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Dynamical estimation of masses of the Main asteroid belt and some individual asteroids within the EPM ephemeris using infrared data
Author(s) -
M. Kan,
Dmitry Pavlov
Publication year - 2022
Publication title -
astronomy at the epoch of multimessenger studies. proceedings of the vak-2021 conference, aug 23–28, 2021
Language(s) - English
Resource type - Conference proceedings
DOI - 10.51194/vak2021.2022.1.1.023
Subject(s) - asteroid , ephemeris , asteroid belt , tikhonov regularization , a priori and a posteriori , infrared , astrobiology , astronomy , physics , mathematics , inverse problem , satellite , mathematical analysis , philosophy , epistemology
The purpose of this work is to estimate the mass of the main asteroid belt and those of the individual asteroids. To solve thistask we propose to use Tikhonov regularization which allows to use a priori information on the asteroids’ masses and theiruncertainties. Each a priori mass and its uncertainty were calculated based on the infrared diameter and density estimatesof a particular asteroid. As a result, we managed to obtain mass estimates consistent with those obtained earlier, and toextend the list of asteroids whose masses are individually determined in the EPM dynamical model.

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