Results 81 to 90 of about 674 (209)
Effect of Lunar Rotation on Antipodal Ejecta Deposition
Abstract The Moon's crust exhibits strong magnetic anomalies that likely record ancient magnetic fields produced by a core dynamo. Lunar materials have low magnetic susceptibility, but impactor material with high susceptibility may record the Moon's ancient dynamo. Some magnetic anomalies are antipodal to lunar basins and it is hypothesized that impact
S. Wakita, B. C. Johnson
wiley +1 more source
Abstract Lava tubes are subsurface volcanic conduits formed during effusive basaltic eruptions and are considered key targets for planetary exploration. Orbital remote sensing on the Moon and Mars has identified numerous collapse pits interpreted as possible surface expressions of underlying lava tube systems. However, the limited resolution of current
A. Ghirotto +8 more
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Lunar meteorites provide access to a geographically unconstrained record of the Moon, offering key insights into crustal diversity and interior evolution beyond the Apollo and Luna landing sites.
Andrew Alberini +11 more
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Emplacement of Venus' Crater Outflows as Impact Melt
Abstract Some of Venus' impact craters are associated with flow features that extend up to hundreds of kilometers from the crater rim, making these flows the longest crater outflows in the solar system. Various mechanisms of formation have been proposed including two end‐member hypotheses (the vapor cloud origin and the impact melt origin).
M. Borrelli, I. Ganesh, L. Bourg
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An Integrated Framework for Global Detection and Quantification of Lunar Pyroclastic Deposits
Lunar pyroclastic deposits (LPDs) composed of Fe–Ti-bearing volcanic glasses are considered one of the best proxies to understand the primitive lunar mantle composition.
Dibyendu Misra +3 more
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Lunar south polar regions have attracted considerable scientific interest due to their potential for preservation of water ice and unique mineralogical compositions.
Rui Ni +5 more
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Abstract The lunar surface charging is controlled mainly by the balance of electron currents near the surface. One of the main electron currents is the photocurrent on the dayside, comprised of photoelectrons produced by solar photons ionizing the lunar surface.
Shaosui Xu +3 more
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Magnetic Mineralogy in Lunar Mare Basalts and Implications for Paleointensity Retrieval
Abstract Lunar paleomagnetic studies have identified multidomain metallic Fe–Ni alloys as the dominant magnetic contributors in mare basalts. Here, we explore the low‐temperature magnetic behavior of standard samples for a suite of opaque minerals that occur within mare basalts (single‐domain and multidomain Fe, wüstite, ulvöspinel ...
Ji‐In Jung +6 more
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Abstract The cause of the observed mare basalt asymmetry between the lunar nearside and farside remains a long‐lasting conundrum. In this study, we characterized the petrology and geochemistry of the Chang'e‐6 low‐Ti basalts from the lunar farside, performed petrological modeling of major elements and conducted Monte Carlo simulation of trace elements,
Ziqing Li +7 more
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Abstract Silicate melt viscosity plays a pivotal role in the evolution of rocky bodies within the Solar System, exerting first‐order control on mantle differentiation and stratification, while dictating the metal‐silicate separation and the subsequent volcanic activity.
Fabrizio Di Fiore, Michele Cassetta
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