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...
| Main Authors: | , |
|---|---|
| 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 |