Advertisement

Introduction

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

Abstract

At present, there is no generally recognized model that can describe the whole diversity of the conditions which led to the formation of the Solar system. The numerous hypotheses in which authors try to solve this problem can be divided into two groups.

Keywords

Solar system Molecular clouds Supernova Meteorite The Earth The Moon Formation 

References

  1. 1.
    Urey H (1951) The origin and development of the Earth and other terrestrial planets. Geochim et Cosmochim Acta 2:209–277CrossRefGoogle Scholar
  2. 2.
    Fisher D (1987) The birth of the Earth. Columbia University Press, New YorkGoogle Scholar
  3. 3.
    Vitjazev A, Pechernikova G, Safronov V (1990) The Earth’s group planets. Nauka, Moscow (in Russian)Google Scholar
  4. 4.
    Miyake Y (1965) Elements of geochemistry. Muruzen, TokyoGoogle Scholar
  5. 5.
    Schmidt O (1962) The origin of the Earth and planets. Academy of Science USSR Press (in Russian)Google Scholar
  6. 6.
    Herbst W, Assouza G (1982) The role of supernova on the star formation and spiral structure. In: Gehrels T (ed) Protostars and planets. The studies of star formation and of the origin of the Solar system. University of Arizona Press. Russian version. Mir, Moscow, pp 421–429Google Scholar
  7. 7.
    Shramm D (1982) Supernova and the solar system formation. In. Gehrels T (ed) The studies of star formation and of the origin of the Solar system. University of Arizona Press. Russian version. Mir, Moscow, pp 440–457Google Scholar
  8. 8.
    Ouellette N, Desh S, Bizzaro M et al (2008) The injection mechanisms of short-living radio nuclides and their homogenization. Geochim et Cosmochim Acta 73:4946–4962CrossRefGoogle Scholar
  9. 9.
    Huss G, Meyer B, Srinivasan B et al (2008) Stellar sources of short-living radionuclides in the early Solar system. Geochim et Cosmochim Acta 73:4922–4945CrossRefGoogle Scholar
  10. 10.
    Grossman L (1972) Condensation in the primitive solar nebula. Geochim et Cosmochim Acta 36:597–619CrossRefGoogle Scholar
  11. 11.
    Amelin Y, Krot A (2007) Pb isotopic age of the Allende chondrules. Meteorit Planet Sci 42:1321–1337CrossRefGoogle Scholar
  12. 12.
    Anfilogov V, Khachay Y (2005) A possible scenario of material differentiation at initial stage of the Earth formation. Doklady Earth Sci 403A:954–947 (in Russian)Google Scholar
  13. 13.
    Anfilogov V, Khachay Y (2013) Origin of the Kimberlite diamond bearing lithosphere of cratons. Dokl Akad Nauk SSSR 451:537–540Google Scholar
  14. 14.
    Anfilogov V, Khachay Y (2013) Evolution of core and silicate envelopes at heterogeneous accumulation of the Earth. Lithosphera 4:146–153 (in Russian)Google Scholar
  15. 15.
    Khachay Y, Anfilogov V (2009) The temperature distribution numerical models for the Earth envelopes at its accumulation stages. Geodynamics. Deep structure. The Earth’s thermal field. Geophysical fields interpretation. In: Proceedings on 5th conference on behalf of Bulashevich. Ekaterinburg, pp 520–522 (in Russian)Google Scholar
  16. 16.
    Khachay Y, Anfilogov V (2009) The variant of the temperature distributions in the Earth on its accumulation. The study of the Earth as a planet by methods of geophysics, geodesy and astronomy. In: Proceedings on 6th Orlov conference. Kiev, pp 197–202Google Scholar
  17. 17.
    Anfilogov V, Khachay Y (2012) Differentiation of mantle material at the Earth’s accumulation and the initial crust formation. Lithosphera 6:3–13 (in Russian)Google Scholar
  18. 18.
    Khachay Y, Anfilogov V (2013) Numerical results of Earth’s core accumulation 3-D modeling. EGU Geophys Res Abs 15:51Google Scholar
  19. 19.
    Anfilogov V, Khachay Y, Antipin A (2014) Numerical 3D simulation of temperature distribution at the stage of the Earth’s accumulation and peculiarity of its initial minerageny. Ural Geophys Bull 1:81–85 (in Russian)Google Scholar
  20. 20.
    Khachay Y, Anfilogov V, Antipin A (2014) Numerical results of 3-D simulation of Moon accumulation. EGU Geophys Res Abs 16:1011Google Scholar
  21. 21.
    Khachay Y, Antipin A (2014) The results of numerical 3D simulation of temperature distribution in the lunar envelopes at its accumulation. Monitoring. Nauka i Technologii 1:28–32 (in Russian)Google Scholar

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

Personalised recommendations