Results 241 to 250 of about 8,311,841 (367)

Science AMA Series: We are Drs. Gulick, Morgan and Lowery. In spring we drilled into the Chicxulub impact crater. Now the whole science party has met for the first time to have a closer look at the cores. AMA! [PDF]

, 2016
Chicxulub Impact, r Science
openalex   +1 more source

Impact Reactivation of a Hydrothermal System in Basalt in the Vargeão Dome Impact Structure, Brazil

Journal of Geophysical Research: Planets, Volume 131, Issue 2, February 2026.
Abstract As hydrous minerals have been observed in impact craters on Mars, impact‐generated hydrothermal systems (IGHSs) have been considered as potential habitats for life on that planet. The Vargeão Dome, a 12 km wide impact structure in southern Brazil, was formed in basalts with at least two hydrothermal alteration stages.
Jitse Alsemgeest, Fraukje M. Brouwer, Luis F. Auqué, Kirsten van Zuilen, Natalia Hauser, Wolf Uwe Reimold   +5 more
wiley   +1 more source

Effect of Different Sand Types and Fractions on Ballistic Resistance of High-Performance Steel Fibre-Reinforced Concrete. [PDF]

Materials (Basel)
Mára M, Fornůsek J, Hrabě T, Sovják R.   +3 more
europepmc   +1 more source

Enhancing regional scientific knowledge for the Ritland Impact Crater: Meteorite classification, mineralogical and impact shock characteristics

, 2020
Linda Cathrin Olsen
openalex   +1 more source

Lunar impact basins: Stratigraphy, sequence and ages from superposed impact crater populations measured from Lunar Orbiter Laser Altimeter (LOLA) data

, 2012
C. Fassett, J. Head, S. Kadish, E. Mazarico, G. Neumann, David E. Smith, M. Zuber   +6 more
semanticscholar   +1 more source

Origin of the Bulge Topography Within Caloris Basin, Mercury

Journal of Geophysical Research: Planets, Volume 131, Issue 2, February 2026.
Abstract Caloris basin on Mercury has a massive circular bulge topography imprinted with unique fault sets. A variety of deformational processes have been proposed to have influenced their formation, including both global contraction and basin evolution, as well as the deposition and weight of the volcanic infill.
G. Schmidt, V. Galluzzi, A. Sepe, S. Buoninfante, B. De Toffoli, L. Ferranti, P. Palumbo   +6 more
wiley   +1 more source

The origin of complex crater formation during high-speed impacts. [PDF]

Sci Adv
Celebi HF, Andrews AJ, Pothos I, Bellefeuille NA, Olson BA, Schwartzentruber TE, Hogan CJ.   +6 more
europepmc   +1 more source

Magnetic signatures of lunar impact craters

Xi Yang, M. A. Wieczorek
openalex   +1 more source

Lightning remagnetization of the Vredefort impact crater: No evidence for impact-generated magnetic fields

, 2012
L. Carporzen, B. Weiss, S. Gilder, A. Pommier, R. Hart   +4 more
semanticscholar   +1 more source

On the Possibility of Melting Water Ice During the Recent Past of Mars: Implications for the Formation of Gullies

Journal of Geophysical Research: Planets, Volume 131, Issue 2, February 2026.
Abstract The formation of gullies on Mars has often been attributed to the melting of (sub)surface water ice. However, melting‐based hypotheses generally overlook key processes: (a) sublimation cooling by latent heat absorption, (b) the non‐stability of ice where melting conditions can be reached, and (c) the particular microclimates of gullied slopes.
L. Lange, F. Forget
wiley   +1 more source