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1 References  





2 External links  














168P/Hergenrother: Difference between revisions






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* [https://arxiv.org/abs/1409.7641 Temporal Correlation Between Outbursts and Fragmentation Events of Comet 168P/Hergenrother] ([[arXiv]]:1409.7641 : 26 Sep 2014)

* [https://arxiv.org/abs/1409.7641 Temporal Correlation Between Outbursts and Fragmentation Events of Comet 168P/Hergenrother] ([[arXiv]]:1409.7641 : 26 Sep 2014)



{{PeriodicComets Navigator|167P/CINEOS|169P/NEAT}}

{{Comets}}

{{Comets}}

{{2019 in space}}

{{2019 in space}}

{{PeriodicComets Navigator|167P/CINEOS|169P/NEAT}}



{{DEFAULTSORT:Hergenrother, 168P}}

{{DEFAULTSORT:Hergenrother, 168P}}

[[Category:Comets]]

[[Category:Periodic comets]]

[[Category:Periodic comets]]

[[Category:Comets in 2019]]

[[Category:Comets in 2019]]


Revision as of 16:33, 17 January 2019

168P/Hergenrother
168P/Hergenrother during its 2012 outburst. By Mount Lemmon Observatory.
Discovery
Discovered byCarl W. Hergenrother
Discovery dateNovember 22, 1998
Designations

Alternative designations

P/1998 W2
P/2005 N2
Orbital characteristics
EpochMarch 6, 2006
Aphelion5.839 AU
Perihelion1.426 AU
Semi-major axis3.632 AU
Eccentricity0.6075
Orbital period6.923 a
Inclination21.8934°
Last perihelionOctober 1, 2012[1]
November 2, 2005
Next perihelionAugust 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] On 19 October 2012, images by the Virtual Telescope Project showed a dust cloud trailing the nucleus.[7] Images by the 2 m (79 in) Faulkes Telescope North on 26 October 2012 confirm a fragmentation event.[8] 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.[9]

References

  1. ^ a b Syuichi Nakano (2009-04-23). "168P/Hergenrother (NK 1778)". OAA Computing and Minor Planet Sections. Retrieved 2012-02-20.
  • ^ "168P/Hergenrother Orbit". Minor Planet Center. Retrieved 2014-06-20.
  • ^ Syuichi Nakano (2012-07-17). "168P/Hergenrother (NK 2283)". OAA Computing and Minor Planet Sections. Retrieved 2012-10-13.
  • ^ IAUC 8560: recovery of comet P/1998 W2
  • ^ Seiichi Yoshida (2012-02-21). "168P/Hergenrother (2012)". Seiichi Yoshida's Comet Catalog. Retrieved 2012-02-25.
  • ^ Math:
  • ^ Gianluca Masi (October 19, 2012). "Comet 168P/Hergenrother: hi-res images (19 Oct. 2012)". Virtual Telescope Project. Retrieved 2016-10-18.
  • ^ Giovanni Sostero; Nick Howes; Ernesto Guido (October 26, 2012). "Splitting event in comet 168P/Hergenrother". Remanzacco Observatory in Italy – Comets & Neo. Retrieved 2012-10-28.
  • ^ Phil Plait (2012-11-05). "Breaking up is easy to do. If you're a comet". Bad Astronomy. Retrieved 2012-11-05.
  • External links

    Numbered comets
    Previous
    167P/CINEOS
    168P/Hergenrother Next
    169P/NEAT


  • t
  • e

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=168P/Hergenrother&oldid=878891834"

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    This page was last edited on 17 January 2019, at 16:33 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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