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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Publishing House "Akademperiodyka"
2017-01-01
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Online Access: | ftp://ftp.nas.gov.ua/akademperiodyka/Downloads/Archive%20SI%20Journal/SI_ukr/2017/N1/Ivanenko.pdf |
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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 |
_version_ |
1724984802274181120 |