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A surface gravity traverse on Mars indicates low bedrock density at Gale crater.
Lewis, Kevin W; Peters, Stephen; Gonter, Kurt; Morrison, Shaunna; Schmerr, Nicholas; Vasavada, Ashwin R; Gabriel, Travis.
Afiliação
  • Lewis KW; Earth and Planetary Sciences Department, Johns Hopkins University, Baltimore, MD 21218, USA. klewis@jhu.edu.
  • Peters S; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
  • Gonter K; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
  • Morrison S; Geophysical Laboratory, Carnegie Institution, Washington, DC 20015, USA.
  • Schmerr N; Department of Geology, University of Maryland, College Park, MD 20742, USA.
  • Vasavada AR; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
  • Gabriel T; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85281, USA.
Science ; 363(6426): 535-537, 2019 02 01.
Article em En | MEDLINE | ID: mdl-30705193
ABSTRACT
Gravimetry, the precise measurement of gravitational fields, can be used to probe the internal structure of Earth and other planets. The Curiosity rover on Mars carries accelerometers normally used for navigation and attitude determination. We have recalibrated them to isolate the signature of the changing gravitational acceleration as the rover climbs through Gale crater. The subsurface rock density is inferred from the measured decrease in gravitational field strength with elevation. The density of the sedimentary rocks in Gale crater is 1680 ± 180 kilograms per cubic meter. This value is lower than expected, indicating a high porosity and constraining maximum burial depths of the rocks over their history.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2019 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2019 Tipo de documento: Article