Origin of α-poor Very Metal-poor Stars
Among very metal-poor (VMP) stars, α -poor VMP ( α -PVMP) stars that have subsolar values of [X/Fe] for Mg and other α elements are rare and are thought to have been formed from gas polluted by Type 1a supernova (SN 1a). However, recent analyses indicate
S. K. Jeena, Projjwal Banerjee
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The martian tropical water ice spatial and temporal distribution was characterized using impact crater ejecta type, location, size, and age in one of two epochs, ≤3.4 Ga and >3.4 Ga, using statistical models designed for spatial and temporal correlation ...
Jamie D. Riggs, Michelle R. Kirchoff
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Contemporaneous formation of self-secondaries and layered ejecta deposits on Mars
Self-secondaries are secondary craters formed in cogenetic ejecta deposits. Bearing important information on cratering mechanics and the applicability of remote age-determination technique using crater statistics, the spatial distribution of self ...
Fanglu Luo +7 more
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Mitigating plume surface interactions using lunar craters. [PDF]
Anderson SL, Saxena P, Metzger PT.
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A southward differentiated impactor forms the tapered shape of the South Pole-Aitken impact basin on the Moon. [PDF]
Wakita S +10 more
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Mobilization of Unconsolidated Granular Material on Asteroid (101955) Bennu by Spacecraft Interaction. [PDF]
Bierhaus EB +22 more
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Thermal runaway-induced short-circuit arc in highly integrated lithium-ion battery systems: mechanisms, thresholds, and mitigation strategies. [PDF]
Yu Z +6 more
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Unraveling the Cretaceous-Paleogene boundary event across the Gulf of Mexico-High-resolution Rayon reef section, Valles-San Luis Potosi platform, Mexico. [PDF]
Bartali R +4 more
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Superluminous supernovae: diverse rise times explain diverse spectra. [PDF]
Nicholl M.
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