Adeona family

The Adeona or Adeonian family (FIN: 505) is a large asteroid family that formed from the parent body 145 Adeona.^[1] Its spectral type is that of a carbonaceous C-type, with currently 2,236 asteroids identified as family members.^[2]^: 23 Based upon simulation studies, the Adeonian family is believed to be no more than 600 million years old, compared to a typical asteroid family age of 1–2 billion years.^[3]

References

^ Zappala, Vincenzo; et al. (December 1990), "Asteroid families. I – Identification by hierarchical clustering and reliability assessment", Astronomical Journal, 100: 2030–2046, Bibcode:1990AJ....100.2030Z, doi:10.1086/115658. In particular, see family #44.
^ 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.
^ Carruba, V.; et al. (2003), "Orbital evolution of the Gefion and Adeona asteroid families: close encounters with massive asteroids and the Yarkovsky effect" (PDF), Icarus, 162 (2): 308–327, Bibcode:2003Icar..162..308C, doi:10.1016/S0019-1035(02)00062-3.

This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it.

[Zappala1990-1] Zappala, Vincenzo; et al. (December 1990), "Asteroid families. I – Identification by hierarchical clustering and reliability assessment", Astronomical Journal, 100: 2030–2046, Bibcode:1990AJ....100.2030Z, doi:10.1086/115658. In particular, see family #44.

[Nesvorny-2014-2] 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.

[Carruba2003-3] Carruba, V.; et al. (2003), "Orbital evolution of the Gefion and Adeona asteroid families: close encounters with massive asteroids and the Yarkovsky effect" (PDF), Icarus, 162 (2): 308–327, Bibcode:2003Icar..162..308C, doi:10.1016/S0019-1035(02)00062-3.

[1]

[2]

[3]