Astronomy:Themis family
The Themis family (adj. Themistian; FIN: 602) is a family of carbonaceous asteroids located in the outer portion of the asteroid belt, at a mean distance of 3.13 AU from the Sun. It is one of the largest families with over 4700 known members,[1] and consists of a well-defined core of larger bodies surrounded by a region of smaller ones. The collisional Themis family is named after its parent body, the asteroid 24 Themis, discovered on 5 April 1853 by Italian astronomer Annibale de Gasparis.[2]
Description
The Themis family is one of the largest and longest-recognized dynamical families of asteroids, and is made up of C-type asteroids with a composition believed to be similar to that of carbonaceous chondrites.[3] To date, the Themis family comprises approximately 535 known asteroids.
Asteroids in the Themis family share the following orbital elements:
- semimajor axes between 3.08 AU and 3.24 AU
- orbital eccentricities between 0.09 and 0.22
- orbital inclinations of less than 3°
List
Some of the largest members of this family include:[4][5]
- 24 Themis
- 62 Erato
- 90 Antiope
- 104 Klymene
- 171 Ophelia
- 222 Lucia
- 223 Rosa
- 316 Goberta
- 379 Huenna
- 383 Janina
- 468 Lina
- 492 Gismonda
- 515 Athalia
- 526 Jena
- 767 Bondia
- 846 Lipperta
See also
References
- ↑ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N.
- ↑ "24 Themis". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=24. Retrieved 7 November 2018.
- ↑ DIVERSITY OF TYPES OF HYDRATED MINERALS ON C≠CLASS ASTEROIDS A. S. Rivkin, Massachusetts Institute of Technology, E. S. Howell, Arecibo Observatory, S. J. Bus, Institute for Astronomy
- ↑ de León, J.; Pinilla-Alonso, N.; Campins, H.; Licandro, J.; Marzo, G. A. (March 2012). "Near-infrared spectroscopic survey of B-type asteroids: Compositional analysis". Icarus 218 (1): 196–206. doi:10.1016/j.icarus.2011.11.024. Bibcode: 2012Icar..218..196D. https://www.researchgate.net/publication/232728965. Retrieved 7 November 2018.
- ↑ Licandro, J.; Hargrove, K.; Kelley, M.; Campins, H.; Ziffer, J.; Alí-Lagoa, V. et al. (January 2012). "5-14 mum Spitzer spectra of Themis family asteroids". Astronomy and Astrophysics 537: 7. doi:10.1051/0004-6361/201118142. Bibcode: 2012A&A...537A..73L. https://www.aanda.org/articles/aa/pdf/2012/01/aa18142-11.pdf. Retrieved 7 November 2018.
- Castillo-Rogez, C.; Schmidt, B. E. (2010). Geophysical Evolution of the Themis Family Parent Body. http://www.lpi.usra.edu/meetings/lpsc2010/pdf/2632.pdf.
External links
- Nesvorny HCM Asteroid Families V3.0, Small Bodies Data Ferret
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