On the Initially Circular Motion of an Orbiter in the Oblate, Rotating, Martian Atmosphere

Details On the Initially Circular Motion of an Orbiter in the Oblate, Rotating, Martian Atmosphere On the Initially Circular Motion of an Orbiter in the Oblate, Rotating, Martian Atmosphere

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..24...15m&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 24, 15

Astronomy and Astrophysics

Astronomy

1

Scientific paper

RESUMEN Usando la ley de distribuci6n de densidad propuesta por Sehnal and Pospisilova (1988), se estudia el movimiento inicial circular de una 6rbita en la atmosfera de Marte (considerada oblicua y en rotaci6n). Se estiman analiticamente la diferencia entre el perfodo nodal y Kepleriano correspondiente, asf como los cambios independientes en cinco elementos orbitales, sobre un perfodo nodal. ABSTRACT Using the density distribution law proposed by Sehnal and Pospisilova (1988), the initially circular motion of an orbiter in Mars' atmosphere (considered as oblate and rotating) is studied. The difference between the nodal period and the corresponding Keplerian one, and the changes of five independent orbital elements, over a nodal period, are analytically estimated. Key words: ORBITAL - PLANETh AND SATELLIThS-ATMOSPHERES - SOLAR SYSThM

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