Antisolar point: Difference between revisions
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The '''antisolar point''' is the [[vanishing point|abstract point]] on the [[celestial sphere]] directly opposite of the [[Sun]] from an observer's [[perspective (graphical)|perspective]].<ref name="timherd">{{cite web |first=Tim |last=Herd |url=http://www.timherd.com/wp-content/uploads/2012/03/angularmeasurements.pdf |title=Angular Measurements in the sky |work=Kaleidoscope Sky |page=27 |publisher=Abrams |year=2007 |isbn=0-8109-9397-X}}</ref> This means that the antisolar point lies above the [[horizon]] when the Sun is below it, and vice versa. On a [[daytime|sunny day]], the antisolar point can be easily found; it is located within the [[shadow]] of the observer's head. Like the [[zenith]] and [[nadir]], the antisolar point is not fixed in [[three-dimensional space]], but is defined relative to the observer. Each observer has their own antisolar point, which moves along with them as they change position. |
The '''antisolar point''' is the [[vanishing point|abstract point]] on the [[celestial sphere]] directly opposite of the [[Sun]] from an observer's [[perspective (graphical)|perspective]].<ref name="timherd">{{cite web |first=Tim |last=Herd |url=http://www.timherd.com/wp-content/uploads/2012/03/angularmeasurements.pdf |title=Angular Measurements in the sky |work=Kaleidoscope Sky |page=27 |publisher=Abrams |year=2007 |isbn=0-8109-9397-X}}</ref> This means that the antisolar point lies above the [[horizon]] when the Sun is below it, and vice versa. On a [[daytime|sunny day]], the antisolar point can be easily found; it is located within the [[shadow]] of the observer's head. Like the [[zenith]] and [[nadir]], the antisolar point is not fixed in [[three-dimensional space]], but is defined relative to the observer. Each observer has their own antisolar point, which moves along with them as they change position. |
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The antisolar point forms the [[centre (geometry)|geometric center]] of several [[optical phenomena]], including subhorizon [[halo (optical phenomenon)|haloes]], [[rainbow]]s,<ref>{{cite web |url=http://www.atoptics.co.uk/rainbows/primary.htm |title=Primary rainbows |publisher=atoptics.co.uk |first=Les |last=Cowley |accessdate=13 September 2013}}</ref> [[glory (optical phenomenon)|glories]],<ref>{{cite web |url=http://www.atoptics.co.uk/droplets/glory.htm |title=The Glory |publisher=atoptics.co.uk |first=Les |last=Cowley}}</ref> and [[heiligenschein]]. Occasionally, around [[sunset]] or [[sunrise]], [[anticrepuscular rays]] appear to converge toward the antisolar point near the horizon.<ref>{{cite web |url=http://www.atoptics.co.uk/atoptics/anti1.htm |title=Anticrepuscular rays |publisher=atoptics.co.uk |first=Les |last=Cowley |accessdate=13 September 2013}}</ref> However, this is an [[optical illusion]] caused by perspective; in reality, the "rays" (i.e. bands of shadow) run near-parallel to each other.<ref>{{cite web |url=http://www.atoptics.co.uk/fz892.htm |title=Antisolar or anticrepuscular rays |publisher=atoptics.co.uk |first=Les |last=Cowley}}</ref> |
The antisolar point forms the [[centre (geometry)|geometric center]] of several [[optical phenomena]], including subhorizon [[halo (optical phenomenon)|haloes]], [[rainbow]]s,<ref>{{cite web |url=http://www.atoptics.co.uk/rainbows/primary.htm |title=Primary rainbows |publisher=atoptics.co.uk |first=Les |last=Cowley |accessdate=13 September 2013}}</ref> [[glory (optical phenomenon)|glories]],<ref>{{cite web |url=http://www.atoptics.co.uk/droplets/glory.htm |title=The Glory |publisher=atoptics.co.uk |first=Les |last=Cowley}}</ref> the [[Brocken spectre]], and [[heiligenschein]]. Occasionally, around [[sunset]] or [[sunrise]], [[anticrepuscular rays]] appear to converge toward the antisolar point near the horizon.<ref>{{cite web |url=http://www.atoptics.co.uk/atoptics/anti1.htm |title=Anticrepuscular rays |publisher=atoptics.co.uk |first=Les |last=Cowley |accessdate=13 September 2013}}</ref> However, this is an [[optical illusion]] caused by perspective; in reality, the "rays" (i.e. bands of shadow) run near-parallel to each other.<ref>{{cite web |url=http://www.atoptics.co.uk/fz892.htm |title=Antisolar or anticrepuscular rays |publisher=atoptics.co.uk |first=Les |last=Cowley}}</ref> |
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Also around the antisolar point, the [[gegenschein]] is often visible in a moonless [[night sky]] away from [[light pollution|city lights]], arising from the [[backscatter]] of [[sunlight]] by [[interplanetary dust]]. In [[astronomy]], the [[full Moon]] or a [[planet]] in [[opposition (planets)|opposition]] lies around the antisolar point. During a total [[lunar eclipse]], the full Moon enters the [[umbra]] of [[Earth's shadow]], which the planet has been casting onto [[atmosphere of Earth|its atmosphere]], into space, and toward the antisolar point. |
Also around the antisolar point, the [[gegenschein]] is often visible in a moonless [[night sky]] away from [[light pollution|city lights]], arising from the [[backscatter]] of [[sunlight]] by [[interplanetary dust]]. In [[astronomy]], the [[full Moon]] or a [[planet]] in [[opposition (planets)|opposition]] lies around the antisolar point. During a total [[lunar eclipse]], the full Moon enters the [[umbra]] of [[Earth's shadow]], which the planet has been casting onto [[atmosphere of Earth|its atmosphere]], into space, and toward the antisolar point. |
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Revision as of 16:26, 24 January 2019
The antisolar point is the abstract point on the celestial sphere directly opposite of the Sun from an observer's perspective.[1] This means that the antisolar point lies above the horizon when the Sun is below it, and vice versa. On a sunny day, the antisolar point can be easily found; it is located within the shadow of the observer's head. Like the zenith and nadir, the antisolar point is not fixed in three-dimensional space, but is defined relative to the observer. Each observer has their own antisolar point, which moves along with them as they change position.
The antisolar point forms the geometric center of several optical phenomena, including subhorizon haloes, rainbows,[2] glories,[3] the Brocken spectre, and heiligenschein. Occasionally, around sunset or sunrise, anticrepuscular rays appear to converge toward the antisolar point near the horizon.[4] However, this is an optical illusion caused by perspective; in reality, the "rays" (i.e. bands of shadow) run near-parallel to each other.[5]
Also around the antisolar point, the gegenschein is often visible in a moonless night sky away from city lights, arising from the backscatter of sunlight by interplanetary dust. In astronomy, the full Moon or a planet in opposition lies around the antisolar point. During a total lunar eclipse, the full Moon enters the umbra of Earth's shadow, which the planet has been casting onto its atmosphere, into space, and toward the antisolar point.
Anthelic point
The anthelic point is often used as a synonym for the antisolar point, but the two should be differentiated.[1] While the antisolar point is directly opposite the sun, always below the horizon when the sun is up, the anthelic point is opposite but at the same elevation as the sun, and is therefore located on the parhelic circle. There are several halo phenomena that are centered on or converge on the anthelic point, such as the anthelion, Wegener arcs, Tricker arcs and the parhelic circle itself.[6][7][8]
See also
References
- ^ a b Herd, Tim (2007). "Angular Measurements in the sky" (PDF). Kaleidoscope Sky. Abrams. p. 27. ISBN 0-8109-9397-X.
- ^ Cowley, Les. "Primary rainbows". atoptics.co.uk. Retrieved 13 September 2013.
- ^ Cowley, Les. "The Glory". atoptics.co.uk.
- ^ Cowley, Les. "Anticrepuscular rays". atoptics.co.uk. Retrieved 13 September 2013.
- ^ Cowley, Les. "Antisolar or anticrepuscular rays". atoptics.co.uk.
- ^ Alexander Wünsche; Jim Foster, Anthelion and anthelic arcs, 2006
- ^ Walter Tape, Atmospheric Halos, ISSN 0066-4634, ISBN 0875908349, American Geophysical Union, 1994, p. 27
- ^ Les Cowley. South Pole Halos – Anthelic View – Atmospheric Optics, accessed 13 September 2013