Physics
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...81...74l&link_type=abstract
Icarus (ISSN 0019-1035), vol. 81, Sept. 1989, p. 74-91.
Physics
57
Chondrule, Magnetic Field Reconnection, Meteoritic Microstructures, Planetary Nebulae, Stellar Flares, Melting Points, Solar System, Meteorites, Chondrules, Origin, Formation, Nebula, Melting, Calculations, Magnetic Effects, Flares, Coronas, Energy, Heating, Temperature, Dust, Magnetic Fields, Remanent Magnetization, Diagrams, Structure
Scientific paper
A possible episodic heating mechanism that could account for chondrule formation is discussed. The mechanism involves the transient release of energy as a result of magnetic flares in the corona of the protosolar nebula. The possible magnetic behavior of the protosolar nebula is outlined, based on meteorite paleomagnetic evidence about the magnetic field of the protoplanetary nebula and observations of the behavior of magnetic fields. The thermal balance in the melting of a chondrule precursor dust ball is examined. Observational evidence supporting the proposed heating mechanism is presented.
Araki Sakae
Levy Eugene H.
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