Moons of Saturn

{{Use mdy dates|date=November 2025}} {{Short description|Natural satellites of the planet Saturn}} [[File:Saturn - September 9 2007 - Annotated (50316920862).jpg|thumb|upright=2|An annotated picture of Saturn's many moons captured by the ''Cassini'' spacecraft. Shown in the image are Dione, Enceladus, Epimetheus, Prometheus, Mimas, Rhea, Janus, Tethys and Titan.]] [[File:Saturn irregular moon orbits tilted annotated 2025.png|thumb|upright=2|Diagram showing the highly clustered orbits of Saturn's 250 known outer irregular moons {{asof|2025|lc=y}}. The majority of these irregular moons orbit retrograde, or opposite to the direction of Saturn's rotation. The orbits of retrograde moons are colored red while the orbits of prograde moons are colored blue.]]

Saturn has 292 moons with confirmed orbits as of 9 April 2026, the most of any planet in the Solar System.<ref name="jplsats-disc"/> Saturn's moons are diverse in size, ranging from tiny moonlets to Titan, which is larger than the planet Mercury and the second largest moon in the Solar System. Three of these moons possess particularly notable features: Titan has a nitrogen-rich, Earth-like atmosphere and a landscape featuring river networks and hydrocarbon lakes,<ref>{{cite web |last=Redd |first=Nola Taylor |url=https://www.space.com/15257-titan-saturn-largest-moon-facts-discovery-sdcmp.html |title=Titan: Facts About Saturn's Largest Moon |work=Space.com |date=27 March 2018 |access-date=7 October 2019 |archive-date=15 October 2017 |archive-url=https://web.archive.org/web/20171015185936/https://www.space.com/15257-titan-saturn-largest-moon-facts-discovery-sdcmp.html |url-status=live}}</ref> Enceladus emits jets of ice from its south-polar region and is covered in a deep layer of snow,<ref>{{cite web|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Enceladus|title=Enceladus - Overview - Planets - NASA Solar System Exploration|url-status=dead|archive-url=https://web.archive.org/web/20130217190247/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Enceladus|archive-date=2013-02-17}}</ref> and Iapetus has contrasting black and white hemispheres as well as an extensive ridge of equatorial mountains which are among the tallest in the Solar System.

Twenty-four of the confirmed moons are regular satellites; they have prograde orbits not greatly inclined to Saturn's equatorial plane (except Iapetus, which has a prograde but significantly inclined orbit).<ref>{{cite web|url=http://abyss.uoregon.edu/~js/ast121/lectures/lec17.html|title=Moons|access-date=2013-02-13|archive-date=2013-04-20|archive-url=https://web.archive.org/web/20130420125226/http://abyss.uoregon.edu/~js/ast121/lectures/lec17.html|url-status=live}}</ref><ref>{{Cite web|url=https://science.nasa.gov/saturn/moons/iapetus/|title=Iapetus - NASA Science|website=science.nasa.gov|date=December 2017 |access-date=2024-01-06|archive-date=2024-01-06|archive-url=https://web.archive.org/web/20240106100409/https://science.nasa.gov/saturn/moons/iapetus/|url-status=live}}</ref><ref>{{cite web | url=https://www.nasa.gov/image-article/view-from-iapetus/#:~:text=the%20Saturn%20System.-,Iapetus%20(1%2C468%20kilometers%2C%20or%20912%20miles%20across)%20is%20the,a%20tilt%2C%20as%20seen%20here | title=The View from Iapetus - NASA | access-date=2024-01-06 | archive-date=2024-06-16 | archive-url=https://web.archive.org/web/20240616103717/https://www.nasa.gov/image-article/view-from-iapetus/#:~:text=the%20Saturn%20System.-,Iapetus%20(1%2C468%20kilometers%2C%20or%20912%20miles%20across)%20is%20the,a%20tilt%2C%20as%20seen%20here | url-status=live}}</ref> They include the seven rounded satellites, and four small moons that exist in a trojan orbit with some of the large moons. Four orbit inside of the diffuse G ring or between the major moons Mimas and Enceladus. Two moons are mutually co-orbital, Janus and Epimetheus. The relatively large Hyperion is locked in an orbital resonance with Titan. The remaining regular moons orbit near the edges of or within gaps in the main rings, some of which act as shepherd moons of the dense A Ring and the narrow F Ring. The regular satellites are traditionally named after Titans and Titanesses or other figures associated with the mythological Saturn, and one, S/2009 S 1, remains unnamed.

The remaining 268 moons, with mean diameters ranging from {{cvt|2 to 213|km|mi|0}}, orbit much farther from Saturn. They are irregular satellites, which have high orbital inclinations and eccentricities mixed between prograde and retrograde. These moons are probably captured minor planets, or fragments from the collisional breakup of such bodies after they were captured, creating collisional families. The irregular satellites are classified by their orbital characteristics into the prograde Inuit and Gallic groups and the large retrograde Norse group, and their names are chosen from the corresponding mythologies (with the Gallic group corresponding to Celtic mythology). Phoebe, the largest irregular Saturnian moon, is the sole exception to this naming system; it is part of the Norse group but named for a Greek Titaness. {{as of|2026|4|post=,}} 228 of Saturn's irregular moons are unnamed.<ref name="SheppardMoons"/>

The rings of Saturn are made of objects ranging in size from microscopic to moonlets hundreds of meters across, each in its own orbit around Saturn.<ref name="Esposito2002" /> The number of moons given above does not include these moonlets, nor hundreds of possible kilometer-sized distant moons that have been observed on single occasions.<ref name="SheppardMoons" /><ref name="Tiscareno2008" /><ref name="Ashton2021" /> Thus an absolute number of Saturnian moons cannot be given, because there is no consensus on a boundary between the countless small unnamed objects that form Saturn's ring system and the larger objects that have been named as moons. Over 150 moonlets embedded in the rings have been detected by the disturbance they create in the surrounding ring material, though this is thought to be only a small sample of the total population of such objects.<ref name=Tiscareno2008/>

==Discovery== ===Early observations=== [[File:Iapetus-2010Mar04.jpg|thumb|Saturn (overexposed) and the moons Iapetus, Titan, Dione, Hyperion, and Rhea viewed through a 12.5-inch telescope|alt=A large bright circle in the center is surrounded by small circles.]] Before the advent of telescopic photography, eight moons of Saturn were discovered by direct observation using optical telescopes. Saturn's largest moon, Titan, was discovered in 1655 by Christiaan Huygens using a {{convert|57|mm|in|1|adj=on|sp=us}} objective lens<ref name="ap050325" /> on a refracting telescope of his own design.<ref name="Baalke" /> Tethys, Dione, Rhea and Iapetus (the "Sidera Lodoicea") were discovered between 1671 and 1684 by Giovanni Domenico Cassini.<ref name=Helden1994/> Mimas and Enceladus were discovered in 1789 by William Herschel.<ref name=Helden1994/> Hyperion was discovered in 1848 by W. C. Bond, G. P. Bond<ref name=Bond1848/> and William Lassell.<ref name=Lassell1848/>

The use of long-exposure photographic plates made possible the discovery of additional moons. The first to be discovered in this manner, Phoebe, was found in 1899 by W. H. Pickering.<ref name=Pickering1899/> In 1966 the tenth satellite of Saturn was discovered by Audouin Dollfus, when the rings were observed edge-on near an equinox.<ref name=Fountain1977/> It was later named Janus. A few years later it was realized that all observations of 1966 could only be explained if another satellite had been present and that it had an orbit similar to that of Janus.<ref name=Fountain1977/> This object is now known as Epimetheus, the eleventh moon of Saturn. It shares the same orbit with Janus—the only known example of co-orbitals in the Solar System.<ref name=Uralskaya1998/> In 1980, three additional Saturnian moons were discovered from the ground and later confirmed by the ''Voyager'' probes. They are trojan moons of Dione (Helene) and Tethys (Telesto and Calypso).<ref name=Uralskaya1998/>

===Observations by spacecraft=== thumb|Five moons in a Cassini image: Rhea bisected in the far-right foreground, Mimas behind it, bright Enceladus above and beyond the rings, Pandora eclipsed by the F Ring, and Janus off to the left

The study of the outer planets has since been revolutionized by the use of uncrewed space probes. The arrival of the ''Voyager'' spacecraft at Saturn in 1980–1981 resulted in the discovery of three additional moons—Atlas, Prometheus and Pandora—bringing the total to 17.<ref name=Uralskaya1998/> In addition, Epimetheus was confirmed as distinct from Janus. In 1990, Pan was discovered in archival ''Voyager'' images.<ref name=Uralskaya1998/>

The ''Cassini'' mission,<ref name="NYT-20151218-jc">{{cite news |last=Corum |first=Jonathan |title=Mapping Saturn's Moons |url=https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |date=December 18, 2015 |work=The New York Times |access-date=December 18, 2015 |archive-date=May 20, 2020 |archive-url=https://web.archive.org/web/20200520124847/https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |url-status=live}}</ref> which arrived at Saturn in July 2004, initially discovered three small inner moons: Methone and Pallene between Mimas and Enceladus, and the second trojan moon of Dione, Polydeuces. It also observed three suspected but unconfirmed moons in the F Ring.<ref name=Porco2005/> In {{Nowrap|November 2004}} Cassini scientists announced that the structure of Saturn's rings indicates the presence of several more moons orbiting within the rings, although only one, Daphnis, had been visually confirmed at the time.<ref name=Britt2004/> In 2007 Anthe was announced.<ref name=IAUC2007/> In 2008 it was reported that ''Cassini'' observations of a depletion of energetic electrons in Saturn's magnetosphere near Rhea might be the signature of a tenuous ring system around Saturn's second largest moon.<ref name=Jones2008/> In {{Nowrap|March 2009}}, Aegaeon, a moonlet within the G Ring, was announced.<ref name="IAUC2009" /> In July of the same year, S/2009 S 1, the first moonlet within the B Ring, was observed.<ref name="IAUC2009b" /> In April 2014, the possible beginning of a new moon, within the A Ring, was reported.<ref name="NASA-20140414a">{{cite web |last1=Platt |first1=Jane |last2=Brown |first2=Dwayne |title=NASA Cassini Images May Reveal Birth of a Saturn Moon |url=http://www.jpl.nasa.gov/news/news.php?release=2014-112 |date=14 April 2014 |work=NASA |access-date=14 April 2014 |archive-date=10 April 2019 |archive-url=https://web.archive.org/web/20190410120305/https://www.jpl.nasa.gov/news/news.php?release=2014-112 |url-status=live}}</ref> (related image)

===Search for irregulars=== [[File:2019 S 1 shift-and-add demonstration.png|thumb|This image demonstrates the application of the shift-and-add technique to the detection of a faint moon of Saturn (S/2019 S 1; circled in red). While the moon is barely visible in an individual image (top panel), it can be seen better when many images of the moon are taken, stacked to the moon's motion and then added together (bottom panel)]] Study of Saturn's moons has also been aided by advances in telescope instrumentation, primarily the introduction of digital charge-coupled devices which replaced photographic plates. For the 20th century, Phoebe stood alone among Saturn's known moons with its highly irregular orbit. Then in 2000, a team of astronomers led by Brett J. Gladman discovered twelve irregular moons of Saturn using various ground-based telescopes around the world.<ref name=Gladman2001/><ref name=Jewitt2007/> The discovery of these irregular moons revealed orbital groupings within Saturn's irregular moon population, which provided the first insights into the collisional history of Saturn's irregular moons.<ref name=Jewitt2007/>

In 2003, a team of astronomers including Scott Sheppard, David C. Jewitt, and Jan Kleyna began using the Subaru 8.2&nbsp;m telescope at Mauna Kea Observatory to search for irregular moons around Saturn, and discovered Narvi.<ref name=Jewitt2007/> Because of the Subaru telescope's very large aperture size alongside its camera's large field of view, it is capable of detecting extremely faint moons, hence Sheppard's team continued using the Subaru telescope for further moon searches.<ref name=Jewitt2007/> In 2005, Sheppard's team announced the discovery of twelve more small outer moons from their Subaru observations.<ref name=Jewitt2005/><ref name=Lakdawalla2005/> Sheppard's team announced nine more irregular moons in 2006<ref name=IAUC8727/> and three more moons in 2007, when Tarqeq was announced in {{Nowrap|April 2007}}, followed by S/2007 S 2 and S/2007 S 3 the following month.<ref name=IAUC8836/>

No new irregular moons of Saturn were reported until 2019, when Sheppard's team identified twenty more irregular satellites of Saturn in archives of their 2004–2007 Subaru observations. This brought Saturn's moon count to 82, which resulted in Saturn overtaking Jupiter as the planet with the most known moons for the first time since 2000.<ref name="Carnegie2019">{{cite web|title=Saturn Surpasses Jupiter After The Discovery Of 20 New Moons And You Can Help Name Them!|url=https://carnegiescience.edu/news/saturn-surpasses-jupiter-after-discovery-20-new-moons-and-you-can-help-name-them|publisher=Carnegie Science|date=7 October 2019|access-date=7 October 2019|archive-date=6 June 2020|archive-url=https://web.archive.org/web/20200606203854/https://carnegiescience.edu/news/saturn-surpasses-jupiter-after-discovery-20-new-moons-and-you-can-help-name-them|url-status=live}}</ref><ref name="SheppardMoons" /> In 2019, researchers Edward Ashton, Brett Gladman, and Matthew Beaudoin conducted a survey of Saturn's Hill sphere using the 3.6-meter Canada–France–Hawaii Telescope (CFHT) and discovered about 80 new Saturnian irregular moons, which were reported to the Minor Planet Center (MPC) for announcement.<ref name="Ashton2021"/><ref name="Ashton2022"/> Follow-up observations of these new moons took place over 2019–2021, eventually leading to S/2019 S 1 being announced in November 2021 and an additional 62 moons being announced from 3–16 May 2023.<ref name="UBC-20230511"/><ref name="MPEC-2023-K118"/> These discoveries brought Saturn's total number of confirmed moons up to 145, making it the first planet known to have over 100 moons.<ref name="UBC-20230511"/><ref name="NYT-20230512">{{cite news |last=O'Callaghan |first=Jonathan |title=With 62 Newly Discovered Moons, Saturn Knocks Jupiter Off Its Pedestal - If all the objects are recognized by scientific authorities, the ringed giant world will have 145 moons in its orbit. |url=https://www.nytimes.com/2023/05/12/science/saturn-moons-jupiter.html |date=12 May 2023 |work=The New York Times |url-status=live |archiveurl=https://archive.today/20230512174454/https://www.nytimes.com/2023/05/12/science/saturn-moons-jupiter.html |archivedate=12 May 2023 |accessdate=13 May 2023}}</ref> Yet another moon, S/2006 S 20, was announced on 23 May 2023, bringing Saturn's total count moons to 146.<ref name="MPEC-2023-K118"/> On 11 March 2025, 128 moons of Saturn were simultaneously announced by the MPC,<ref name="MPEC-2025-E155">{{cite web |date=11 March 2025 |title=MPEC 2025-E155 : THIRTY-THREE NEW SATURNIAN SATELLITES |url=https://minorplanetcenter.net/mpec/K25/K25EF5.html |accessdate=11 March 2025 |publisher=Minor Planet Center}}</ref> bringing the total number of confirmed moons to 274.<ref name="Ashton2025b" /><ref name="UBC2025">{{Cite news |date=11 March 2025 |title=2025 Discovery of more Saturnian Moons |url=https://phas.ubc.ca/2025-discovery-more-saturnian-moons |accessdate=12 March 2025 |work=The University of British Columbia |publisher=The University of British Columbia}}</ref><ref>{{Cite news |date=11 March 2025 |title=Saturn has 128 new moons – more than the rest of the planets combined |url=https://www.newscientist.com/article/2471071-saturn-has-128-new-moons-more-than-the-rest-of-the-planets-combined/ |accessdate=12 March 2025 |work=New Scientist |publisher=New Scientist}}</ref> These moons were found by Ashton, Gladman, Mike Alexandersen, and Jean-Marc Petit, using the CFHT in 2023, as a continuation of their survey.<ref name="Ashton2025b" /><ref name="UBC2025" /> Ashton's team also searched in CFHT images taken by a separate team consisting of Wesley Fraser, Samantha Lawler, and John Kavelaars.<ref name="MPEC-2025-E155" /> Many of these moons were traced back to earlier observations from 2004 to 2021, which correspond to their discovery dates.<ref name="MPEC-2025-E155" /> In 2026, 11 moons were announced on 16 March,<ref name="MPEC-2026-F14" /> and an additional seven more on 9 April, bringing the total number of Saturnian moons to 292.

All of these recently announced moons are small and faint, with diameters over {{cvt|3|km|mi|sigfig=1}} and apparent magnitudes of 25–27.<ref name="Ashton2021"/> These extremely dim moons could only be seen via the shift-and-add technique, where multiple long-exposure images are overlaid, shifted to follow the motion of Saturn in the sky, and then additively combined to bring out the signal of faint moons that follow Saturn in the sky.<ref name="Ashton2021"/> The researchers found that the Saturnian irregular moon population is more abundant at smaller sizes, suggesting that they are likely fragments from a collision that occurred a few hundred million years ago. The researchers extrapolated that the true population of Saturnian irregular moons larger than {{cvt|2.8|km|mi|sigfig=2}} in diameter amounts to {{val|150|30}}, which is approximately three times as many Jovian irregular moons down to the same size. If this size distribution applies to even smaller diameters, Saturn would therefore intrinsically have more irregular moons than Jupiter.<ref name="Ashton2021"/>

==Naming== {{Main|Naming of moons}} The modern names for Saturnian moons were suggested by John Herschel in 1847.<ref name=Helden1994/> He proposed to name them after mythological figures associated with the Roman god of agriculture and harvest, Saturn (equated to the Greek Cronus).<ref name=Helden1994/> In particular, the then known seven satellites were named after Titans, Titanesses and Giants – brothers and sisters of Cronus.<ref name=Pickering1899/> The idea was similar to Simon Marius' scheme for naming moons of Jupiter after children of Zeus.<ref name=Helden>{{cite journal |last1=van Helden |first1=Albert |title=Naming the Satellites of Jupiter and Saturn |journal=The Newsletter of the Historical Astronomy Division of the American Astronomical Society |date=August 1994 |issue=32 |url=https://had.aas.org/sites/had.aas.org/files/HADN32.pdf |access-date=10 March 2023 |archive-date=7 December 2022 |archive-url=https://web.archive.org/web/20221207151902/https://had.aas.org/sites/had.aas.org/files/HADN32.pdf |url-status=live}}</ref> <blockquote>As Saturn devoured his children, his family could not be assembled around him, so that the choice lay among his brothers and sisters, the Titans and Titanesses. The name ''Iapetus'' seemed indicated by the obscurity and remoteness of the exterior satellite, ''Titan'' by the superior size of the Huyghenian, while the three female appellations [''Rhea'', ''Dione'', and ''Tethys''] class together the three intermediate Cassinian satellites. The minute interior ones seemed appropriately characterized by a return to male appellations [''Enceladus'' and ''Mimas''] chosen from a younger and inferior (though still superhuman) brood. [''Results of the Astronomical Observations made ... at the Cape of Good Hope'', p.&nbsp;415]</blockquote>

In 1848, Lassell proposed that the eighth satellite of Saturn be named Hyperion after another Titan.<ref name=Lassell1848/><ref name=Helden/> When in the 20th century the names of Titans were exhausted, the moons were named after different characters of the Greco-Roman mythology or giants from other mythologies.<ref name=Gazetteer/> All the irregular moons (except Phoebe, discovered about a century before the others) are named after Inuit, and Gallic gods, and after Norse ice giants.<ref name=Grav2007/> The International Astronomical Union's (IAU) Committee for Planetary System Nomenclature, which oversees the naming of Solar System moons, rules that Saturnian moons that are smaller than 3&nbsp;km in diameter (absolute magnitude H_V&nbsp;>&nbsp;16.5){{efn|If assuming an albedo of 0.04, H_V&nbsp;{{=}}&nbsp;16.5 corresponds to a diameter of 3.3&nbsp;km. The formula for the calculation can be found in absolute magnitude#Small Solar System bodies (H).}} should only be named if they are of scientific interest.<ref name="IAU-rules">{{cite web|title=IAU Rules and Conventions|url=https://planetarynames.wr.usgs.gov/Page/Rules|work=Gazetteer of Planetary Nomenclature|publisher=USGS Astrogeology Science Center|accessdate=16 March 2025}}</ref>

Some asteroids share the same names as moons of Saturn: 55 Pandora, 106 Dione, 577 Rhea, 1809 Prometheus, 1810 Epimetheus, and 4450 Pan. In addition, three more asteroids would share the names of Saturnian moons if not for spelling differences made permanent by the IAU: Calypso and asteroid 53 Kalypso; Helene and asteroid 101 Helena; and Gunnlod and asteroid 657 Gunlöd.

==Formation== There are three main scenarios proposed to explain how the regular moons of Saturn formed. The first scenario proposes that they are remnants of the debris of a giant impact or the disruption of a previous moon system. It is thought that the Saturnian system of Titan, mid-sized moons, and rings developed from a set-up closer to the Galilean moons of Jupiter, though the details are unclear. It has been proposed either that a second Titan-sized moon broke up, producing the rings and inner mid-sized moons,<ref>{{cite journal | last1 = Canup | first1 = R. | author-link = Robin Canup | title = Origin of Saturn's rings and inner moons by mass removal from a lost Titan-sized satellite | journal = Nature | volume = 468| issue = 7326| pages = 943–6| doi = 10.1038/nature09661 | pmid=21151108 | date=December 2010|bibcode = 2010Natur.468..943C | s2cid = 4326819}}</ref> or that two large moons fused to form Titan, with the collision scattering icy debris that formed the mid-sized moons.<ref name="Asphaug2013" /> Studies based on Enceladus's tidal-based geologic activity and the lack of evidence of extensive past resonances in Tethys, Dione, and Rhea's orbits suggest that the moons up to and including Rhea may be only 100 million years old.<ref>{{cite magazine|url=http://www.astronomy.com/news/2016/03/moons-of-saturn-may-be-younger-than-the-dinosaurs|title=Moons of Saturn may be younger than the dinosaurs|author=SETI Institute|magazine=Astronomy|date=March 25, 2016|author-link=SETI Institute|access-date=March 30, 2016|archive-date=December 6, 2019|archive-url=https://web.archive.org/web/20191206163235/https://astronomy.com/news/2016/03/moons-of-saturn-may-be-younger-than-the-dinosaurs|url-status=live}}</ref>

Another more generic theory proposes that they that formed directly from the original circumplanetary disk around Saturn. The gas giants, Jupiter and Saturn, are expected to have had circumplanetary disks, while this is considered unlikely for the ice giants Uranus and Neptune. The moons may have originated from the higher-density regions within the disk, and the mass of the system may be a reflection of the mass of the disk. Alternatively, several sets of moons may have formed then fallen out of their orbits due to drag with the disk, leading to the survival of only one large moon (Titan).<ref name="Blanc2025"/>

The third idea is that moons coalesced from a previously much more massive set of rings. This would explain the existence of the small regular moons and the mid-sized moons interior to Titan. The ring system would have spread outward over time, some of it beyond the Roche limit of Saturn, allowing that material to accrete into moons. The moons would continue migrating outwards due to gravitation interactions with the rings but slow down the further away they move, leading to them colliding and merging. This means that moons farther away are older and tend to be more massive. This model does not address the origin of the ring system itself.<ref name="Blanc2025"/>

==Mass distribution== Saturn's satellite system is very lopsided: the largest moon, Titan, comprises 96% of the mass in orbit around the planet. The six other planemo (ellipsoidal) moons constitute 4% of the mass. These seven moons are large enough to have collapsed into a relaxed, ellipsoidal shape, though only one or two, Titan and possibly<!--shape of Rhea consistent w HE, but not demonstrated to be in HE since it spun down--> Rhea, are currently in hydrostatic equilibrium. The remaining small moons, together with the rings, comprise only 0.04% of the orbiting mass.{{refn | group = lower-alpha | The mass of the rings is about 0.40 times the mass of Mimas, whereas the combined mass of Janus, Hyperion and Phoebe—the most massive of the remaining moons—is about one-third. The total mass of the rings and small moons is around {{val|5.5|e=19|u=kg}}.}}

{{image frame |content=<div style="display:flex; justify-content: center;">{{Pie chart |1= [ {"value":0.04, "label": "Mimas $d"}, {"value":0.11, "label": "Enceladus $d"}, {"value":0.62, "label": "Tethys $d"}, {"value":1.1, "label": "Dione $d"}, {"value":2.3, "label": "Rhea $d"}, {"value":134.5, "label": "Titan $d"}, {"value":1.8, "label": "Iapetus $d"}, ] |legend=true |autoscale=true |radius=100 |border=no }} {{Pie chart |1= [ {"value":0.04, "label": "Mimas $d"}, {"value":0.11, "label": "Enceladus $d"}, {"value":0.62, "label": "Tethys $d"}, {"value":1.1, "label": "Dione $d"}, {"value":2.3, "label": "Rhea $d"}, {"value":0, "label": "[Titan omitted] $d"}, {"value":1.8, "label": "Iapetus $d"}, ] |legend=true |autoscale=true |radius=100 |border=no }}</div> |max-width=670 |align=none |caption=The relative masses of Saturn's moons. Values are ×10²¹&nbsp;kg. With Titan in the comparison (left), Mimas and Enceladus are invisible at this scale. Even excluding Titan (right), Phoebe, Hyperion, the smaller moons and the rings are invisible. |border=no |mode=scrollable }}

{| class="wikitable sortable" style="clear:left;text-align:center;" |+ Saturn's major satellites, compared with the Moon |- ! Name<br> ! data-sort-type="number" | Diameter<br>(km)<ref name="Thomas2010" /> ! data-sort-type="number" | Mass<br>(kg)<ref name="Jacobson Antreasian et al. 2006" /> ! data-sort-type="number" | Orbital radius<br>(km)<ref name="NASA" /> ! data-sort-type="number" | Orbital period<br>(days)<ref name="NASA" /> |- | '''Mimas''' || 396<br>(0.12&nbsp;''D''_☾) || data-sort-value="4.0E19" | 4×10¹⁹<br>(0.0005&nbsp;''M''_☾) || 185,539<br>(0.48&nbsp;''a''_☾) || 0.9<br>(0.03&nbsp;''T''_☾) |- | '''Enceladus''' || 504<br>(0.14&nbsp;''D''_☾) || data-sort-value="1.1E20" | 1.1×10²⁰<br>(0.002&nbsp;''M''_☾) || 237,948<br>(0.62&nbsp;''a''_☾) || 1.4<br>(0.05&nbsp;''T''_☾) |- | '''Tethys''' || 1,062<br>(0.30&nbsp;''D''_☾) || data-sort-value="6.2E20" | 6.2×10²⁰<br>(0.008&nbsp;''M''_☾) || 294,619<br>(0.77&nbsp;''a''_☾) || 1.9<br>(0.07&nbsp;''T''_☾) |- | '''Dione''' || 1,123<br>(0.32&nbsp;''D''_☾) || data-sort-value="1.1E21" | 1.1×10²¹<br>(0.015&nbsp;''M''_☾) || 377,396<br>(0.98&nbsp;''a''_☾) || 2.7<br>(0.10&nbsp;''T''_☾) |- | '''Rhea''' || 1,527<br>(0.44&nbsp;''D''_☾) || data-sort-value="2.3E21" | 2.3×10²¹<br>(0.03&nbsp;''M''_☾) || 527,108<br>(1.37&nbsp;''a''_☾) || 4.5<br>(0.20&nbsp;''T''_☾) |- | '''Titan''' || 5,149<br>(1.48&nbsp;''D''_☾)<br>(0.75&nbsp;''D''_♂) || data-sort-value="1.35E23" | 1.35×10²³<br>(1.80&nbsp;''M''_☾)<br>(0.21&nbsp;''M''_♂) || 1,221,870<br>(3.18&nbsp;''a''_☾) || 16<br>(0.60&nbsp;''T''_☾) |- | '''Iapetus''' || 1,470<br>(0.42&nbsp;''D''_☾) || data-sort-value="1.8E21" | 1.8×10²¹<br>(0.025&nbsp;''M''_☾) || 3,560,820<br>(9.26&nbsp;''a''_☾) || 79<br>(2.90&nbsp;''T''_☾) |}

==Characteristics and groups== thumb|upright=2.0|Artist conception of Saturn, its rings and major icy moons—from Mimas to Rhea Although the boundaries may be somewhat vague, Saturn's moons can be divided into several groups according to their orbital characteristics. Many of them, such as Pan and Daphnis, orbit within Saturn's ring system and have orbital periods only slightly longer than the planet's rotation period.<ref name="Porco2007" /> The innermost moons and most regular satellites all have mean orbital inclinations ranging from less than a degree to about 1.5 degrees (except Iapetus, which has an inclination of 7.57 degrees) and small orbital eccentricities.<ref name="SheppardMoons" /> Some of the small inner moons are shepherd satellites, which have the effect of sculpting the rings: giving them sharp edges, and creating gaps between them. On the other hand, irregular satellites in the outermost regions of Saturn's moon system, in particular the Norse group, have orbital radii of millions of kilometers and orbital periods lasting several years. The moons of the Norse group also orbit in the opposite direction to Saturn's rotation.<ref name="Grav2007" />

=== Inner moons ===

==== Inner ring moons ==== {{multiple image | caption_align = center | align = right | width = 200 | direction = vertical | image1 = PIA21056 - Daphnis Up Close.jpg | caption1 = Shepherd moon Daphnis creating waves in Saturn's A Ring | image2 = PIA12684 F Ring.png | caption2 = Shepherd moon Prometheus disturbing Saturn's F Ring }}

These satellites orbit the closest to Saturn, occupying spaces between the gaps or on the edges of the main rings.<ref name="Ciarniello et al. 2024">{{Cite journal |last=Ciarniello|first=Mauro|last2=Filacchione|first2=Gianrico|last3=Nicholson|first3=Philip D.|last4=Hedman|first4=Matthew M.|last5=Charnoz|first5=Sebastien|last6=Cuzzi|first6=Jeffrey N.|last7=El Moutamid|first7=Maryame|last8=Hendrix|first8=Amanda R.|last9=Rambaux|first9=Nicolas|last10=Miller|first10=Kelly E.|last11=Mousis|first11=Olivier|last12=Baillié|first12=Kevin|last13=Estrada|first13=Paul R.|last14=Waite|first14=J. Hunter|date=2024-09-17|title=The Origin and Composition of Saturn’s Ring Moons|url=https://doi.org/10.1007/s11214-024-01103-z|journal=Space Science Reviews|language=en|volume=220|issue=7|pages=72|doi=10.1007/s11214-024-01103-z|issn=1572-9672|doi-access=free}}</ref> Several act as shepherd moons, and they are Pan (Encke gap), Daphnis (Keeler gap), and Prometheus (F Ring).<ref name="Porco2005" /> Atlas and Pandora orbit on the outside edge of the A Ring and F Ring respectively, and were long thought to be shepherds as well, until more recent studies began to indicate otherwise. These moons likely formed as a result of accretion of the friable ring material on preexisting denser cores. The cores with sizes from one-third to one-half the present-day moons may be themselves collisional shards formed when a parental satellite of the rings disintegrated.<ref name="Porco2007" />

==== Co-orbitals ==== Janus and Epimetheus are co-orbital moons.<ref name="Uralskaya1998" /> They are of similar size, with Janus being somewhat larger than Epimetheus.<ref name="Porco2007" /> They have orbits with less than a 100-kilometer difference in semi-major axis, close enough that they would collide if they attempted to pass each other. Instead of colliding, their gravitational interaction causes them to swap orbits every four years.<ref name="Spitale Jacobson et al. 2006" /> Both moons additionally act as shepherds for the A Ring.<ref name="Porco2005" />

==== {{anchor|The Alkyonides|Alkyonides}} Ring-embedded moons ==== [[File:Aegaeon (2008 S1).jpg|thumb|right|Sequence of ''Cassini'' images of Aegaeon embedded within the bright arc of Saturn's G Ring]] These four moons' orbits are embedded within their own faint rings or partial arcs, and serve as sources of material within their respective ring structures. They are some of the smallest moons in the Saturnian system.<ref name="Ciarniello et al. 2024" /> Aegaeon resides within the bright arc of G Ring, while the other three moons, Methone, Anthe, and Pallene, orbit between the major moons Mimas and Enceladus. The latter three are sometimes collectively referred to as the Alkyonides, named after those of Greek mythology.

Aegaeon is trapped in the 7:6 mean-motion resonance with Mimas,<ref name="IAUC2009" /> meaning that it makes exactly seven revolutions around Saturn while Mimas makes exactly six. The moon is the largest among the population of bodies that are sources of dust in the G ring.<ref name="Hedman2007" /> Aegaeon, Anthe, and Methone are involved in orbital resonances, resulting in ring arcs along their orbits. Ejecta from their surfaces remains locked in the same resonance as the moon is, shaping into an arc instead of a uniform ring. In contrast, Pallene, which is not in resonance, possesses a faint, complete ring.<ref name="Alkyonides" /><ref>{{Cite journal|title=The Origin and Composition of Saturn’s Ring Moons|url=https://doi.org/10.1007/s11214-024-01103-z|journal=Space Science Reviews|date=2024-09-17|issn=1572-9672|pages=72|volume=220|issue=7|doi=10.1007/s11214-024-01103-z|language=en|first=Mauro|last=Ciarniello|first2=Gianrico|last2=Filacchione|first3=Philip D.|last3=Nicholson|first4=Matthew M.|last4=Hedman|first5=Sebastien|last5=Charnoz|first6=Jeffrey N.|last6=Cuzzi|first7=Maryame|last7=El Moutamid|first8=Amanda R.|last8=Hendrix|first9=Nicolas|last9=Rambaux|first10=Kelly E.|last10=Miller|first11=Olivier|last11=Mousis|first12=Kevin|last12=Baillié|first13=Paul R.|last13=Estrada|first14=J. Hunter|last14=Waite|doi-access=free}}</ref>

Imagery shows that Aegaeon, Methone, and Pallene are much darker than expected, possibly due to exposure to high-energy radiation.<ref name="Hedman2020"/> Methone and Pallene are the only moons that have been imaged in any detail, revealing them to be morphologically different from any small moon, asteroid, or comet imaged previously.<ref>{{Cite journal |ref={{sfnRef|Thomas et al.|2013}}|last=Thomas |first=P. C. |last2=Burns |first2=J. A. |last3=Hedman |first3=M. |last4=Helfenstein |first4=P. |last5=Morrison |first5=S. |last6=Tiscareno |first6=M. S. |last7=Veverka |first7=J. |date=2013-09-01 |title=The inner small satellites of Saturn: A variety of worlds |url=https://www.sciencedirect.com/science/article/pii/S0019103513003230 |journal=Icarus |volume=226 |issue=1 |pages=999–1019 |doi=10.1016/j.icarus.2013.07.022 |issn=0019-1035|url-access=subscription }}</ref> Of the two, only Methone has been imaged from close range, showing it to be egg-shaped with very few or no craters.<ref>{{cite web |last1=Lakdawalla |first1=Emily |author-link1=Emily Lakdawalla |title=Methone, an egg in Saturn orbit? |url=http://www.planetary.org/blogs/emily-lakdawalla/2012/05211206.html |website=Planetary Society |access-date=27 April 2019 |archive-date=27 April 2019 |archive-url=https://web.archive.org/web/20190427233242/http://www.planetary.org/blogs/emily-lakdawalla/2012/05211206.html |url-status=live}}</ref>

==== Trojans ====

Trojan moons are a unique feature only known from the Saturnian system. A trojan body orbits at either the leading L₄ or trailing L₅ Lagrange point of a much larger object, such as a large moon or planet. Tethys has two trojan moons, Telesto (leading) and Calypso (trailing), and Dione also has two, Helene (leading) and Polydeuces (trailing).<ref name="Porco2005" /> Helene is the largest trojan moon, while Polydeuces is by far the smallest and has the most chaotic orbit.<ref name="Spitale Jacobson et al. 2006" /> These moons are coated with dusty material that has smoothed out their surfaces.<ref>{{Cite web|url=https://www.planetary.org/articles/2078|title=Cassini goodies: Telesto, Janus, Prometheus, Pandora, F ring|website=The Planetary Society}}</ref>

===Major moons=== {{multiple image | header = Saturn's major moons | caption_align = center | align = right | direction = vertical | image1 = Mimas.jpg | caption1 = Image of Mimas from ''Cassini''. The large crater Herschel is visible. | image2 = Fountains of Enceladus PIA07758.jpg | caption2 = Enceladus ejecting icy particles from its south polar plumes | image3 = PIA18355-SaturnMoon-Tethys-20151123.jpg | caption3 = Tethys and the rings of Saturn | image4 = Dione and Saturn.jpg | caption4 = Color view of Dione in front of Saturn | image5 = PIA08148 (Rhea-Splat).jpg | caption5 = Inktomi or "The Splat", a relatively young crater with prominent butterfly-shaped ejecta on Rhea's leading hemisphere | alt5 = A spherical body is almost fully illuminated. Its grayish surface is covered by numerous circular craters. The terminator is located near the upper-right limb. A large crater can be seen near the limb in the upper-left part of the body. Another smaller bright crater can be seen in the center. It is surrounded by a large bright patch having the shape of a five-pointed star. | image6 = Ringside with Titan and Dione.jpg | caption6 = Titan in front of Dione and the rings of Saturn | image7 = PIA17193-SaturnMoon-Hyperion-20150531.jpg | caption7 = ''Cassini'' image of Hyperion | alt7 = An irregularly-shaped and heavily cratered body, pock-marked with dark pits and ridges on its tan-colored icy surface. | image8 = Iapetus equatorial ridge.jpg | caption8 = Equatorial ridge on Iapetus | alt8 = A part of a spherical body illuminated from the above and behind. The convex limb runs from the lower-left to the upper-right corner. The black outer space is in the upper-left corner. The terminator is near the bottom. The surface of the body is covered with numerous craters. A large ridge runs in the center from the top to bottom. }}

In the Saturnian system, there are seven moons large enough to be ellipsoidal, though Hyperion is often taken with them to make eight major moons. Sometimes Phoebe is included as well, though usually it is placed with the irregular satellites (see below). The moons inward of Titan orbit within Saturn's tenuous E Ring. The three smaller moons of the Alkyonides group and the trojan moons orbit with the innermost four moons. *Mimas is the smallest and least massive of the round moons, although its mass is sufficient to alter the orbit of Methone.<ref name="Spitale Jacobson et al. 2006" /> It is noticeably ovoid-shaped, having been made shorter at the poles and longer at the equator (by about 20&nbsp;km) by the effects of Saturn's gravity.<ref name="Thomas2007" /> Mimas has a large impact crater one-third its diameter, Herschel, situated on its leading hemisphere.<ref name="Moore Schenk et al. 2004" /> Mimas has no known past or present geologic activity and its surface is dominated by impact craters, though it does have a water ocean 20–30&nbsp;km beneath the surface.<ref>{{Cite journal |last1=Lainey |first1=V |last2=Rambaux |first2=N |last3=Tobie |first3=G |last4=Cooper |first4=N |last5=Zhang |first5=Q |last6=Noyelles |first6=B |last7=Baillié |first7=K |date=2024-02-07 |title=A recently formed ocean inside Saturn's moon Mimas |url=https://www.nature.com/articles/s41586-023-06975-9.epdf?sharing_token=vYAG4f049M5kK2gX7OfZg9RgN0jAjWel9jnR3ZoTv0MN0ukW__TUAf43EkTwisrqQJAdNax6CY-KTbuDYP9edZjI9EdTKQHqBQ7K4elhr_eA7eCcg60b2Fa-ecxLjrdaHL789s2t1YlS3e4-7nwjkbYcddy-Gnh3L73x_IXMKpuk6IXunnHmMERXqVHjOrcX0QRIEEolq8Efgnu3Kz1-6vBxMaerFbOz8sldPmErHwqNcmCFFYGSE3pLfIeaGK87Lisfz_gHA_dN9cqMDnl_asFvF8X4cvtD9qTYp0xwrzzdoKkTp2J5UhquPn7vGF4R |journal=Nature |language=en |volume=626 |issue=7998 |pages=280–282 |doi=10.1038/s41586-023-06975-9 |pmid=38326592 |bibcode=2024Natur.626..280L |s2cid=267546453 |issn=1476-4687 |access-date=2024-02-07 |archive-date=2024-06-16 |archive-url=https://web.archive.org/web/20240616103720/https://www.nature.com/articles/s41586-023-06975-9.epdf?sharing_token=vYAG4f049M5kK2gX7OfZg9RgN0jAjWel9jnR3ZoTv0MN0ukW__TUAf43EkTwisrqQJAdNax6CY-KTbuDYP9edZjI9EdTKQHqBQ7K4elhr_eA7eCcg60b2Fa-ecxLjrdaHL789s2t1YlS3e4-7nwjkbYcddy-Gnh3L73x_IXMKpuk6IXunnHmMERXqVHjOrcX0QRIEEolq8Efgnu3Kz1-6vBxMaerFbOz8sldPmErHwqNcmCFFYGSE3pLfIeaGK87Lisfz_gHA_dN9cqMDnl_asFvF8X4cvtD9qTYp0xwrzzdoKkTp2J5UhquPn7vGF4R |url-status=live}}</ref> The only tectonic features known are a few arcuate and linear troughs, which probably formed when Mimas was shattered by the Herschel impact.<ref name="Moore Schenk et al. 2004" /> *Enceladus is one of the smallest of Saturn's moons that is spherical in shape—only Mimas is smaller—yet is the only small Saturnian moon that is currently endogenously active, and the smallest known body in the Solar System that is geologically active today.<ref name="Porco Helfenstein et al. 2006" /> Its surface is morphologically diverse; it includes ancient heavily cratered terrain as well as younger smooth areas with few impact craters. Many plains on Enceladus are fractured and intersected by systems of lineaments. The area around its south pole was found by ''Cassini'' to be unusually warm and cut by a system of fractures about 130&nbsp;km long called "tiger stripes", some of which emit jets of water vapor and dust.<ref name="Porco Helfenstein et al. 2006" /> These jets form a large plume off its south pole, which replenishes Saturn's E ring<ref name="Porco Helfenstein et al. 2006" /> and serves as the main source of ions in the magnetosphere of Saturn.<ref name="Pontius2006" /> The gas and dust are released with a rate of more than 100&nbsp;kg/s. Enceladus may have liquid water underneath the south-polar surface.<ref name="Porco Helfenstein et al. 2006" /> The source of the energy for this cryovolcanism is thought to be a 2:1 mean-motion resonance with Dione. The pure ice on the surface makes Enceladus one of the brightest known objects in the Solar System—its geometrical albedo is more than 140%.<ref name="Porco Helfenstein et al. 2006" /> *Tethys is the fifth largest of Saturn's moons. Its most prominent features are a large (400&nbsp;km diameter) impact crater named Odysseus on its leading hemisphere and a vast canyon system named Ithaca Chasma extending at least 270° around Tethys.<ref name="Moore Schenk et al. 2004" /> The Ithaca Chasma is concentric with Odysseus, and these two features may be related. Tethys appears to have no current geological activity. A heavily cratered hilly terrain occupies the majority of its surface, while a smaller and smoother plains region lies on the hemisphere opposite to that of Odysseus. The plains contain fewer craters and are apparently younger. A sharp boundary separates them from the cratered terrain. There is also a system of extensional troughs radiating away from Odysseus.<ref name="Moore Schenk et al. 2004" /> The density of Tethys (0.985&nbsp;g/cm³) is less than that of water, indicating that it is made mainly of water ice with only a small fraction of rock.<ref name="Thomas2010" /> * Dione is the fourth-largest moon of Saturn. It has a higher density than the geologically dead Rhea, but lower than that of active Enceladus.<ref name="Thomas2007" /> While the majority of Dione's surface is heavily cratered old terrain, this moon is also covered with an extensive network of troughs and lineaments, indicating that in the past it had global tectonic activity.<ref name="Wagner2009" /> The troughs and lineaments are especially prominent on the trailing hemisphere, where several intersecting sets of fractures form what is called "wispy terrain".<ref name="Wagner2009" /> The cratered plains have a few large impact craters reaching 250&nbsp;km in diameter.<ref name="Moore Schenk et al. 2004" /> Smooth plains with low impact-crater counts are also present on a small fraction of its surface.<ref name="Schenk2009b" /> They were probably tectonically resurfaced relatively later in the geological history of Dione. At two locations within smooth plains strange landforms (depressions) resembling oblong impact craters have been identified, both of which lie at the centers of radiating networks of cracks and troughs;<ref name="Schenk2009b" /> these features may be cryovolcanic in origin. Dione may be geologically active even now, although on a scale much smaller than the cryovolcanism of Enceladus. This follows from Cassini magnetic measurements that show Dione is a net source of plasma in the magnetosphere of Saturn, much like Enceladus.<ref name="Schenk2009b" /> *Rhea is the second-largest of Saturn's moons. It is even slightly larger than Oberon, the second-largest moon of Uranus.<ref name="Thomas2007" /> In 2005, ''Cassini'' detected a depletion of electrons in the plasma wake of Rhea, which forms when the co-rotating plasma of Saturn's magnetosphere is absorbed by the moon.<ref name="Jones2008" /> The depletion was hypothesized to be caused by the presence of dust-sized particles concentrated in a few faint equatorial rings. Such a ring system would make Rhea the only moon in the Solar System known to have rings.<ref name="Jones2008" /> Subsequent targeted observations of the putative ring plane from several angles by ''Cassini'''s narrow-angle camera turned up no evidence of the expected ring material, leaving the origin of the plasma observations unresolved.<ref name="Tiscareno2010">{{Cite journal |last1=Tiscareno |first1=Matthew S. |last2=Burns |first2=Joseph A. |last3=Cuzzi |first3=Jeffrey N. |last4=Hedman |first4=Matthew M. |date=July 2010 |title=Cassini imaging search rules out rings around Rhea |journal=Geophysical Research Letters |language=en |volume=37 |issue=14 |pages=L14205 |arxiv=1008.1764 |bibcode=2010GeoRL..3714205T |doi=10.1029/2010GL043663 |issn=0094-8276 |s2cid=59458559}}</ref> : Otherwise Rhea has rather a typical heavily cratered surface,<ref name="Moore Schenk et al. 2004" /> with the exceptions of a few large Dione-type fractures (wispy terrain) on the trailing hemisphere<ref name="Wagner2008" /> and a very faint "line" of material at the equator that may have been deposited by material deorbiting from present or former rings.<ref name="Schenk2009" /> Rhea also has two very large impact basins on its anti-Saturnian hemisphere, which are about 400 and 500&nbsp;km across.<ref name="Wagner2008" /> The first, Tirawa, is roughly comparable to the Odysseus basin on Tethys.<ref name="Moore Schenk et al. 2004" /> There is also a 48&nbsp;km-diameter impact crater called Inktomi at 112°W that is prominent because of an extended system of bright rays,<ref name="Splat" /> which may be one of the youngest craters on the inner moons of Saturn.<ref name="Wagner2008" />{{Failed verification|date=February 2026|reason=No mention of comparison to other moons, nor what an 'inner moon' is}} No evidence of any endogenic activity has been discovered on the surface of Rhea.<ref name="Wagner2008" /> *Titan, at 5,149&nbsp;km diameter, is the second largest moon in the Solar System and Saturn's largest.<ref name="Zebker 2009" /><ref name="Jacobson Antreasian et al. 2006" /> Out of all the large moons, Titan is the only one with a dense (surface pressure of 1.5&nbsp;atm), cold atmosphere, primarily made of nitrogen with a small fraction of methane.<ref name="Porco2005c" /> The dense atmosphere frequently produces bright white convective clouds, especially over the south pole region.<ref name="Porco2005c" /> On 6 June 2013, scientists at the IAA-CSIC reported the detection of polycyclic aromatic hydrocarbons in the upper atmosphere of Titan.<ref name="IAA-20130606">{{cite news |last=López-Puertas |first=Manuel |url=http://www.iaa.es/content/pahs-titans-upper-atmosphere |title=PAH's in Titan's Upper Atmosphere |date=6 June 2013 |work=CSIC |access-date=6 June 2013 |archive-date=22 August 2016 |archive-url=https://web.archive.org/web/20160822010505/http://www.iaa.es/content/pahs-titans-upper-atmosphere |url-status=dead}}</ref> On 23 June 2014, NASA claimed to have strong evidence that nitrogen in the atmosphere of Titan came from materials in the Oort cloud, associated with comets, and not from the materials that formed Saturn in earlier times.<ref name="NASA-201450623">{{cite press release |last1=Dyches |first1=Preston |last2=Clavin |first2=Whitney |title=Titan's Building Blocks Might Pre-date Saturn |url=http://www.jpl.nasa.gov/news/news.php?release=2014-200 |date=23 June 2014 |publisher=Jet Propulsion Laboratory |access-date=28 June 2014 |archive-date=9 September 2018 |archive-url=https://web.archive.org/web/20180909162240/https://www.jpl.nasa.gov/news/news.php?release=2014-200 |url-status=live}}</ref>

: The surface of Titan, which is difficult to observe due to persistent atmospheric haze, shows only a few impact craters and is probably very young.<ref name="Porco2005c" /> It contains a pattern of light and dark regions, flow channels and possibly cryovolcanos.<ref name="Porco2005c" /><ref name="Lopes2007" /> Some dark regions are covered by longitudinal dune fields shaped by tidal winds, where sand is made of frozen water or hydrocarbons.<ref name="Lorenz2006" /> Titan is the only body in the Solar System beside Earth with bodies of liquid on its surface, in the form of methane–ethane lakes in Titan's north and south polar regions.<ref name="Stofan2007" /> The largest lake, Kraken Mare, is larger than the Caspian Sea.<ref name="KrakenMare" /> Like the moons Europa and Ganymede of Jupiter, it is believed that Titan has a subsurface ocean made of water mixed with ammonia, which can erupt to the surface of the moon and lead to cryovolcanism.<ref name="Lopes2007" /> On 2 July 2014, NASA reported the ocean inside Titan may be "as salty as the Earth's Dead Sea".<ref name="NASA-20140702">{{cite web |last1=Dyches |first1=Preston |last2=Brown |first2=Dwayne |title=Ocean on Saturn Moon Could be as Salty as the Dead Sea |url=http://www.jpl.nasa.gov/news/news.php?release=2014-217 |date=2 July 2014 |work=NASA |access-date=July 2, 2014 |archive-date=9 July 2014 |archive-url=https://web.archive.org/web/20140709165628/http://www.jpl.nasa.gov/news/news.php?release=2014-217 |url-status=live}}</ref><ref name="ICARUS-2014">{{cite journal |last1=Mitri |first1=Giuseppe |last2=Meriggiola |first2=Rachele |last3=Hayes |first3=Alex |last4=Lefevre |first4=Axel |last5=Tobie | first5=Gabriel |last6=Genova |first6=Antonio |last7=Lunine |first7=Jonathan I. |last8=Zebker |first8=Howard |title=Shape, topography, gravity anomalies and tidal deformation of Titan |date=1 July 2014 |journal=Icarus |doi=10.1016/j.icarus.2014.03.018 |volume=236 |pages=169–177 |bibcode = 2014Icar..236..169M}}</ref> *Hyperion is Titan's nearest neighbor in the Saturnian system. The two moons are locked in a 4:3 mean-motion resonance with each other, meaning that while Titan makes four revolutions around Saturn, Hyperion makes exactly three.<ref name="Jacobson Antreasian et al. 2006" /> With an average diameter of about 270&nbsp;km, Hyperion is smaller and lighter than Mimas.<ref name="Thomas2007b" /> It has an extremely irregular shape, and a very odd, tan-colored icy surface resembling a sponge, though its interior may be partially porous as well. The average density of about 0.55&nbsp;g/cm³ indicates that the porosity exceeds 40% even assuming it has a purely icy composition. The surface of Hyperion is covered with numerous impact craters—those with diameters 2–10&nbsp;km are especially abundant. It is the only moon besides some of the small moons of Pluto known to have a chaotic rotation, which means Hyperion has no well-defined poles or equator. While on short timescales the satellite approximately rotates around its long axis at a rate of 72–75° per day, on longer timescales its axis of rotation (spin vector) wanders chaotically across the sky.<ref name="Thomas2007b" /> This makes the rotational behavior of Hyperion essentially unpredictable.<ref name="Thomas1995" /> *Iapetus is the third-largest of Saturn's moons.<ref name="Thomas2007" /> Orbiting the planet at {{Nowrap|3.5 million}} km, it is by far the most distant of Saturn's round moons, and also has the largest orbital inclination, at 15.47°.<ref name="NASA" /> Iapetus has long been known for its unusual two-toned surface; its leading hemisphere is pitch-black and its trailing hemisphere is almost as bright as fresh snow.<ref name="Porco2005b" /> ''Cassini'' images showed that the dark material is confined to a large near-equatorial area on the leading hemisphere called Cassini Regio, which extends approximately from 40°N to 40°S. The pole regions of Iapetus are as bright as its trailing hemisphere. ''Cassini'' also discovered a 20&nbsp;km tall equatorial ridge, which spans nearly the moon's entire equator. Otherwise both dark and bright surfaces of Iapetus are old and heavily cratered. The images revealed at least four large impact basins with diameters from 380 to 550&nbsp;km and numerous smaller impact craters. No evidence of any endogenic activity has been discovered.<ref name="Porco2005b" />

: A clue to the origin of the dark material covering part of Iapetus's starkly dichromatic surface may have been found in 2009, when NASA's Spitzer Space Telescope discovered a vast, nearly invisible disk around Saturn, just inside the orbit of the moon Phoebe &ndash; the Phoebe ring.<ref name="Verbiscer2009" /> Scientists believe that the disk originates from dust and ice particles kicked up by impacts on Phoebe. Because the disk particles, like Phoebe itself, orbit in the opposite direction to Iapetus, Iapetus collides with them as they drift in the direction of Saturn, darkening its leading hemisphere slightly.<ref name="Verbiscer2009" /> Once a difference in albedo, and hence in average temperature, was established between different regions of Iapetus, a thermal runaway process of water ice sublimation from warmer regions and deposition of water vapor onto colder regions ensued. Iapetus's present two-toned appearance results from the contrast between the bright, primarily ice-coated areas and regions of dark lag, the residue left behind after the loss of surface ice.<ref name="Denk">{{Cite journal | last = Denk | first = T. |display-authors=etal | title = Iapetus: Unique Surface Properties and a Global Color Dichotomy from Cassini Imaging | journal = Science | volume = 327| issue =5964 | pages =435–9 | date = 2009-12-10 | doi = 10.1126/science.1177088 | pmid = 20007863|bibcode = 2010Sci...327..435D | s2cid = 165865}}</ref><ref name="Spencer">{{Cite journal | last = Spencer | first = J. R. |author2=Denk, T. | title = Formation of Iapetus' Extreme Albedo Dichotomy by Exogenically Triggered Thermal Ice Migration | journal = Science | volume = 327| issue =5964 | pages =432–5 | date = 2009-12-10 | doi = 10.1126/science.1177132 | pmid = 20007862|bibcode = 2010Sci...327..432S | citeseerx = 10.1.1.651.4218 | s2cid = 20663944}}</ref>

{{clear|left}}

===Irregular moons=== thumb|upright=1.25|Orbits and positions of Saturn's 250 irregular moons as of March 2025. Prograde orbits are colored blue while retrograde orbits are colored red. Saturn's outermost regular moons, Titan, Hyperion, and Iapetus, are also shown with turquoise orbits.

Irregular moons are small satellites with distant, inclined, and frequently retrograde orbits, believed to have been acquired by the parent planet through a capture process. They often occur as collisional families or groups.<ref name="Jewitt2007" /> The precise size and albedo of many of the irregular moons are not known because they are too small to be resolved by telescopes on Earth and in space, so their sizes are estimated from their brightness by assuming a dark surface or low albedo of around 6% (albedo of Phoebe) or less.<ref name="Gladman2001" /> The irregular moons generally have featureless visible and near infrared spectra dominated by water absorption bands.<ref name="Jewitt2007" /> They are typically gray (spectrally neutral) or moderately red in color—similar to C-type, P-type, or D-type asteroids,<ref name="Grav2007" /> though they are much less red than Kuiper belt objects.<ref name="Jewitt2007" />{{refn | group = lower-alpha | The photometric color may be used as a proxy for the chemical composition of satellites' surfaces.}}

====Inuit==== {{Main|Inuit group}}

The Inuit group includes 39<!--for a count of 292--> prograde outer moons that are similar enough in their distances from the planet (190–300 radii of Saturn), their orbital inclinations (43–51°) and their colors that they can be considered a group.<ref name="Gladman2001" /><ref name="Grav2007" /> The Inuit group is further split into three distinct subgroups at different semi-major axes, and are named after their respective largest members. Ordered by increasing semi-major axis, these subgroups are the Kiviuq subgroup (188 Saturn radii), Paaliaq (249 Saturn radii), and the Siarnaq subgroup (297 Saturn radii).<ref name="Sheppard2023" /><ref name="Ashton2025a" /><ref name="jplsats-elem" /> It is unknown whether all of these subgroups of the Inuit group share a common origin.<ref name="Ashton2025a" />

The Kiviuq group includes 23 members, with the only named members being Ijiraq and the group's largest member and namesake Kiviuq. Kiviuq has a diameter of about 17&nbsp;km and has a highly elongated shape, which may indicate it is a contact binary.<ref name="Denk2018" /> The Siarnaq group includes 15 members, with the only named members being Tarqeq and the group's namesake Siarnaq.<ref name="jplsats-elem" /> Siarnaq is the largest member of its subgroup and the entire Inuit group, with an estimated diameter of about 39&nbsp;km.<ref name="Grav2015" /> The moons of the Kiviuq and Siarnaq subgroups are tightly clustered in semi-major axis and inclination with respect to their namesake moon, which makes them distinct collisional families.<ref name="Ashton2025a" /><ref name="Ashton2025b" /> In contrast to Kiviuq and Siarnaq, Paaliaq (diameter ~25&nbsp;km) does not have an associated subgroup.<ref name="Ashton2025a" /><ref name="Sheppard2023" />

====Gallic==== {{Main|Gallic group}}

The Gallic group includes 19<!--for a count of 292--> prograde outer moons that are similar in their orbital inclination (34–41°), their orbital eccentricity, and their color that they can be considered a group.<ref name="Gladman2001" /><ref name="Grav2007" /> The named members of the Gallic group are Albiorix, Bebhionn, Erriapus, and Tarvos.<ref name="jplsats-elem" /> The largest of these moons is Albiorix with an estimated diameter of about 29&nbsp;km.<ref name="Grav2015" /> The Gallic group may be divided into the Albiorix subgroup, which consists of 16 moons with semi-major axes between 200–330 radii of Saturn, and the outlier moon S/2004 S 24 which has a lower eccentricity and a much more distant semi-major axis of ~400 Saturn radii.<ref name="jplsats-elem" /><ref name="Ashton2025a" /> S/2004 S 24 may not be directly related to the Gallic group, although it is possible that it could have formed as a fragment of an Albiorix subgroup member that was collisionally disrupted when it was at its farthest distance from Saturn in its elliptical orbit.<ref name="Ashton2025a" />

====Norse==== {{Main|Norse group}}

[[File:Phoebe cassini full.jpg|thumb|Phoebe, Saturn's largest irregular moon]]

All 210<!--for a count of 292--> retrograde outer moons of Saturn are broadly classified into the Norse group.<ref name="Gladman2001" /><ref name="Grav2007" /> Only 31 moons of the Norse group have been named: Aegir, Angrboda, Alvaldi, Beli, Bergelmir, Bestla, Eggther, Farbauti, Fenrir, Fornjot, Geirrod, Gerd, Greip, Gridr, Gunnlod, Hati, Hyrrokkin, Jarnsaxa, Kari, Loge, Mundilfari, Narvi, Phoebe, Skathi, Skoll, Skrymir, Surtur, Suttungr, Thiazzi, Thrymr, and Ymir.<ref name="jplsats-elem" />

Although the Norse group does not show obvious clustering in orbital elements, researchers led by Edward Ashton have proposed splitting the Norse group into four different subgroups by inclination.<ref name="Ashton2025a" /> These subgroups still have a broad range of orbital semi-major axes, inclinations, and eccentricities, and may not necessarily have an impact origin.<ref name="Ashton2025a" />

*The Phoebe subgroup consists of moons between inclinations 172° and 180° and is named after Phoebe,<ref name="Ashton2025a" /> by far the largest irregular moon of Saturn with a diameter of {{val|213|1.4|u=km}}.<ref name="Jewitt2007" /> It has a retrograde orbit and rotates on its axis every 9.3 hours.<ref name="Giese2006" /> Phoebe was the first moon of Saturn to be studied in detail by ''Cassini'', in {{Nowrap|June 2004}}; during this encounter ''Cassini'' was able to map nearly 90% of the moon's surface. Phoebe has a nearly spherical shape and a relatively high density of about 1.6&nbsp;g/cm³.<ref name="Jewitt2007" /> ''Cassini'' images revealed a dark surface scarred by numerous impacts—there are about 130 craters with diameters exceeding 10&nbsp;km. Such impacts may have ejected fragments of Phoebe into orbit around Saturn—two of these may be S/2006 S 20 and S/2006 S 9, whose orbits are similar to Phoebe.<ref name="Sheppard2023" /><ref>{{Cite web |title=S/2006 S 20 – Tilmann Denk |url=https://tilmanndenk.de/outersaturnianmoons/s2006_s20/ |access-date=2024-01-23 |language=en-US |archive-date=2024-06-16 |archive-url=https://web.archive.org/web/20240616103718/https://tilmanndenk.de/outersaturnianmoons/s2006_s20/ |url-status=live}}</ref><ref>{{Cite web |title=S/2006 S 9 – Tilmann Denk |url=https://tilmanndenk.de/outersaturnianmoons/s2006_s9/ |access-date=2024-01-23 |language=en-US |archive-date=2023-12-24 |archive-url=https://web.archive.org/web/20231224062938/https://tilmanndenk.de/outersaturnianmoons/s2006_s9/ |url-status=live}}</ref> Spectroscopic measurement showed that the surface is made of water ice, carbon dioxide, phyllosilicates, organics and possibly iron-bearing minerals.<ref name="Jewitt2007" /> Phoebe is believed to be a captured centaur that originated in the Kuiper belt.<ref name="Jewitt2007" /> It also serves as a source of material for the largest known ring of Saturn, which darkens the leading hemisphere of Iapetus (see above).<ref name="Verbiscer2009" />

*The Mundilfari subgroup consists of moons between inclinations 157° and 172° and is the most populated of the four Norse subgroups proposed by Ashton and collaborators.<ref name="Ashton2025a" /> Named after its largest member Mundilfari (diameter ~7&nbsp;km), this subgroup is dominated by tiny moons smaller than 4&nbsp;km in diameter, which suggests they were formed by a relatively recent collisional event that destroyed a progenitor moon at least 100 million years ago.<ref name="Ashton2025a" /><ref name="Ashton2025b" /> Ashton and collaborators proposed that this progenitor moon of the Mundifari subgroup would have orbited Saturn at a semi-major axis of ~19.5&nbsp;million&nbsp;km (~320 Saturn radii), inclination ~165°, and eccentricity ~0.28.<ref name="Ashton2025a" /> The collision that destroyed this progenitor moon would have to eject its fragments at a speed of at least 200&nbsp;m/s, and subsequent collisions of its fragments may further disperse their orbits to produce the broad orbital distribution of the Mundilfari group observed today.<ref name="Ashton2025a" />

*The Kari subgroup consists of moons between inclinations 151.7° and 157° and appears mostly concentrated around the orbit of its namesake and largest member Kari (diameter ~6&nbsp;km) with a semi-major axis range between {{convert|0.14–0.16|AU|e6km|abbr=unit}} from Saturn.<ref name="Ashton2025a" /> This tight clustering may be a collisional family.<ref name="Ashton2025a" /> There are several other moons in the Kari subgroup's inclination range that have semi-major axes less than the aforementioned range, and thus may not be related to the proposed collisional family.<ref name="Ashton2025a" /><ref name="Ashton2025b" />

*The remaining Norse group moons with inclinations below 151.7° are sparse in number and are assigned to the low-inclination subgroup by Ashton and collaborators.<ref name="Ashton2025a" /> Of the moons of the low-inclination subgroup, Narvi and S/2019 S 11 have the most similar orbits to each other, which suggests these two moons share an origin.<ref name="Ashton2025a" />

==List== [[File:Saturnmoonsdiagram.png|thumb|upright=4|center|Orbital diagram of the orbital inclination and orbital distances for Saturn's rings and moon system at various scales. Notable moons, moon groups, and rings are individually labeled. Open the image for full resolution.]]

The Saturnian moons are listed here by orbital period (or semi-major axis), from shortest to longest. Moons massive enough for their surfaces to have collapsed into a spheroid are highlighted in bold and marked with a blue background, while the irregular moons are listed in red, orange, and gray background. The orbits and mean distances of the irregular moons are strongly variable over short timescales due to frequent planetary and solar perturbations, so the orbital elements of irregular moons listed here are averaged over a 5,000-year numerical integration by the Jet Propulsion Laboratory. These may sometimes strongly differ from the osculating orbital elements orbital elements provided by other sources.<ref name="jplsats-elem" /><ref name="Jacobson2022b" /> Otherwise, recently discovered irregular moons without published proper elements are temporarily listed here with inaccurate osculating orbital elements that are ''italicized'' to distinguish them from other irregular moons with proper orbital elements. The mean orbital elements are based on a reference epoch of 1 January 2000.<ref name="jplsats-elem">{{cite web|title=Planetary Satellite Mean Elements|url=https://ssd.jpl.nasa.gov/sats/elem/|publisher=Jet Propulsion Laboratory|access-date=10 November 2025|archive-date=November 16, 2025|archive-url=https://web.archive.org/web/20251116001458/https://ssd.jpl.nasa.gov/sats/elem/|url-status=live}}</ref>

<div style="float:left"> {| class="wikitable" style="margin:0; font-size:90%; text-align:left" |- |+ Key |- | style="background:#fff;" |&nbsp; ''Other regular moons (17)'' | style="background:#ccf;" | ♠ '''''Round moons''' (7)'' | style="background:#f4c2c2" | ♦ ''Inuit group (39)'' | style="background:#fdd5b1" | ♣ ''Gallic group (19)'' | style="background:#d3d3d3" | ‡ ''Norse group (210)'' |}</div>

{{Clear}} {{sort under}} {{sticky table start}} {| class="wikitable sortable sort-under sticky-table-row1 sticky-table-col1" style="font-size:85%" |- ! Label<br>{{refn|group=lower-alpha|A confirmed moon is given a permanent designation by the IAU consisting of a name and a Roman numeral.<ref name="Gazetteer" /> The eight moons that were known before 1850 are numbered in order of their distance from Saturn; the rest are numbered in the order by which they received their permanent designations. Many small moons have not yet received a permanent designation.}} ! Name ! class="unsortable" |Pronunciation ! class="unsortable" |Image ! data-sort-type="number" | Abs.<br>magn.<br />{{refn|group=lower-alpha|Absolute magnitudes of regular satellites are calculated from their mean diameters and geometric albedos given in NASA's Saturnian Satellite Fact Sheet.<ref name="NASA"/> Absolute magnitude estimates for some small inner moons are not available as they do not have measured geometric albedos. Absolute magnitudes of irregular satellites were taken from the Minor Planet Center's Natural Satellites Ephemeris Service.<ref name="MPC-NatSats"/>|name=absmag}} ! data-sort-type="number" | Diameter<br>(km)<br />{{refn|group=lower-alpha|The diameters and dimensions of the small inner moons, from Pan to Helene, are taken from Thomas et al., 2020, Table 1.<ref name="Thomas2020"/> Diameters and dimensions of Mimas, Enceladus, Tethys, Dione, Rhea, Iapetus, and Phoebe are from Thomas 2010, Table 1.<ref name="Thomas2010"/> Diameters of Siarnaq and Albiorix are from Grav et al., 2015, Table 3.<ref name="Grav2015"/> The approximate sizes of all other irregular satellites are calculated from their absolute magnitudes with an assumed geometric albedo of 0.04, which is the average value for that population.<ref name="Grav2015"/> Calculations were made with NASA/JPL's Asteroid Size Estimator.<ref name="SizeEstimator"/>|name=diameter}} ! data-sort-type="number" | Mass<br>({{e|15}} kg)<br />{{refn|group=lower-alpha|Masses of the large round moons, including Hyperion, Phoebe, and Helene, were taken from Jacobson et al., 2022, Table 5.<ref name="Jacobson2022a"/> Masses of Atlas, Prometheus, Pandora, Epimetheus, and Janus were taken from Lainey et al., 2023, Table 1.<ref name="Lainey2023"/> Masses of Pan, Daphnis, Aegaeon, Methone, and Pallene were taken from Thomas et al., 2020, Table 2.<ref name="Thomas2020"/> Masses of other regular satellites were calculated by multiplying their volumes with an assumed density of 500 kg/m³ (0.5&nbsp;g/cm³), while masses of irregular satellites were calculated with an assumed density of 1000 kg/m³ (1.0&nbsp;g/cm³).}} ! data-sort-type="number" | Semi-major<br>axis<br>(km)<br /><ref name="jplsats-elem"/> ! data-sort-type="number" | Orbital period (d)<br /><ref name="jplsats-elem"/>{{refn|group=lower-alpha|Negative orbital periods indicate a retrograde orbit around Saturn (opposite to the planet's rotation). Orbital periods of irregular satellites may not directly correlate with their semi-major axes due to perturbations.}} ! data-sort-type="number" | Inclination<br />(°)<br /><ref name="jplsats-elem"/>{{refn|group=lower-alpha|Orbital inclinations of regular satellites and Phoebe are with respect to their Laplace planes. Orbital inclinations of irregular satellites are with respect to the ecliptic.<ref name="jplsats-elem"/>|name=inclination}} ! data-sort-type="number"| Eccentricity<br /><ref name="jplsats-elem"/> ! Group<br>{{refn|group=lower-alpha|The irregular moons are categorized as described in Ashton et al., 2025a. Otherwise, for the 128 newly discovered satellites not included in the paper, they are sorted into their categories based on the inclination and semi-major axis criteria stated in Ashton et al., 2025a.<ref name="Ashton2025a"/>}} ! Discovery<br>year<br /><ref name="jplsats-disc">{{cite web|title=Planetary Satellite Discovery Circumstances|url=https://ssd.jpl.nasa.gov/sats/discovery.html|publisher=Jet Propulsion Laboratory|date=23 May 2023|access-date=11 April 2026|archive-date=27 September 2021|archive-url=https://web.archive.org/web/20210927162554/https://ssd.jpl.nasa.gov/sats/discovery.html|url-status=live}}</ref> ! Year announced ! Discoverer<br /><ref name="Gazetteer" /><ref name="jplsats-disc" /> |-style="background:#fff;" | {{sort|Q|}} || {{hid|S/2009}} <small>S/2009 S 1</small> || — || style="background:white;"| frameless|upright=0.3|center || {{sort|98|—}} || 0.3 || {{nowrap|{{sort|0.0000071|≈&thinsp;{{val|0.0000071}}}}}} || {{sort|116900|&thinsp;{{val|116900}}}}|| {{sort|0.47150|&thinsp;{{val|0.47150}}}}|| {{sort|0|≈&thinsp;{{val|0.0}}}} || {{sort|0|≈&thinsp;{{val|0.000}}}} || &nbsp; || 2009 || 2009 || ''Cassini''<ref name="IAUC2009b" /> |-style="background:#fff;" | {{sort|18|XVIII}} || {{hid|Pan}} Pan || {{IPAc-en|ˈ|p|æ|n}} || style="background:black;"| frameless|upright=0.3|center|alt=An irregularly shaped body with a prominent equatorial ridge. It is illuminated from the bottom right.|| 9.2 || {{sort|28.2|28.2<br>(35 × 28 × 21)}} || {{val|4.30}} || {{val|133600}} || {{sort|0.57505|+{{val|0.57505}}}} || 0.0 || 0.000 || inner ring || 1990 || 1990 || Showalter |-style="background:#fff;" | {{sort|35|XXXV}} || {{hid|Daphnis}} Daphnis || {{IPAc-en|ˈ|d|æ|f|n|ə|s}} || style="background:black;"| frameless|upright=0.3|center|alt=A small, irregularly shaped body elongated from the bottom left to top right. It is illuminated from the bottom left. || {{sort|99|—}} || {{sort|7.6|7.6<br>(9.8 × 8.4 × 5.6)}}|| {{val|0.068}} || {{val|136500}} || {{sort|0.59408|+{{val|0.59408}}}} || 0.0 || 0.000 || inner ring || 2005 || 2005 || ''Cassini'' |-style="background:#fff;" | {{sort|15|XV}} || {{hid|Atlas}} Atlas || {{IPAc-en|ˈ|æ|t|l|ə|s}} || style="background:black;"| frameless|upright=0.3|center|alt=An irregularly shaped body is fully illuminated. The body, which looks like a cone viewed from the south pole, is elongated downward. || 8.5 || {{sort|30.2|30.2<br>(41 × 35 × 19)}} || {{val|5.490}} || {{val|137700}} || {{sort|0.60460|+{{val|0.60460}}}} || 0.0 || 0.001 || inner ring || 1980 || 1980 || ''Voyager 1'' |-style="background:#fff;" | {{sort|16|XVI}} || {{hid|Prometheus}} Prometheus || {{IPAc-en|p|r|oʊ|ˈ|m|iː|θ|i|ə|s}} || style="background:black;"| frameless|upright=0.3|center|alt=An irregularly shaped oblong body is fully illuminated. It is elongated in the direction from the top left to bottom left. Its surface is covered by craters. || 6.7 || {{sort|86.2|86.2<br>(137 × 81 × 56)}} || {{val|159.72}} || {{val|139400}} || {{sort|0.61588|+{{val|0.61588}}}} || 0.0 || 0.002 || inner ring || 1980 || 1980 || ''Voyager 1'' |-style="background:#fff;" | {{sort|17|XVII}} || {{hid|Pandora}} Pandora || {{IPAc-en|p|æ|n|ˈ|d|ɔər|ə}} || style="background:black;"| alt=An irregularly shaped body is half illuminated from the bottom. The terminator runs from the left to right. The surface is covered by numerous craters.|center|frameless|upright=0.3 || 6.5 || {{sort|81.4|81.4<br>(104 × 81 × 64)}} || {{val|135.7}} || {{val|141700}} || {{sort|0.63137|+{{val|0.63137}}}} || 0.0 || 0.004 || inner ring || 1980 || 1980 || ''Voyager 1'' |-style="background:#fff;" | {{sort|11|XI}} || {{hid|Epimetheus}} Epimetheus || {{IPAc-en|ɛ|p|ə|ˈ|m|iː|θ|i|ə|s}} || style="background:black;"| frameless|upright=0.3|center|alt=A partially-illuminated irregular body, which has a shape remotely resembling a cube. The body's surface consists of ridges and valleys and is covered by craters. || 5.5 || {{sort|116.2|116.2<br>(130 × 114 × 106)}} || {{val|525.607}} || {{val|151400}} || {{sort|0.69701|+{{val|0.69701}}}} || 0.3 || 0.020 || co-orbital (with Janus) || 1966 || 1967 || Fountain & Larson |-style="background:#fff;" | {{sort|10|X}} || {{hid|Janus}} Janus || {{IPAc-en|ˈ|dʒ|eɪ|n|ə|s}} || style="background:black;"| frameless|upright=0.3|alt=An irregular body, whose outline looks like an approximate circle in this image. It is illuminated from the bottom-left. The terminator runs from the top-left to bottom-right. The surface is covered by craters. || 4.5 || {{sort|179|179<br>(203 × 185 × 153)}} || {{val|1893.88}} || {{val|151500}} || {{sort|0.69735|+{{val|0.69735}}}} || 0.2 || 0.007 || co-orbital (with Epimetheus) || 1966 || 1967 || Dollfus |-style="background:#fff;" | {{sort|53|LIII}} || {{hid|Aegaeon}} Aegaeon || {{IPAc-en|iː|ˈ|dʒ|iː|ɒ|n}} || style="background:black;"| frameless|upright=0.3|center|alt=Image of Aegaeon by Cassini. || {{sort|99|—}} || {{sort|0.66|0.66<br>(1.4 × 0.5 × 0.4)}} || {{val|0.0000782}} ||| {{val|167500}} || {{sort|0.80812|+{{val|0.80812}}}} || 0.0 || 0.000 || ring-embedded || 2008 || 2009 || ''Cassini'' |- style="background:#ccf;" | {{sort|01|I}} || {{hid|Mimas}} ♠'''Mimas''' || {{IPAc-en|ˈ|m|aɪ|m|ə|s}} || style="background:black;"| frameless|upright=0.3|center|alt=A spherical body is half illuminated from the left. The terminator runs from the top to bottom in the vicinity of the right limb. A large crater with a central peak sits on the terminator slightly to the right and above the center of the body. It makes the body look like the Death Star. There are numerous smaller craters. || 3.2 || {{sort|396.4|396.4<br>(416 × 393 × 381)}} || {{val|37509.4}} || {{val|186000}} || {{sort|0.94242|+{{val|0.94242}}}} || 1.6 || 0.020 || &nbsp; || 1789 || 1789 || Herschel |-style="background:#fff;" | {{sort|32|XXXII}} || {{hid|Methone}} Methone || {{IPAc-en|m|ə|ˈ|θ|oʊ|n|iː}} || style="background:black;"| frameless|upright=0.3|center|alt=A smooth, featureless ellipsoidal object illuminated from the top right, distinctly looking like an egg. || {{sort|99|—}} || {{sort|2.9|2.9<br>(4.0 × 2.6 × 2.4)}} || {{val|0.00392}} ||| {{val|194700}} || {{sort|1.00955|+{{val|1.00955}}}} || 0.0 || 0.002 || ring-embedded || 2004 || 2004 || ''Cassini'' |-style="background:#fff;" | {{sort|49|XLIX}} || {{hid|Anthe}} Anthe || {{IPAc-en|ˈ|æ|n|θ|iː}} || style="background:black;"| frameless|upright=0.3|center|alt=A blurry ellipsoidal object in the center of the image || {{sort|99|—}} || 1.8 || {{sort|0.0015|≈&thinsp;{{val|0.0015}}}} ||| {{val|198100}} || {{sort|1.03890|+{{val|1.03890}}}} || 0.0 || 0.002 || ring-embedded || 2007 || 2007 || ''Cassini'' |-style="background:#fff;" | {{sort|33|XXXIII}} || {{hid|Pallene}} Pallene || {{IPAc-en|p|ə|ˈ|l|iː|n|iː}} || style="background:#bab271;"| frameless|upright=0.3|center|alt=A small, half-illuminated ellipsoidal object in front of Saturn as a backdrop || {{sort|99|—}} || {{sort|4.44|4.44<br>(5.8 × 4.2 × 3.7)}} || {{sort|0.023|≈&thinsp;{{val|0.023}}}} ||| {{val|212300}} || {{sort|1.15606|+{{val|1.15606}}}} || 0.2 || 0.004 || ring-embedded || 2004 || 2004 || ''Cassini'' |- style="background:#ccf;" | {{sort|02|II}} || {{hid|Enceladus}} ♠'''Enceladus''' || {{IPAc-en|ɛ|n|ˈ|s|ɛ|l|ə|d|ə|s}} || style="background:black;"| frameless|upright=0.3|center || 2.1 || {{sort|504.2|504.2<br>(513 × 503 × 497)}} || {{val|108031.8}} || {{val|238400}} || {{sort|1.37022|+{{val|1.37022}}}} || 0.0 || 0.005 || &nbsp; || 1789 || 1789 || Herschel |- style="background:#ccf;" | {{sort|03|III}} || {{hid|Tethys}} ♠'''Tethys''' || {{IPAc-en|ˈ|t|iː|θ|ə|s}} || style="background:black;"| center|frameless|upright=0.3|| 0.7 || {{sort|1062.2|1062.2<br>(1077 × 1057 × 1053)}} || {{val|617495.9}} || {{val|295000}} || {{sort|1.887802|+{{val|1.88780}}}}|| 1.1 || 0.001 || &nbsp; || 1684 || 1684 || Cassini |-style="background:#fff;" | {{sort|13|XIII}} || {{hid|Telesto}} Telesto || {{IPAc-en|t|ə|ˈ|l|ɛ|s|t|oʊ}} || style="background:black;"| frameless|upright=0.3|center|alt=An oblong object with a few large craters and a smooth surface || 8.7 || {{sort|24.8|24.8<br>(33 × 23 × 19)}} || {{sort|3.9|≈&thinsp;{{val|3.9}}}} || {{val|295000}} || {{sort|1.887802|+{{val|1.88780}}}}|| 1.2 || 0.001 || trojan (Tethys {{L4}}) || 1980 || 1980 || Smith et al. |-style="background:#fff;" | {{sort|14|XIV}} || {{hid|Calypso}} Calypso || {{IPAc-en|k|ə|ˈ|l|ɪ|p|s|oʊ}} || style="background:black;" | frameless|upright=0.3|center|alt=An oblong body is seen in this low resolution image. || 9.2 || {{sort|21.4|21.4<br>(29 × 19 × 13)}} || {{sort|1.8|≈&thinsp;{{val|1.8}}}} || {{val|295000}} || {{sort|1.887803|+{{val|1.88780}}}}|| 1.5 || 0.001 || trojan (Tethys {{L5}}) || 1980 || 1980 || Pascu et al. |-style="background:#fff;" | {{sort|12|XII}} || {{hid|Helene}} Helene || {{IPAc-en|ˈ|h|ɛ|l|ə|n|iː}} || style="background:black;" | frameless|upright=0.3|center|alt=An irregularly shaped body illuminated from the left. Its surface is covered by numerous impact craters. || 8.2 || {{sort|35.2|35.2<br>(45 × 39 × 27)}} || {{val|7.1}} || {{val|377600}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.2 || 0.007 || trojan (Dione {{L4}}) || 1980 || 1980 || Laques & Lecacheux |-style="background:#fff;" | {{sort|34|XXXIV}} || {{hid|Polydeuces}} Polydeuces || {{IPAc-en|p|ɒ|l|i|ˈ|dj|uː|s|iː|z}} || style="background:black;" | frameless|upright=0.3|center|alt=A small oblong body is barely resolved in this image. || {{sort|99|—}} || {{sort|2.6|2.6<br>(3.5 × 3.1 × 2.7)}} || {{sort|0.0075|≈&thinsp;{{val|0.0075}}}} || {{val|377600}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.2 || 0.019 || trojan (Dione {{L5}}) || 2004 || 2004 || ''Cassini'' |- style="background:#ccf;" | {{sort|04|IV}} || {{hid|Dione}} ♠'''Dione''' || {{IPAc-en|d|aɪ|ˈ|oʊ|n|iː}} || style="background:black;" | center|frameless|upright=0.3|| 0.8 || {{sort|1122.8|1122.8<br>(1128 × 1123 × 1119)}} || {{val|1095486.8}} || {{val|377700}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.0 || 0.002 || &nbsp; || 1684 || 1684 || Cassini |- style="background:#ccf;" | {{sort|05|V}} || {{hid|Rhea}} ♠'''Rhea''' || {{IPAc-en|ˈ|r|eɪ|ə}} || style="background:black;"| frameless|upright=0.3|center || 0.1 || {{sort|1527.6|1527.6<br>{{nowrap|(1530 × 1526 × 1525)}}}} || {{val|2306485.4}} || {{val|527200}} || {{sort|4.51750|+{{val|4.51750}}}} || 0.3 || 0.001 || &nbsp; || 1672 || 1673 || Cassini |- style="background:#ccf;" | {{sort|06|VI}} || {{hid|Titan}} ♠'''Titan''' || {{IPAc-en|ˈ|t|aɪ|t|ən}} || style="background:black;"| frameless|upright=0.3|center || –1.3 || {{sort|5149.46|5149.46<br>{{nowrap|({{val|5149}} × {{val|5149}} × {{val|5150}})}}}} || {{val|134518035.4}} || {{val|1221900}} || {{sort|15.9454|+{{val|15.9454}}}} || 0.3 || 0.029 || &nbsp; || 1655 || 1656 || Huygens |-style="background:#fff;" | {{sort|07|VII}} || {{hid|Hyperion}} Hyperion || {{IPAc-en|h|aɪ|ˈ|p|ɪər|i|ə|n}} || style="background:black;"| frameless|upright=0.3|center|alt=An irregularly shaped oblong body is illuminated from the left. The terminator is near the right limb. The body is elongated in the top-bottom direction. The surface is punctured by numerous impact craters, which make it look like a sponge or cheese. || 4.8 || {{sort|270.0|270.0<br>(360 × 266 × 205)}} || {{val|5551.0}} || {{val|1481500}} || {{sort|21.2767|+{{val|21.2767}}}} || 0.6 || 0.105 || &nbsp; || 1848 || 1848 || Bond & Lassell |- style="background:#ccf;" | {{sort|08|VIII}} || {{hid|Iapetus}} ♠'''Iapetus''' || {{IPAc-en|aɪ|ˈ|æ|p|ə|t|ə|s}} || style="background:black;"| frameless|upright=0.3|center || 1.2 || {{sort|1468.6|1468.6<br>{{nowrap|(1491 × 1491 × 1424)}}}} || {{val|1805659.1}} || {{val|3561700}} || {{sort|79.3310|+{{val|79.3310}}}} || 7.6 || 0.028 || &nbsp; || 1671 || 1673 || Cassini |- id="S/2023 S 1" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 1</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11205400}} || {{sort|442.86|+{{val|442.86}}}} || 48.8 || 0.386 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 1" style="background:#F4C2C2;" | {{sort|R|}} || {{hid|S/2019A}} ♦<small>S/2019 S 1</small> || — || style="background:black;"| frameless|upright=0.3|center || 15.3 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|11245400}}|| {{sort|445.17|+{{val|445.17}}}} || 49.5 || 0.383 || Inuit group (Kiviuq) || 2019 || 2021 || Ashton et al. |- id="S/2004 S 54" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 54</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11277500}} || {{sort|447.14|+{{val|447.14}}}} || 48.1 || 0.373 || Inuit group (Kiviuq) || 2004 || 2025 || Sheppard et al. |- id="S/2023 S 56" style="background: #f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 56</small> || ― || style="background:black;"| || 17.1 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11287500}} || {{sort|447.75|+{{val|447.75}}}} || 45.4 || 0.358 || Inuit group (Kiviuq) || 2023 || 2026 || Ashton et al. |- id="S/2004 S 55" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 55</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11294700}} || {{sort|448.16|+{{val|448.16}}}} || 48.9 || 0.260 || Inuit group (Kiviuq) || 2004 || 2025 || Sheppard et al. |- id="S/2020 S 11" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 11</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11295600}} || {{sort|448.21|+{{val|448.21}}}} || 48.2 || 0.372 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 22" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 22</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11305100}} || {{sort|448.78|+{{val|448.48}}}} || 47.3 || 0.369 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 49" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 49</small> || ― || style="background:black;"| || 16.9 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|11305900}} || {{sort|448.84|+{{val|448.84}}}} || 48.0 || 0.373 || Inuit group (Kiviuq) || 2020 || 2026 || Ashton et al. |- id="Kiviuq" style="background:#F4C2C2;" | {{sort|24|XXIV}} || {{hid|Kiviuq}} ♦Kiviuq || {{IPAc-en|ˈ|k|ɪ|v|i|ə|k}} || style="background:black;" | frameless|upright=0.3|center || 12.7 || {{sort|17|≈&thinsp;{{val|17}}}}|| {{sort|3.6|≈&thinsp;{{val|3.6}}}} || {{val|11307400}}|| {{sort|448.91|+{{val|448.91}}}} || 48.0 || 0.275 || Inuit group (Kiviuq) || 2000 || 2000 || Gladman et al. |- id="S/2023 S 2" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 2</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11309900}} || {{sort|449.05|+{{val|449.05}}}} || 45.7 || 0.339 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 23" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 23</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11310200}} || {{sort|449.08|+{{val|449.08}}}} || 48.7 || 0.255 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 12" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 12</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11314500}} || {{sort|449.33|+{{val|449.33}}}} || 50.8 || 0.260 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al. |- id="S/2005 S 4" style="background:#f4c2c2;" | {{sort|Zza|}} || {{hid|S/2005A}} ♦<small>S/2005 S 4</small> || — || style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|11324500}} || {{sort|449.93|+{{val|449.93}}}} || 48.0 || 0.315 || Inuit group (Kiviuq) || 2005 || 2023 || Sheppard et al. |- id="S/2019 S 25" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 25</small> || ― || style="background:black;"| || 16.4 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11329400}} || {{sort|450.22|+{{val|450.22}}}} || 48.1 || 0.271 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 1" style="background:#F4C2C2;" | {{sort|S|}} || {{hid|S/2020A}} ♦<small>S/2020 S 1</small> || — || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11338600}} || {{sort|450.77|+{{val|450.77}}}} || 48.2 || 0.337 || Inuit group (Kiviuq) || 2020 || 2023 || Ashton et al. |- id="Ijiraq" style="background:#F4C2C2;" | {{sort|22|XXII}} || {{hid|Ijiraq}} ♦Ijiraq || {{IPAc-en|ˈ|iː|ɪ|r|ɒ|k}} || style="background:black;" | frameless|upright=0.3|center || 13.2 || {{sort|13|≈&thinsp;{{val|13}}}}|| {{sort|1.8|≈&thinsp;{{val|1.8}}}} || {{val|11344700}} || {{sort|451.12|+{{val|451.12}}}} || 49.2 || 0.293 || Inuit group (Kiviuq) || 2000 || 2000 || Gladman et al. |- id="S/2020 S 48" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 48</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11355100}} || {{sort|451.75|+{{val|451.75}}}} || 45.9 || 0.373 || Inuit group (Kiviuq) || 2020 || 2026 || Ashton et al. |- id="S/2019 S 24" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 24</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11360500}} || {{sort|452.07|+{{val|452.07}}}} || 46.7 || 0.345 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al. |- id="S/2007 S 10" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2007 S 10</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11364900}} || {{sort|452.36|+{{val|452.36}}}} || 45.8 || 0.367 || Inuit group (Kiviuq) || 2007 || 2025 || Sheppard et al. |- id="S/2019 S 26" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 26</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11390900}} || {{sort|453.89|+{{val|453.89}}}} || 48.1 || 0.365 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 13" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 13</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11415600}} || {{sort|455.39|+{{val|455.39}}}} || 48.0 || 0.373 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 50" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 50</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11656500}} || {{sort|469.82|−{{val|469.82}}}} || 166.1 || 0.263 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 6" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 6</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11953100}} || {{sort|487.91|+{{val|487.91}}}} || 47.4 || 0.336 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 7" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 7</small> || ― || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|12133700}} || {{sort|499.01|+{{val|499.01}}}} || 44.7 || 0.284 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 38" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 38</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|12823500}} || {{sort|546.31|−{{val|546.31}}}} || 149.2 || 0.909 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al. |- id="Phoebe" style="background:#d3d3d3;" | {{sort|09|IX}} || {{hid|Phoebe}} ‡Phoebe || {{IPAc-en|ˈ|f|iː|b|i}} || style="background:black;"| frameless|upright=0.3|center|alt=An approximately spherical heavily cratered body is illuminated from the bottom-right. The terminator runs near the left and top limbs. There is huge crater at the top, which affects the shape, and another slightly smaller at the bottom. || 6.7 || {{sort|213.0|213.0<br>(219 × 217 × 204)}} || {{val|8312.3}} || {{val|12929400}} || {{sort|550.30|{{val|−550.30}}}} || 175.2 || 0.164 || Norse group (Phoebe) || 1898 || 1899 || Pickering |- id="S/2023 S 9" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 9</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|13167500}} || {{sort|564.11|−{{val|564.11}}}} || 172.2 || 0.141 || Norse group (Phoebe) || 2023 || 2025 || Ashton et al. |- id="S/2006 S 20" style="background:#d3d3d3;" | {{sort|Zzzc|}} || {{hid|S/2006N}} ‡<small>S/2006 S 20</small> || — || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|13193700}} || {{sort|565.79|{{val|−565.79}}}} || 173.1 || 0.206 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al. |- id="S/2004 S 56" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 56</small> || ― || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|13670200}} || {{sort|596.69|−{{val|596.69}}}} || 161.6 || 0.339 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al. |- id="S/2023 S 8" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 8</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14018800}} || {{sort|619.69|−{{val|619.69}}}}|| 166.9 || 0.122 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 62" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 62</small> || ― || style="background:black;"| || 16.9 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|14025900}} || {{sort|620.15|−{{val|620.15}}}} || 155.6 || 0.467 || Norse group (Kari) || 2023 || 2026 || Ashton et al. |- id="S/2023 S 11" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 11</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14046100}} || {{sort|621.49|−{{val|621.49}}}} || 170.9 || 0.300 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2006 S 9" style="background:#d3d3d3;" | {{sort|T|}} || {{hid|S/2006C}} ‡<small>S/2006 S 9</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14406700}} || {{sort|645.58|{{val|−645.58}}}} || 173.0 || 0.249 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al. |- id="S/2006 S 21" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 21</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14976500}} || {{sort|684.28|−{{val|684.28}}}} || 169.8 || 0.204 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al. |- id="Paaliaq" style="background:#F4C2C2;" | {{sort|20|XX}} || {{hid|Paaliaq}} ♦Paaliaq || {{IPAc-en|ˈ|p|ɑː|l|i|ɒ|k}} || style="background:black;"| frameless|upright=0.3|center || 11.7 || {{sort|25|≈&thinsp;25<ref>{{Cite web|url=https://tilmanndenk.de/outersaturnianmoons/paaliaq/|title=Paaliaq (S/2000 S 2) – Tilmann Denk}}</ref>}}|| {{sort|14|≈&thinsp;{{val|14}}}} || {{val|14997700}} || {{sort|685.72|+{{val|685.72}}}} || 48.5 || 0.378 || Inuit group{{refn|group=lower-alpha|The moon has a similar inclination, but a significantly different semi-major axis. Therefore, it is uncertain whether it comes from the same parent body as the rest of the Inuit group.<ref name="Ashton2025a"/>}} || 2000 || 2000 || Gladman et al. |- id="S/2006 S 22" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 22</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15109500}} || {{sort|693.41|−{{val|693.41}}}} || 172.0 || 0.246 || Norse group (Phoebe){{efn|group=lower-alpha|This moon's inclination of 172.0° is at the exact boundary between the Phoebe (i > 172°) and Mundilfari subgroups (172° > i > 157°). Because neither group's range is inclusive of the boundary value, S/2006 S 22 has been arbitrarily assigned to the Phoebe subgroup.}} || 2006 || 2025 || Sheppard et al. |- id="S/2023 S 13" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 13</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15193000}} || {{sort|699.18|−{{val|699.18}}}} || 168.5 || 0.179 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 10" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 10</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15500200}} || {{sort|720.49|−{{val|720.49}}}} || 163.0 || 0.302 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Skathi" style="background:#d3d3d3;" | {{sort|27|XXVII}} || {{hid|Skathi}} ‡Skathi || {{IPAc-en|ˈ|s|k|ɑː|ð|i}} || style="background:black;"| frameless|upright=0.3|center || 14.3 || {{sort|8|≈&thinsp;8}} || {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|15575400}} || {{sort|725.73|{{val|−725.73}}}} || 151.6 || 0.281 || Norse group (low-inclination) || 2000 || 2000 || Gladman et al. |- id="S/2023 S 12" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 12</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15805900}} || {{sort|741.92|−{{val|741.92}}}} || 168.8 || 0.601 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2007 S 5" style="background:#d3d3d3;" | {{sort|U|}} || {{hid|S/2007C}} ‡<small>S/2007 S 5</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15835600}} || {{sort|744.01|{{val|−744.01}}}} || 158.4 || 0.104 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al. |- id="S/2007 S 7" style="background:#d3d3d3;" | {{sort|Zzb|}} || {{hid|S/2007E}} ‡<small>S/2007 S 7</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15931600}} || {{sort|750.80|{{val|−750.80}}}} || 169.3 || 0.217 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al. |- id="S/2007 S 2" style="background:#d3d3d3;" | {{sort|O|}} || {{hid|S/2007A}} ‡<small>S/2007 S 2</small> || —|| style="background:black;"| || 15.6 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|15939100}} || {{sort|751.33|{{val|−751.33}}}} || 174.0 || 0.232 || Norse group (Phoebe){{refn|group=lower-alpha|name="Phoebe/Mundilfari"|The moon has been identified as potentially belonging to the Mundilfari subgroup due to its inclination and semi-major axis.<ref name="Ashton2025a"/>}} || 2007 || 2007 || Sheppard et al. |- id="S/2004 S 37" style="background:#d3d3d3;" | {{sort|K|}} || {{hid|S/2004T}} ‡<small>S/2004 S 37</small> || —|| style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15956300}} || {{sort|752.55|{{val|−752.55}}}} || 158.2 || 0.448 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2004 S 47" style="background:#d3d3d3;" | {{sort|Zu|}} || {{hid|S/2004Zd}} ‡<small>S/2004 S 47</small> || — || style="background:black;"| || 16.3 || {{sort|4|��&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|16050700}} || {{sort|759.22|{{val|−759.22}}}} || 160.9 || 0.291 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2004 S 40" style="background:#d3d3d3;" | {{sort|V|}} || {{hid|S/2004W}} ‡<small>S/2004 S 40</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|16075600}} || {{sort|761.00|{{val|−761.00}}}} || 169.2 || 0.297 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2020 S 14" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 14</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16186200}} || {{sort|768.86|−{{val|768.86}}}} || 161.7 || 0.313 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 27" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 27</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16267000}} || {{sort|774.63|−{{val|774.63}}}} || 162.1 || 0.420 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="Albiorix" style="background:#FDD5B1;" | {{sort|26|XXVI}} || {{hid|Albiorix}} ♣Albiorix || {{IPAc-en|ˌ|æ|l|b|i|ˈ|ɒr|ɪ|k|s}} || style="background:black;"| frameless|upright=0.3|center || 11.2 || 28.6 || {{sort|12|≈&thinsp;{{val|12}}}} || {{val|16329200}} || {{sort|779.07|+{{val|779.07}}}} || 36.8 || 0.482 || Gallic group || 2000 || 2000 || Holman |- id="S/2019 S 2" style="background:#d3d3d3;" | {{sort|W|}} || {{hid|S/2019B}} ‡<small>S/2019 S 2</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16560300}} || {{sort|795.67|{{val|−795.67}}}} || 173.3 || 0.279 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al. |- id="S/2020 S 15" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2020 S 15</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16729200}} || {{sort|807.82|+{{val|807.82}}}} || 37.1 || 0.462 || Gallic group || 2020 || 2025 || Ashton et al. |- id="S/2023 S 14" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 14</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16853000}} || {{sort|816.86|−{{val|816.86}}}} || 171.6 || 0.497 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 55" style="background: #fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 55</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16875100}} || {{sort|818.51|+{{val|818.51}}}} || 35.9 || 0.491 || Gallic group || 2023 || 2026 || Ashton et al. |- id="S/2020 S 16" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 16</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16963400}} || {{sort|824.92|−{{val|824.92}}}} || 167.3 || 0.405 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 16" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 16</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17005300}} || {{sort|827.91|−{{val|827.81}}}} || 162.6 || 0.270 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Bebhionn" style="background:#FDD5B1;" | {{sort|37|XXXVII}} || {{hid|Bebhionn}} ♣Bebhionn || {{IPAc-en|ˈ|b|eɪ|v|ɪ|n}} || style="background:black;"| frameless|upright=0.3|center || 15.0 || {{sort|6|≈&thinsp;6}} || {{sort|0.18|≈&thinsp;{{val|0.18}}}} || {{val|17027300}} || {{sort|829.64|+{{val|829.64}}}} || 38.6 || 0.459 || Gallic group || 2004 || 2005 || Sheppard et al. |- id="S/2007 S 8" style="background:#FDD5B1;" | {{sort|Zzc|}} || {{hid|S/2007F}} ♣<small>S/2007 S 8</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17048900}} || {{sort|831.21|+{{val|831.21}}}} || 36.2 || 0.490 || Gallic group || 2007 || 2023 || Sheppard et al. |- id="Saturn LX" style="background:#FDD5B1;" | {{sort|60|LX}} || {{hid|S/2004M}} ♣<small>S/2004 S 29</small> || —|| style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17063900}} || {{sort|832.27|+{{val|832.27}}}} || 38.6 || 0.485 || Gallic group || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 3" style="background:#d3d3d3;" | {{sort|X|}} || {{hid|S/2019C}} ‡<small>S/2019 S 3</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17077400}} || {{sort|833.19|{{val|−833.19}}}} || 166.9 || 0.248 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2020 S 17" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 17</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17094200}} || {{sort|834.45|−{{val|834.45}}}} || 148.9 || 0.378 || Norse group (low-inclination) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 53" style="background: #d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 53</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17181100}} || {{sort|840.82|−{{val|840.82}}}} || 171.2 || 0.103 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2023 S 58" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 58</small> || ― || style="background:black;"| || 16.9 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|17206000}} || {{sort|842.68|−{{val|842.68}}}} || 169.6 || 0.093 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2023 S 20" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 20</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17261000}} || {{sort|846.77|−{{val|846.77}}}} || 136.5 || 0.442 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 29" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 29</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17353900}} || {{sort|853.62|+{{val|853.62}}}} || 37.7 || 0.441 || Gallic group || 2019 || 2025 || Ashton et al. |- id="S/2023 S 18" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 18</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17381700}} || {{sort|855.65|+{{val|855.65}}}} || 36.7 || 0.448 || Gallic group || 2023 || 2025 || Ashton et al. |- id="S/2023 S 17" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 17</small> || ― || style="background:black;"| || 17.1 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17385300}} || {{sort|855.94|+{{val|855.94}}}} || 35.9 || 0.498 || Gallic group || 2023 || 2025 || Ashton et al. |- id="S/2020 S 7" style="background:#d3d3d3;" | {{sort|Zzd|}} || {{hid|S/2020G}} ‡<small>S/2020 S 7</small> || — || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17394000}} || {{sort|856.53|{{val|−856.53}}}} || 161.4 || 0.500 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="S/2007 S 11" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2007 S 11</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17434400}} || {{sort|859.53|+{{val|859.53}}}} || 35.5 || 0.499 || Gallic group || 2007 || 2025 || Sheppard et al. |- id="S/2023 S 54" style="background: #fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 54</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17485100}} || {{sort|863.35|+{{val|863.35}}}} || 37.8 || 0.480 || Gallic group || 2023 || 2026 || Ashton et al. |- id="S/2023 S 60" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 60</small> || ― || style="background:black;"| || 16.8 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|17493700}} || {{sort|863.96|−{{val|863.96}}}} || 170.7 || 0.206 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2019 S 28" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 28</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17496000}} || {{sort|864.09|−{{val|864.09}}}} || 158.4 || 0.199 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2004 S 31" style="background:#F4C2C2;" | {{sort|I|}} || {{hid|S/2004O}} ♦<small>S/2004 S 31</small> || —|| style="background:black;"| || 15.6 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17497100}} || {{sort|863.92|+{{val|863.92}}}} || 48.0 || 0.159 || Inuit group (Siarnaq) || 2004 || 2019 || Sheppard et al. |- id="Erriapus" style="background:#FDD5B1;" | {{sort|28|XXVIII}} || {{hid|Erriapus}} ♣Erriapus || {{IPAc-en|ɛ|r|i|ˈ|æ|p|ə|s}} || style="background:black;"| frameless|upright=0.3|center || 13.7 || {{sort|10|≈&thinsp;10}} || {{sort|0.95|≈&thinsp;{{val|0.95}}}} || {{val|17506900}} || {{sort|864.92|+{{val|864.92}}}} || 37.1 || 0.475 || Gallic group || 2000 || 2000 || Gladman et al. |- id="S/2023 S 19" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 19</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17590300}} || {{sort|870.92|+{{val|870.92}}}} || 48.2 || 0.092 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al. |- id="Skoll" style="background:#d3d3d3;" | {{sort|47|XLVII}} || {{hid|Skoll}} ‡Skoll || {{IPAc-en|ˈ|s|k|ɒ|l}} || style="background:black;"| frameless|upright=0.3|center || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|17623400}} || {{sort|873.57|{{val|−873.57}}}} || 159.4 || 0.463 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al. |- id="S/2023 S 3" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 3</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17646400}} || {{sort|875.00|+{{val|875.00}}}} || 46.9 || 0.178 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 30" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 30</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17709900}} || {{sort|879.97|−{{val|879.97}}}} || 168.3 || 0.107 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 19" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 19</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17726700}} || {{sort|881.04|+{{val|881.04}}}} || 48.1 || 0.159 || Inuit group (Siarnaq) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 31" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 31</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17739100}} || {{sort|882.24|+{{val|882.24}}}} || 39.8 || 0.488 || Gallic group || 2019 || 2025 || Ashton et al. |- id="Tarqeq" style="background:#F4C2C2;" | {{sort|52|LII}} || {{hid|Tarqeq}} ♦Tarqeq || {{IPAc-en|ˈ|t|ɑːr|k|eɪ|k}} ||style="background:black;"| frameless|upright=0.3|center || 14.8 || {{sort|7|≈&thinsp;7}}|| {{sort|0.18|≈&thinsp;{{val|0.18}}}} || {{val|17751000}} || {{sort|882.85|+{{val|882.85}}}} || 48.7 || 0.144 || Inuit group (Siarnaq) || 2007 || 2007 || Sheppard et al. |- id="S/2023 S 21" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 21</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17755400}} || {{sort|883.31|−{{val|883.31}}}} || 157.3 || 0.077 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 4" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 4</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17764600}} || {{sort|884.11|−{{val|884.11}}}} || 170.0 || 0.276 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 18" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 18</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17777900}} || {{sort|885.12|−{{val|885.12}}}} || 168.9 || 0.180 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 14" style="background:#F4C2C2;" | {{sort|Zze|}} || {{hid|S/2019N}} ♦<small>S/2019 S 14</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17852800}} || {{sort|893.15|+{{val|890.59}}}} || 46.2 || 0.172 || Inuit group (Siarnaq) || 2019 || 2023 || Ashton et al. |- id="S/2020 S 2" style="background:#d3d3d3;" | {{sort|Y|}} || {{hid|S/2020B}} ‡<small>S/2020 S 2</small> || — || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17869000}} || {{sort|891.86|{{val|−891.86}}}} || 170.7 || 0.152 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="Siarnaq" style="background:#F4C2C2;" | {{sort|29|XXIX}} || {{hid|Siarnaq}} ♦Siarnaq || {{IPAc-en|ˈ|s|iː|ɑːr|n|ə|k}} || style="background:black;"| frameless|upright=0.3|center || 10.6 || 39.3 || {{sort|32|≈&thinsp;{{val|32}}}} || {{val|17881100}} || {{sort|892.68|+{{val|892.68}}}} || 47.8 || 0.308 || Inuit group (Siarnaq) || 2000 || 2000 || Gladman et al. |- id="S/2019 S 4" style="background:#d3d3d3;" | {{sort|Za|}} || {{hid|S/2019D}} ‡<small>S/2019 S 4</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17951900}} || {{sort|898.09|{{val|−898.09}}}} || 170.1 || 0.408 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2019 S 32" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 32</small> || ― || style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17960500}} || {{sort|898.71|+{{val|898.71}}}} || 46.2 || 0.276 || Inuit group (Siarnaq) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 20" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 20</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17997300}} || {{sort|901.53|−{{val|901.53}}}} || 169.8 || 0.133 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2020 S 3" style="background:#F4C2C2;" | {{sort|Z|}} || {{hid|S/2020C}} ♦<small>S/2020 S 3</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18056800}} || {{sort|905.84|+{{val|905.84}}}} || 46.0 || 0.142 || Inuit group (Siarnaq) || 2020 || 2023 || Ashton et al. |- id="S/2023 S 61" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 61</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18067700}} || {{sort|906.85|−{{val|906.85}}}} || 158.0 || 0.557 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2004 S 41" style="background:#d3d3d3;" | {{sort|Zb|}} || {{hid|S/2004X}} ‡<small>S/2004 S 41</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18095400}} || {{sort|908.89|{{val|−908.89}}}} || 165.7 || 0.301 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2005 S 6" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2005 S 6</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18107300}} || {{sort|909.58|+{{val|909.58}}}} || 47.7 || 0.084 || Inuit group (Siarnaq) || 2005 || 2025 || Sheppard et al. |- id="S/2004 S 57" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 57</small> || ― || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18150500}} || {{sort|913.07|−{{val|913.07}}}} || 167.9 || 0.263 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al. |- id="S/2019 S 6" style="background:#F4C2C2;" | {{sort|Zn|}} || {{hid|S/2019F}} ♦<small>S/2019 S 6</small> || — || style="background:black;" | || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18205600}} || {{sort|917.11|+{{val|917.11}}}} || 46.4 || 0.120 || Inuit group (Siarnaq)|| 2019 || 2023 || Ashton et al. |- id="S/2006 S 24" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 24</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18210700}} || {{sort|917.56|−{{val|917.56}}}} || 165.9 || 0.352 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al. |- id="Tarvos" style="background:#FDD5B1;" | {{sort|21|XXI}} || {{hid|Tarvos}} ♣Tarvos || {{IPAc-en|ˈ|t|ɑːr|v|ə|s}} || style="background:black;"| frameless|upright=0.3|center || 13.1 || {{sort|15|≈&thinsp;15}} || {{sort|2.1|≈&thinsp;{{val|2.1}}}} || {{val|18216600}} || {{sort|917.98|+{{val|917.98}}}} || 37.8 || 0.522 || Gallic group || 2000 || 2000 || Gladman et al. |- id="S/2020 S 4" style="background:#FDD5B1;" | {{sort|Zc|}} || {{hid|S/2020D}} ♣<small>S/2020 S 4</small> || — || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18236400}} || {{sort|919.52|+{{val|919.52}}}} || 40.1 || 0.496 || Gallic group || 2020 || 2023 || Ashton et al. |- id="S/2023 S 30" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 30</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18238300}} || {{sort|919.71|−{{val|919.71}}}} || 142.4 || 0.493 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 42" style="background:#d3d3d3;" | {{sort|Zf|}} || {{hid|S/2004Y}} ‡<small>S/2004 S 42</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18240700}} || {{sort|919.88|{{val|−919.88}}}} || 165.7 || 0.158 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2023 S 15" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 15</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18241300}} || {{sort|919.93|−{{val|919.93}}}} || 161.9 || 0.549 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 58" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 58</small> || ― || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18254500}} || {{sort|920.80|+{{val|920.80}}}} || 45.7 || 0.249 || Inuit group (Siarnaq) || 2004 || 2025 || Sheppard et al. |- id="S/2006 S 23" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2006 S 23</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18269700}} || {{sort|921.86|+{{val|921.86}}}} || 43.8 || 0.190 || Inuit group (Siarnaq) || 2006 || 2025 || Sheppard et al. |- id="Hyrrokkin" style="background:#d3d3d3;" | {{sort|44|XLIV}} || {{hid|Hyrrokkin}} ‡Hyrrokkin || {{IPAc-en|h|ɪ|ˈ|r|ɒ|k|ə|n}} ||style="background:black;"| frameless|upright=0.3|center || 14.3 || {{sort|8|≈&thinsp;8}} || {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|18340900}} || {{sort|927.46|{{val|−927.46}}}} || 149.9 || 0.336 || Norse group (low-inclination) || 2004 || 2005 || Sheppard et al. |- id="S/2023 S 24" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 24</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18351800}} || {{sort|928.25|−{{val|928.25}}}} || 169.7 || 0.374 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Greip" style="background:#d3d3d3;" | {{sort|51|LI}} || {{hid|Greip}} ‡Greip || {{IPAc-en|ˈ|ɡ|r|eɪ|p}} || style="background:black;"| frameless|upright=0.3|center || 15.3 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|18380000}} || {{sort|930.44|{{val|−930.44}}}} || 174.2 || 0.317 || Norse group (Phoebe) || 2006 || 2006 || Sheppard et al. |- id="S/2020 S 5" style="background:#F4C2C2;" | {{sort|Zc|}} || {{hid|S/2020E}} ♦<small>S/2020 S 5</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18391000}} || {{sort|931.19|+{{val|931.19}}}} || 48.2 || 0.220 || Inuit group (Siarnaq) || 2020 || 2023 || Ashton et al. |- id="S/2019 S 34" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 34</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18446800}} || {{sort|935.45|+{{val|935.45}}}} || 37.6 || 0.536 || Gallic group || 2019 || 2025 || Ashton et al. |- id="S/2004 S 13" style="background:#d3d3d3;" | {{sort|D|}} || {{hid|S/2004C}} ‡<small>S/2004 S 13</small> || —|| style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18453700}} || {{sort|936.09|{{val|−936.09}}}} || 169.0 || 0.265 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2023 S 63" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 63</small> || ― || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18482600}} || {{sort|938.25|−{{val|938.25}}}} || 165.0 || 0.266 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2005 S 7" style="background:#fdd5b1;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2005 S 7</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18502500}} || {{sort|939.75|+{{val|939.75}}}} || 34.6 || 0.565 || Gallic group || 2005 || 2025 || Sheppard et al. |- id="S/2007 S 6" style="background:#d3d3d3;" | {{sort|Ze|}} || {{hid|S/2007D}} ‡<small>S/2007 S 6</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18545000}} || {{sort|942.98|{{val|−942.98}}}} || 166.5 || 0.168 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al. |- id="S/2019 S 35" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 35</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18557800}} || {{sort|944.00|−{{val|944.00}}}} || 157.3 || 0.577 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2006 S 25" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 25</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18572400}} || {{sort|945.07|−{{val|945.07}}}} || 158.8 || 0.303 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al. |- id="S/2023 S 22" style="background:#f4c2c2;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 22</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18577500}} || {{sort|945.37|+{{val|945.37}}}} || 47.5 || 0.182 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al. |- id="Mundilfari" style="background:#d3d3d3;" | {{sort|25|XXV}} || {{hid|Mundilfari}} ‡Mundilfari || {{IPAc-en|m|ʊ|n|d|əl|ˈ|v|ær|i}} || style="background:black;"| frameless|upright=0.3|center || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|18588200}} || {{sort|946.29|{{val|−946.29}}}} || 167.1 || 0.211 || Norse group (Mundilfari) || 2000 || 2000 || Gladman et al. |- id="S/2006 S 26" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 26</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18619300}} || {{sort|948.67|−{{val|948.67}}}} || 171.9 || 0.248 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al. |- id="S/2019 S 33" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 33</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18696100}} || {{sort|954.53|−{{val|954.53}}}} || 170.4 || 0.289 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2006 S 1" style="background:#d3d3d3;" | {{sort|M|}} || {{hid|S/2006A}} ‡<small>S/2006 S 1</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18746300}} || {{sort|958.32|{{val|−958.32}}}} || 156.1 || 0.105 || Norse group (Kari) || 2006 || 2006 || Sheppard et al. |- id="S/2023 S 23" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 23</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18783700}} || {{sort|961.22|−{{val|961.22}}}} || 164.8 || 0.350 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 21" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 21</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18862100}} || {{sort|967.26|−{{val|967.26}}}} || 169.9 || 0.307 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2020 S 46" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 46</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18892100}} || {{sort|969.60|−{{val|969.60}}}} || 167.3 || 0.207 || Norse group (Mundilfari) || 2020 || 2026 || Ashton et al. |- id="S/2004 S 43" style="background:#d3d3d3;" | {{sort|Zi|}} || {{hid|S/2004Z}} ‡<small>S/2004 S 43</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18935700}} || {{sort|972.85|{{val|−972.85}}}} || 171.1 || 0.432 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2006 S 10" style="background:#d3d3d3;" | {{sort|Zg|}} || {{hid|S/2006D}} ‡<small>S/2006 S 10</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18979900}} || {{sort|976.34|{{val|−976.34}}}} || 161.6 || 0.151 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2019 S 5" style="background:#d3d3d3;" | {{sort|Zh|}} || {{hid|S/2019E}} ‡<small>S/2019 S 5</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19090100}} || {{sort|984.87|{{val|−984.87}}}} || 158.8 || 0.216 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2023 S 25" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 25</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19136600}} || {{sort|988.53|−{{val|988.53}}}} || 166.4 || 0.281 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 59" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 59</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19170700}} || {{sort|991.18|−{{val|991.18}}}} || 167.3 || 0.262 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al. |- id="S/2006 S 27" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 27</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19205700}} || {{sort|993.79|−{{val|993.79}}}} || 170.5 || 0.140 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al. |- id="Gridr" style="background:#d3d3d3;" | {{sort|54|LIV}} || {{hid|Gridr}} ‡Gridr || {{IPAc-en|ˈ|g|r|i:|D|@r}} ||style="background:black;"| || 15.8 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19250600}} || {{sort|997.33|{{val|−997.33}}}} || 163.9 || 0.187 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="Bergelmir" style="background:#d3d3d3;" | {{sort|38|XXXVIII}} || {{hid|Bergelmir}} ‡Bergelmir || {{IPAc-en|b|ɛər|ˈ|j|ɛ|l|m|ɪər}} || style="background:black;"| frameless|upright=0.3|center || 15.2 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19268100}} || {{sort|998.62|{{val|−998.62}}}} || 158.8 || 0.145 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="Jarnsaxa" style="background:#d3d3d3;" | {{sort|50|L}} || {{hid|Jarnsaxa}} ‡Jarnsaxa || {{IPAc-en|j|ɑːr|n|ˈ|s|æ|k|s|ə}} ||style="background:black;"| || 15.6 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19273500}} || {{sort|999.13|{{val|−999.13}}}} || 163.0 || 0.218 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al. |- id="Narvi" style="background:#d3d3d3;" | {{sort|31|XXXI}} || {{hid|Narvi}} ‡Narvi || {{IPAc-en|ˈ|n|ɑːr|v|i}} || style="background:black;"| frameless|upright=0.3|center || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|19285000}} || {{sort|999.94|{{val|−999.94}}}} || 142.2 || 0.441 || Norse group (low-inclination) || 2003 || 2003 || Sheppard et al. |- id="S/2023 S 44" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 44</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19292400}} || {{sort|1000.47|−{{val|1000.47}}}} || 167.4 || 0.434 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Suttungr" style="background:#d3d3d3;" | {{sort|23|XXIII}} || {{hid|Suttungr}} ‡Suttungr || {{IPAc-en|ˈ|s|ʊ|t|ʊ|ŋ|ɡ|ər}} ||style="background:black;"| frameless|upright=0.3|center || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|19391900}} || {{sort|1008.25|{{val|−1008.25}}}} || 175.7 || 0.116 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al. |- id="S/2020 S 22" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 22</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19443000}} || {{sort|1012.24|−{{val|1012.24}}}} || 161.3 || 0.059 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2004 S 44" style="background:#d3d3d3;" | {{sort|Zj|}} || {{hid|S/2004Za}} ‡<small>S/2004 S 44</small> || — || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19515400}} || {{sort|1017.91|{{val|−1017.91}}}} || 167.7 || 0.129 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2004 S 60" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 60</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19517000}} || {{sort|1018.13|−{{val|1018.13}}}} || 173.8 || 0.280 || Norse group (Phoebe) || 2004 || 2025 || Sheppard et al. |- id="S/2006 S 12" style="background:#FDD5B1;" | {{sort|Zm|}} || {{hid|S/2006F}} ♣<small>S/2006 S 12</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19570300}} || {{sort|1022.29|+{{val|1022.29}}}} || 38.6 || 0.542 || Gallic group{{refn|group=lower-alpha|Sheppard et al. suggested in 2023 that the moon's identification with the Gallic group is uncertain,<ref name="Sheppard2023"/> but a later study from Ashton et al. considers it confidently Gallic and associated with Albiorix, unlike S/2004 S 24.<ref name="Ashton2025a"/>}} || 2006 || 2023 || Sheppard et al. |- id="S/2007 S 3" style="background:#d3d3d3;" | {{sort|P|}} || {{hid|S/2007B}} ‡<small>S/2007 S 3</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19614400}} || {{sort|1025.70|{{val|−1025.70}}}} || 173.8 || 0.150 || Norse group (Phoebe) || 2007 || 2007 || Sheppard et al. |- id="S/2004 S 45" style="background:#d3d3d3;" | {{sort|Zk|}} || {{hid|S/2004Zb}} ‡<small>S/2004 S 45</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19693700}} || {{sort|1031.86|{{val|−1031.86}}}} || 154.0 || 0.551 || Norse group (Kari) || 2004 || 2023 || Sheppard et al. |- id="Hati" style="background:#d3d3d3;" | {{sort|43|XLIII}} || {{hid|Hati}} ‡Hati || {{IPAc-en|ˈ|h|ɑː|t|i}} || style="background:black;"| frameless|upright=0.3|center || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19695000}} || {{sort|1032.02|{{val|−1032.02}}}} || 165.4 || 0.372 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2004 S 17" style="background:#d3d3d3;" | {{sort|E|}} || {{hid|S/2004D}} ‡<small>S/2004 S 17</small> || —||style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19699000}} || {{sort|1032.37|{{val|−1032.37}}}} || 167.9 || 0.162 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2006 S 11" style="background:#d3d3d3;" | {{sort|Zl|}} || {{hid|S/2006E}} ‡<small>S/2006 S 11</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19711900}} || {{sort|1033.35|{{val|−1033.35}}}} || 174.1 || 0.143 || Norse group (Phoebe) || 2004 || 2023 || Sheppard et al. |- id="S/2004 S 12" style="background:#d3d3d3;" | {{sort|C|}} || {{hid|S/2004B}} ‡<small>S/2004 S 12</small> || —||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19801000}} || {{sort|1040.39|{{val|−1040.39}}}} || 164.7 || 0.337 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2020 S 23" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 23</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19801500}} || {{sort|1040.38|−{{val|1040.38}}}} || 165.0 || 0.089 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 27" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 27</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19820100}} || {{sort|1041.85|−{{val|1041.85}}}} || 151.1 || 0.652 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al. |- id="Eggther" style="background:#d3d3d3;" | {{sort|59|LIX}} || {{hid|Eggther}} ‡Eggther || {{IPAc-en|ˈ|E|g|T|E@r}} ||style="background:black;"| || 15.4 || {{sort|6|≈&thinsp;6}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19844600}} || {{sort|1043.80|{{val|−1043.80}}}} || 165.0 || 0.157 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2023 S 28" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 28</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19881000}} || {{sort|1046.56|−{{val|1046.56}}}} || 168.7 || 0.575 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 37" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 37</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19889800}} || {{sort|1047.39|−{{val|1047.39}}}} || 172.3 || 0.215 || Norse group (Phoebe) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 26" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 26</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19894300}} || {{sort|1047.76|−{{val|1047.76}}}} || 163.9 || 0.306 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 36" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 36</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19903200}} || {{sort|1048.42|−{{val|1048.42}}}} || 166.9 || 0.161 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2006 S 13" style="background:#d3d3d3;" | {{sort|Zo|}} || {{hid|S/2006G}} ‡<small>S/2006 S 13</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19953300}} || {{sort|1052.32|{{val|−1052.32}}}} || 162.0 || 0.313 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2019 S 37" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 37</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19996900}} || {{sort|1055.78|−{{val|1055.78}}}} || 149.9 || 0.404 || Norse group (low-inclination) || 2019 || 2025 || Ashton et al. |- id="S/2023 S 48" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 48</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20029200}} || {{sort|1058.35|−{{val|1058.35}}}} || 169.7 || 0.022 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 29" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 29</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20042400}} || {{sort|1059.42|−{{val|1059.42}}}} || 172.2 || 0.141 || Norse group (Phoebe) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 59" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 59</small> || ― || style="background:black;"| || 16.9 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|20064000}} || {{sort|1061.04|−{{val|1061.04}}}} || 169.5 || 0.467 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2007 S 9" style="background:#d3d3d3;" | {{sort|Zzy|}} || {{hid|S/2007G}} ‡<small>S/2007 S 9</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20174600}} || {{sort|1069.81|{{val|−1069.81}}}} || 159.3 || 0.360 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al. |- id="S/2019 S 7" style="background:#d3d3d3;" | {{sort|Zp|}} || {{hid|S/2019G}} ‡<small>S/2019 S 7</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20185100}} || {{sort|1070.80|{{val|−1070.80}}}} || 174.2 || 0.233 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al. |- id="S/2019 S 8" style="background:#d3d3d3;" | {{sort|Zq|}} || {{hid|S/2019H}} ‡<small>S/2019 S 8</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20287400}} || {{sort|1078.86|{{val|−1078.86}}}} || 172.8 || 0.311 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al. |- id="Farbauti" style="background:#d3d3d3;" | {{sort|40|XL}} || {{hid|Farbauti}} ‡Farbauti || {{IPAc-en|f|ɑːr|ˈ|b|aʊ|t|i}} ||style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|20290700}} || {{sort|1079.12|{{val|−1079.12}}}} || 156.2 || 0.249 || Norse group (Kari) || 2004 || 2005 || Sheppard et al. |- id="Thrymr" style="background:#d3d3d3;" | {{sort|30|XXX}} || {{hid|Thrymr}} ‡Thrymr || {{IPAc-en|ˈ|θ|r|ɪ|m|ər}} || style="background:black;"| frameless|upright=0.3|center || 14.3 || {{sort|8|≈&thinsp;8}}|| {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|20330500}} || {{sort|1082.23|{{val|−1082.23}}}} || 175.0 || 0.467 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al. |- id="Bestla" style="background:#d3d3d3;" | {{sort|39|XXXIX}} || {{hid|Bestla}} ‡Bestla || {{IPAc-en|ˈ|b|ɛ|s|t|l|ə}} || style="background:black;"| frameless|upright=0.3|center || 14.6 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|20337800}} || {{sort|1082.94|{{val|−1082.94}}}} || 138.3 || 0.486 || Norse group (low-inclination) || 2004 || 2005 || Sheppard et al. |- id="S/2019 S 9" style="background:#d3d3d3;" | {{sort|Zr|}} || {{hid|S/2019I}} ‡<small>S/2019 S 9</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20359700}} || {{sort|1084.62|{{val|−1084.62}}}} || 159.5 || 0.433 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2023 S 32" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 32</small> || ― || style="background:black;"| || 17.2 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|20454400}} || {{sort|1092.24|−{{val|1092.24}}}} || 169.8 || 0.037 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 46" style="background:#d3d3d3;" | {{sort|Zs|}} || {{hid|S/2004Zc}} ‡<small>S/2004 S 46</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20513800}} || {{sort|1096.99|{{val|−1096.99}}}} || 177.2 || 0.249 || Norse group (Phoebe) || 2004 || 2023 || Sheppard et al. |- id="S/2023 S 57" style="background: #d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 57</small> || ― || style="background:black;"| || 17.2 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|20536100}} || {{sort|1098.83|−{{val|1098.83}}}} || 168.0 || 0.245 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="Angrboda" style="background:#d3d3d3;" | {{sort|55|LV}} || {{hid|Angrboda}} ‡Angrboda || {{IPAc-en|'|A:|N|g|@r|b|ou|D|@}} ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20591500}} || {{sort|1103.20|{{val|−1103.20}}}} || 177.7 || 0.216 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al. |- id="S/2020 S 24" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 24</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20618300}} || {{sort|1105.41|−{{val|1105.41}}}} || 159.6 || 0.230 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 11" style="background:#d3d3d3;" | {{sort|Zv|}} || {{hid|S/2019K}} ‡<small>S/2019 S 11</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20664200}} || {{sort|1109.11|{{val|−1109.11}}}} || 144.6 || 0.513 || Norse group (low-inclination) || 2019 || 2023 || Ashton et al. |- id="Aegir" style="background:#d3d3d3;" | {{sort|36|XXXVI}} || {{hid|Aegir}} ‡Aegir || {{IPAc-en|ˈ|aɪ|.|ɪər}} ||style="background:black;"| || 15.5 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|20664400}} || {{sort|1109.13|{{val|−1109.13}}}} || 166.1 || 0.255 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2019 S 10" style="background:#d3d3d3;" | {{sort|Zt|}} || {{hid|S/2019J}} ‡<small>S/2019 S 10</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20700300}} || {{sort|1111.99|{{val|−1111.99}}}} || 163.9 || 0.248 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="Beli" style="background:#d3d3d3;" | {{sort|61|LXI}} || {{hid|Beli}} ‡Beli || {{IPAc-en|ˈ|b|eI|l|i}} ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}}|| {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20703700}} || {{sort|1112.27|{{val|−1112.27}}}} || 158.9 || 0.087 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2023 S 31" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 31</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20729200}} || {{sort|1114.29|−{{val|1114.29}}}} || 163.0 || 0.182 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 25" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 25</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20763700}} || {{sort|1117.09|−{{val|1117.09}}}} || 171.8 || 0.316 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 34" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 34</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20803900}} || {{sort|1120.38|−{{val|1120.38}}}} || 168.4 || 0.570 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2023 S 39" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 39</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20824500}} || {{sort|1121.99|−{{val|1121.99}}}} || 164.8 || 0.124 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 12" style="background:#d3d3d3;" | {{sort|Zx|}} || {{hid|S/2019L}} ‡<small>S/2019 S 12</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20895000}} || {{sort|1127.60|{{val|−1127.60}}}} || 167.1 || 0.476 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="Gerd" style="background:#d3d3d3;" | {{sort|57|LVII}} || {{hid|Gerd}} ‡Gerd || {{IPAc-en|ˈ|j|E@r|D}} ||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}}|| {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20947500}} || {{sort|1131.91|{{val|−1131.91}}}} || 174.4 || 0.517 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 13" style="background:#d3d3d3;" | {{sort|Zz|}} || {{hid|S/2019M}} ‡<small>S/2019 S 13</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20964500}} || {{sort|1133.27|{{val|−1133.27}}}} || 177.3 || 0.318 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al. |- id="S/2004 S 61" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 61</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20986900}} || {{sort|1135.06|−{{val|1135.06}}}} || 168.4 || 0.466 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al. |- id="S/2006 S 14" style="background:#d3d3d3;" | {{sort|Zw|}} || {{hid|S/2006H}} ‡<small>S/2006 S 14</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21062300}} || {{sort|1141.27|{{val|−1141.27}}}} || 166.7 || 0.060 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2023 S 40" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 40</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21065100}} || {{sort|1141.48|−{{val|1141.48}}}} || 169.6 || 0.342 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Gunnlod" style="background:#d3d3d3;" | {{sort|62|LXII}} || {{hid|Gunnlod}} ‡Gunnlod || {{IPAc-en|ˈ|g|U|n|l|Q|D}} ||style="background:black;"| || 15.7 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21141800}} || {{sort|1147.74|{{val|−1147.74}}}} || 160.4 || 0.251 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 15" style="background:#d3d3d3;" | {{sort|Zzf|}} || {{hid|S/2019O}} ‡<small>S/2019 S 15</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21191100}} || {{sort|1151.66|{{val|−1151.66}}}} || 157.8 || 0.257 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2020 S 6" style="background:#d3d3d3;" | {{sort|Zy|}} || {{hid|S/2020F}} ‡<small>S/2020 S 6</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21253300}} || {{sort|1156.81|{{val|−1156.81}}}} || 166.9 || 0.480 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="S/2020 S 26" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 26</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21264400}} || {{sort|1157.77|−{{val|1157.77}}}} || 163.2 || 0.273 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 41" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 41</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21286400}} || {{sort|1159.52|−{{val|1159.52}}}} || 172.1 || 0.279 || Norse group (Phoebe) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 7" style="background:#d3d3d3;" | {{sort|B|}} || {{hid|S/2004A}} ‡<small>S/2004 S 7</small> || —||style="background:black;"| || 15.5 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21327600}} || {{sort|1162.93|{{val|−1162.93}}}} || 164.8 || 0.511 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2006 S 3" style="background:#d3d3d3;" | {{sort|N|}} || {{hid|S/2006B}} ‡<small>S/2006 S 3</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21353100}} || {{sort|1165.02|{{val|−1165.02}}}} || 156.1 || 0.432 || Norse group (Kari) || 2006 || 2006 || Sheppard et al. |- id="S/2005 S 5" style="background:#d3d3d3;" | {{sort|Zzg|}} || {{hid|S/2005B}} ‡<small>S/2005 S 5</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21364900}} || {{sort|1165.96|{{val|−1165.96}}}} || 169.5 || 0.588 || Norse group (Mundilfari) || 2005 || 2023 || Sheppard et al. |- id="S/2020 S 47" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 47</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21397400}} || {{sort|1168.58|−{{val|1168.58}}}} || 146.1 || 0.564 || Norse group (low-inclination) || 2020 || 2026 || Ashton et al. |- id="Skrymir" style="background:#d3d3d3;" | {{sort|56|LVI}} || {{hid|Skrymir}} ‡Skrymir || {{IPAc-en|ˈ|s|k|r|I|m|ɪər}} ||style="background:black;"| || 15.5 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21447400}} || {{sort|1172.72|{{val|−1172.72}}}} || 175.6 || 0.437 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al. |- id="S/2023 S 33" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 33</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21621900}} || {{sort|1187.07|−{{val|1187.07}}}} || 155.8 || 0.665 || Norse group (Kari) || 2023 || 2025 || Ashton et al. |- id="S/2006 S 16" style="background:#d3d3d3;" | {{sort|Zzi|}} || {{hid|S/2006J}} ‡<small>S/2006 S 16</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21721200}} || {{sort|1195.13|{{val|−1195.13}}}} || 164.1 || 0.204 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2023 S 49" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 49</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21766500}} || {{sort|1198.99|−{{val|1198.99}}}} || 171.7 || 0.026 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 30" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 30</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21790700}} || {{sort|1201.02|−{{val|1201.02}}}} || 154.2 || 0.601 || Norse group (Kari) || 2020 || 2025 || Ashton et al. |- id="S/2006 S 15" style="background:#d3d3d3;" | {{sort|Zzh|}} || {{hid|S/2006I}} ‡<small>S/2006 S 15</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|21799600}} || {{sort|1201.69|{{val|−1201.69}}}} || 161.1 || 0.117 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2020 S 27" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 27</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21802300}} || {{sort|1202.02|−{{val|1202.02}}}} || 145.3 || 0.255 || Norse group (low-inclination) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 42" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 42</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21837000}} || {{sort|1204.81|−{{val|1204.81}}}} || 166.7 || 0.059 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 28" style="background:#d3d3d3;" | {{sort|H|}} || {{hid|S/2004L}} ‡<small>S/2004 S 28</small> || — ||style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21865900}} || {{sort|1207.18|{{val|−1207.18}}}} || 167.9 || 0.159 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2020 S 32" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 32</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21884100}} || {{sort|1208.85|−{{val|1208.85}}}} || 169.1 || 0.502 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2006 S 28" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 28</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|21955100}} || {{sort|1214.53|−{{val|1214.53}}}} || 172.9 || 0.210 || Norse group (Phoebe) || 2006 || 2025 || Sheppard et al. |- id="S/2020 S 8" style="background:#d3d3d3;" | {{sort|Zzl|}} || {{hid|S/2020H}} ‡<small>S/2020 S 8</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21967200}} || {{sort|1215.61|{{val|−1215.61}}}} || 161.8 || 0.252 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="S/2020 S 28" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 28</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21993700}} || {{sort|1217.81|−{{val|1217.81}}}} || 160.1 || 0.474 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="Alvaldi" style="background:#d3d3d3;" | {{sort|65|LXV}} || {{hid|Alvaldi}} ‡Alvaldi || {{IPAc-en|O:|l|ˈ|v|O:|l|d|i}} ||style="background:black;"| || 15.6 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21993800}} || {{sort|1217.80|{{val|−1217.80}}}} || 177.4 || 0.238 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 38" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 38</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21998400}} || {{sort|1218.27|−{{val|1218.27}}}} || 163.0 || 0.399 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="Kari" style="background:#d3d3d3;" | {{sort|45|XLV}} || {{hid|Kari}} ‡Kari || {{IPAc-en|ˈ|k|ɑːr|i}} || style="background:black;"| frameless|upright=0.3|center || 14.5 || {{sort|6|≈&thinsp;6}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|22032100}} || {{sort|1220.98|{{val|−1220.98}}}} || 153.0 || 0.469 || Norse group (Kari) || 2006 || 2006 || Sheppard et al. |- id="S/2004 S 48" style="background:#d3d3d3;" | {{sort|Zzk|}} || {{hid|S/2004Ze}} ‡<small>S/2004 S 48</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22137400}} || {{sort|1229.86|{{val|−1229.86}}}} || 161.9 || 0.374 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2023 S 36" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 36</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22230600}} || {{sort|1237.61|−{{val|1237.61}}}} || 166.3 || 0.359 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="Geirrod" style="background:#d3d3d3;" | {{sort|66|LXVI}} || {{hid|Geirrod}} ‡Geirrod || {{IPAc-en|ˈ|j|ei|r|Q|d}} ||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22259400}} || {{sort|1240.05|{{val|−1240.05}}}} || 154.4 || 0.539 || Norse group (Kari) || 2004 || 2019 || Sheppard et al. |- id="S/2023 S 35" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 35</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22269700}} || {{sort|1240.76|−{{val|1240.76}}}} || 168.5 || 0.151 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 29" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 29</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22301400}} || {{sort|1243.45|−{{val|1243.45}}}} || 169.1 || 0.047 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="Fenrir" style="background:#d3d3d3;" | {{sort|41|XLI}} || {{hid|Fenrir}} ‡Fenrir || {{IPAc-en|ˈ|f|ɛ|n|r|ɪər}} ||style="background:black;"| || 15.8 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22330800}} || {{sort|1245.92|{{val|−1245.92}}}} || 164.5 || 0.137 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2004 S 50" style="background:#d3d3d3;" | {{sort|Zzn|}} || {{hid|S/2004Zg}} ‡<small>S/2004 S 50</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22345000}} || {{sort|1247.19|{{val|−1247.19}}}} || 164.0 || 0.450 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2006 S 17" style="background:#d3d3d3;" | {{sort|Zzj|}} || {{hid|S/2006K}} ‡<small>S/2006 S 17</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22384200}} || {{sort|1250.46|{{val|−1250.46}}}} || 168.7 || 0.425 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2004 S 49" style="background:#d3d3d3;" | {{sort|Zzm|}} || {{hid|S/2004Zf}} ‡<small>S/2004 S 49</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22399400}} || {{sort|1251.68|{{val|−1251.68}}}} || 159.8 || 0.453 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2020 S 34" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 34</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22435600}} || {{sort|1254.61|−{{val|1254.61}}}} || 160.6 || 0.154 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2020 S 31" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 31</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22457300}} || {{sort|1256.50|−{{val|1256.50}}}} || 163.8 || 0.238 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2023 S 52" style="background: #d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 52</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22528000}} || {{sort|1262.34|−{{val|1262.34}}}} || 146.2 || 0.124 || Norse group (low-inclination) || 2023 || 2026 || Ashton et al. |- id="S/2023 S 43" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 43</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22563900}} || {{sort|1265.57|−{{val|1265.57}}}} || 170.3 || 0.264 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2019 S 17" style="background:#d3d3d3;" | {{sort|Zzq|}} || {{hid|S/2019Q}} ‡<small>S/2019 S 17</small> || — || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22722700}} || {{sort|1278.96|{{val|−1278.96}}}} || 155.5 || 0.546 || Norse group (Kari) || 2019 || 2023 || Ashton et al. |- id="Surtur" style="background:#d3d3d3;" | {{sort|48|XLVIII}} || {{hid|Surtur}} ‡Surtur || {{IPAc-en|ˈ|s|ɜːr|t|ər}} ||style="background:black;"| || 15.7 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|22748000}} || {{sort|1281.14|{{val|−1281.14}}}} || 168.4 || 0.448 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al. |- id="S/2006 S 18" style="background:#d3d3d3;" | {{sort|Zzo|}} || {{hid|S/2006L}} ‡<small>S/2006 S 18</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22760600}} || {{sort|1282.09|{{val|−1282.09}}}} || 169.5 || 0.131 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al. |- id="S/2020 S 36" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 36</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22806200}} || {{sort|1286.03|−{{val|1286.03}}}} || 168.8 || 0.336 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="Loge" style="background:#d3d3d3;" | {{sort|46|XLVI}} || {{hid|Loge}} ‡Loge || {{IPAc-en|ˈ|l|ɔɪ|.|eɪ}} || style="background:black;"| frameless|upright=0.3|center || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|22919200}} || {{sort|1295.52|{{val|−1295.52}}}} || 168.1 || 0.191 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al. |- id="S/2020 S 33" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 33</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22922500}} || {{sort|1295.85|−{{val|1295.85}}}} || 162.8 || 0.555 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="Ymir" style="background:#d3d3d3;" | {{sort|19|XIX}} || {{hid|Ymir}} ‡Ymir || {{IPAc-en|ˈ|iː|m|ɪər}} || style="background:black;"| frameless|upright=0.3|center || 12.2 || {{sort|19|≈&thinsp;19}}|| {{sort|5.6|≈&thinsp;{{val|5.6}}}} || {{val|22955600}} || {{sort|1298.68|{{val|−1298.68}}}} || 172.3 || 0.338 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al. |- id="S/2020 S 35" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 35</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23030300}} || {{sort|1304.97|−{{val|1304.97}}}} || 174.9 || 0.225 || Norse group (Phoebe) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 19" style="background:#d3d3d3;" | {{sort|Zzs|}} || {{hid|S/2019S}} ‡<small>S/2019 S 19</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23044400}} || {{sort|1306.16|{{val|−1306.16}}}} || 151.8 || 0.458 || Norse group (Kari) || 2019 || 2023 || Ashton et al. |- id="S/2019 S 18" style="background:#d3d3d3;" | {{sort|Zzr|}} || {{hid|S/2019R}} ‡<small>S/2019 S 18</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23139500}} || {{sort|1314.27|{{val|−1314.27}}}} || 154.6 || 0.509 || Norse group (Kari) || 2019 || 2023 || Ashton et al. |- id="S/2004 S 21" style="background:#d3d3d3;" | {{sort|F|}} || {{hid|S/2004E}} ‡<small>S/2004 S 21</small> || — ||style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23160900}}|| {{sort|1316.12|{{val|−1316.12}}}}|| 153.2 || 0.394 || Norse group (Kari) || 2004 || 2019 || Sheppard et al. |- id="S/2004 S 39" style="background:#d3d3d3;" | {{sort|L|}} || {{hid|S/2004V}} ‡<small>S/2004 S 39</small> || — || style="background:black;" | || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23192400}} || {{sort|1318.74|{{val|−1318.74}}}} || 165.9 || 0.100 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 16" style="background:#d3d3d3;" | {{sort|Zzp|}} || {{hid|S/2019P}} ‡<small>S/2019 S 16</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23265200}} || {{sort|1324.95|{{val|−1324.95}}}} || 162.0 || 0.250 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2004 S 53" style="background:#d3d3d3;" | {{sort|Zzz|}} || {{hid|S/2004Zj}} ‡<small>S/2004 S 53</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23279800}} || {{sort|1326.18|{{val|−1326.18}}}} || 162.6 || 0.240 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2004 S 24" style="background:#FDD5B1;" | {{sort|G|}} || {{hid|S/2004H}} ♣<small>S/2004 S 24</small> || — || style="background:black;" | || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23338200}} || {{sort|1331.32|+{{val|1331.32}}}} || 37.4 || 0.071 || Gallic group{{refn|group=lower-alpha|The moon has a similar inclination, but a significantly larger semi-major axis. Therefore, it is uncertain whether it comes from the same parent body as the rest of the Gallic group.<ref name="Sheppard2023"/><ref name="Ashton2025a"/>}} || 2004 || 2019 || Sheppard et al. |- id="S/2004 S 36" style="background:#d3d3d3;" | {{sort|J|}} || {{hid|S/2004S}} ‡<small>S/2004 S 36</small> || — || style="background:black;" | || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23390800}} || {{sort|1335.80|{{val|−1335.80}}}} || 153.3 || 0.625 || Norse group (Kari) || 2004 || 2019 || Sheppard et al. |- id="S/2023 S 51" style="background: #d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 51</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23431500}} || {{sort|1339.21|−{{val|1339.21}}}} || 163.3 || 0.191 || Norse group (Mundilfari) || 2023 || 2026 || Ashton et al. |- id="S/2023 S 45" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 45</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23438400}} || {{sort|1339.85|−{{val|1339.85}}}} || 157.4 || 0.633 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 45" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 45</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23507700}} || {{sort|1345.79|−{{val|1345.79}}}} || 172.8 || 0.199 || Norse group (Phoebe) || 2020 || 2026 || Ashton et al. |- id="Thiazzi" style="background:#d3d3d3;" | {{sort|63|LXIII}} || {{hid|Thiazzi}} ‡Thiazzi || {{IPAc-en|T|i|ˈ|ae|t|s|i}} || style="background:black;" | || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23577500}}|| {{sort|1351.83|{{val|−1351.83}}}} || 158.8 || 0.511 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2020 S 38" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 38</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23583900}} || {{sort|1352.43|−{{val|1352.43}}}} || 159.7 || 0.513 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 20" style="background:#d3d3d3;" | {{sort|Zzt|}} || {{hid|S/2019T}} ‡<small>S/2019 S 20</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23677900}} || {{sort|1360.47|{{val|−1360.47}}}} || 156.0 || 0.354 || Norse group (Kari) || 2019 || 2023 || Ashton et al. |- id="S/2020 S 37" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 37</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23751800}} || {{sort|1366.82|−{{val|1366.82}}}} || 174.8 || 0.344 || Norse group (Phoebe) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 39" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 39</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23784500}} || {{sort|1369.64|−{{val|1369.64}}}} || 174.5 || 0.098 || Norse group (Phoebe) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 40" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 40</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23785900}} || {{sort|1369.76|−{{val|1369.76}}}} || 167.3 || 0.412 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2006 S 19" style="background:#d3d3d3;" | {{sort|Zzu|}} || {{hid|S/2006M}} ‡<small>S/2006 S 19</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23800500}} || {{sort|1371.02|{{val|−1371.02}}}} || 175.5 || 0.467 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al. |- id="S/2019 S 40" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 40</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24087800}} || {{sort|1395.88|−{{val|1395.88}}}} || 161.8 || 0.088 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2019 S 42" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 42</small> || ― || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|24111600}} || {{sort|1397.98|−{{val|1397.98}}}} || 163.2 || 0.121 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="Saturn LXIV" style="background:#d3d3d3;" | {{sort|64|LXIV}} || {{hid|S/2004Q}} ‡<small>S/2004 S 34</small> || — ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|24145800}} || {{sort|1400.93|{{val|−1400.93}}}} || 168.3 || 0.279 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al. |- id="S/2020 S 39" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 39</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24262400}} || {{sort|1411.15|−{{val|1411.15}}}} || 160.1 || 0.305 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 41" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 41</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24493600}} || {{sort|1431.30|−{{val|1431.30}}}} || 157.1 || 0.257 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2023 S 46" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 46</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24708900}} || {{sort|1450.27|−{{val|1450.27}}}} || 143.2 || 0.336 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al. |- id="Fornjot" style="background:#d3d3d3;" | {{sort|42|XLII}} || {{hid|Fornjot}} ‡Fornjot || {{IPAc-en|ˈ|f|ɔːr|n|j|ɒ|t}} || style="background:black;"| frameless|upright=0.3|center || 14.7 || {{sort|6|≈&thinsp;6}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|24936800}} || {{sort|1470.36|{{val|−1470.36}}}} || 170.0 || 0.213 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al. |- id="S/2023 S 47" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 47</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25102300}} || {{sort|1485.04|−{{val|1485.04}}}} || 162.5 || 0.101 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2004 S 51" style="background:#d3d3d3;" | {{sort|Zzv|}} || {{hid|S/2004Zh}} ‡<small>S/2004 S 51</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|25207100}} || {{sort|1494.41|{{val|−1494.41}}}} || 171.2 || 0.201 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2006 S 29" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 29</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25212100}} || {{sort|1494.78|−{{val|1494.78}}}} || 156.2 || 0.239 || Norse group (Kari) || 2006 || 2025 || Sheppard et al. |- id="S/2020 S 10" style="background:#d3d3d3;" | {{sort|Zzza|}} || {{hid|S/2020J}} ‡<small>S/2020 S 10</small> || — || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25315300}} || {{sort|1503.97|{{val|−1503.97}}}} || 165.6 || 0.296 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="S/2020 S 42" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 42</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25329400}} || {{sort|1505.31|−{{val|1505.31}}}} || 157.5 || 0.506 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2020 S 9" style="background:#d3d3d3;" | {{sort|Zzw|}} || {{hid|S/2020I}} ‡<small>S/2020 S 9</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|25408700}} || {{sort|1512.38|{{val|−1512.38}}}} || 161.4 || 0.531 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al. |- id="S/2023 S 5" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 5</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25583500}} || {{sort|1528.04|−{{val|1528.04}}}} || 168.8 || 0.599 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al. |- id="S/2020 S 41" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 41</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25876400}} || {{sort|1554.40|−{{val|1554.40}}}} || 160.2 || 0.402 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="Saturn LVIII" style="background:#d3d3d3;" | {{sort|58|LVIII}} || {{hid|S/2004J}} ‡<small>S/2004 S 26</small> || — ||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|26097500}} || {{sort|1574.25|{{val|−1574.25}}}} || 172.9 || 0.147 || Norse group (Phoebe){{refn|group=lower-alpha|name="Phoebe/Mundilfari"}} || 2004 || 2019 || Sheppard et al. |- id="S/2019 S 21" style="background:#d3d3d3;" | {{sort|Zzzb|}} || {{hid|S/2019U}} ‡<small>S/2019 S 21</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|26439500}} || {{sort|1605.28|{{val|−1605.28}}}} || 171.9 || 0.155 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al. |- id="S/2004 S 52" style="background:#d3d3d3;" | {{sort|Zzx|}} || {{hid|S/2004Zi}} ‡<small>S/2004 S 52</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26446400}} || {{sort|1605.89|{{val|−1605.89}}}} || 165.4 || 0.291 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al. |- id="S/2020 S 43" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 43</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26657400}} || {{sort|1625.29|−{{val|1625.29}}}} || 164.6 || 0.203 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |- id="S/2019 S 43" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 43</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26664100}} || {{sort|1625.90|−{{val|1625.90}}}} || 165.3 || 0.277 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al. |- id="S/2019 S 44" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 44</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26796900}} || {{sort|1638.11|−{{val|1638.11}}}} || 172.6 || 0.512 || Norse group (Phoebe) || 2019 || 2025 || Ashton et al. |- id="S/2020 S 44" style="background:#d3d3d3;" | {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 44</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|27259400}} || {{sort|1680.64|−{{val|1680.64}}}} || 168.5 || 0.199 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al. |} {{sticky table end}}

==Other objects==

=== Ring moonlets ===

Also existing in Saturn's ring system are moonlets: objects generally too small to be treated as moons or directly imaged, and usually short-lived or transient bodies.

During late July 2009, a moonlet, S/2009 S 1, was discovered in the B Ring, 480&nbsp;km from the outer edge of the ring, by the shadow it cast.<ref name="IAUC2009b" /> It is estimated to be 300&nbsp;m in diameter. Unlike the A Ring moonlets, it does not induce a 'propeller' feature, probably due to the density of the B Ring.<ref name="2009s1" /> Unlike most other objects referred to as 'moonlets', S/2009 S 1 is technically counted as a moon of Saturn, though it is almost never discussed in the same context as other inner moons.

In 2006, four tiny moonlets were found in ''Cassini'' images of the A Ring.<ref name="Tiscareno2006" /> Before this discovery only two larger moons had been known within gaps in the A Ring, Pan and Daphnis, which are large enough to clear continuous gaps in the ring.<ref name="Tiscareno2006" /> In contrast, a moonlet is only massive enough to clear two small—about 10&nbsp;km across—partial gaps in the immediate vicinity of the moonlet itself creating a structure shaped like an airplane propeller.<ref name="Sremcevic2007" /> The moonlets themselves are tiny, ranging from about 40 to 500&nbsp;meters in diameter, and are too small to be seen directly.<ref name="Tiscareno2008" />

In 2007, the discovery of 150 more moonlets revealed that they (with the exception of two that have been seen outside the Encke gap) are confined to three narrow bands in the A Ring between 126,750 and 132,000&nbsp;km from Saturn's center. Each band is about a thousand kilometers wide, which is less than 1% the width of Saturn's rings.<ref name="Tiscareno2008" /> This region is relatively free from the disturbances caused by resonances with larger satellites,<ref name="Tiscareno2008" /> although other areas of the A Ring without disturbances are apparently free of moonlets. The moonlets were probably formed from the breakup of a larger satellite.<ref name="Sremcevic2007" /> It is estimated that the A Ring contains 7,000–8,000 propellers larger than 0.8&nbsp;km in size and millions larger than 0.25&nbsp;km.<ref name="Tiscareno2008" /> In April 2014, NASA scientists reported the possible consolidation of a new moon within the A Ring, implying that Saturn's present moons may have formed in a similar process in the past when Saturn's ring system was much more massive.<ref name="NASA-20140414a"/>

Similar moonlets may reside in the F Ring.<ref name="Tiscareno2008" /> They have not been confirmed as solid bodies; it is not yet clear if these are real satellites or merely persistent clumps within the F Ring. There, "jets" of material may be due to collisions, initiated by perturbations from the nearby small moon Prometheus, of these moonlets with the core of the F Ring. One of the largest F Ring moonlets may be the as-yet unconfirmed object S/2004 S 6. The F Ring also contains transient "fans" which are thought to result from even smaller moonlets, about 1&nbsp;km in diameter, orbiting near the F Ring core.<ref name=Murray2008/>

The following is a table of selected moonlets observed by ''Cassini'', including unconfirmed bodies.<ref name=Porco2005/>

{| class="wikitable" |- ! Name ! Image ! Diameter (km) ! Semi-major<br>axis (km) ! Orbital<br>period (d) ! Position ! Discovery year ! Status |- | A Ring moonlets<ref name="Tiscareno2008" /> || style="background:black;" |frameless|upright=0.3|center|alt=A noisy image showing a few bright dots marked by circles || {{sort|0.22|0.04–0.4}} || {{sort|130000|≈&thinsp;{{val|130000}}}} || {{sort|0.55|≈&thinsp;+{{val|0.55}}}}|| Three 1,000&nbsp;km bands within A Ring || 2006 || — |- | S/2004 S 3 and S 4<ref name="Spitale Jacobson et al. 2006" />|| style="background:black;" |frameless|upright=0.3|| ≈&thinsp;3–5 || ≈&thinsp;{{val|140300}}|| ≈&thinsp;+{{val|0.619}} | rowspan="2" |uncertain objects around the F Ring|| 2004 |Were undetected in thorough imaging of the region in November 2004, making their existence improbable. S/2004 S 4 was most likely a transient clump—it has not been recovered since the first sighting.<ref name="Porco2005" /> |- | S/2004 S 6<ref name="Spitale Jacobson et al. 2006" />|| style="background:black;" |frameless|upright=0.3|alt=A bright narrow band runs from the top to bottom. To the right of it in the diffuse halo the is a bright small object.|| ≈&thinsp;3–5 || ≈&thinsp;{{val|140130}}|| +{{val|0.61801}} || 2004 |Consistently detected into 2005, may be surrounded by fine dust and have a very small physical core |}

===Spurious=== Two moons were claimed to be discovered by different astronomers but never seen again. Both moons were said to orbit between Titan and Hyperion.<ref name=Solarviews/> *Chiron which was supposedly sighted by Hermann Goldschmidt in 1861, but never observed by anyone else.<ref name=Solarviews/> *Themis was allegedly discovered in 1905 by astronomer William Pickering, but never seen again. Nevertheless, it was included in numerous almanacs and astronomy books until the 1960s.<ref name=Solarviews/>

===Hypothetical=== In 2022, scientists of the Massachusetts Institute of Technology proposed the hypothetical former moon Chrysalis, using data from the Cassini–Huygens mission. Chrysalis would have orbited between Titan and Iapetus, but its orbit would have gradually become more eccentric until it was torn apart by Saturn. 99% of its mass would have been absorbed by Saturn, while the remaining 1% would have formed Saturn's rings.<ref>{{Cite web|url=https://www.newscientist.com/article/2337884-saturns-rings-could-have-come-from-a-destroyed-moon-named-chrysalis/|title=Saturn's rings could have come from a destroyed moon named Chrysalis|date=15 September 2022|website=New Scientist|access-date=16 September 2022|archive-date=16 September 2022|archive-url=https://web.archive.org/web/20220916161501/https://www.newscientist.com/article/2337884-saturns-rings-could-have-come-from-a-destroyed-moon-named-chrysalis/|url-status=live}}</ref><ref>{{Cite journal|url=https://www.science.org/doi/10.1126/science.abn1234|title=Loss of a satellite could explain Saturn's obliquity and young rings|first1=Jack|last1=Wisdom|first2=Rola|last2=Dbouk|first3=Burkhard|last3=Militzer|first4=William B.|last4=Hubbard|first5=Francis|last5=Nimmo|first6=Brynna G.|last6=Downey|first7=Richard G.|last7=French|date=September 16, 2022|journal=Science|volume=377|issue=6612|pages=1285–1289|doi=10.1126/science.abn1234|pmid=36107998|bibcode=2022Sci...377.1285W |hdl=1721.1/148216 |s2cid=252310492 |url-access=subscription|hdl-access=free}}</ref>

===Temporary=== Much like Jupiter, asteroids and comets will infrequently make close approaches to Saturn, even more infrequently becoming captured into orbit of the planet. The comet P/2020 F1 (Leonard) is calculated to have made a close approach of {{val|978000|65000}} km ({{val|608000|40000}} mi) to Saturn on 8 May 1936, closer than the orbit of Titan to the planet, with an orbital eccentricity of only {{val|1.098|0.007}}. The comet may have been orbiting Saturn prior to this as a temporary satellite, but difficulty modelling the non-gravitational forces makes whether or not it was indeed a temporary satellite uncertain.<ref>{{cite web |last1=Deen |first1=Sam |title=P/2020 F1 (Leonard): A previous-perihelion precovery, and a very, very young comet. |url=https://groups.io/g/mpml/message/35416 |website=groups.io |access-date=27 March 2020 |archive-date=27 March 2020 |archive-url=https://web.archive.org/web/20200327032811/https://groups.io/g/mpml/message/35416 |url-status=live}}</ref>

Other comets and asteroids may have temporarily orbited Saturn at some point, but none are presently known to have.

==See also== *List of natural satellites

==Notes== {{Reflist|30em| group = lower-alpha}}

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==External links== {{Commons category}} *Scott S. Sheppard: [https://sites.google.com/carnegiescience.edu/sheppard/moons/saturnmoons Saturn Moons] *{{cite web |url=http://orinetz.com/planet/animatesystem.php?ephid=Q07IAL5QATR7V073RO44XQVPA00001 |title=Simulation showing the position of Saturn's Moons |access-date=26 May 2010 |url-status=dead |archive-url=https://web.archive.org/web/20110823202308/http://orinetz.com/planet/animatesystem.php?ephid=Q07IAL5QATR7V073RO44XQVPA00001 |archive-date=23 August 2011}} *{{cite web|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Rings|title=Saturn's Rings|publisher=NASA's Solar System Exploration|access-date=26 May 2010|url-status=dead|archive-url=https://web.archive.org/web/20100527141504/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Rings|archive-date=27 May 2010}} *{{cite web|url=http://www.astronomycast.com/astronomy/episode-61-saturns-moons/|title=Saturn's Moons|date=6 November 2007 |publisher=Astronomy Cast episode No. 61, includes full transcript|access-date=26 May 2010}} *{{cite video|url=https://www.youtube.com/watch?v=xxXa9pxwzoY|people=Carolyn Porco|title=Fly me to the moons of Saturn|access-date=26 May 2010}} *[https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html Rotate and Spin Maps of 7 Moons] at ''The New York Times'' *Planetary Society [http://www.planetary.org/blogs/emily-lakdawalla/2017/0517-saturns-small-satellites-to-scale.html blog post] (2017-05-17) by Emily Lakdawalla with images giving comparative sizes of the moons *Tilmann Denk: [https://tilmanndenk.de/outersaturnianmoons/ Outer Moons of Saturn]

{{Moons of Saturn}} {{Saturn}} {{Solar System moons (compact)}} {{Solar System}} {{Portal bar|Stars|Spaceflight|Outer space|Science}} {{Authority control}}

{{DEFAULTSORT:Moons Of Saturn}} Category:Moons of Saturn Category:Lists of moons Category:Solar System