Results 251 to 260 of about 78,262 (284)

Hydrogenotrophic methanogenesis at 7-12 mbar by Methanosarcina barkeri under simulated martian atmospheric conditions. [PDF]

Sci Rep
Harris RL, Schuerger AC.
europepmc   +1 more source

Percolative sulfide core formation in oxidized planetary bodies. [PDF]

Nat Commun
Crossley SD, Setera JB, Anzures BA, Iacovino K, Buckley WP, Eckley SA, O'Neal EW, Maisano JA, Simon JI, Righter K.   +9 more
europepmc   +1 more source

On Martian Longitudes

The Astrophysical Journal, 1895
openaire   +2 more sources

Time-series variations of recurring slope lineae on Mars compatible with contemporary water activity from bedrock aquifer melting. [PDF]

Sci Rep
Liu S, Wu B, Krasilnikov S, Zhu J, Chen Z, Chai S, Zhao Q, Li Y, Michalski J.   +8 more
europepmc   +1 more source

Seismic evidence of liquid water at the base of Mars' upper crust. [PDF]

Natl Sci Rev
Sun W, Tkalčić H, Malusà MG, Pan Y.
europepmc   +1 more source

The effect of vibrotactile feedback on performance, perception and trust when balancing in different analog g-levels. [PDF]

Exp Brain Res
Vimal VP, DiZio P, Lackner JR.
europepmc   +1 more source

Aeroponic Technology for Accelerated Weathering of Extraterrestrial Regolith to Extract Plant Essential Nutrients and Generate Arable Soils. [PDF]

ACS Earth Space Chem
Coker HR, Denvir AC, Robertson IJ, Shackelford CEB, Li WH, Lin CW, Watters RM, Sparks DL, Smith AP, Howe JA.   +9 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Martian chronicler

Science, 2020
NASA's Perseverance rover aims to find out whether ancient Mars was warm and wet or cold and dry.
openaire   +2 more sources

The Martian Rose

Leonardo, 2009
This artwork explores extreme environments and life beyond terrestrial settings. Using a planetary simulation chamber, a rose was exposed to Martian environment for six hours at the Mars Simulation Laboratory, University of Aarhus, Denmark.
Boland, Howard, Cinti, Laura
openaire   +3 more sources