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Three TIF files are provided that each have raster data for the Montes Apenninus region of the Moon. The images have been derived from the continuum-corrected and smoothed spectra following algorithms for glass band parameter, and 1 and 2 micron band depths. For these, we follow the methods of Horgan et al., 2014 and Bennett et al., 2016, see manuscript for details.
The original geologic maps of the Apennine-Hadley region (I-723) were published in 1971 as two map sheets (1:250,000 and 1:50,000) in a Transverse Mercator projection to support the Apollo 15 mission, the fourth crewed mission to land on the Moon (July 26 – August 7, 1971). These renovated versions of the 1:50k and 1:250k maps represent a best effort to capture and preserve the fidelity of the original mapping effort in an interactive digital format. These maps are not updated versions or reinterpretations of the original geologic maps which were based on Lunar Orbiter images, but spatial adjustments to a Lunar Reconnaissance Orbiter (LRO) Wide Angle Camera (WAC) basemap to make the maps more compatible with current...
Data for Journal article: Relationship between explosive and effusive volcanism in the Montes Apenninus region of the Moon in JGR: Planets
Categories: Data;
Tags: Lunar,
Planetary,
Planetary Sciences,
Pyroclastic,
USGS Science Data Catalog (SDC),
Geologic Map of the Descartes Region of the Moon, Apollo 16 Pre-Mission Map Renovation, 1:250k, 2022
The original geologic maps of the Descartes region (I-748) were published in 1972 as two map sheets (1:250,000 and 1:50,000) in a Transverse Mercator projection to support the Apollo 16 mission, the fifth crewed mission to land on the Moon (April 16 – 27, 1972). These renovated versions of the 1:50K and 1:250k maps represent a best effort to capture and preserve the fidelity of the original mapping effort in an interactive digital format. These maps are not updated versions or reinterpretations of the original geologic maps which were based on Lunar Orbiter images and Apollo 14 photography, but spatial adjustments to a Lunar Reconnaissance Orbiter (LRO) Wide Angle Camera (WAC) basemap to make the maps more compatible...
This file is a list of the wavelengths that are associated with the M3 bands, expressed in nanometers
The original geologic maps of the Taurus-Littrow region (I-800) were published in 1972 as two map sheets (1:250,000 and 1:50,000) in a Transverse Mercator projection to support the Apollo 17 mission, the sixth and final crewed mission to land on the Moon (December 7 – 19, 1972). These renovated versions of the 1:50k and 1:250k maps represent a best effort to capture and preserve the fidelity of the original mapping effort in an interactive digital format. These maps are not updated versions or reinterpretations of the original geologic maps which were based on Apollo 15 metric photographs, but spatial adjustments to a Lunar Reconnaissance Orbiter (LRO) Wide Angle Camera (WAC) basemap to make the maps more compatible...
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