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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Minimum velocity for impact ejecta to form secondaries on terrestrial bodies
The minimum velocity (v) for impact ejecta to form secondary craters (secondaries) remains enigmatic, but it is a crucial parameter in untangling the fate of impact ejecta on planetary surfaces.
Rui Xu +4 more
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The First Day of a Type Ia Supernova from a Double-degenerate Binary
Supernovae in binary star systems involve a hydrodynamical interaction between the ejecta and a binary companion. This collision results in shock heating and a modified density structure for the ejecta, both of which affect the light curve.
Gabriel Kumar +2 more
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Superluminous supernovae: diverse rise times explain diverse spectra. [PDF]
Nicholl M.
europepmc +1 more source
Searching for surficial water ice in lunar permanently shaded regions (PSRs) with ShadowCam. [PDF]
Li S +7 more
europepmc +1 more source
Direct detection of an asteroid's heliocentric deflection: The Didymos system after DART. [PDF]
Makadia R +13 more
europepmc +1 more source
Southward impact excavated magma ocean at the lunar South Pole-Aitken basin. [PDF]
Andrews-Hanna JC +12 more
europepmc +1 more source
Increased small impactor flux on the Moon as inferred from regolith thickness at the Chang'E-5 Region. [PDF]
Zhang M, Jia B, Eke VR, Fa W.
europepmc +1 more source
Extremophile survives the transient pressures associated with impact-induced ejection from Mars. [PDF]
Zhao L +3 more
europepmc +1 more source

