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<ref name="NK1778">{{cite web |
<ref name="NK1778">{{cite web |
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|date=2009-04-23 |
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|title=168P/Hergenrother (NK 1778) |
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|publisher=OAA Computing and Minor Planet Sections |
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|author=Syuichi Nakano |
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|author-link=Syuichi Nakano |
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|url=http://www.oaa.gr.jp/~oaacs/nk/nk1778.htm |
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|accessdate=2012-02-20 |
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}}</ref> |
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<ref name="NK2283">{{cite web |
<ref name="NK2283">{{cite web |
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|date=2012-07-17 |
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|title=168P/Hergenrother (NK 2283) |
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|publisher=OAA Computing and Minor Planet Sections |
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|author=Syuichi Nakano |
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|author-link=Syuichi Nakano |
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|url=http://www.oaa.gr.jp/~oaacs/nk/nk2283.htm |
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|accessdate=2012-10-13 |
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}}</ref> |
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<ref name="recovery">[http://www.cbat.eps.harvard.edu/iauc/08500/08560.html IAUC 8560: recovery of comet P/1998 W2]</ref> |
<ref name="recovery">[http://www.cbat.eps.harvard.edu/iauc/08500/08560.html IAUC 8560: recovery of comet P/1998 W2]</ref> |
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<ref name="Yoshida-2012">{{cite web |
<ref name="Yoshida-2012">{{cite web |
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|date=2012-02-21 |
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|title=168P/Hergenrother (2012) |
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|publisher=Seiichi Yoshida's Comet Catalog |
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|author=Seiichi Yoshida |
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|url=http://www.aerith.net/comet/catalog/0168P/2012.html |
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|accessdate=2012-02-25 |
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}}</ref> |
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<ref name=outburst-math>[[Apparent magnitude#Calculations|Math]]: <math>(\sqrt[5]{100})^{15.2-8}\approx 758</math></ref> |
<ref name=outburst-math>[[Apparent magnitude#Calculations|Math]]: <math>(\sqrt[5]{100})^{15.2-8}\approx 758</math></ref> |
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<ref name="Faulkes">{{cite web |
<ref name="Faulkes">{{cite web |
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|date=October 26, 2012 |
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|title=Splitting event in comet 168P/Hergenrother |
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|publisher=Remanzacco Observatory in Italy – Comets & Neo |
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|author=Giovanni Sostero |
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|author-link=Giovanni Sostero |
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|author2=Nick Howes |
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|author2-link= |
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|author3=Ernesto Guido |
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|url=http://remanzacco.blogspot.it/2012/10/splitting-event-in-comet.html |
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|accessdate=2012-10-28 |
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}}</ref> |
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<ref name="badastronomy">{{cite web |
<ref name="badastronomy">{{cite web |
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|date=2012-11-05 |
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|title=Breaking up is easy to do. If you’re a comet. |
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|publisher=Bad Astronomy |
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|author=Phil Plait |
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|author-link=Phil Plait |
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|url=http://blogs.discovermagazine.com/badastronomy/2012/11/05/breaking-up-is-easy-to-do-if-youre-a-comet/ |
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|accessdate=2012-11-05 |
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}}</ref> |
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<ref name=MPC>{{cite web |
<ref name=MPC>{{cite web |
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|title=168P/Hergenrother Orbit |
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|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=168P |
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|publisher=[[Minor Planet Center]] |
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|accessdate=2014-06-20 |
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}}</ref> |
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}} |
}} |
Discovery | |
---|---|
Discovered by | Carl W. Hergenrother |
Discovery date | November 22, 1998 |
Designations | |
P/1998 W2 P/2005 N2 | |
Orbital characteristics | |
Epoch | March 6, 2006 |
Aphelion | 5.839 AU |
Perihelion | 1.426 AU |
Semi-major axis | 3.632 AU |
Eccentricity | 0.6075 |
Orbital period | 6.923 a |
Inclination | 21.8934° |
Last perihelion | October 1, 2012[1] November 2, 2005 |
Next perihelion | August 5, 2019[2][3] |
168P/Hergenrother is a periodic comet in the solar system. The comet originally named P/1998 W2 returned in 2005 and got the temporary name P/2005 N2.[4]
The comet came to perihelion on 1 October 2012,[1] and was expected to reach about apparent magnitude 15.2, but due to an outburst the comet reached apparent magnitude 8.[5] As a result of the outburst of gas and dust, the comet was briefly more than 500 times brighter than it would have been without the outburst.[6] Images by the 2 m (79 in) Faulkes Telescope North on 26 October 2012 confirm a fragmentation event.[7] The secondary fragment was about magnitude 17. Further observations by the 8.1 m (320 in) Gemini telescope show that the comet fragmented into at least 4 parts.[8]
Numbered comets | ||
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Previous 167P/CINEOS |
168P/Hergenrother | Next 169P/NEAT |
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