The mass of (1) Ceres obtained from four close encounters
Author(s) -
Andjelka B. Kovačević,
M. Kuzmanoski
Publication year - 2005
Publication title -
serbian astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.196
H-Index - 16
eISSN - 1820-9289
pISSN - 1450-698X
DOI - 10.2298/saj0571037k
Subject(s) - physics , asteroid , perturbation (astronomy) , astrophysics , astronomy , theoretical physics
The technique of asteroid mass determination from perturbation during close approach requires as many as possible different close approaches in order to derive reliable mass of a perturber. Here are presented some results for the mass of (1) Ceres obtained using newly found close approaches
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