C/1911 S3
Semi-major axis 2064.11 AU | | |
| Eccentricity | 0.997005 | |
|---|---|---|
| Orbital period | n/a | |
| Inclination | 96.4659° | |
| Last perihelion | October 10, 1911 | |
| Next perihelion | unknown | |
Comet Beljawsky is also known as 1911 IV and 1911g according to the naming conventions at the time. The
perihelion, as an evening object. It faded rapidly, becoming visible only in telescopes and was last seen on February 17, 1912.[1][3][4] The comet sported a tail 8 to 10 degrees in length.[2] In mid-October, the comet was visible in the evening sky together with another bright comet, C/1911 O1 Brooks.[5]
Comet Beljawsky is a
inner Solar System.[1]
References
- ^ a b c JPL Small-Body Database
- ^ a b Curtis, HD [1], Publications of the Astronomical Society of the Pacific, 1911
- ^ Leon, Luis G. (1911). Popular Astronomy. Vol. 19. Goodsell Observatory of Carleton College. p. 575.
- ^ Leonard, Frederick C. (1911). The Monthly Register of the Society for Practical Astronomy. Vol. 3. Society for Practical Astronomy, Chicago. p. 56.
- ^ Bortle, J The Bright Comet Chronicles, International Comet Quarterly, 1998
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