Radiometric tracking data collected by NASA's Deep Space Network (DSN) for
Mariner 9, Viking 1 and 2 orbiters, and Mars Global Surveyor (MGS) have bee
n analyzed to determine the gravity field of Mars. The gravity solution (MG
S75D) is a complete spherical harmonics model to degree and order 75. Also
parts of the solution are the gravitational constants of Mars, Phobos, and
Deimos. The significant improvement in the MGS75D Mars gravity model is mai
nly a consequence of globally distributed data set collected from the MGS m
apping orbits, the use of optimal weighting and constrained least squares s
olution techniques, and improved force and measurement models in the orbit
determination process. The gravity anomaly map reveals significantly more d
etail and larger amplitudes than any previous Mars gravity map over the maj
or impact and volcanic areas on Mars. Olympus Mons remains the largest know
n gravity anomaly in our solar system and Isidis Planitia, the highest-ampl
itude mascon. There are mascons in the Hellas, Argyre, and Utopia basins. V
alles Marineris has distinctive negative anomalies, and all volcanic featur
es are positive. Gravity anomalies over several craters have also been reso
lved. The overall correlation of the MGS75D gravity anomaly map with topogr
aphy derived from the Mars Orbiter Laser Altimeter (MOLA) is very high, whi
le the polar regions display relatively poor correlation.