Mineralogical clues to the origins of asteroid dynamical families

Details Mineralogical clues to the origins of asteroid dynamical families Mineralogical clues to the origins of asteroid dynamical families

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...78..426b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 78, April 1989, p. 426-440.

Mathematics

Logic

26

Asteroids, Chemical Composition, Cosmology, Mineralogy, Planetology, Astronomical Models, Classifying, Orbital Elements, Orbital Resonances (Celestial Mechanics), Solar System, Asteroids, Mineralogy, Dynamics, Origin, Formation, Parent Bodies, Composition, Infrared, Radar Methods, Procedure, Classification, Catalog, Comparisons, Asteroid Families

Scientific paper

Remote-sensing data are the bases of the present tabulation of the mineralogical composition of the asteroid dynamical families' parent bodies, in which correlations are presented between Tholen's (1984) taxonomic types and the family-membership lists of Hirayama (1933), Brouwer (1951), Arnold (1969), Carusi and Massaro (1978), Kozai (1979), and Williams (1979). In conjunction with recently obtained IR and radar data, these tables suggest that most of the smaller proposed families cannot share the origin of the larger, well-defined families as fragments of collisionally disrupted parent bodies.

Affiliated with

Also associated with

No associations

Rating

Mineralogical clues to the origins of asteroid dynamical families does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mineralogical clues to the origins of asteroid dynamical families, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mineralogical clues to the origins of asteroid dynamical families will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1737542