Results 71 to 80 of about 813 (198)
Impact craters serve as recorders of lunar evolutionary history, and determining the stratigraphic ages of craters is crucial. However, the age of many craters on the Moon remains undetermined.
Ke Zhang +8 more
doaj +1 more source
X‐ray computed tomography study of terrestrial analog cores in preparation for Mars sample return
Abstract Mars Sample Return (MSR) is expected to transform planetary science by providing unprecedented access to pristine Martian material. Initial characterization in the sample receiving facility (SRF) will rely on nondestructive techniques such as X‐ray computed tomography (XCT) to document the condition, distribution, and internal features of ...
Sophie Benaroya +3 more
wiley +1 more source
Evaluating Lunar Crater Ejecta Maturation across Wavelengths
Ejecta blankets of young lunar craters provide an important window into the maturation processes of material at the lunar surface. As freshly exposed material degrades, the signature of that material changes in remote sensing data.
Angela M. Stickle +3 more
doaj +1 more source
Central peaks in lunar craters [PDF]
Central peak features in 580 craters on the lunar near side were systematically studied, and detailed studies were made of several features of interest, in an attempt to define the mechanism of central peak formation. The peaks tend to be elongated along the preferred directions of the lunar grid.
openaire +1 more source
The Challenge of Icy Sample Return Begins With Artemis
Abstract Throughout the Solar System, volatiles are found as solid ices. Returning ices to Earth for scientific analysis is critical to understanding the formation of a Solar System that bears life. This challenge begins with the Artemis missions to the lunar south polar region, where the coldest lunar regolith is enriched in H2O and other ices—systems
D. L. Gilbertson +7 more
wiley +1 more source
The regolith temperature of the Moon is strongly influenced by direct solar radiation and multiple-scattered thermal radiation from the surrounding terrains.
Zhen Yang +4 more
doaj +1 more source
The Moon’s surface, marked by craters, serves as a crucial record of the Solar System's impact history, offering key insights into planetary formation and evolution.
Mimansa Sinha, Sanchita Paul
doaj +1 more source
Freeze‐Thaw Cycling Accelerated Olivine Weathering and Water Sequestration on Icy Mars
Abstract Geological evidence and paleoclimate models suggest that freeze‐thaw (FT) cycling has played a pivotal role in shaping the Martian surface composition throughout geological time. Here we show the experimental investigation of the sulfuric acid weathering of olivine under simulated FT conditions (193–293 K).
Jing Liu +8 more
wiley +1 more source
SCCA-YOLO: Spatial Channel Fusion and Context-Aware YOLO for Lunar Crater Detection
Lunar crater detection plays a crucial role in geological analysis and the advancement of lunar exploration. Accurate identification of craters is also essential for constructing high-resolution topographic maps and supporting mission planning in future ...
Jiahao Tang +3 more
doaj +1 more source
Shock Metamorphism of Lunar Minerals
Impact events have played a crucial role in the formation and evolution of the Moon, as evidenced by the numerous of impact craters on its surface, indicating a long history spanning over 4 billion years characterized by numerous such occurrences. As the
Jianxi Zhu +6 more
doaj +1 more source

