Results 211 to 220 of about 64,792 (321)

Is the transition impact to post‐impact rock complete? Some remarks based on XRF scanning, electron microprobe, and thin section analyses of the Yaxcopoil‐1 core in the Chicxulub crater [PDF]

, 2004
Jan Smit, Sjerry van der Gaast, W. J. Lustenhouwer   +2 more
openalex   +1 more source

Theoretical prediction of crater size for hypervelocity impact by reduced-density particles, 18 May 1966 - 17 August 1967 [PDF]

Theoretical prediction of crater size in Al alloy for hypervelocity impact by reduced density ...
Heyda, J. F., Riney, T. D.
core   +1 more source

Silicate–sulfide interaction within quenched melts of space weathered Ryugu grains

Meteoritics &Planetary Science, EarlyView.
Abstract The first few microns of the surface of airless bodies are subject to severe changes due to the harsh environment of space, known as space weathering. The Hayabusa2 sample return mission from the asteroid Ryugu provides the first opportunity to study these effects on a carbonaceous and hydrated body.
Sylvain Laforet, Hugues Leroux, Corentin Le Guillou, Maya Marinova, Adrien Néri, Adrien Teurtrie, Francisco de la Peña, Damien Jacob, Alexandre Fadel, David Troadec   +9 more
wiley   +1 more source

Reply to Mizera and Strunga: Evidence for the Bolaven impact crater and its ejecta. [PDF]

Proc Natl Acad Sci U S A
Sieh K, Herrin J, Schonwalder Angel D.
europepmc   +1 more source

Secondary alteration of the impactite and mineralization in the basal Tertiary sequence, Yaxcopoil‐1, Chicxulub impact crater, Mexico [PDF]

, 2004
D E Ames, I M Kjarsgaard, Kevin Pope, B. O. Dressler, Mark Pilkington   +4 more
openalex   +1 more source

Selective sampling of asteroids, the Moon, and Mars: Factors affecting the numerical abundances of members of meteorite groups

Meteoritics &Planetary Science, EarlyView.
Abstract Meteorite collection inventories show that many related meteorite groups have very different numerical abundances (e.g., lunar versus Martian meteorites; Eagle Station pallasites versus main‐group pallasites; eucrites versus diogenites; ungrouped Antarctic irons versus ungrouped non‐Antarctic irons; carbonaceous chondrite‐related (CC) iron ...
Alan E. Rubin
wiley   +1 more source

Proximal ejecta of the putative parent impact crater for Australasian tektites at the Bolaven Plateau. [PDF]

Proc Natl Acad Sci U S A
Mizera J, Strunga V.
europepmc   +1 more source

Discovery of the largest impact crater field on Earth in the Gilf Kebir region, Egypt [PDF]

, 2004
Philippe Paillou, A. El Barkooky, A. A. Barakat, Jean-Marie Malézieux, Bruno Reynard, Jean Dejax, Essam Heggy   +6 more
openalex   +1 more source

Low‐temperature dissociation of zircon in highly alkaline conditions: A cautionary note for studies on natural glasses of debated origin

Meteoritics &Planetary Science, EarlyView.
Abstract Dissociated zircon is largely used as a robust indicator of glasses generated by impact cratering and airbursts. The reaction of zircon dissociation, i.e. ‘ZrSiO4 → ZrO2 + SiO2’, requires high temperatures (>1670°C) only reached by extreme geological processes. Using high‐temperature experiments, this study shows that zircon can dissociate and
A. Musolino, B. Devouard, P. Rochette, P. Roperch, P. M. Zanetta, A.‐M. Seydoux‐Guillaume, A. Licht, D. Ferry, A. Campos   +8 more
wiley   +1 more source

Pseudo-Spectral Spatial Feature Extraction and Enhanced Fusion Image for Efficient Meter-Sized Lunar Impact Crater Automatic Detection in Digital Orthophoto Map. [PDF]

Sensors (Basel)
Liu H, Lu YB, Zhang L, Liu F, Tian Y, Du H, Yao J, Yu Z, Li D, Lin X.   +9 more
europepmc   +1 more source