Investigation of Light Pressure Influence on Dynamics of Near-Earth Objects with Reverse Motion


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

In this paper we consider the joint influence of secular resonances and light pressure on the long-term orbital evolution of objects with reverse motion in the near-Earth space with semimajor axes of orbits from 15000 to 45000 km. The orbital evolution of each object is considered for three values of the area-to-mass ratio of the object: 0.001, 1, and 10 m2/kg.

作者简介

A. Aleksandrova

National Research Tomsk State University

编辑信件的主要联系方式.
Email: aleksann@sibmail.com
俄罗斯联邦, Tomsk

T. Bordovitsyna

National Research Tomsk State University

Email: aleksann@sibmail.com
俄罗斯联邦, Tomsk

V. Aleksandrov

National Research Tomsk State University

Email: aleksann@sibmail.com
俄罗斯联邦, Tomsk

补充文件

附件文件
动作
1. JATS XML

版权所有 © Springer Science+Business Media, LLC, part of Springer Nature, 2019