Characterization of the Martian Surface Deposits by the Mars Pathfinder Rover, Sojourner
- 5 December 1997
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 278 (5344) , 1765-1768
- https://doi.org/10.1126/science.278.5344.1765
Abstract
Sojourner, the Mars Pathfinder rover, discovered pebbles on the surface and in rocks that may be sedimentary—not volcanic—in origin. Surface pebbles may have been rounded by Ares flood waters or liberated by weathering of sedimentary rocks called conglomerates. Conglomerates imply that water existed elsewhere and earlier than the Ares flood. Most soil-like deposits are similar to moderately dense soils on Earth. Small amounts of dust are currently settling from the atmosphere.Keywords
This publication has 8 references indexed in Scilit:
- Overview of the Mars Pathfinder Mission and Assessment of Landing Site PredictionsScience, 1997
- The Chemical Composition of Martian Soil and Rocks Returned by the Mobile Alpha Proton X-ray Spectrometer: Preliminary Results from the X-ray ModeScience, 1997
- The Pathfinder MicroroverJournal of Geophysical Research, 1997
- Viking landing sites, remote-sensing observations, and physical properties of Martian surface materialsIcarus, 1989
- The Martian surface as imaged, sampled, and analyzed by the Viking landersReviews of Geophysics, 1989
- A summary of Viking sample‐trench analyses for angles of internal friction and cohesionsJournal of Geophysical Research, 1982
- Properties and effects of dust particles suspended in the Martian atmosphereJournal of Geophysical Research, 1979
- The geology of the Viking Lander 2 siteJournal of Geophysical Research, 1977