Themis family: Difference between revisions
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== Description == |
== Description == |
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The Themis family is one of the largest and longest-recognized dynamical families of asteroids, and is made up of [[C-type asteroid]]s with a composition believed to be similar to that of [[carbonaceous chondrite]]s.<ref>[http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1646.pdf 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</ref> To date, the Themis family comprises approximately 535 known asteroids. |
The Themis family is one of the largest and biggest even longest-recognized dynamical families of asteroids, and is made up of [[C-type asteroid]]s with a composition believed to be similar to that of [[carbonaceous chondrite]]s.<ref>[http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1646.pdf 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</ref> To date, the Themis family comprises approximately 535 known asteroids. |
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Asteroids in the Themis family share the following orbital elements: |
Asteroids in the Themis family share the following orbital elements: |
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Revision as of 18:53, 9 February 2023
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 biggest even 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]
See also
References
- ^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). Identification and Dynamical Properties of Asteroid Families. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. S2CID 119280014.
{{cite book}}:|journal=ignored (help) - ^ "24 Themis". Minor Planet Center. 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. Bibcode:2012Icar..218..196D. doi:10.1016/j.icarus.2011.11.024. 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" (PDF). Astronomy and Astrophysics. 537: 7. Bibcode:2012A&A...537A..73L. doi:10.1051/0004-6361/201118142. Retrieved 7 November 2018.
- Castillo-Rogez, C. & Schmidt, B. E. (2010). "Geophysical Evolution of the Themis Family Parent Body" (PDF).
{{cite journal}}: Cite journal requires|journal=(help)
External links
- Nesvorny HCM Asteroid Families V3.0, Small Bodies Data Ferret