Discovery | |
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Discovered by: | Coggia, Jerome E. |
Discovery date: | January 22, 1867 |
Alternate designations: | P/1980 L2, P/1942 V1, P/1867 B1, 38P |
Orbital characteristics A | |
Epoch: | 1981-Apr-26 (JD 2444720.5)[1] |
Aphelion: | 20.920 AU (near Uranus) |
Perihelion: | 1.5744 AU (near Mars) |
Semi-major axis: | 11.247 AU |
Eccentricity: | 0.86002 |
Orbital period: | 37.72 yr |
Inclination: | 17.981° |
Last perihelion: | December 5, 1980[2][1] |
Next perihelion: | November 10, 2018[2] |
38P/Stephan–Oterma (also known as Comet Stephan–Oterma) is a periodic comet discovered in January 1867, by Jerome Coggia at Marseilles Observatory, France.[1]
It has perihelion near the orbit of Mars and has aphelion near the orbit of Uranus. Acting like a centaur-hybrid, between the years 1982 and 2067, this object will make close approaches to the giant planets Jupiter, Saturn, and Uranus.[3] If this object did not show a coma and had a perihelion beyond Jupiter (5AU), we would be calling it a centaur.
Periodic comets (by number) | ||
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38P/Stephan–Oterma | Next 39P/Oterma |