DATA_SET_DESCRIPTION |
Data Set Overview
=================
This collection of asteroid masses and densities has been compiled from
the published literature by Jim Baer, Steve Chesley, and Dan Britt. It
also includes asteroid size and shape information, also collected from the
published literature, to show the source of the tabulated bulk density.
The version included in this data set is dated April 18, 2012. This data
set supersedes the older PDS Asteroid Densities data set,
EAR-A-5-DDR-ASTEROID-DENSITIES-V1.1.
In addition to the asteroid mass and density file, astmass12.tab, the file
astmassrefs12.tab lists the full references of the published sources of
the mass and size data. Only published values are included; a few
unpublished values included in the original file have been removed.
In selecting size information for computing the bulk density, preference
was given to the source with the most plausible greatest precision. In
general, this yielded the following order of preference:
- direct imagery (including adaptive optics)
- radar
- occultation
- light curves
- radiometric (especially SIMPS).
In addition to asteroids, entries for the Pluto/Charon/Nix/Hydra system
are included. For comet masses, see the data set Properties of Comet
Nuclei, EAR-C-COMPIL-5-COMET-NUC-PROPERTIES-V1.0.
Since the cited publication Standish (2001) is of limited availability, it
has been provided in the document directory of this data set with
permission from the author.
Standish, E. M., Suggested GM values for Ceres, Pallas, and Vesta, JPL
Interoffice Memorandum 312.F-01-006, April 11, 2001. [Standish2001]
Modification History
====================
This data set was first archived in 2009 and has been updated since by
adding additional asteroid masses that have been published since the
previous update. The number of asteroid masses given in each version are
V1.0 - 151
V2.0 - 222
V3.0 - 248
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CITATION_DESCRIPTION |
Baer, J., Chesley, S., and Britt, D., Eds., Asteroid Masses V3.0.
EAR-A-COMPIL-5-ASTMASS-V3.0. NASA Planetary Data System, 2012.
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