Interior Structure and Seasonal Mass Redistribution of Mars from Radio Tracking of Mars Pathfinder
W. M. Folkner,
*
C. F. Yoder,
D. N. Yuan,
E. M. Standish,
R. A. Preston
Doppler and range measurements to the Mars Pathfinder lander
made using its radio communications system have been combined with
similar measurements from the Viking landers to estimate improved
values of the precession of Mars' pole of rotation and the variation
in Mars' rotation rate. The observed precession of -7576 ± 35 milliarc seconds of angle per year implies a dense core and constrains
possible models of interior composition. The estimated annual variation
in rotation is in good agreement with a model of seasonal mass exchange
of carbon dioxide between the atmosphere and ice caps.
Jet Propulsion Laboratory, California Institute of Technology,
4800 Oak Grove Drive, Pasadena, CA 91109, USA.
*
To whom correspondence should be addressed. E-mail:
william.folkner{at}jpl.nasa.gov