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Conclusions

  • Vsevolod N. AnfilogovEmail author
  • Yurij V. Khachay
Chapter
  • 432 Downloads
Part of the SpringerBriefs in Earth Sciences book series (BRIEFSEARTH)

Abstract

The content of short-living radioactive elements in the silicate part of the proto-planetary cloud matter is sufficient, in the inner part of even small proto-planetary bodies with a radius of about 50 km, to provide a temperature higher than the melting temperature of iron.

Keyword

Dynamics Bodies collision Proto-planetary body Differentiation 3-D model P-T distribution Accumulation process 

Copyright information

© The Author(s) 2015

Authors and Affiliations

  1. 1.Institute of MineralogyRussian Academy of SciencesMiassRussia
  2. 2.Institute of GeophysicsRussian Academy of SciencesEkaterinburgRussia

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