 | |
| Discovery | |
|---|---|
| Discovered by: | Klim Ivanovich Churyumov and Svetlana Ivanovna Gerasimenko |
| Discovery date: | September 20, 1969 |
| Alternate designations: | 1982 VIII; 1982f; 1989 VI; 1988i; 1969 R1; 1969 IV; 1969h; 1975 P1; 1976 VII; 1975i |
| Orbital characteristics A | |
| Epoch: | September 3, 2002 (JD 2452520.5) |
| Aphelion distance: | 5.722 AU |
| Perihelion distance: | 1.2923 AU |
| Semi-major axis: | 3.5072973258 AU |
| Eccentricity: | 0.6315 |
| Orbital period: | 6.568 a |
| Inclination: | 7.1205° |
| Last perihelion: | February 28, 2009 |
| Next perihelion: | August 13, 2015[1] |
67P/Churyumov-Gerasimenko is the designation of a comet with a current orbital period of 6.6 years. It is the destination[2] of the European Space Agency's Rosetta spacecraft mission, launched on March 2, 2004.
Comet physical parameters
Diameter: 4 km
Hubble pictures
As preparation for the Rosetta mission Hubble Space Telescope pictures taken on March 12, 2003, were closely analyzed. An overall 3-D model was constructed and computer generated images from various view angles are shown in this composite picture.
Discovery
This comet was discovered by Klim Ivanovich Churyumov who examined a photograph exposed for periodic comet 32P/Comas Solá by Svetlana Gerasimenko on September 11, 1969 at the Alma-Ata Astrophysical Institute. He found a cometary object near the edge of the plate, but assumed that this was Comas Solá. After returning to his home institute in Kiev, all photographic plates were investigated closely. About a month after the photograph was taken (October 22), it was discovered that the object could not be the assumed comet, because it was about 1.8 degrees off the expected position. Further scrutiny produced a faint picture of Comas Solá at its expected position on the plate, thus proving that the other object was a newly discovered comet.
Orbital history
Churyumov-Gerasimenko has a rather interesting orbital history. Comets are regularly nudged from one orbit to another when they encounter Jupiter or Saturn in close proximity. For this comet it was calculated, that before the year 1840 it was completely unobservable due to its perihelion distance of about 4.0 AU. At this time Jupiter shifted that distance to about 3.0 AU. Later on, in the year 1959, another encounter with Jupiter pushed it to about 1.28 AU, where it is now.
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