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C/1992 J1 (Spacewatch)
Non-periodic comet
Non-periodic comet
| Field | Value |
|---|---|
| name | C/1992 J1 (Spacewatch) |
| image | CometSpacewatch.png |
| caption | Simulated orbit of C/1992 J1 (Spacewatch) as of 12 January 2012 |
| discovery_ref | |
| discoverer | David Rabinowitz |
| Spacewatch Project | |
| discovery_site | Kitt Peak Observatory |
| discovery_date | 1 May 1992 |
| designations | 1992h |
| 1993 XV | |
| orbit_ref | |
| epoch | 3 August 1993 (JD 2449202.5) |
| observation_arc | 1,007 days (2.76 years) |
| obs | 240 |
| perihelion | 3.007 AU |
| aphelion | ~75,000 AU (inbound) |
| ~3,700 AU (outbound) | |
| eccentricity | 0.99996 |
| period | ~78,000 years (outbound) |
| inclination | 124.32° |
| asc_node | 203.32° |
| arg_peri | 83.40° |
| tjup | –1.212 |
| Earth_moid | 2.541 AU |
| Jupiter_moid | 0.127 AU |
| M1 | 8.3 |
| M2 | 14.2 |
| last_p | 6 September 1993 |
Spacewatch Project 1993 XV ~3,700 AU (outbound)
C/1992 J1 (Spacewatch) is a comet that was discovered 1 May 1992 by David Rabinowitz of the Spacewatch Project. This was the first comet to be discovered using an automated system.
Orbit
Using a generic heliocentric (two-body) solution calculated near the time of perihelion (closest approach to the Sun), it is estimated to have an aphelion (Q) (furthest distance from the Sun) of 154202 AU. But the orbit of a long-period comet is properly obtained when the osculating orbit is computed at an epoch after leaving the planetary region and is calculated with respect to the center of mass of the Solar System. After leaving the planetary region of the Solar System, the post-perihelion orbital period is estimated to be about 78,000 years with aphelion around 3,650 AU. In 2007 it reached more than 30 AU from the Sun.
References
| access-date= 31 January 2010 }}
| access-date= 15 April 2009
| access-date= 15 April 2009 | archive-date= 29 October 2008 | archive-url= https://web.archive.org/web/20081029054125/http://spacewatch.lpl.arizona.edu/outerss_text.html | url-status= dead }}
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