The moon and the planets

, Volume 20, Issue 3, pp 241–249 | Cite as

Early collisional heating of the Moon

  • G. P. Horedt


It is shown that, because of the occurrence of ‘fall-back’ craters, there could occur considerable heating of the Moon above the melting point of silicates during accretional time scales of order 106–108 yr.


Silicate Melting Point Considerable Heating Collisional Heating Accretional Time 
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Copyright information

© D. Reidel Publishing Co 1979

Authors and Affiliations

  • G. P. Horedt
    • 1
  1. 1.Physics Dept.Universitatea ClujRomania

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