Magmatic differentiation of the moon's interior, confirmed through calculations of thermal history, was studied. It appears that differentiation was a result of the moon's initial temperature whose origin remains unknown. In solving this problem, convective models of the moon were considered as well as a two layered differentiated model of the moon, operative over the past 3.5 billion years. The high content of long lived radioactive elements present was investigated in explaining the moon's current thermal properties. The controversy concerning the true nature of magmatic differentiation continues to be unsolved.


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    Titel :

    Riddles about the origin and thermal history of the moon


    Beteiligte:
    Levin, B. Y. (Autor:in) / Mayeva, S. V. (Autor:in)


    Erscheinungsdatum :

    1977-01-01


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :



    Origin and history of the moon

    Urey, H. C. | NTRS | 1969


    Solving riddles of aviation medicine

    Engineering Index Backfile | 1941


    Thermal History of the Moon

    Lucas, John W. | AIAA | 1972


    On the thermal history of the moon

    Arkani-Hamed, J. | NTRS | 1973