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Lunar science for landed missions workshop findings report
Abstract The Lunar Science for Landed Missions workshop was convened at the National
Aeronautics and Space Administration Ames Research Center on 10–12 January, 2018 …
Aeronautics and Space Administration Ames Research Center on 10–12 January, 2018 …
Lunar irregular Mare patches: Classification, characteristics, geologic settings, updated catalog, origin, and outstanding questions
One of the most mysterious lunar features discovered during the Apollo era was Ina, a~ 2× 3‐
km depression composed of bleb‐like mounds surrounded by hummocky and blocky …
km depression composed of bleb‐like mounds surrounded by hummocky and blocky …
Ina pit crater on the Moon: Extrusion of waning-stage lava lake magmatic foam results in extremely young crater retention ages
The enigmatic Ina feature on the Moon was recently interpreted to represent extrusive
basaltic volcanic activity within the past 100 my of lunar history, an extremely young age for …
basaltic volcanic activity within the past 100 my of lunar history, an extremely young age for …
Constraining formation hypotheses for irregular mare patches on the Moon with orbital reflectance spectra
Irregular mare patches (IMPs) are enigmatic volcanic features on the Moon's surface, whose
lack of cratering and crisp appearance imply they formed< 100 Ma ago,∼ 1 Ga after the …
lack of cratering and crisp appearance imply they formed< 100 Ma ago,∼ 1 Ga after the …
The role of substrate characteristics in producing anomalously young crater retention ages in volcanic deposits on the Moon: Morphology, topography, subresolution …
Lunar irregular mare patches (IMP s) comprise dozens of small, distinctive, and enigmatic
lunar mare features. Characterized by their irregular shapes, well‐preserved state of relief …
lunar mare features. Characterized by their irregular shapes, well‐preserved state of relief …
The lunar mare ring‐moat dome structure (RMDS) age conundrum: Contemporaneous with Imbrian‐aged host lava flows or emplaced in the Copernican?
F Zhang, JW Head, C Wöhler… - Journal of …, 2021 - Wiley Online Library
Ring‐moat dome structures (RMDSs) are small circular mounds of diameter typically about
200 m and∼ 3–4 m in height, surrounded by narrow, shallow moats. They occur in clusters …
200 m and∼ 3–4 m in height, surrounded by narrow, shallow moats. They occur in clusters …
Geological characterization of the Ina shield volcano summit pit crater on the Moon: Evidence for extrusion of waning‐stage lava lake magmatic foams and …
Abstract Ina, a distinctive~ 2× 3 km D‐shaped depression, is composed of unusual bulbous‐
shaped mounds surrounded by optically immature hummocky/blocky floor units. The crisp …
shaped mounds surrounded by optically immature hummocky/blocky floor units. The crisp …
Thermophysical properties of lunar irregular mare patches from LRO diviner radiometer data
Irregular mare patches (IMPs) are enigmatic features in the lunar maria that are
characterized as having smooth mounds surrounded by uneven or blocky terrain. The IMPs …
characterized as having smooth mounds surrounded by uneven or blocky terrain. The IMPs …
The Cauchy 5 small, low‐volume lunar shield volcano: Evidence for volatile exsolution‐eruption patterns and type 1/type 2 hybrid irregular mare patch formation
The lunar shield volcano Cauchy 5, sitting at the low diameter‐height‐volume end of the
population, is the only known example containing two different types of Irregular Mare …
population, is the only known example containing two different types of Irregular Mare …
Lunar Crater Ina: Analysis of the morphology of intracrater landforms
AT Basilevsky, GG Michael - Solar System Research, 2021 - Springer
We present the results of geological and morphological analysis of LROC NAC images of a
small volcanic crater Ina, D-shaped in plan view (2.9× 1.9 km), and its immediate …
small volcanic crater Ina, D-shaped in plan view (2.9× 1.9 km), and its immediate …