Thermal metamorphism of the C, G, B, and F asteroids seen from the 0.7 μm, 3 μm, and UV absorption strengths in comparison with carbonaceous chondrites

Author:

Hiroi Takahiro,Zolensky Michael E.,Pieters Carlé M.,Lipschutz Michael E.

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference46 articles.

1. Incompletely transformed serpentine-type phyllosilicates in the matrix of Antarctic CM chondrites;Akai;Geochim. Cosmochim. Acta,1988

2. Mineralogical evidence of heating events in Antarctic carbonaceous chondrites, Y-86720 and Y-82162;Akai;Proc. NIPR Symp. Antarct. Meteorites,1990

3. T-T-T diagram of serpentine and saponite, and estimation of metamorphic heating degree of Antarctic carbonaceous chondrites;Akai;Proc. NIPR Symp. Antarct. Meteorites,1992

4. The 52-color asteroid survey: Final results and interpretation (abstract);Bell;Lunar Planet. Sci.,1988

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