Masses and densities of asteroidsCeres, Pallas, and Vesta allow a determination of mass from gravitational effects in the motion of another asteroid. An extended and partly corrected set of observations of 197 Arete leads to an increase of 15% in the resulting mass of Vesta that was first determined by Hertz. Other possibilities of mass determination and estimates of the total mass of asteroids are mentioned. The available diameter determinations and adopt preferred values are reviewed. The densities for Ceres, Pallas, and Vesta are respectively 2.3 plus or minus 1.1 g/cu cm, 2.6 plus or minus 0.9 g/cu cm and 3.3 plus or minus 1.5 g/cu cm.
Document ID
19800040386
Acquisition Source
Legacy CDMS
Document Type
Other - Collected Works
Authors
Schubart, J. (Heidelberg, Universitaet Heidelberg, Germany)
Matson, D. L. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)