1508 Kemi
| Discovery | |
|---|---|
| Discovered by | H. Alikoski |
| Discovery site | Turku |
| Discovery date | 21 October 1938 |
| Designations | |
| MPC designation | 1508 |
Named after | Kemi |
| 1938 UP | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 80.38 yr (29360 days) |
| Aphelion | 3.9274277 AU (587.53482 Gm) |
| Perihelion | 1.6164689 AU (241.82031 Gm) |
| 2.771948 AU (414.6775 Gm) | |
| Eccentricity | 0.4168474 |
| 4.62 yr (1685.7 d) | |
| 268.61999° | |
| 0° 12m 48.828s / day | |
| Inclination | 28.72352° |
| 14.29863° | |
| 92.89361° | |
| Earth MOID | 0.874895 AU (130.8824 Gm) |
| Jupiter MOID | 2.15143 AU (321.849 Gm) |
| Jupiter Tisserand parameter | 3.041 |
| Physical characteristics | |
| Dimensions | ~17 km[2] |
| 9.196 h (0.3832 d) | |
Sidereal rotation period | 9.196 h[1] |
| BCF/C[1] | |
| 12.03[1] | |
|
| |
1508 Kemi (1938 UP) is a large Mars-crossing asteroid discovered on October 21, 1938, by H. Alikoski at Turku, and independently discovered on October 30, 1938, by György Kulin at Budapest.[3] At roughly 17 km in diameter,[2] it is one of the largest Mars-crossing asteroids. It has been grouped with the Pallas family because of its high inclination, similar to other objects in that family,[4] but has different spectral characteristics than many Pallas asteroids.[5] It is classified as a BCF-type asteroid.
It is named after the town of Kemi, in Finland, and the Kemi River, the largest river in Finland, on which the town lies, in keeping with a pattern of giving high-inclination asteroids four-letter names.[3]
References
- 1 2 3 4 "JPL Small-Body Database Browser: 1508 Kemi (1938 UP)". Jet Propulsion Laboratory. Retrieved 27 April 2016.
- 1 2 "Absolute Magnitude (H)". NASA/JPL. Retrieved 2015-05-08.
- 1 2 Schmadel, Lutz (2003), Dictionary of Minor Planet Names, 1, Springer Science & Business Media, p. 120, ISBN 9783540002383.
- ↑ Novaković, Bojan; Cellino, Alberto; Knežević, Zoran (November 2011), "Families among high-inclination asteroids", Icarus, 216 (1): 69–81, arXiv:1108.3740
, Bibcode:2011Icar..216...69N, doi:10.1016/j.icarus.2011.08.016. - ↑ Jenniskens, Peter; Vaubaillon, Jérémie; Binzel, Richard P.; DeMeo, Francesca E.; Nesvorný, David; Bottke, William F.; Fitzsimmons, Alan; Hiroi, Takahiro; Marchis, Franck; Bishop, Janice L.; Vernazza, Pierre; Zolensky, Michael E.; Herrin, Jason S.; Welten, Kees C.; Meier, Matthias M. M.; Shaddad, Muawia H. (October 2010), "Almahata Sitta (=asteroid 2008 TC3) and the search for the ureilite parent body" (PDF), Meteoritics & Planetary Science, 45 (10-11): 1590–1617, Bibcode:2010M&PS...45.1590J, doi:10.1111/j.1945-5100.2010.01153.x.
Additional reading
- Holliday, B. (December 1995), "Lightcurve Observations of Minor Planets 1508 Kemi and 2014 Vasilevskis", Minor Planet Bulletin, 22: 43, Bibcode:1995MPBu...22...43H
- Jamieson, Q.; Klinglesmith, D. A., III (December 2004), "Period determination of asteroids 1508 Kemi and 5036 Tuttle", Minor Planet Bulletin, 31: 88–89, Bibcode:2004MPBu...31...88J.
External links
- 1508 Kemi at the JPL Small-Body Database
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