Results 81 to 90 of about 36,481 (263)
Martian Surface and Atmosphere Workshop
Eos, Transactions American Geophysical Union, 1992 The NASA‐sponsored Martian Surface and Atmosphere Through Time Study Project convened its first major meeting at the University of Colorado in Boulder, September 23–25, 1991. The workshop, co‐sponsored by the Lunar and Planetary Institute (LPI) and the Laboratory for Atmospheric and Space Physics at the University of Colorado, brought together an ...
openaire +1 more source
Hypogravity simulation using the Variable Gravity Suspension System: A technical report
Experimental Physiology, EarlyView.Abstract Human movement has evolved within Earth's gravitational environment (1 g; −9.81 m s−2). Future human exploration of terrestrial bodies, including the Moon (0.17 g; −1.62 m s−2) and Mars (0.38 g; −3.71 m s−2), will require astronauts to live and work within reduced gravitational environments (hypogravity).
Patrick Swain +7 more
wiley +1 more source
Directionality of the Martian Surface Radiation and Derivation of the Upward Albedo Radiation [PDF]
, 2021 Jingnan Guo +10 more
openalex +1 more source
What martian meteorites reveal about the interior and surface of Mars
, 2020 Arya Udry +5 more
+4 more sources
Life, 2018 Minerals might have played critical roles for the origin and evolution of possible life forms on Mars. The study of the interactions between the “building blocks of life„ and minerals relevant to Mars mineralogy under conditions mimicking the
Teresa Fornaro +2 more
doaj +1 more source
Evolution of Water Reservoirs on Mars: Constraints from Hydrogen Isotopes in Martian Meteorites
, 2014 Martian surface morphology implies that Mars was once warm enough to maintain persistent liquid water on its surface. While the high D/H ratios (~6 times the Earth's ocean water) of the current martian atmosphere suggest that significant water has been ...
Dohm, James M. +6 more
core +1 more source
Hypotheses for near-surface exchange of methane on Mars [PDF]
, 2016 The Curiosity rover recently detected a background of 0.7 ppb and spikes of 7 ppb of methane on Mars. This in situ measurement reorients our understanding of the Martian environment and its potential for life, as the current theories do not entail any ...
Bloom, A. Anthony +4 more
core +3 more sources
Martian surface temperatures [PDF]
Reduction of infrared scan data on Martian surface ...
Morrison, D.
core +1 more source
Laboratory and field analogs of the Martian (sub)surface [PDF]
, 2023 Karolina Anna Poplawska-Kopacz
openalex +1 more source
Seasonal Ice Cover Could Allow Liquid Lakes to Persist in a Cold Mars Paleoclimate
AGU Advances, Volume 7, Issue 1, February 2026.Abstract Geomorphic and stratigraphic studies of Mars prove that extensive liquid water flowed and pooled on the surface early in Mars' history. Martian paleoclimate models, however, have difficulty simulating climate conditions warm enough to maintain liquid water on early Mars.
Eleanor L. Moreland +8 more
wiley +1 more source