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Emergence of two types of terrestrial planet on solidification of magma ocean

Author

Listed:
  • Keiko Hamano

    (The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan)

  • Yutaka Abe

    (The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan)

  • Hidenori Genda

    (The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
    Earth-Life Science Institute, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan)

Abstract

Terrestrial planets can be divided into two distinct types on the basis of their evolutionary history during solidification from their initial molten state: type I planets (such as Earth) solidify within several million years and retain most of their water, and type II planets (possibly such as Venus), formed inside a critical distance, are desiccated by hydrodynamic escape.

Suggested Citation

  • Keiko Hamano & Yutaka Abe & Hidenori Genda, 2013. "Emergence of two types of terrestrial planet on solidification of magma ocean," Nature, Nature, vol. 497(7451), pages 607-610, May.
  • Handle: RePEc:nat:nature:v:497:y:2013:i:7451:d:10.1038_nature12163
    DOI: 10.1038/nature12163
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    Cited by:

    1. Suraj K. Bajgain & Aaron Wolfgang Ashley & Mainak Mookherjee & Dipta B. Ghosh & Bijaya B. Karki, 2022. "Insights into magma ocean dynamics from the transport properties of basaltic melt," Nature Communications, Nature, vol. 13(1), pages 1-10, December.

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