Results 11 to 20 of about 1,847 (170)
Terraced depressions in Lunar Maria [PDF]
Some shallow, irregularly shaped mare depressions are bordered by terraces. Morphologic study suggests that some of these depressions are drained lava lakes. If so, mare materials in which they occur originated as lava. Some associated sinuous rills and craters may have had volcanic origins.
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Special Thermophysical Features of Floor Materials in Mare Smythii Indicated by CE-2 CELMS Data
Mare Smythii is a special basin, which is one of the oldest mare basins with the considerably young mare basalts and the high density of floor-fractured craters.
Cai Liu +8 more
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The Variability of Lunar Mare Basalt Properties from Surface Rock Abundance
We use the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment surface rock abundance data set to investigate how rock content changes with surface age in the maria. We find that surface rock abundance decreases with unit age as expected for
Catherine M. Elder +7 more
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On the Possible Origin of the Lunar Maria [PDF]
RECENT close-up photographs of the lunar surface on the western shores of Oceanus Procellarum, televized back to Earth by the Russian soft-lander Luna 9 on February 4, revealed for the first time the detailed micro-structure of typical mare ground down to a cm–mm scale.
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Distribution characteristics of hydrogen elements on lunar surface based on CE2-GRS data
BackgroundWater is the primary resource required for the exploitation of lunar resources. Investigating the distribution of water on the surface of the moon has become a focal point in the lunar exploration plans of several nations.PurposeThis study aims
LI Yonghui +5 more
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Chronology of the Basalt Units Surrounding Chang’e-4 Landing Area
The Chang’e-4 (CE-4) lunar probe, the first soft landing spacecraft on the far side of the Moon, successfully landed in the Von Kármán crater on 3 January 2019. Geological studies of the landing area have been conducted and more intensive studies will be
Zongyu Yue +6 more
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Recent Tectonic Deformation of the Lunar Farside Mare and South Pole–Aitken Basin
The timing and scale of lunar tectonism provide a crucial insight into the geologic evolution of Earth’s Moon. Within the nearside lunar maria, wrinkle ridges formed during and after the emplacement of the mare basalts as a result of subsidence-induced ...
C. A. Nypaver +2 more
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Diverse Geological Evolution of Impact Basins on the Moon
Impact basins are the dominant landforms on the lunar surface, and their geological evolution varies. This research studied the diversity in the geological evolution of three impact basins: the Dirichlet–Jackson Basin, the Nectaris Basin, and the ...
Jiayin Deng, Weiming Cheng, Yimeng Jiao
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Abstract New data on the equine aortic valve obtained using advanced techniques is especially important given the greater availability of animal models for translational research. Here we characterized the morphological and morphometric aspects of the equine aortic valve from 60 healthy hearts collected at equine abattoirs.
Vitor Pires Pereira +3 more
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Abstract Macaws are renowned for processing dry, mechanically resistant fruits, yet the species‐level anatomical and functional correlates of this performance remain incompletely resolved. We examined the feeding apparatus of the Blue‐and‐yellow Macaw (Ara ararauna) using an integrated approach that combines osteology, myology, and bite‐force estimates
Sérgio R. Posso +2 more
wiley +1 more source

