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Masses of asteroids and total mass of the main asteroid belt. / Pitjeva, E. V.; Pitjev, N. P.
в: Proceedings of the International Astronomical Union, Том 10, 2016, стр. 212-217.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Masses of asteroids and total mass of the main asteroid belt
AU - Pitjeva, E. V.
AU - Pitjev, N. P.
N1 - Publisher Copyright: Copyright © 2016 International Astronomical Union. Copyright: Copyright 2016 Elsevier B.V., All rights reserved.
PY - 2016
Y1 - 2016
N2 - An estimation of the mass of the main asteroid belt was made on the basis of the new version of EPM2014 ephemerides of the Institute of Applied Astronomy of Russian Academy of Sciences using about 800000 positional observations of planets and spacecraft. We obtained the individual estimations of masses of large asteroids from radar data, as well as estimates of the masses of asteroids by using known diameters and estimated average densities for the three taxonomic types (C, S, M), and used the known mass values of binary asteroids and asteroids to which spacecraft approached. A two-dimensional homogeneous annulus with dimensions corresponding observed width of the main asteroid belt (2.06 au and 3.27 au) was used instead of a previous massive one-dimensional ring for modeling total perturbations from small asteroids. The obtained value of the total mass of the main asteroid belt is (12.25 ± 0.19)10-10 M.
AB - An estimation of the mass of the main asteroid belt was made on the basis of the new version of EPM2014 ephemerides of the Institute of Applied Astronomy of Russian Academy of Sciences using about 800000 positional observations of planets and spacecraft. We obtained the individual estimations of masses of large asteroids from radar data, as well as estimates of the masses of asteroids by using known diameters and estimated average densities for the three taxonomic types (C, S, M), and used the known mass values of binary asteroids and asteroids to which spacecraft approached. A two-dimensional homogeneous annulus with dimensions corresponding observed width of the main asteroid belt (2.06 au and 3.27 au) was used instead of a previous massive one-dimensional ring for modeling total perturbations from small asteroids. The obtained value of the total mass of the main asteroid belt is (12.25 ± 0.19)10-10 M.
KW - asteroids
KW - data analysis
KW - ephemerides
KW - methods: analytical
KW - minor planets
KW - numerical
UR - http://www.scopus.com/inward/record.url?scp=84959542005&partnerID=8YFLogxK
U2 - 10.1017/S1743921315008388
DO - 10.1017/S1743921315008388
M3 - Article
AN - SCOPUS:84959542005
VL - 10
SP - 212
EP - 217
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
SN - 1743-9213
ER -
ID: 75815746