Time-dependent model of the Martian atmosphere for use in orbit lifetime and sustenance studies

Astronomy and Astrophysics – Astronomy

Scientific paper

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Artificial Satellites, Atmospheric Models, Low Altitude, Mars Atmosphere, Satellite Drag, Time Dependence, Diurnal Variations, Dust Storms, Fortran, Satellite Lifetime, Solar Radiation

Scientific paper

A time-dependent model of the Martian atmosphere suitable for calculation of long-term aerodynamic effects on low altitude satellites is presented. The atmospheric model is both position dependent, through latitude and longitude effects, and time dependent. The time dependency includes diurnal and seasonal effects, effects of annual motion, long and short term solar activity effects, and periodic dust storm effects. Nine constituent gases are included in the model. Uncertainties in exospheric temperature, turbidity, and turbopause altitude are used to produce bounds on the expected density. A computer model - a Fortran subroutine which, when given the Julian date, Cartesian position of the sun and the spacecraft in aerocentric coordinates, returns the local values of mass density, temperature, scale height, and upper and lower bounds on the mass density is presented.

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