335P/Gibbs
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This is an old revision of this page, as edited by Citation bot (talk | contribs) at 06:27, 21 September 2023 (Alter: title. | Use this bot. Report bugs. | Suggested by Eastmain | #UCB_webform 92/624). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Revision as of 06:27, 21 September 2023 by Citation bot (talk | contribs) (Alter: title. | Use this bot. Report bugs. | Suggested by Eastmain | #UCB_webform 92/624)
Discovery | |
---|---|
Discovered by | Alex R. Gibbs |
Discovery date | 31 December 2008 |
Designations | |
2008 Y2, 2016 A9 | |
Orbital characteristics | |
Epoch | 2022-08-09.0 |
Aphelion | 5.532 AU |
Perihelion | 1.624 AU |
Semi-major axis | 3.578 AU |
Eccentricity | 0.546 |
Orbital period | 6.77 a |
Inclination | 7.293° |
Last perihelion | 2015-11-05 |
Next perihelion | 2022-08-12[1][2] |
335P/Gibbs is a periodic comet in the Solar System. It last came to perihelion in August 2022. Together with 266P/Christensen, it was proposed as the source of the 1977 "Wow! Signal".[3]
References
- ^ "335P/Gibbs Orbit". Minor Planet Center. Retrieved 2017-06-08.
- ^ Syuichi Nakano (2016-02-09). "335P/Gibbs (NK 3062)". OAA Computing and Minor Planet Sections. Retrieved 2017-06-08.
- ^ Paris, Antonio (Winter 2015). "Hydrogen Clouds from Comets 266/P Christensen and P/2008 Y2 (Gibbs) are Candidates for the Source of the 1977 "WOW" Signal" (PDF). Washington Academy of Sciences. Retrieved 7 June 2017.
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- 335P on Seiichi Yoshida's comet list
- Elements and Ephemeris for 335P/Gibbs[permanent dead link] – Minor Planet Center
Numbered comets | ||
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Previous 334P/NEAT |
335P/Gibbs | Next 336P/McNaught |
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