Results 101 to 110 of about 2,638 (227)
Comparisons of Mercury and the Moon [PDF]
Papers are presented outlining various comparisons of Mercury and the moon. Topics include the planetary magnetism and the interiors of the moon and Mercury, the relationship between crustal tectonics and internal evolution, global tectonics, the origin ...
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Global Distribution of Large Lunar Craters: Implications for Resurfacing and Impactor Populations
Lunar Reconnaissance The Lunar Reconnaissance Orbiter reached lunar orbit on 23 June 2009. Global data acquired since then now tell us about the impact history of the Moon and the igneous processes that shaped it.
James W. Head +6 more
core +1 more source
Lunar ejecta as the missing piece to resolving lunar cratering asymmetry
The leading-trailing asymmetry in lunar crater distribution provides a critical record of inner Solar System dynamics, yet the long-standing discrepancy between the observed higher asymmetry and lower theoretical predictions indicates a gap in our understanding of the impactor population.
Hailiang Li +2 more
openaire +2 more sources
Slope Map between Shackleton and de Gerlache Craters, Lunar South Pole
This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 10-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith
https://orcid.org/0000-0002-4964-1138 +13 more
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Planetary science : a lunar perspective [PDF]
An interpretative synthesis of current knowledge on the moon and the terrestrial planets is presented, emphasizing the impact of recent lunar research (using Apollo data and samples) on theories of planetary morphology and evolution.Stuart Ross TaylorThe
Taylor, Stuart Ross, 1925-
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Catalogue of lunar craters cross sections. I - Craters with peaks Research report no. 16
Lunar craters with centrally located peaks - tables and profile ...
Zack, W. H. +2 more
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China's Chang'e‐6 (CE‐6) mission has returned the first‐ever lunar farside samples from a mare plain on the southern Apollo basin floor. The crater statistics of the CE‐6 mare unit and the provenance of the samples are crucial in interpreting the CE‐6 ...
Luyuan Xu +5 more
doaj +1 more source
Impact Melt in Small Lunar Highlands Craters
Impact-melt deposits are a typical characteristic of complex impact craters, occurring as thick pools on the crater floor, ponds on wall terraces, veneers on the walls, and flows outside and inside the rim.
Barnouin, O. +4 more
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Two fundamental questions face lunar scientists: (1) What is the absolute age of each lunar impact basin and thus the early impact flux curve? (2) To what degree did basin impact melt seas undergo differentiation? We compiled a 1:200,000-scale geological
Kirby Runyon +7 more
doaj +1 more source

