A new gravity field determination that has been produced combines both
the Pioneer Venus Orbiter (PVO) and the Magellan Doppler radio data.
Comparisons between this estimate, a spherical harmonic model of degre
e and order 21, and previous models show that significant improvements
have been made. Results are displayed as gravity contours overlaying
a topographic map. We also calculate a new spherical harmonic model of
topography based on Magellan altimetry, with PVO altimetry included w
here gaps exist in the Magellan data. This model is also of degree and
order 21, so in conjunction with the gravity model, Bouguer and isost
atic anomaly maps can be produced. These results are very consistent w
ith previous results, but reveal more spatial resolution in the higher
latitudes.