# Kappa Lupi

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Binary star in the constellation Lupus

Kappa Lupi Location of κ Lupi (circled in red) Observation data Epoch J2000.0 Equinox ICRS Constellation Lupus[1][2] κ1 Lup Right ascension 15h 11m 56.07286s[3] Declination −48° 44′ 16.1692″[3] Apparent magnitude (V) 3.86[4] κ2 Lup Right ascension 15h 11m 57.67537s[5] Declination −48° 44′ 37.2684″[5] Apparent magnitude (V) 5.70[2] Characteristics κ1 Lup Spectral type B9.5 Vne[6] U−B color index −0.08[4] B−V color index −0.05[4] κ2 Lup Evolutionary stage main sequence[5] Spectral type A3/5V[7] B−V color index +0.144±0.008[2] Astrometry κ1 Lup Radial velocity (Rv) −6.6±2.9[8] km/s Proper motion (μ) RA: −96.50[3] mas/yr Dec.: −49.86[3] mas/yr Parallax (π) 18.12±0.47 mas[3] Distance 180 ± 5 ly (55 ± 1 pc) κ2 Lup Radial velocity (Rv) +0.0±3.7[9] km/s Proper motion (μ) RA: −98.497 mas/yr[5] Dec.: −43.645 mas/yr[5] Parallax (π) 17.906±0.0587 mas[5] Distance 182.1 ± 0.6 ly (55.8 ± 0.2 pc) Absolute magnitude (MV) +1.84[10] Details κ1 Lup Mass 2.89±0.03[11] M☉ Radius 3.0[12] R☉ Luminosity 90[12] L☉ Surface gravity (log g) 3.99±0.14[13] cgs Temperature 10,280[12] K Rotational velocity (v sin i) 191±16[11] km/s Age 121[13] Myr κ2 Lup Mass 2.0[12] M☉ Radius 1.8[12] R☉ Luminosity 13[12] L☉ Surface gravity (log g) 4.26[12] cgs Temperature 8,255[12] K Metallicity [Fe/H] −0.01[14] dex Rotational velocity (v sin i) 160.4±1.0[15] km/s Age 653[5] Myr Other designations κ1 Lup: CD−48°9704, FK5 1398, HD 134481, HIP 74376, HR 5646, SAO 225525[16] κ2 Lup: CD−48°9705, HD 134482, HIP 74380, HR 5647, SAO 225526[17] Database references SIMBAD κ1 Lup SIMBAD κ2 Lup

**Kappa Lupi** is a [binary star](/source/Binary_star)[18] in the constellation of Lupus. With a combined [apparent magnitude](/source/Apparent_magnitude) of 3.70,[19] it is visible to the [naked eye](/source/Naked_eye). The average distance to this system, based on [parallax](/source/Parallax) measurements, is 180 [light-years](/source/Light-year).

The stars in the system are separated by an [angular separation](/source/Angular_separation) of 26.44[″](/source/Second_of_arc).[18] At their distance, this corresponds to a [projected separation](/source/Projected_separation) of 1,450 [astronomical units](/source/Astronomical_unit).[20] They are members of the [Hyades Stream](/source/Hyades_Stream), which is a [moving group](/source/Moving_group) that is coincident with the [proper motions](/source/Proper_motion) of the [Hyades](/source/Hyades_(star_cluster)) cluster.[21]

The primary, Kappa1 Lupi, has an [apparent magnitude](/source/Apparent_magnitude) of 3.86.[4] It is a [B-type main sequence star](/source/B-type_main_sequence_star) with a [stellar classification](/source/Stellar_classification) of B9.5 Vne.[6] The 'n' suffix indicates the [spectrum](/source/Spectrum) shows "nebulous" [absorption lines](/source/Absorption_line) due to rapid rotation, while the 'e' means this is a [Be star](/source/Be_star) that displays [Balmer series](/source/Balmer_series) emission lines. With an estimated age of 195 million years,[6] it is about 75% of the way through its life span on the [main sequence](/source/Main_sequence).[11] The star is rotating with a [projected rotational velocity](/source/Projected_rotational_velocity) of 191 km/s.[11] This rate of spin is giving the star an [oblate](/source/Oblate_spheroid) shape with an [equatorial bulge](/source/Equatorial_bulge) that is an estimated 9% larger than the polar radius.[22]

The secondary, Kappa2 Lupi, has an [apparent magnitude](/source/Apparent_magnitude) of 5.70.[2] It is an [A-type main-sequence star](/source/A-type_main-sequence_star) with a [stellar classification](/source/Stellar_classification) of A3/5V.[7] The star has a high rotation rate, showing a [projected rotational velocity](/source/Projected_rotational_velocity) of 160 km/s.[15] It is 2.0 times more massive and 1.8 times larger than the Sun, with 13 times the Sun's luminosity and an [effective temperature](/source/Effective_temperature) of 8,255 K.[12]

In [Chinese astronomy](/source/Chinese_astronomy), Kappa1 Lupi is called 騎陣將軍, [Pinyin](/source/Pinyin): Qízhènjiāngjūn, meaning *Chariots and Cavalry General*, because this star is marking itself and stand alone in *Chariots and Cavalry General* asterism, [Root](/source/Root_(Chinese_constellation)) mansion (see : [Chinese constellation](/source/Chinese_constellation)).[23]

## References

1. **[^](#cite_ref-XHIP-k1_1-0)** Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". *[Astronomy Letters](/source/Astronomy_Letters)*. **38** (5): 331. [arXiv](/source/ArXiv_(identifier)):[1108.4971](https://arxiv.org/abs/1108.4971). [Bibcode](/source/Bibcode_(identifier)):[2012AstL...38..331A](https://ui.adsabs.harvard.edu/abs/2012AstL...38..331A). [doi](/source/Doi_(identifier)):[10.1134/S1063773712050015](https://doi.org/10.1134%2FS1063773712050015). [XHIP record for this object](https://vizier.cds.unistra.fr/viz-bin/VizieR-4?-ref=VIZ681510a8389ecb&-out.src=V%2F137D%2FXHIP&-nav=cat%3AV%2F137D%26tab%3A{V%2F137D%2FXHIP}%26key%3Asource%3DV%2F137D%2FXHIP%26HTTPPRM%3A&-source=V%2F137D%2FXHIP&-out=HIP&HIP=74376&-out=Comp&-out=Gr&-out=RAJ2000&-out=DEJ2000&-out=Dist&-out=X&-out=Y&-out=Z&-out=SpType&-out=Simbad&-out=Hpmag&-out=Lum&-out=Cst) at [VizieR](/source/VizieR).

1. ^ [***a***](#cite_ref-XHIP-k2_2-0) [***b***](#cite_ref-XHIP-k2_2-1) [***c***](#cite_ref-XHIP-k2_2-2) [***d***](#cite_ref-XHIP-k2_2-3) Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". *[Astronomy Letters](/source/Astronomy_Letters)*. **38** (5): 331. [arXiv](/source/ArXiv_(identifier)):[1108.4971](https://arxiv.org/abs/1108.4971). [Bibcode](/source/Bibcode_(identifier)):[2012AstL...38..331A](https://ui.adsabs.harvard.edu/abs/2012AstL...38..331A). [doi](/source/Doi_(identifier)):[10.1134/S1063773712050015](https://doi.org/10.1134%2FS1063773712050015). [XHIP record for this object](https://vizier.cds.unistra.fr/viz-bin/VizieR-4?-ref=VIZ681510a8389ecb&-out.src=V%2F137D%2FXHIP&-nav=cat%3AV%2F137D%26tab%3A{V%2F137D%2FXHIP}%26key%3Asource%3DV%2F137D%2FXHIP%26HTTPPRM%3A&-source=V%2F137D%2FXHIP&-out=HIP&HIP=74380&-out=Comp&-out=Gr&-out=RAJ2000&-out=DEJ2000&-out=Dist&-out=X&-out=Y&-out=Z&-out=SpType&-out=Simbad&-out=Hpmag&-out=Lum&-out=Cst) at [VizieR](/source/VizieR).

1. ^ [***a***](#cite_ref-vanLeeuwen2007_3-0) [***b***](#cite_ref-vanLeeuwen2007_3-1) [***c***](#cite_ref-vanLeeuwen2007_3-2) [***d***](#cite_ref-vanLeeuwen2007_3-3) [***e***](#cite_ref-vanLeeuwen2007_3-4) van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", *Astronomy and Astrophysics*, **474** (2): 653–664, [arXiv](/source/ArXiv_(identifier)):[0708.1752](https://arxiv.org/abs/0708.1752), [Bibcode](/source/Bibcode_(identifier)):[2007A&A...474..653V](https://ui.adsabs.harvard.edu/abs/2007A&A...474..653V), [doi](/source/Doi_(identifier)):[10.1051/0004-6361:20078357](https://doi.org/10.1051%2F0004-6361%3A20078357), [S2CID](/source/S2CID_(identifier)) [18759600](https://api.semanticscholar.org/CorpusID:18759600).

1. ^ [***a***](#cite_ref-Mermilliod1986_4-0) [***b***](#cite_ref-Mermilliod1986_4-1) [***c***](#cite_ref-Mermilliod1986_4-2) [***d***](#cite_ref-Mermilliod1986_4-3) Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", *Catalogue of Eggen's UBV Data*, [SIMBAD](/source/SIMBAD), [Bibcode](/source/Bibcode_(identifier)):[1986EgUBV........0M](https://ui.adsabs.harvard.edu/abs/1986EgUBV........0M).

1. ^ [***a***](#cite_ref-GaiaDR3-k2_5-0) [***b***](#cite_ref-GaiaDR3-k2_5-1) [***c***](#cite_ref-GaiaDR3-k2_5-2) [***d***](#cite_ref-GaiaDR3-k2_5-3) [***e***](#cite_ref-GaiaDR3-k2_5-4) [***f***](#cite_ref-GaiaDR3-k2_5-5) Vallenari, A.; et al. (Gaia collaboration) (2023). ["*Gaia* Data Release 3. Summary of the content and survey properties"](https://doi.org/10.1051%2F0004-6361%2F202243940). *Astronomy and Astrophysics*. **674**: A1. [arXiv](/source/ArXiv_(identifier)):[2208.00211](https://arxiv.org/abs/2208.00211). [Bibcode](/source/Bibcode_(identifier)):[2023A&A...674A...1G](https://ui.adsabs.harvard.edu/abs/2023A&A...674A...1G). [doi](/source/Doi_(identifier)):[10.1051/0004-6361/202243940](https://doi.org/10.1051%2F0004-6361%2F202243940). [S2CID](/source/S2CID_(identifier)) [244398875](https://api.semanticscholar.org/CorpusID:244398875). [Gaia DR3 record for this source](https://vizier.cds.unistra.fr/viz-bin/VizieR-4?-source=+I%2F355&-from=nav&-nav=cat%3AI%2F355%26tab%3A%7BI%2F355%2Fgaiadr3%7D%26key%3Asource%3D1355%2Fgaiadr3%26HTTPPRM%3A%26-out.add%3D.%26Source%3D%3D%3D5902489102985502208%26-go+%25%23Sesame%23%25%26) at [VizieR](/source/VizieR).

1. ^ [***a***](#cite_ref-levenhagen2006_6-0) [***b***](#cite_ref-levenhagen2006_6-1) [***c***](#cite_ref-levenhagen2006_6-2) Levenhagen, R. S.; Leister, N. V. (2006), "Spectroscopic analysis of southern B and Be stars", *Monthly Notices of the Royal Astronomical Society*, **371** (1): 252–262, [arXiv](/source/ArXiv_(identifier)):[astro-ph/0606149](https://arxiv.org/abs/astro-ph/0606149), [Bibcode](/source/Bibcode_(identifier)):[2006MNRAS.371..252L](https://ui.adsabs.harvard.edu/abs/2006MNRAS.371..252L), [doi](/source/Doi_(identifier)):[10.1111/j.1365-2966.2006.10655.x](https://doi.org/10.1111%2Fj.1365-2966.2006.10655.x), [S2CID](/source/S2CID_(identifier)) [16492030](https://api.semanticscholar.org/CorpusID:16492030).

1. ^ [***a***](#cite_ref-houk1978_7-0) [***b***](#cite_ref-houk1978_7-1) Houk, Nancy (1978), *Michigan catalogue of two-dimensional spectral types for the HD stars*, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, [Bibcode](/source/Bibcode_(identifier)):[1978mcts.book.....H](https://ui.adsabs.harvard.edu/abs/1978mcts.book.....H).

1. **[^](#cite_ref-deBruijne2012_8-0)** de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", *Astronomy & Astrophysics*, **546**: 14, [arXiv](/source/ArXiv_(identifier)):[1208.3048](https://arxiv.org/abs/1208.3048), [Bibcode](/source/Bibcode_(identifier)):[2012A&A...546A..61D](https://ui.adsabs.harvard.edu/abs/2012A&A...546A..61D), [doi](/source/Doi_(identifier)):[10.1051/0004-6361/201219219](https://doi.org/10.1051%2F0004-6361%2F201219219), [S2CID](/source/S2CID_(identifier)) [59451347](https://api.semanticscholar.org/CorpusID:59451347), A61.

1. **[^](#cite_ref-Kharchenko2007_9-0)** Kharchenko, N. V.; et al. (2007), "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations", *Astronomische Nachrichten*, **328** (9): 889, [arXiv](/source/ArXiv_(identifier)):[0705.0878](https://arxiv.org/abs/0705.0878), [Bibcode](/source/Bibcode_(identifier)):[2007AN....328..889K](https://ui.adsabs.harvard.edu/abs/2007AN....328..889K), [doi](/source/Doi_(identifier)):[10.1002/asna.200710776](https://doi.org/10.1002%2Fasna.200710776), [S2CID](/source/S2CID_(identifier)) [119323941](https://api.semanticscholar.org/CorpusID:119323941).

1. **[^](#cite_ref-ap1999_10-0)** Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". *Astronomy and Astrophysics*. **352**: 555. [arXiv](/source/ArXiv_(identifier)):[astro-ph/9911002](https://arxiv.org/abs/astro-ph/9911002). [Bibcode](/source/Bibcode_(identifier)):[1999A&A...352..555A](https://ui.adsabs.harvard.edu/abs/1999A&A...352..555A).

1. ^ [***a***](#cite_ref-Zorec2012_11-0) [***b***](#cite_ref-Zorec2012_11-1) [***c***](#cite_ref-Zorec2012_11-2) [***d***](#cite_ref-Zorec2012_11-3) Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", *Astronomy & Astrophysics*, **537**: A120, [arXiv](/source/ArXiv_(identifier)):[1201.2052](https://arxiv.org/abs/1201.2052), [Bibcode](/source/Bibcode_(identifier)):[2012A&A...537A.120Z](https://ui.adsabs.harvard.edu/abs/2012A&A...537A.120Z), [doi](/source/Doi_(identifier)):[10.1051/0004-6361/201117691](https://doi.org/10.1051%2F0004-6361%2F201117691), [S2CID](/source/S2CID_(identifier)) [55586789](https://api.semanticscholar.org/CorpusID:55586789).

1. ^ [***a***](#cite_ref-tic_12-0) [***b***](#cite_ref-tic_12-1) [***c***](#cite_ref-tic_12-2) [***d***](#cite_ref-tic_12-3) [***e***](#cite_ref-tic_12-4) [***f***](#cite_ref-tic_12-5) [***g***](#cite_ref-tic_12-6) [***h***](#cite_ref-tic_12-7) [***i***](#cite_ref-tic_12-8) Stassun, Keivan G.; et al. (2019). ["The Revised TESS Input Catalog and Candidate Target List"](https://doi.org/10.3847%2F1538-3881%2Fab3467). *The Astronomical Journal*. **158** (4): 138. [arXiv](/source/ArXiv_(identifier)):[1905.10694](https://arxiv.org/abs/1905.10694). [Bibcode](/source/Bibcode_(identifier)):[2019AJ....158..138S](https://ui.adsabs.harvard.edu/abs/2019AJ....158..138S). [doi](/source/Doi_(identifier)):[10.3847/1538-3881/ab3467](https://doi.org/10.3847%2F1538-3881%2Fab3467).

1. ^ [***a***](#cite_ref-David2015_13-0) [***b***](#cite_ref-David2015_13-1) David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", *The Astrophysical Journal*, **804** (2): 146, [arXiv](/source/ArXiv_(identifier)):[1501.03154](https://arxiv.org/abs/1501.03154), [Bibcode](/source/Bibcode_(identifier)):[2015ApJ...804..146D](https://ui.adsabs.harvard.edu/abs/2015ApJ...804..146D), [doi](/source/Doi_(identifier)):[10.1088/0004-637X/804/2/146](https://doi.org/10.1088%2F0004-637X%2F804%2F2%2F146), [S2CID](/source/S2CID_(identifier)) [33401607](https://api.semanticscholar.org/CorpusID:33401607).

1. **[^](#cite_ref-Netopil2017_14-0)** Netopil, Martin (August 2017), "Metallicity calibrations for dwarf stars and giants in the Geneva photometric system", *Monthly Notices of the Royal Astronomical Society*, **469** (3): 3042–3055, [arXiv](/source/ArXiv_(identifier)):[1705.00883](https://arxiv.org/abs/1705.00883), [Bibcode](/source/Bibcode_(identifier)):[2017MNRAS.469.3042N](https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.3042N), [doi](/source/Doi_(identifier)):[10.1093/mnras/stx1077](https://doi.org/10.1093%2Fmnras%2Fstx1077), [S2CID](/source/S2CID_(identifier)) [119034918](https://api.semanticscholar.org/CorpusID:119034918).

1. ^ [***a***](#cite_ref-Diaz2011_15-0) [***b***](#cite_ref-Diaz2011_15-1) Díaz, C. G.; et al. (July 2011), "Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum", *Astronomy & Astrophysics*, **531**: A143, [arXiv](/source/ArXiv_(identifier)):[1012.4858](https://arxiv.org/abs/1012.4858), [Bibcode](/source/Bibcode_(identifier)):[2011A&A...531A.143D](https://ui.adsabs.harvard.edu/abs/2011A&A...531A.143D), [doi](/source/Doi_(identifier)):[10.1051/0004-6361/201016386](https://doi.org/10.1051%2F0004-6361%2F201016386), [S2CID](/source/S2CID_(identifier)) [119286673](https://api.semanticscholar.org/CorpusID:119286673).

1. **[^](#cite_ref-SIMBAD-k1_16-0)** ["kap01 Lup"](http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=kap01+Lup). *[SIMBAD](/source/SIMBAD)*. [Centre de données astronomiques de Strasbourg](/source/Centre_de_donn%C3%A9es_astronomiques_de_Strasbourg). Retrieved 2017-03-07.{{[cite web](https://en.wikipedia.org/wiki/Template:Cite_web)}}: CS1 maint: postscript ([link](https://en.wikipedia.org/wiki/Category:CS1_maint:_postscript))

1. **[^](#cite_ref-SIMBAD-k2_17-0)** ["kap02 lup"](http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=kap02+lup). *[SIMBAD](/source/SIMBAD)*. [Centre de données astronomiques de Strasbourg](/source/Centre_de_donn%C3%A9es_astronomiques_de_Strasbourg). Retrieved 2019-09-14.

1. ^ [***a***](#cite_ref-Eggleton2008_18-0) [***b***](#cite_ref-Eggleton2008_18-1) Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", *[Monthly Notices of the Royal Astronomical Society](/source/Monthly_Notices_of_the_Royal_Astronomical_Society)*, **389** (2): 869–879, [arXiv](/source/ArXiv_(identifier)):[0806.2878](https://arxiv.org/abs/0806.2878), [Bibcode](/source/Bibcode_(identifier)):[2008MNRAS.389..869E](https://ui.adsabs.harvard.edu/abs/2008MNRAS.389..869E), [doi](/source/Doi_(identifier)):[10.1111/j.1365-2966.2008.13596.x](https://doi.org/10.1111%2Fj.1365-2966.2008.13596.x), [S2CID](/source/S2CID_(identifier)) [14878976](https://api.semanticscholar.org/CorpusID:14878976).

1. **[^](#cite_ref-Ducati2002_19-0)** Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". *VizieR Online Data Catalog*. **2237**. [Bibcode](/source/Bibcode_(identifier)):[2002yCat.2237....0D](https://ui.adsabs.harvard.edu/abs/2002yCat.2237....0D).

1. **[^](#cite_ref-20)** 26.44" • 55 pc = 1,450 AU.

1. **[^](#cite_ref-eggen1996_21-0)** Eggen, Olin J. (1996), "The Stellar Content of Star Stream I", *Astronomical Journal*, **111**: 1615, [Bibcode](/source/Bibcode_(identifier)):[1996AJ....111.1615E](https://ui.adsabs.harvard.edu/abs/1996AJ....111.1615E), [doi](/source/Doi_(identifier)):[10.1086/117901](https://doi.org/10.1086%2F117901)

1. **[^](#cite_ref-belle2012_22-0)** Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", *The Astronomy and Astrophysics Review*, **20** (1): 51, [arXiv](/source/ArXiv_(identifier)):[1204.2572](https://arxiv.org/abs/1204.2572), [Bibcode](/source/Bibcode_(identifier)):[2012A&ARv..20...51V](https://ui.adsabs.harvard.edu/abs/2012A&ARv..20...51V), [doi](/source/Doi_(identifier)):[10.1007/s00159-012-0051-2](https://doi.org/10.1007%2Fs00159-012-0051-2), [S2CID](/source/S2CID_(identifier)) [119273474](https://api.semanticscholar.org/CorpusID:119273474).

1. **[^](#cite_ref-23)** (in Chinese) [AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 29 日](http://aeea.nmns.edu.tw/2006/0606/ap060629.html) [Archived](https://web.archive.org/web/20210605100121/http://aeea.nmns.edu.tw/2006/0606/ap060629.html) 2021-06-05 at the [Wayback Machine](/source/Wayback_Machine)

## External links

- Kaler, James B. (August 17, 2012), ["Kappa Lupi"](https://web.archive.org/web/20190117031227/http://stars.astro.illinois.edu/sow/kappalup.html), *Stars*, University of Illinois, archived from [the original](http://stars.astro.illinois.edu/sow/kappalup.html) on January 17, 2019, retrieved March 8, 2017.

v t e Constellation of Lupus List of stars in Lupus Lupus in Chinese astronomy Stars Bayer α (Uridim) β γ δ ε ζ η θ ι κ λ μ ν1 ν2 ξ ο π ρ σ τ1 τ2 υ φ1 φ2 χ ψ1 ψ2 ω Flamsteed 1 (i) 2 (f) Variable RU EX GG GQ HR II IL IM KT (d) V407 V462 HR 5362 5364 5401 5651 (e) 5724 (k) 5825 (g) 5943 5967 HD 134004 135344 136164 141943 142527 143811 Other Gliese 588 HIP 70849 Lupus-TR-3 SSSPM J1549−3544 WASP-132 Exoplanets GQ Lupi b HIP 70849 b Lupus-TR-3b WASP-178b Star clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category

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Adapted from the Wikipedia article [Kappa Lupi](https://en.wikipedia.org/wiki/Kappa_Lupi) by Wikipedia contributors ([contributor history](https://en.wikipedia.org/wiki/Kappa_Lupi?action=history)). Available under [Creative Commons Attribution-ShareAlike 4.0 International](https://creativecommons.org/licenses/by-sa/4.0/). Changes may have been made.