![]() “Low resolution”, scientific layers and public domain image libraries). In order to make this new version available for those who do not have a high speed Internet connection to download it (8 GB with modules, textures, scientific layers, image libraries), or for those who wish to support our action, we are now editing an SD distribution card that installs the entire VMA version 7.0 (Command Center, ATLUN ©, PHOTLUN ©, DATLUN ©, WEBLUN ©, databases, “high resolution” textures, dynamic shadows directly on the PC. This documentation now also exists in PDF format. We have updated the illustrated documentation of the VMA with screenshots and photos in situation showing the new possibilities offered by this new version 7. Another big thank you to Luc for sharing his remarkable work! ![]() We have therefore produced what is becoming the largest of the VMA amateur image libraries containing 679 training images under different lighting. He gave us permission to build a “Best of Cathala” image library with his production. With a QHYSIII178M camera, he takes pictures sometimes reaching a resolution of 300 m. ![]() Luc Cathala is one of the best lunar imagers in France using a 625 mm diameter Dobsonian of personal production. Integration of the NELIOTA database produced by the National Observatory of Athens which identifies contemporary meteoritic impacts on behalf of ESA. These maps obviously only show the Visible Face of the Moon and there are sometimes significant differences in the position of the formations, although these are becoming more and more reduced with the last two proposed: You can now compare the work of these pioneers of lunar exploration with current data. We have collected and processed the best digitized versions of old lunar maps that have fallen into the public domain. We thank a lot David and the LPI for giving us the authorization tu use them in VMA.Īll these textures complement each other because the lighting conditions of each texture change, thus showing different details for each of the formations. Harrel (SD Mines) for the US Geologic Survey / Astrogeology Science Center in Flagstaff.ĭavid O’Brien of the Planetary Science Institute (PSI) has realized a texture with the “Lunar Astronautical Charts” (LAC) drawn on 1965 by the United States Air Force (USAF) and published by the Lunar and Planetary Institute. Put online last month, it is a color texture showing the different types of lunar terrain established from the results of several probes and produced by Corey M. The texture “USGS Unified Geological 2020” This particularly highlights the ejecta from recent craters. It is a black and white albedo texture, but the gray levels are reversed as in a photo negative. The initial texture only includes the zones between -60 ° and + 60 ° latitude and the polar zones have been reconstructed from other LRO data. It is not a photograph because it was established by computer from the altimetric data collected by the two probes to create a DEM (Digital Elevation Model). This texture has a variable resolution reaching 60 m / pixel in the best places. Mosaic of the original images of the Lunar Reconnaissance Orbiter (USA) and Kaguya (Japan) probes assembled from USGS data. The reconstructed texture “LOLA-Kaguya-Shaded” The one we are introducing today in the VMA corresponds to the highest resolution available to date. As full coverage at a given resolution progresses, Mark Robinson of Arizona State University and his LRO team publish new global maps of the Moon. Lunar Reconnaissance Orbiter, currently in lunar orbit, transmits images of the lunar surface reaching a resolution of 1 m. The level 6 “LRO / Lunar Reconnaissance Orbiter” photographic texture: Introduction of various translations of the VMA interface or of certain databases in German, Catalan, Croatian, Spanish, Greek, Dutch, Hungarian, Italian and Lithuanian, in addition to French and English.
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