The stability of the 24-hour satellite

1Citations
Citations of this article
1Readers
Mendeley users who have this article in their library.
Get full text

Abstract

The perturbations of the 24-hour satellite, produced by the Moon, Sun and the aspherical shape of the Earth, are investigated. The most important influence of the lunar gravitational attraction is studied with the aid of numerical integration of the equations of motion. The shift of the satellite from its initial position is studied for an ideal 24-orbit. The principal shift will have a periodical character with an amplitude of about 10°. © 1961.

Cite

CITATION STYLE

APA

Sehnal, L. (1961). The stability of the 24-hour satellite. Astronautica Acta, 7(5–6), 445–455. https://doi.org/10.1007/978-3-7091-5470-0_8

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free