In this study we use recent images and topographic data to map the geology and geomorphology of the lunar South Pole quadrangle (LQ-30) at 1:2.5M scale [1-4] in accordance with the Lunar Geologic Mapping Program. Mapping of LQ-30 began during Mest's postdoctoral appointment and has continued under the PG&G Program, from which funding became available in February 2009. Preliminary map-ping and analyses have been done using base materials compiled by Mest, but properly mosaicked and spatially registered base materials are being compiled by the USGS and should be received by the end of June 2009. The overall objective of this research is to constrain the geologic evolution of the lunar South Pole (LQ-30: 60deg -90deg S, 0deg - +/-180deg ) with...
During the Earth-Moon flyby the Galileo Solid State Imaging System obtained new information on the l...
Apollo basin (10°–60°S, 125°–175°W, 492 km diameter) lies within the northeastern edge of the ~2500 ...
We analyze Clementine altimetry to constrain the size and location of proposed permanently shadowed ...
In this study we use recent image, spectral and topographic data to map the geology of the lunar Sou...
Data from recent lunar orbital missions have provided critical insight into the surface composition,...
The first systematic lunar geologic maps were completed at 1:1M scale for the lunar near side during...
The Moon's South Pole-Aitken basin (SPA) is a high priority target for Solar System exploration, and...
The authors seek to construct a 1:2,500,000-scale map of Lunar Quadrangle 10 (LQ10 or the Marius Qua...
Modern high-resolution remote sensing datasets for the Moon provide a detailed view of the lunar sur...
During the December 1992 Galileo Earth/Moon encounter the northern half of the nearside, the eastern...
Aitken Basin region that we have probed with Lunar Reconnaissance Orbiter, Moon Mineralogy Mapper 20...
Mineralogy of South Pole-Aitken Basin (SPA) (the largest confirmed impact basin on the Moon) is eval...
Abstract The Schrödinger basin on the south polar lunar far side has been highlighted as a ...
The Schrödinger basin on the south polar lunar far side has been highlighted as a promising target f...
The South Pole-Aitken (SPA) basin, located on the lunar far side, is one of the oldest and largest r...
During the Earth-Moon flyby the Galileo Solid State Imaging System obtained new information on the l...
Apollo basin (10°–60°S, 125°–175°W, 492 km diameter) lies within the northeastern edge of the ~2500 ...
We analyze Clementine altimetry to constrain the size and location of proposed permanently shadowed ...
In this study we use recent image, spectral and topographic data to map the geology of the lunar Sou...
Data from recent lunar orbital missions have provided critical insight into the surface composition,...
The first systematic lunar geologic maps were completed at 1:1M scale for the lunar near side during...
The Moon's South Pole-Aitken basin (SPA) is a high priority target for Solar System exploration, and...
The authors seek to construct a 1:2,500,000-scale map of Lunar Quadrangle 10 (LQ10 or the Marius Qua...
Modern high-resolution remote sensing datasets for the Moon provide a detailed view of the lunar sur...
During the December 1992 Galileo Earth/Moon encounter the northern half of the nearside, the eastern...
Aitken Basin region that we have probed with Lunar Reconnaissance Orbiter, Moon Mineralogy Mapper 20...
Mineralogy of South Pole-Aitken Basin (SPA) (the largest confirmed impact basin on the Moon) is eval...
Abstract The Schrödinger basin on the south polar lunar far side has been highlighted as a ...
The Schrödinger basin on the south polar lunar far side has been highlighted as a promising target f...
The South Pole-Aitken (SPA) basin, located on the lunar far side, is one of the oldest and largest r...
During the Earth-Moon flyby the Galileo Solid State Imaging System obtained new information on the l...
Apollo basin (10°–60°S, 125°–175°W, 492 km diameter) lies within the northeastern edge of the ~2500 ...
We analyze Clementine altimetry to constrain the size and location of proposed permanently shadowed ...