{{Short description|Distinct parts of a shadow}} thumb|275px|right|Umbra, penumbra and antumbra of Earth and images that could be seen at some points in these areas (Note: the relative size and distance of the bodies shown are not to scale.) thumb|Umbra (A) and penumbra (B) The '''umbra''', '''penumbra''' and '''antumbra''' are three distinct parts of a shadow, created by any light source after impinging on an opaque object of lesser size. In cases of equal or larger impinging objects, only an umbra and penumbra are generated. Assuming no diffraction, for a collimated beam (such as a point source) of light, only the umbra is cast.<ref name=TandD></ref>
These phenomena are generally observed within solar systems, as the size of the stars within the system are larger than the orbiting satellites, hence these terms are most often used for the shadows cast by celestial bodies, though they are sometimes used to describe levels of darkness, such as in sunspots.<ref>{{cite book |author1=Vázquez, M. |editor1-last=Murdin |editor1-first=P. |title=Encyclopedia of Astronomy & Astrophysics |date=31 December 2000 |publisher=Institute of Physics Publishing |location=Bristol |doi=10.1201/9781003220435 |isbn=9781003220435 |page=2082 |edition=1st |url=https://www.taylorfrancis.com/books/mono/10.1201/9781003220435/encyclopedia-astronomy-astrophysics-murdin |access-date=18 March 2026 |format=Hardcover}}</ref>
==Umbra== {{Redirect|Umbra}} thumb|200px|right|Umbra, penumbra and antumbra formed through windows and shutters
The '''umbra''' ({{langnf|la||shadow}}) is the innermost and darkest part of a shadow, where the light source is completely blocked by the occluding body.<ref>{{cite web |url=https://www.merriam-webster.com/dictionary/umbra |title=umbra |website=Merriam-Webster |access-date=August 4, 2025 |archive-url=https://web.archive.org/web/20250608074031/https://www.merriam-webster.com/dictionary/umbra |archive-date=June 8, 2025 |url-status=live}}</ref> An observer within the umbra experiences a total occultation. The umbra of a round body occluding a round light source forms a right circular cone. When viewed from the cone's apex, the two bodies appear the same size.<ref>{{cite web |last1=Bikos |first1=Konstantin |title=Eclipses: What Is the Umbra? |url=https://www.timeanddate.com/eclipse/umbra-shadow.html |website=timeanddate |publisher=© Time and Date AS |access-date=18 March 2026}}</ref>
The distance from the Moon to the apex of its umbra is roughly equal to that between the Moon and Earth: {{cvt|384402|km|mi}}. Since Earth's diameter is 3.7 times the Moon's, its umbra extends correspondingly farther: roughly {{convert|1.4|e6km|mi|abbr=unit}}.<ref>{{cite web |url=http://www.astronomy.ohio-state.edu/~pogge/Ast161/Unit2/eclipses.html |title=Lecture 9: Eclipses of the Sun & Moon |work=Astronomy 161: An Introduction to Solar System Astronomy |first=Richard |last=Pogge |publisher=Ohio State University |access-date=July 16, 2015}}</ref>
== Penumbra == {{redirect|Penumbra}}
The '''penumbra''' ({{etymology|la|{{wikt-lang|la|paene}}|almost, nearly||{{wikt-lang|la|umbra}}|shadow}}) is the region in which only a portion of the light source is obscured by the occluding body, and an observer in the penumbra experiences a partial eclipse.<ref>{{cite web |last1=Bikos |first1=Konstantin |title=Eclipses: What Is the Penumbra? |url=https://www.timeanddate.com/eclipse/penumbra-shadow.html |website=timeanddate |publisher=© Time and Date AS |access-date=18 March 2026}}</ref>
An alternative definition is that the penumbra is the region where ''some or all'' of the light source is obscured (i.e., the umbra is a subset of the penumbra). For example, NASA's Navigation and Ancillary Information Facility defines that a body in the umbra is also within the penumbra.<ref>[http://naif.jpl.nasa.gov/pub/naif/misc/toolkit_docs_N0061/Tutorials/pdf/individual_docs/45_event_finding_preview.pdf ''Event Finding Subsystem Preview''] Navigation and Ancillary Information Facility.</ref>
[[File:Earth umbral cone (partial).png|thumb|center|upright=3|Scale diagram of Earth's shadow, showing how the umbral cone extends beyond the orbit of the Moon (The Moon is indicated by the yellow dot.)]] thumb|upright=3|center|Earth's umbra, as seen during a partial lunar eclipse {{clear}}
== Antumbra == [[File: Transit Of Mercury, May 9th, 2016.png|thumb|Transit of Mercury in front of the Sun, an extreme version of an annular eclipse. Mercury is visible as a black dot below and to the left of the center. The dark area above the center of the solar disk is a sunspot.]]
The '''antumbra''' ({{etymology|la|{{wikt-lang|la|ante}}|before||{{wikt-lang|la|umbra}}|shadow}}) is the region from which the occluding body appears entirely within the disc of the light source. An observer in this region experiences an annular eclipse, in which a bright ring is visible around the eclipsing body.<ref name=TandD>{{cite web |last1=Bikos |first1=Konstantin |title=Eclipses: What Is the Antumbra? |url=https://www.timeanddate.com/eclipse/antumbra-shadow.html |website=timeanddate |publisher=© Time and Date AS |access-date=18 March 2026}}</ref> If the observer moves closer to the light source, the apparent size of the occluding body increases until it causes a full umbra.<ref name=TandD></ref>
== See also == * Antisolar point * Earth's shadow * Umbrella
==References== {{reflist}}
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Category:Optical phenomena Category:Shadows