Results 61 to 70 of about 36,538 (226)
Jumping on the moon as a potential exercise countermeasure
Experimental Physiology, EarlyView.Abstract The Moon's gravitational field strength (17% Earth's gravity) may facilitate the use of bodyweight jumping as an exercise countermeasure against musculoskeletal and cardiovascular deconditioning in reduced gravity settings. The present study characterised the acute physiological and kinetic responses to bodyweight jumping in simulated Lunar ...
Patrick Swain +4 more
wiley +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
Martian meso/micro-scale winds and surface energy budget [PDF]
, 2011 Regional, diurnal and seasonal variations of surface temperature are particularly large on Mars. This is mostly due to the Martian surface remaining close to radiative equilibrium.
Forget, F. +6 more
core
Laboratory and field analogs of the Martian (sub)surface [PDF]
, 2023 Karolina Anna Poplawska-Kopacz
openalex +1 more source
Mars base buildup scenarios [PDF]
, 1985 Two Mars surface based build-up scenarios are presented in order to help visualize the mission and to serve as a basis for trade studies. In the first scenario, direct manned landings on the Martian surface occur early in the missions and scientific ...
Blacic, J. D.
core +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
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
What martian meteorites reveal about the interior and surface of Mars
, 2020 Arya Udry +5 more
+4 more sources
The Sands of Phobos: The Martian moon's eccentric orbit refreshes its surface
, 2018 The surface of the Martian moon Phobos exhibits two distinct geologic units, known as the red and blue units. The provenance of these regions is uncertain yet crucial to understanding the origin of the Martian moon and its interaction with the space ...
Ballouz, Ronald-Louis +4 more
core +1 more source
Characterizing Martian Primary Crustal Compositions With Gamma Ray Spectroscopy
Geophysical Research Letters, Volume 53, Issue 2, 28 January 2026.Abstract Mars's global‐scale chemical maps of the midlatitudes, derived from Mars Odyssey gamma and neutron spectroscopy, have constrained martian geology across a multitude of processes. However, the chemical maps are often used to analyze pre‐defined regions based on mapped geology and/or mineralogy.
Carlos E. Gary‐Bicas +5 more
wiley +1 more source