Statistics – Computation
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985em%26p...33..215b&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 33, Dec. 1985, p. 215-218.
Statistics
Computation
Artificial Satellites, Lunar Effects, Lunar Shadow, Orbit Perturbation, Satellite Orbits, Circular Orbits, Orbit Calculation, Orbital Elements
Scientific paper
The change in the eccentricity of the orbit of an artificial earth satellite (AES) as a result of one passage through the moon's shadow is estimated. The shadow is assumed to be of cylindrical shape. For the AES 1963-30D, a perturbation in the heights of perigee and apogee of the orbit of 31.26 m is found, compared to 115.38 m for passage through the earth's shadow. This change cannot be neglected if an accurate computation of the orbit is needed and the satellite has sufficiently large area to mass ratio.
Batrakov Iu. V.
Helali Y. E.
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