Library · IAA RAS

Papers

Consistent Masses of Asteroids Obtained by the Dynamical Method

Transactions of IAA RAS, issue 31, 66–72 (2014)

Keywords: asteroid, mass of asteroid, orbit, test particle, dynamical method of mass determination

Abstract

An important stage of the dynamical method of asteroid mass determination from observations of other perturbed asteroids is selection of such asteroids. Our previous papers considered observations of a number of perturbed asteroids (test particles) to estimate the mass of one separate perturbing asteroid. This paper describes a possibility to determine masses of 48 perturbing asteroids simultaneously, from their mutual perturbations. The ephemerides DE405 and ЕРМ2011 are used to take into account perturbations caused by major planets and the Moon. Advantages and disadvantages of the previous and the new approaches are discussed.

Citation

Text

BibTeX

RIS

O. M. Kochetova , Yu. A. Chernetenko. Consistent Masses of Asteroids Obtained by the Dynamical Method // Transactions of IAA RAS. — 2014. — Issue 31. — P. 66–72.

@article{kochetova2014,
  abstract = {An important stage of the dynamical method of asteroid mass determination from observations of other perturbed asteroids is selection of such asteroids. Our previous papers considered observations of a number of perturbed asteroids (test particles) to estimate the mass of one separate perturbing asteroid. This paper describes a possibility to determine masses of 48 perturbing asteroids simultaneously, from their mutual perturbations. The ephemerides DE405 and ЕРМ2011 are used to take into account perturbations caused by major planets and the Moon. Advantages and disadvantages of the previous and the new approaches are discussed.},
  author = {O.~M. Kochetova and Yu.~A. Chernetenko},
  issue = {31},
  journal = {Transactions of IAA RAS},
  keyword = {asteroid, mass of asteroid, orbit, test particle, dynamical method of mass determination},
  pages = {66--72},
  title = {Consistent Masses of Asteroids Obtained by the Dynamical Method},
  url = {http://iaaras.ru/en/library/paper/1033/},
  year = {2014}
}

TY  - JOUR
TI  - Consistent Masses of Asteroids Obtained by the Dynamical Method
AU  - Kochetova, O. M.
AU  - Chernetenko, Yu. A.
PY  - 2014
T2  - Transactions of IAA RAS
IS  - 31
SP  - 66
AB  - An important stage of the dynamical method of asteroid mass
determination from observations of other perturbed asteroids is
selection of such asteroids. Our previous papers considered
observations of a number of perturbed asteroids (test particles) to
estimate the mass of one separate perturbing asteroid. This paper
describes a possibility to determine masses of 48 perturbing
asteroids simultaneously, from their mutual perturbations. The
ephemerides DE405 and ЕРМ2011 are used to take into account
perturbations caused by major planets and the Moon. Advantages and
disadvantages of the previous and the new approaches are discussed.
UR  - http://iaaras.ru/en/library/paper/1033/
ER  -