Quantitative mass distribution models for Mare OrientaleSix theoretical models for the mass distribution of Mare Orientale were tested using five gravity profiles extracted from radio-tracking data of orbiting spacecraft. The models with surface mass and moho relief produced the best results. Although there is a mascon-type anomaly in the central maria region, Mare Orientale is a large negative gravity anomaly. This is produced primarily by the empty ring basin. Had the basin filled with maria material it seems likely that it would have produced a mascon such as those presently existing in flooded frontside circular basins.
Document ID
19770051946
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Sjogren, W. L. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Smith, J. C. (Pennsylvania State University State College, Pa., United States)