Results 201 to 210 of about 62,716 (304)
Recent explosive lava-water interaction in Tharsis, Mars. [PDF]
Pieterek B, Jones TJ.
europepmc +1 more source
Life on Mars? The physiological perspective
Experimental Physiology, EarlyView.
Ronan M. G. Berg, Damian M. Bailey
wiley +1 more source
Widespread Impact‐Induced Crustal Permeability on the Early Earth
Abstract The early Earth (i.e., Archean and Hadean Eons, 2.5–4.0 and 4.0–4.5 Ga, respectively) experienced frequent cosmic bombardment. Impacts have been shown to stimulate crustal alteration, for instance via hydrothermal systems active for up to millions of years post‐impact.
A. M. Alexander +2 more
wiley +1 more source
Lunar origin of Earth quasi-satellite Kamo'oalewa. [PDF]
Zhu MH +9 more
europepmc +1 more source
Abstract The study of planetary surface processes has traditionally relied on the manual interpretation of spacecraft images. While manual image analysis methods are robust and well‐established, they become impractical when the volume of available data is large and may introduce observer bias.
Yasmin Hayat, Lior Rubanenko
wiley +1 more source
Numerical Prediction on the Impact Resistance of UHMWPE Flexible Film Against Hypervelocity Particles. [PDF]
Liu H +6 more
europepmc +1 more source
Terrestrial Analogs to Titan for Geophysical Research
Abstract Saturn's moon Titan exhibits remarkable parallels to the Earth in many geophysical and geological processes not found elsewhere in the solar system at the present day. These include a nitrogen atmosphere with a condensible gas—methane—replacing the Earth's water, leading to an active meteorology with rainfall and surface manifestations ...
Conor A. Nixon +21 more
wiley +1 more source
Complex crater formation by low energy impactors. [PDF]
Tardini Paulino R +4 more
europepmc +1 more source
Arc Heat Flow and Magmatic Heat Budgets
Abstract We evaluate hydrothermal heat loss from 11 volcanic‐arc segments (∼6,000 km of arc length, ∼10% of the global total), motivated by the observation that much magmatic heat ultimately crosses the land surface as heated aqueous fluid. Heat loss takes place by volcanic eruption, geothermal heat conduction to the surface, fumarolic (vapor ...
S. E. Ingebritsen +7 more
wiley +1 more source
Recent production rates of cosmogenic nuclides in the igneous rocks of Jezero crater floor, Mars. [PDF]
Zorzano M- +2 more
europepmc +1 more source

