69519

Автор(ы): 

Автор(ов): 

2

Параметры публикации

Тип публикации: 

Статья в журнале/сборнике

Название: 

Probability for Cosmic Masses of the Main Asteroid Belt to Approach the Earth

ISBN/ISSN: 

0094-5765

DOI: 

10.1016/j.actaastro.2021.09.036

Наименование источника: 

  • Acta Astronautica

Обозначение и номер тома: 

Volume 194

Город: 

  • Oxford, United Kingdom

Издательство: 

  • Elsevier Ltd., Pergamon Press Ltd.

Год издания: 

2022

Страницы: 

411-416
Аннотация
The problem of space flights safety arose with the beginning of the first launches of artificial Earth satellites. With expansion of the boundaries of space flights, the area of outer space that must be controlled to ensure flight safety is significantly increasing. In this study, we consider the possibility of capturing space objects into near-planetary space and further movement of these objects. Such statistical analysis is very important when planning the long-term flights. The objects of our research are both: the particles that came from deep space and the evolving asteroids of the Main asteroid belt. A special attention is paid to the evolution of the Griqua family of asteroids, which belong to the main asteroid belt, and move in orbital resonance with Jupiter.

Библиографическая ссылка: 

Сальникова Т.В., Самохин А.С. Probability for Cosmic Masses of the Main Asteroid Belt to Approach the Earth // Acta Astronautica. 2022. Volume 194. С. 411-416.