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Asteroid Families in the Hilda Group

T. A. Vinogradova

Transactions of IAA RAS, issue 31, 73–78 (2014)

Keywords: asteroids, asteroid families, proper elements, resonance, Hildas

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Abstract

It is possible to calculate proper elements with a limited accuracy using distributions of osculating elements, such as the longitude of the ascending node - inclination and the longitude of the perihelion - eccentricity. The proposed empirical method allows to calculate proper elements even in the vicinity of resonances. The method was used to search for asteroid families in the intricate resonance region of Hildas. As a result, two families were found: (1911) Schubart and (153) Hilda.

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T. A. Vinogradova. Asteroid Families in the Hilda Group // Transactions of IAA RAS. — 2014. — Issue 31. — P. 73–78. @article{vinogradova2014, abstract = {It is possible to calculate proper elements with a limited accuracy using distributions of osculating elements, such as the longitude of the ascending node - inclination and the longitude of the perihelion - eccentricity. The proposed empirical method allows to calculate proper elements even in the vicinity of resonances. The method was used to search for asteroid families in the intricate resonance region of Hildas. As a result, two families were found: (1911) Schubart and (153) Hilda.}, author = {T.~A. Vinogradova}, issue = {31}, journal = {Transactions of IAA RAS}, keyword = {asteroids, asteroid families, proper elements, resonance, Hildas}, pages = {73--78}, title = {Asteroid Families in the Hilda Group}, url = {http://iaaras.ru/en/library/paper/1034/}, year = {2014} } TY - JOUR TI - Asteroid Families in the Hilda Group AU - Vinogradova, T. A. PY - 2014 T2 - Transactions of IAA RAS IS - 31 SP - 73 AB - It is possible to calculate proper elements with a limited accuracy using distributions of osculating elements, such as the longitude of the ascending node - inclination and the longitude of the perihelion - eccentricity. The proposed empirical method allows to calculate proper elements even in the vicinity of resonances. The method was used to search for asteroid families in the intricate resonance region of Hildas. As a result, two families were found: (1911) Schubart and (153) Hilda. UR - http://iaaras.ru/en/library/paper/1034/ ER -