302 Clarissa
.png) A three-dimensional model of 302 Clarissa based on its lightcurve | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 14 November 1890 |
| Designations | |
| A890 VA; 1909 YA 1929 CK1; 1946 UN 1948 ED; 1953 NN | |
| Main belt | |
| Orbital characteristics | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 124.04 yr (45,305 d) |
| Aphelion | 2.67 AU (400.04 Gm) |
| Perihelion | 2.14 AU (319.61 Gm) |
| 2.41 AU (359.82 Gm) | |
| Eccentricity | 0.11175 |
| 3.73 yr (1,362.5 d) | |
| 213.798° | |
| 0° 15m 51.174s / day | |
| Inclination | 3.41369° |
| 7.85637° | |
| 54.5926° | |
| Physical characteristics | |
| 43 ± 4 km 43 ± 11 km (alternate) | |
Mean density | 1.5 g cm−3 |
| 14.47670 h (0.603196 d) | |
Pole ecliptic longitude | 28° 190° (alternate) |
Pole ecliptic latitude | −72° |
| 0.0524±0.010 | |
| F | |
| 10.89 | |
302 Clarissa is a typical main-belt asteroid. The asteroid was discovered by the French astronomer Auguste Charlois on 14 November 1890 in Nice. The origin of the name is unknown. In 1991, 302 Clarissa was being considered as a possible flyby target for the Cassini spacecraft, but was later removed from consideration.
This body is orbiting the Sun with a period of 3.73 years and an eccentricity (ovalness) of 0.11. The orbital plane is inclined by 3.4° to the plane of the ecliptic. There are no major planetary resonances near the orbit of 302 Clarissa. It has a retrograde spin with a rotation period of 14.4797 hours. Stellar occultation data provides a size estimate of 43±4 km, while IRAS data gives a diameter of 38.5±3.1 km. It is classified as a F-type asteroid and is probably composed of carbonaceous material.
302 Clarissa provides the eponym for a small collisional asteroid family of mostly C-type asteroids. This group consists of 179 bodies with orbits clustered around 302 Clarissa. The family has a small extent of semi-major axis values, suggesting this is a young group; its estimated age is 56±5 Myr. Seventy to ninety percent of the objects in this family have a retrograde spin, suggesting the parent body may have possessed a similar rotation. This family is one of five that are candidate sources for the near-Earth asteroids 101955 Bennu and 162173 Ryugu.
Spacecraft visits
At present, Clarissa has not been visited by any spacecraft. As of 1991, mission planning for the Cassini–Huygens spacecraft included a flyby of Clarissa while leaving the inner solar system in November 1998; however, due to delays, the launch of Cassini–Huygens was moved from November 1995 to October 1997, thus negating the option to pass near Clarissa. Cassini–Huygens passed by asteroid 2685 Masursky on 23 January 2000 instead.
References
- 1 2 3 "302 Clarissa". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- 1 2 3 4 Ďurech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanuš, Josef; Frappa, Eric; Talbot, John; Hayamizu, Tsutomu; Warner, Brian D.; Pilcher, Frederick; Galád, Adrián (1 August 2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes". Icarus. 214 (2): 652–670. arXiv:1104.4227. Bibcode:2011Icar..214..652D. doi:10.1016/j.icarus.2011.03.016. ISSN 0019-1035. S2CID 119271216.
- 1 2 3 Lowry, Vanessa C.; et al. (September 2020), "Clarissa Family Age from the Yarkovsky Effect Chronology", The Astronomical Journal, 160 (3): 127, arXiv:2009.06030, Bibcode:2020AJ....160..127L, doi:10.3847/1538-3881/aba4af, 127
- ↑ Schmadel, Lutz D. (11 November 2013), Dictionary of Minor Planet Names, Berlin Heidelberg: Springer, p. 61, ISBN 9783662066157
- ↑ Chevreton, M.; et al. (August 1993), "Observations of the asteroid 302 Clarissa by fast multichannel photometer", Planetary and Space Science, 41 (8): 563–567, Bibcode:1993P&SS...41..563C, doi:10.1016/0032-0633(93)90076-E
- ↑ Morate, David; et al. (February 2018), "Visible spectroscopy of the Sulamitis and Clarissa primitive families: a possible link to Erigone and Polana", Astronomy & Astrophysics, 610: 14, Bibcode:2018A&A...610A..25M, doi:10.1051/0004-6361/201731407, A25
- ↑ Outward to the Beginning: the CRAF and Cassini Missions of the Mariner Mark 2 Program; NASA Contractor Report CR-183133, 1 June 1988
External links
- 302 Clarissa at AstDyS-2, Asteroids—Dynamic Site
- 302 Clarissa at the JPL Small-Body Database
