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Pallas family

From Wikipedia, the free encyclopedia
Asteroid family

ThePallas family (adj. Palladian;FIN:801) is a smallasteroid family ofB-type asteroids at very highinclinations in the intermediateasteroid belt.[1][2] The family was identified byKiyotsugu Hirayama in 1928.

The namesake of the family is2 Pallas, an extremely large asteroid with amean diameter of about 512 km.[3] The remaining Palladian asteroids are far smaller; the largest is5222 Ioffe with an estimated diameter of 22 km. This, along with the preponderance of the otherwise rare B spectral type among its members, indicates that this is likely acratering family composed of ejecta from impacts on Pallas.

Another suspected Palladian is3200 Phaethon, the parent body of theGeminid meteor shower.[4]

Location and structure of the Pallas family.

From the diagram, theirproper orbital elements lie in the approximate ranges

apepip
min2.71AU0.2532°
max2.79 AU0.3134°

At the presentepoch, the range ofosculatingorbital elements of the members (by comparison to the MPCORB database[1]) is about

aei
min2.71AU0.1330°
max2.79 AU0.3738°

References

[edit]
  1. ^Cellino, A.; Bus, S. J.; Doressoundiram, A.; Lazzaro, D. (March 2002)."Spectroscopic Properties of Asteroid Families".Asteroids III:633–643.Bibcode:2002aste.book..633C. Retrieved14 December 2018. (see Table on p.636)
  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.
  3. ^Carry, Benoît; Dumas, Christophe; Kaasalainen, Mikko; Berthier, Jérôme; Merline, William J.; Erard, Stéphane; et al. (February 2010). "Physical properties of (2) Pallas".Icarus.205 (2):460–472.arXiv:0912.3626.Bibcode:2010Icar..205..460C.doi:10.1016/j.icarus.2009.08.007.
  4. ^Jaggard, Victoria (12 October 2010)."Exploding Clays Drive Geminids Sky Show?". National Geographic. Retrieved14 December 2018.

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