Results 61 to 70 of about 2,638 (227)
Impact provenance and age of a unique basalt found in Apollo 12 regolith
Abstract Basaltic sample 12032,366‐18 from the Apollo 12 landing site is distinct among basalts collected at this site, other Apollo landing sites, and lunar meteorites in terms of its age, bulk rock composition, and isotopic composition. We present new Pb isotopic data obtained by in situ Secondary Ion Mass Spectrometry on multiple mineral phases in ...
C. Deligny +5 more
wiley +1 more source
It is extremely difficult to collect deep lunar soil samples during lunar exploration, as the average thickness of lunar soils is very large, and the power of lunar soil sampling systems is inherently limited.
Xuyan Hou +6 more
doaj +1 more source
A New Global Catalog LU1319381 of Lunar Craters (≥1 km)
The new global catalog LU1319381 includes approximately 1.32 million lunar craters, which extends the existing global catalogs to craters with diameters of 1 km or larger and is enriched with 3D morphological information on the ...
Bo Wu, Yiran Wang
core +1 more source
Super‐Resolution of Planetary Images Based on Generative Adversarial Network
Abstract Currently, satellite imagery serves as the primary means of observing terrestrial planets such as the Mars, the Moon, and Mercury. Enhancing the resolution and quality of these images can provide more detailed insights into planetary surfaces. However, improvements in image quality are often limited by the constraints of sensor technology and ...
Xiaoran Zhang, Yiran Wang, Miao Zhuo
wiley +1 more source
Lunar Polar Volatile Remobilization in Regolith-Filled Craters
Jupyter Notebooks modeling volatile stability in lunar polar cold trap craters. The hypothesis is that volatiles in cold lunar regolith may experience temperature-dependent slow mobility.THIS DATASET IS ARCHIVED AT DANS/EASY, BUT NOT ACCESSIBLE HERE.
Danque, H (via Mendeley Data)
core +2 more sources
Automated Mineral Identification and Rock‐Type Classification of Lunar Mare Basalts Using SEM Images
Abstract We present an automated system for identifying minerals and classifying rock types in Apollo lunar mare basalts using scanning electron microscopy (SEM) imagery. Mineral segmentation is based on a U‐Net architecture, supplemented by two scale‐aware models designed to incorporate pixel size information.
Ji‐In Jung +3 more
wiley +1 more source
Alteration of a Mantle‐Derived Dunite Boulder in Jezero Crater, Mars
Abstract In 2023, the Mars 2020 Perseverance rover explored the youngest preserved deposits on the Western fan of Jezero crater, Mars: a field of meter‐scale boulders dispersed above the previously explored sandstone and siltstone units. Reflectance spectra of the boulders delineated two classes, one olivine‐bearing and one pyroxene‐bearing.
E. L. Moreland +10 more
wiley +1 more source
Astronaut's guide to terrestrial impact craters [PDF]
Impact cratering of the Earth's surface is discussed and compared with lunar craters. Known craters on earth are ordered by location and a few principal facts are given for each crater and the general terrain in which it is located.
core
Surface Geology and Evolution of Asteroid Ryugu: Insights From Hayabusa2 Global Mapping
Abstract Rubble‐pile asteroids, characterized by loose aggregates of debris held together by gravity, represent both a significant planetary hazard and a key to understanding planetesimal formation. Geologic mapping of these bodies provides essential insights into their origins, evolution, and surface processes.
Lisa M. Vincent +8 more
wiley +1 more source
Abstract The Taruntius crater, situated between Maria Fecunditatis, Crisium, and Tranquillitatis, is characterized by a prominent bright ray system and a floor‐fractured morphology and has long been interpreted as a relatively young Eratosthenian or Copernican crater.
Longjiao Yu +3 more
wiley +1 more source

