76P/West–Kohoutek–Ikemura: Difference between revisions
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'''76P/West–Kohoutek–Ikemura''' is a Jupiter-family periodic comet in our Solar System with a current orbital period of 6.48 years. <ref> {{cite web|url = http://cometography.com/pcomets/076P.html| title= 76P/West-Kohoutek-Ikemura|accessdate = 25 February 2015}} </ref> <ref> {{cite web|url = http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=c&o=0076P|title= Elements and Ephemeris for 76P/West-Kohoutek-Ikemura|publisher= International Astronomical Union|accessdate = 25 February 2015}} </ref> |
'''76P/West–Kohoutek–Ikemura''' is a Jupiter-family periodic comet in our Solar System with a current orbital period of 6.48 years. <ref> {{cite web|url = http://cometography.com/pcomets/076P.html| title= 76P/West-Kohoutek-Ikemura|accessdate = 25 February 2015}} </ref> <ref> {{cite web|url = http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=c&o=0076P|title= Elements and Ephemeris for 76P/West-Kohoutek-Ikemura|publisher= International Astronomical Union|accessdate = 25 February 2015}} </ref> |
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The comet was initially spotted on a photographic plate by [[Richard M. West]] at the [[European Southern Observatory]] Sky Atlas Laboratory, Geneva in January 1975, when it had a brightness of [[Magnitude (astronomy)|magnitude]] 12. |
The comet was initially spotted on a photographic plate by [[Richard M. West]] at the [[European Southern Observatory]] Sky Atlas Laboratory, Geneva in January 1975, when it had a brightness of [[Magnitude (astronomy)|magnitude]] 12. Inability to predict its movement from a single image meant the comet had to be presumed lost. |
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In late February it was accidentally rediscovered by [[Lubos Kohoutek]] at the [[Hamburg Observatory]], Germany and independently on 1 March by [[Toshihiko Ikemura]] in Shinshiro, Japan. After further observations the comets parabolic orbit was computed, which gave a perihelion date of 23 March 1975 and proved that all three sightings were of the same object, which was accordingly designated 76P/West–Kohoutek–Ikemura. |
In late February it was accidentally rediscovered by [[Lubos Kohoutek]] at the [[Hamburg Observatory]], Germany and independently on 1 March by [[Toshihiko Ikemura]] in Shinshiro, Japan. After further observations the comets parabolic orbit was computed, which gave a perihelion date of 23 March 1975 and proved that all three sightings were of the same object, which was accordingly designated 76P/West–Kohoutek–Ikemura. |
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The comet has been observed at its successive returns in 1987, 1993, 2000, 2006 and 2013. |
The comet has been observed at its successive returns in 1987, 1993, 2000, 2006 and 2013. |
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==References== |
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{{reflist}} |
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==See also== |
==See also== |
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Revision as of 11:21, 25 February 2015
| Discovery | |
|---|---|
| Discovered by | Richard M. West at the European Southern Observatory Sky Atlas Laboratory, Geneva, Lubos Kohoutek at the Hamburg Observatory, Germany and Toshihiko Ikemura in Shinshiro, Japan |
| Discovery date | January-March 1975 |
| Orbital characteristics | |
| Epoch | 2014-Dec-9 |
| Aphelion | 5.345 AU |
| Perihelion | 1.6012 AU |
| Semi-major axis | 3.4707 AU |
| Eccentricity | 0.5387 |
| Orbital period | 6.48 yr |
| Inclination | 30.48° |
| Last perihelion | 7 May 2013 |
| Next perihelion | 26 Oct 2019 |
76P/West–Kohoutek–Ikemura is a Jupiter-family periodic comet in our Solar System with a current orbital period of 6.48 years. [1] [2]
The comet was initially spotted on a photographic plate by Richard M. West at the European Southern Observatory Sky Atlas Laboratory, Geneva in January 1975, when it had a brightness of magnitude 12. Inability to predict its movement from a single image meant the comet had to be presumed lost.
In late February it was accidentally rediscovered by Lubos Kohoutek at the Hamburg Observatory, Germany and independently on 1 March by Toshihiko Ikemura in Shinshiro, Japan. After further observations the comets parabolic orbit was computed, which gave a perihelion date of 23 March 1975 and proved that all three sightings were of the same object, which was accordingly designated 76P/West–Kohoutek–Ikemura.
Further calculations by Brian G. Marsden determined the comet's elliptical orbit and revealed that it had passed only 0.012 AU from Jupiter on 22 March 1972. This close approach had reduced its orbital frequency from some 30 years to the current 6.48 years and its perihelion distance from 4.78 AU to 1.60 AU.
The comet has been observed at its successive returns in 1987, 1993, 2000, 2006 and 2013.
See also
References
- ^ "76P/West-Kohoutek-Ikemura". Retrieved 25 February 2015.
- ^ "Elements and Ephemeris for 76P/West-Kohoutek-Ikemura". International Astronomical Union. Retrieved 25 February 2015.
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