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Updated: Jul 12, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

Magnetita en CI Meteoritos carbonáceos: origen por actividad acuosa en una superficie planetesimal

J F Kerridge, A L Mackay, W V Boynton

    Science (New York, N.Y.)
    |July 27, 1979
    PubMed
    Resumen

    La magnetita en los meteoritos carbonáceos probablemente se formó en su cuerpo progenitor, no en la nebulosa solar temprana. Este hallazgo vuelve a fechar el meteorito.

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