Results 131 to 140 of about 56,805 (216)
On the helium abundance of Nova Cephei 1971 ejecta [PDF]
J. A. de Freitas Pacheco
openalex +1 more source
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
doaj +1 more source
Explosive volcanic eruptions - VI. Ejecta dispersal in plinian eruptions: the control of eruption conditions and atmospheric properties [PDF]
Lionel Wilson, George P. L. Walker
openalex +1 more source
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
doaj +1 more source
14. Pseudomyrma ejecta. Worker. Length 1 1/2 line.-Rufo-testaceous, smooth and shining: the head, hinder part of the thorax, femora and tibiae, darker-coloured; abdomen blackish-brown; the thorax strangulated in the middle, the first node of the petiole subelongate, a minute tooth at the base of the petiole beneath, both the nodes rufo-testaceous; the ...
openaire +2 more sources
On the possibility of dust condensation in the ejecta of supernova 1987a [PDF]
R. D. Gehrz, E. P. Ney
openalex +1 more source
Confirmation of dust condensation in the ejecta of supernova 1987a. [PDF]
R. D. Gehrz, E. P. Ney
openalex +1 more source
DART Impact Ejecta Plume Evolution: Implications for Dimorphos
The NASA Double Asteroid Redirection Test (DART) spacecraft impacted the moon Dimorphos of the [65803] Didymos binary system and changed the binary orbit period, demonstrating asteroid deflection by a kinetic impact and indicating that more momentum was ...
Andrew F. Cheng+31 more
doaj +1 more source
Chemical Routes to Dust Formation in the Ejecta of Novae [PDF]
J. M. C. Rawlings, D. A. Williams
openalex +1 more source
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
doaj +1 more source