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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 изданияхстатьяРецензирование

Harvard

Pitjeva, EV & Pitjev, NP 2016, 'Masses of asteroids and total mass of the main asteroid belt', Proceedings of the International Astronomical Union, Том. 10, стр. 212-217. https://doi.org/10.1017/S1743921315008388

APA

Pitjeva, E. V., & Pitjev, N. P. (2016). Masses of asteroids and total mass of the main asteroid belt. Proceedings of the International Astronomical Union, 10, 212-217. https://doi.org/10.1017/S1743921315008388

Vancouver

Pitjeva EV, Pitjev NP. Masses of asteroids and total mass of the main asteroid belt. Proceedings of the International Astronomical Union. 2016;10:212-217. https://doi.org/10.1017/S1743921315008388

Author

Pitjeva, E. V. ; Pitjev, N. P. / Masses of asteroids and total mass of the main asteroid belt. в: Proceedings of the International Astronomical Union. 2016 ; Том 10. стр. 212-217.

BibTeX

@article{4d0c42110ead4a8bbdaca62f209643a4,
title = "Masses of asteroids and total mass of the main asteroid belt",
abstract = "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.",
keywords = "asteroids, data analysis, ephemerides, methods: analytical, minor planets, numerical",
author = "Pitjeva, {E. V.} and Pitjev, {N. P.}",
note = "Publisher Copyright: Copyright {\textcopyright} 2016 International Astronomical Union. Copyright: Copyright 2016 Elsevier B.V., All rights reserved.",
year = "2016",
doi = "10.1017/S1743921315008388",
language = "English",
volume = "10",
pages = "212--217",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",

}

RIS

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