Pyroclastic Deposits in Floor-Fractured Craters: A Unique Style or Lunar Basaltic Volcanism?
The lunar maria were formed by effusive fissure flows of low-viscosity basalt. Regional pyroclastic deposits were formed by deep-sourced fire-fountain eruptions dominated by basaltic glass.
Pieters, Carle M. +7 more
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Is the Moon\u27s Orbit Ringing from an Asteroid Collision Event which Triggered the Flood?
We use ordinary Newtonian orbital mechanics to explore the possibility that near side lunar maria are giant impact basins left over from a catastrophic impact event that caused the present orbital configuration of the moon.
Samec, Ronald G.
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Special Thermophysical Features of Floor Materials in Mare Smythii Indicated by CE-2 CELMS Data
Mare Smythii is a special basin, which is one of the oldest mare basins with the considerably young mare basalts and the high density of floor-fractured craters.
Cai Z. +8 more
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Lunar Advanced Radar Orbiter for Subsurface Sounding (LAROSS): Lava Tube Exploration mission
With the goal of expanding human presence beyond Earth, sub-surface empty lava tubes on other worlds form ideal candidates for creating a permanent habitation environment safe from cosmic radiation, microm-eteorite impacts and temperature extremes.
Howell, Kathleen +2 more
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Lunar maria and related deposits: Preliminary Galileo imaging results
During the Earth-Moon flyby the Galileo Solid State Imaging system obtained new information on lunar media. Imaging data in spectral bands from 0.4 to 1.0 micron wavelength provide color data for deposits on the western limb.
Belton, M. +9 more
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Remote Compositional Analyses of Space-Weathered Lunar Maria
This repository is for the paper "Remote Compositional Analyses of Space-Weathered Lunar Maria" by Jung, Lapotre, Milliken, and Minson. It is associated with the manuscript number AAS63572.Space-WeatheringThis repository provides a space weathering correction based on Hapke-based spectral unmixing framework.
Jung, Ji In +2 more
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THE ORIGIN OF CERTAIN CLASSES OF LUNAR MARIA RIDGES
Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items ...
Cruikshank, Dale P. +2 more
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Long-wavelength Radar Studies of the Lunar Maria
Radar measurements at 70 cm and 7.5 m wavelengths provide insight into the structure and chemical properties of the upper 5-100 m of the lunar regolith and crust.
Thompson, Thomas W. +2 more
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On the depths and shapes of the freshest kilometer-scale simple craters on the lunar maria: A new crater shape model. [PDF]
Chappelow JE.
europepmc +1 more source
Geology of the Apollo 17 landing site [PDF]
The topics covered include the following: petrology, lithology, lunar rocks, lunar soil, geochemistry, lunar geology, lunar resources, oxygen production, ilmenite, volcanism, highlands, lunar maria, massifs, impact melts, breccias, lunar crust, Taurus ...
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