The Clementine mission is the result of those early investigations. A mission was conceived to test the latest in space-based imaging components, using the moon and a near-earth asteroid as celestial targets. That request was given to the then Strategic Defense Initiative Organization (SDIO) to investigate. The Clementine story began in 1990 when NASA administrator Richard Truly asked the Department of Defense to consider a joint NASA/DOD mission that would achieve goals mutually beneficial to both organizations. Copyright 2011 by the American Geophysical Union. Absorption band minimums are difficult to compare due to the significantly different spectral resolutions. The 1 m absorption band depths may be comparable between the instruments, but Clementine data consistently exhibit shallower 2 m band depths than M 3. M3 spectra show the Moon to be redder, that is, have a steeper continuum slope, than indicated by Clementine. We have found that M3 reflectance values are lower across all wavelengths compared with albedos from both of Clementine's UV-VIS and NIR cameras. The Clementine mission provided the first global multispectral maps the lunar surface in 11 spectral bands across the UV-VIS and NIR. In an effort to understand how M3 improves our ability to analyze and interpret lunar data, we compare M3 spectra with those from Clementine's UV-VIS and NIR cameras. The Clementine mission provided the first global multispectral maps the lunar surface in 11 spectral bands across the ultraviolet-visible (UV-VIS) and near-infrared (NIR). The Moon Mineralogy Mapper (M3) provided the first global hyperspectral data of the lunar surface in 85 bands from 460 to 2980 nm. Newer views of the Moon: Comparing spectra from Clementine and the Moon Mineralogy Mapper About 500 images from NASA's Clementine spacecraft were processed and combined into a multispectral mosaic of this region. The Aristarchus region is one of the most diverse and interesting areas on the Moon. Multispectral Mosaic of the Aristarchus Crater and Plateau Concepts for two such efforts are described: glogal multispectral imaging of the moon and videos of Geographos. Effective scientific analyses of such large datasets require systematic processing efforts. If fully successful, the Clementine mission will return about 3,000,000 lunar images and more than 5000 images of Geographos. Systematic Processing of Clementine Data for Scientific Analyses The two views of southeastern Africa were acquired by the UVVIS camera while Clementine was in low Earth orbit early in the mission. The top right image shows the Earth as viewed by the UVVIS camera while Clementine was in transit to the Moon swirling white cloud patterns indicate storms. The Earth actually appeared about twice as far above the lunar horizon as shown. The image on the left shows the Earth as seen across the lunar north pole the large crater in the foreground is Plaskett. This collection of UVVIS camera Clementine images shows the Earth from the Moon and 3 images of the Earth. The two views of southeastern Africa were acquired by the UVVIS camera while Clementine was in low Earth orbit early in the missionĭuring its flight and lunar orbit, NASA’s Clementine spacecraft returned images of the planet Earth and the Moon. During its flight and lunar orbit, the Clementine spacecraft returned images of the planet Earth and the Moon.
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