The Maria family (adj. Marian; FIN: 506; also known as the Roma family) is a collisional asteroid family located in the inner parts of the intermediate asteroid belt, near the 1:3 Kirkwood gap. The family consist of several thousand stony S-type asteroids. It is named after its parent body and lowest numbered member, the asteroid 170 Maria. It is also known as the Roma family, named after its alternative parent body, 472 Roma.
The family was initially identified by Japanese astronomer Kiyotsugu Hirayama in 1918. Asteroids in this family typically have a semi-major axis between 2.52−2.62 AU, and an inclination of 12 to 17°.
Members
The family consists of 2940 known members based on the HCM method. Its largest members are the asteroids 170 Maria and 472 Roma. A complete synthetic HCM-listing for all members can be obtained by using the Ferret Interactive Search.
Name | a | e | i | SBDB |
---|---|---|---|---|
170 Maria | 2.553 | 0.065 | 14.40° | JPL |
472 Roma | 2.545 | 0.094 | 15.80° | JPL |
Name | a | e | i | SBDB |
---|---|---|---|---|
292 Ludovica | 2.529 | 0.034 | 14.92° | JPL |
652 Jubilatrix | 2.554 | 0.127 | 15.77° | JPL |
714 Ulula | 2.535 | 0.058 | 14.27° | JPL |
787 Moskva | 2.539 | 0.129 | 14.84° | JPL |
875 Nymphe | 2.552 | 0.151 | 14.59° | JPL |
879 Ricarda | 2.531 | 0.155 | 13.68° | JPL |
897 Lysistrata | 2.541 | 0.094 | 14.32° | JPL |
1158 Luda | 2.564 | 0.112 | 14.85° | JPL |
1215 Boyer | 2.578 | 0.133 | 15.91° | JPL |
2089 Cetacea | 2.533 | 0.156 | 15.39° | JPL |
3066 McFadden | 2.527 | 0.133 | 15.57° | JPL |
Interlopers
Although asteroid 695 Bella has orbital properties that make it a candidate for this family, the spectral properties of the object indicate it is most likely an interloper. Instead, it may have been spalled off from 6 Hebe, or its parent body.
References
- ^ Fieber-Beyer, Sherry K.; Gaffey, Michael J.; Kelley, Michael S.; Reddy, Vishnu; Reynolds, Chalbeth M.; Hicks, Tony (June 2011). "The Maria asteroid family: Genetic relationships and a plausible source of mesosiderites near the 3:1 Kirkwood Gap". Icarus. 213 (2): 524–537. Bibcode:2011Icar..213..524F. doi:10.1016/j.icarus.2011.03.009. Retrieved 25 April 2018.
- ^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
- Masiero, Joseph R.; Mainzer, A. K.; Bauer, J. M.; Grav, T.; Nugent, C. R.; Stevenson, R. (June 2013). "Asteroid Family Identification Using the Hierarchical Clustering Method and WISE/NEOWISE Physical Properties". The Astrophysical Journal. 770 (1): 22. arXiv:1305.1607. Bibcode:2013ApJ...770....7M. doi:10.1088/0004-637X/770/1/7.
- EasySky – Screenshots
- "Small Bodies Data Ferret". Synthetic Family (170) Maria – Nesvorny HCM Asteroid Families V3.0. Archived from the original on 2 August 2017. Retrieved 22 July 2017. (Query)
Small Solar System bodies | |||||||
---|---|---|---|---|---|---|---|
Minor planets |
| ||||||
Comets | |||||||
Other |