Some Dynamic Characteristics of Binary Near-Earth Asteroids

Tidal acceleration exerted by the terrestrial planets and Jupiter’s are determined, orbital resonances to evaluate the motion stability in binary asteroid systems are calculated. Radius of the Hill sphere surrounding the main component in approximation of the planetary three-body problem — the Sun-m...

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Main Authors: Ivanenko, N.V., Bazyey, О.A.
Format: Article
Language:Ukrainian
Published: Publishing House "Akademperiodyka" 2017-01-01
Series:Nauka ta Innovacii
Subjects:
Online Access:ftp://ftp.nas.gov.ua/akademperiodyka/Downloads/Archive%20SI%20Journal/SI_ukr/2017/N1/Ivanenko.pdf
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spelling doaj-adb6d08a25ca44d59599eaf1db9b1e332020-11-25T01:55:08ZukrPublishing House "Akademperiodyka"Nauka ta Innovacii1815-20662413-497X2017-01-01131343710.15407/scin13.01.034Some Dynamic Characteristics of Binary Near-Earth AsteroidsIvanenko, N.V.0Bazyey, О.A.1Odessa I.I. Mechnikov National UniversityOdessa I.I. Mechnikov National UniversityTidal acceleration exerted by the terrestrial planets and Jupiter’s are determined, orbital resonances to evaluate the motion stability in binary asteroid systems are calculated. Radius of the Hill sphere surrounding the main component in approximation of the planetary three-body problem — the Sun-main component-satellite is calculated. Escape velocities from the surface of the asteroid satellites are found and the conclusion on the possibility of substance loss is made.ftp://ftp.nas.gov.ua/akademperiodyka/Downloads/Archive%20SI%20Journal/SI_ukr/2017/N1/Ivanenko.pdfbinary NEAHill sphereresonance
collection DOAJ
language Ukrainian
format Article
sources DOAJ
author Ivanenko, N.V.
Bazyey, О.A.
spellingShingle Ivanenko, N.V.
Bazyey, О.A.
Some Dynamic Characteristics of Binary Near-Earth Asteroids
Nauka ta Innovacii
binary NEA
Hill sphere
resonance
author_facet Ivanenko, N.V.
Bazyey, О.A.
author_sort Ivanenko, N.V.
title Some Dynamic Characteristics of Binary Near-Earth Asteroids
title_short Some Dynamic Characteristics of Binary Near-Earth Asteroids
title_full Some Dynamic Characteristics of Binary Near-Earth Asteroids
title_fullStr Some Dynamic Characteristics of Binary Near-Earth Asteroids
title_full_unstemmed Some Dynamic Characteristics of Binary Near-Earth Asteroids
title_sort some dynamic characteristics of binary near-earth asteroids
publisher Publishing House "Akademperiodyka"
series Nauka ta Innovacii
issn 1815-2066
2413-497X
publishDate 2017-01-01
description Tidal acceleration exerted by the terrestrial planets and Jupiter’s are determined, orbital resonances to evaluate the motion stability in binary asteroid systems are calculated. Radius of the Hill sphere surrounding the main component in approximation of the planetary three-body problem — the Sun-main component-satellite is calculated. Escape velocities from the surface of the asteroid satellites are found and the conclusion on the possibility of substance loss is made.
topic binary NEA
Hill sphere
resonance
url ftp://ftp.nas.gov.ua/akademperiodyka/Downloads/Archive%20SI%20Journal/SI_ukr/2017/N1/Ivanenko.pdf
work_keys_str_mv AT ivanenkonv somedynamiccharacteristicsofbinarynearearthasteroids
AT bazyeyoa somedynamiccharacteristicsofbinarynearearthasteroids
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