The Magellan and Pioneer Venus Orbiter radiometric tracking data sets
have been combined to produce a 60th degree and order spherical harmon
ic gravity field. The Magellan data include the high-precision X-band
gravity tracking from September 1992 to May 1993 and post-aerobraking
data up to January 5, 1994. Gravity models are presented from the appl
ication of Kaula's power rule for Venus and an alternative a priori me
thod using surface accelerations. Results are given as vertical gravit
y acceleration at the reference surface, geoid, vertical Bouguer, and
vertical isostatic maps with errors for the vertical gravity and geoid
maps included. Correlation of the gravity with topography for the dif
ferent models is also discussed. (C) 1994 Academic Press, Inc.