http://podideployment.blogspot.co.uk/2012/10/a-comet.html Kitt Peak 3.5m] (30 Oct 2012)
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* [http://podideployment.blogspot.co.uk/2012/10/a-comet.html Comet 168P and fragment] as seen by Kitt Peak WIYN {{convert|3.5|m|in|adj=on}} on 30 Oct 2012
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Line 67: | Line 67: | ||
* [http://www.youtube.com/watch?v=aFcwzQe_hHc Comet 168P Hergenrother in outburst] (Google+ chat archive Oct 12, 2012) |
* [http://www.youtube.com/watch?v=aFcwzQe_hHc Comet 168P Hergenrother in outburst] (Google+ chat archive Oct 12, 2012) |
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* [http://transientsky.wordpress.com/2012/10/20/comet-hergenrother-in-outburst/ Comet Hergenrother in Outburst] (Carl Hergenrother : 20 Oct 2012) |
* [http://transientsky.wordpress.com/2012/10/20/comet-hergenrother-in-outburst/ Comet Hergenrother in Outburst] (Carl Hergenrother : 20 Oct 2012) |
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*[http://podideployment.blogspot.co.uk/2012/10/a-comet.html Kitt Peak 3. |
* [http://podideployment.blogspot.co.uk/2012/10/a-comet.html Comet 168P and fragment] as seen by [[Kitt Peak National Observatory|Kitt Peak]] [[WIYN Observatory|WIYN]] {{convert|3.5|m|in|adj=on}} on 30 Oct 2012 |
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{{PeriodicComets Navigator|167P/CINEOS|169P/NEAT}} |
{{PeriodicComets Navigator|167P/CINEOS|169P/NEAT}} |
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] |
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.[3]
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.[4] 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.[5] Images by the 2 m (79 in) Faulkes Telescope North on 26 October 2012 confirm a fragmentation event.[6] The secondary fragment was about magnitude 17.
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