A shallow volatile layer at Chryse Planitia, Mars

• Demura Hirohide

  Department of Earth and Planetary Physics, University of Tokyo

• Kurita Kei

  Department of Earth and Planetary Physics, University of Tokyo

Abstract

We have investigated size distribution of rampart craters in the east edge of Chryse Planitia on Mars by Viking high resolution images. Clear existence of the onset diameter of rampart crater, which defines the minimum size of the rampart crater, has been recognized. If this diameter corresponds to the depth to the top of the volatile layer, the converted depth ranges from -20 m to 60 m. These values are systematically shallower than the previous estimates (Kuzmin, 1988). Martian volatile layer is thought as a main reservoir of the ancient fluvial processes and atmospheric water vapor. This shallow volatile layer gives us information of the inventory of Martian water and conditions of cryosphere.

Journal

• Earth, Planets and Space

  Earth, Planets and Space 50 (5), 423-429, 1998

  Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan, The Volcanological Society of Japan , The Geodetic Society of Japan , The Japanese Society for Planetary Sciences

Keywords

• Space and Planetary Science
• Geology

Details

• CRID: 1390001206510999424
• NII Article ID: 10002206681
• NII Book ID: AA11211921
• DOI: 10.1186/bf03352129
• ISSN: 18805981
• ISSN: 13438832
• Web Site: https://link.springer.com/content/pdf/10.1186/BF03352129.pdf
• Web Site: https://link.springer.com/article/10.1186/BF03352129/fulltext.html
• Web Site: http://link.springer.com/content/pdf/10.1186/BF03352129
• Text Lang: en
• Data Source:
  • JaLC
  • Crossref
  • CiNii Articles
• Abstract License Flag: Disallowed