SATELLITE LIBRATIONS ON AN ELLIPTIC ORBIT
Abstract
The first-order effect of orbital eccentricity on the planar tumbling or oscillatory motion of a dumbbell-shaped satellite is discussed. This has been done by assuming that the angular orientation angle psi can be represented by a power series in eccentricity e, in which the co efficient of the e to the o power term was set equal to the circular solution psi-c available from earlier investigations. The differential equation for the coefficient of the e to the 1 power term is shown to be of an inhomogeneous Mathieu type, the particular solutions of which can be readily obtained if certain weak restrictions are placed on the initial magnitude of the dumbbell's angular velocity. The analysis indicated that the orientation of the satellite in the elliptic orbit can differ substantially from the one determined for the circular orbit. (Author) 8 AD-407 928
Document Details
- Document Type
- Technical Report
- Publication Date
- May 01, 1963
- Accession Number
- AD0407928
Entities
People
- H. B. Schechter
Organizations
- RAND Corporation