Computer Science
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...78..402h&link_type=abstract
Icarus (ISSN 0019-1035), vol. 78, April 1989, p. 402-410.
Computer Science
36
Asteroids, Cosmology, Induction Heating, Solar Planetary Interactions, Chemical Composition, Pre-Main Sequence Stars, Solar Wind, Spatial Distribution, Asteroids, Electric Properties, Heading, Induction, Composition, Size, Distance, Thermal Properties, Evolution, Electromagnetic Effects, Models, Distribution, Conductivity, Parameters, Diagrams, Carbonaceous Material, Hypotheses, Solar Wind, Formation, Origin
Scientific paper
The driving of primordial asteroidal thermal evolution by EM induction in a dense, premain-sequence solar wind is presently hypothesized to be the basis for recently observed systematic trends of asteroidal composition with respect to both size and heliocentric distance. Good correlation is obtainable between the spatial distribution of induction heating and the spatial distribution inferred from the current distribution of asteroid-composition types, assuming reasonable protosolar-system characteristics; on the basis of this agreement, an approximate constraint on the induction-heating epoch's duration is deduced, together with the temperature-dependent electrical conductivity of the protoasteroidal material.
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