67P/Churyumov–Gerasimenko

67P/Churyumov–Gerasimenko
67P/Churyumov–Gerasimenko
Comet 67P Churyumov-Gerasimenko.jpg
Discovery
Discovered by Klim Ivanovich Churyumov and
Svetlana Ivanovna Gerasimenko
Designations
Alternate name(s) 1982 VIII; 1982f;
1989 VI; 1988i;
1969 R1; 1969 IV;
1969h; 1975 P1;
1976 VII; 1975i
Epoch September 3, 2002 (JD 2452520.5)
Aphelion 5.722 AU
Perihelion 1.2923 AU
Semi-major axis 3.5072973258 AU
Eccentricity 0.6315
Orbital period 6.568 a
Inclination 7.1205°
Physical characteristics
Dimensions 4 km in diameter[1]

Comet Churyumov–Gerasimenko, officially designated 67P/Churyumov–Gerasimenko, is a comet with a current orbital period of 6.6 years. It is the destination of the European Space Agency's Rosetta spacecraft mission, launched on March 2, 2004.[2]

Contents

Discovery

The comet was discovered by Klim Ivanovich Churyumov, who examined a photograph that had been exposed for periodic comet 32P/Comas Solá by Svetlana Gerasimenko on September 11, 1969 at the Alma-Ata Astrophysical Institute. Churyumov 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, Churyumov examined all the photographic plates more closely. About a month after the photograph was taken (October 22), he discovered that the object could not be Comas Solá, because it was about 1.8 degrees off the expected position. Further scrutiny produced a faint image of Comas Solá at its expected position on the plate, thus proving that the other object was a newly discovered comet.

Observations

3-D illustration of the nucleus of Churyumov–Gerasimenko from Hubble telescope observations.

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 created.

Orbital history

Comets are regularly nudged from one orbit to another when they encounter Jupiter or Saturn in close proximity. It has been calculated that before the year 1959 Churyumov–Gerasimenko had perihelion distance of about 2.7 AU. In 1959 a close encounter with Jupiter pushed its perihelion distance to about 1.3 AU, where it remains today.[3]

References

  1. ^ NASA JPL Small-Body Database Browser on 67P/Churyumov–Gerasimenko
  2. ^ Krolikowska, Malgorzata (2003). "67P/Churyumov–Gerasimenko – potential target for the Rosetta mission". Acta Astronomica 53: 195–209. arXiv:astro-ph/0309130. Bibcode 2003AcA....53..195K. 
  3. ^ 67P orbital history at Kazuo Kinoshita home page

External links

Periodic comets (by number)
Previous
66P/du Toit
67P/Churyumov–Gerasimenko Next
68P/Klemola

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