Asteroid Families in the Hilda Group
Transactions of IAA RAS, issue 31, 73–78 (2014)
Keywords: asteroids, asteroid families, proper elements, resonance, Hildas
About the paperAbstract
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.
Citation
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 -