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Multiple parent bodies of ordinary chondritesThermal histories of chondrite parent bodies are calculated from an initial state with material in a powder-like form, taking into account the effect of consolidation state on thermal conductivity. The very low thermal conductivity of the starting materials makes it possible for a small body with a radius of less than 100 km to be heated by several hundred degrees even if long-lived radioactive elements in chondritic abundances are the only source of heat. The maximum temperature is determined primarily by the temperature at which sintering of the constituent materials occurs. The thermal state of the interior of a chondrite parent body after sintering has begun is nearly isothermal. Near the surface, however, where the material is unconsolidated and the thermal conductivity is much lower, the thermal gradient is quite large. This result contradicts the conventional 'onion-shell' model of chondrite parent bodies. But because the internal temperature is almost constant through the whole body, it supports a 'multiple-parent bodies' model, according to which each petrologic type of chondrite comes from a different parent body.
Document ID
19840051235
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Yomogida, K.
(MIT Cambridge, MA, United States)
Matsui, T.
(Tokyo, University Tokyo, Japan)
Date Acquired
August 12, 2013
Publication Date
April 1, 1984
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 68
Issue: 1 Ap
ISSN: 0012-821X
Subject Category
Lunar And Planetary Exploration
Accession Number
84A34022
Funding Number(s)
CONTRACT_GRANT: NSG-7081
Distribution Limits
Public
Copyright
Other

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