Electronic Resource
Springer
Celestial mechanics and dynamical astronomy
4 (1971), S. 295-308
ISSN:
1572-9478
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract The equations of motion are derived for the case of a spinning satellite which has a central rigid body, and long flexible appendages which are nominally in the spin plane. The ‘major-axis theorem’ is found to be necessary, but not sufficient for this case, and appropriate sufficiency criteria are derived from a Liapunov function. The results are presented in a form amenable to satellite design.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF01231392
|
Location |
Call Number |
Expected |
Availability |