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Clementine Project Information. Clementine was a joint project between the Strategic Defense Initiative Organization and NASA. The objective of the mission was to test sensors and spacecraft components under extended exposure to the space environment and to make scientific observations of the Moon and the near-Earth asteroid 1620 Geographos.
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Clementine (officially called the Deep Space Program Science Experiment (DSPSE)) was a joint space project between the Ballistic Missile Defense Organization (previously the Strategic Defense Initiative Organization) and NASA, launched on January 25, 1994.Its objective was to test sensors and spacecraft components in long-term exposure to space and to make scientific observations of both the.
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Clementine data offers compositional information of the upper microns of the lunar surface. The only way to get information about the deep crust is to have a drill core. Without a mission to return to the Moon and bring back drill cores, researchers must rely upon a natural means of excavation. Impact craters excavate rocks from the interior of.
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Mission Summary. Over the course of 71 days in orbit, Clementine systematically mapped the 38 million square kilometers of the Moon at eleven different wavelengths, from the ultraviolet (415 nm) to the near-infrared (2800 nm) parts of the spectrum (nearly 1,000,000 images). In addition, the spacecraft took 620,000 high-resolution CCD images and.
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Clementine: 1024x768x3: PIA18159: Clementine Fully Deployed (Artist's Concept). Clementine MESSENGER Mariner Venus Mercury (Mariner 10) 1248x624x1: PIA14823: The Whole of the Moon Full Resolution: TIFF (779.8 kB) JPEG (103.9 kB) Currently displaying images:.
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A lunar mosaic of 1,500 Clementine images of the south pole of the Moon. Credit: NASA. Clementine rose from Space Launch Complex 4 West at California's Vandenberg Air Force Base atop a Titan IIG.
Clementine Mission Images
Clementine Data. Scientists at the LPI are using data acquired by Clementine to answer important questions about the Moon. These questions include the global three-dimensional composition of the lunar crust, the possibility of ice at the south pole, the composition of mare basalts on the Moon's farside, and the chemical heterogeneity of the Apollo 16 landing site.
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As a secondary mission, Clementine would observe the Moon for two months using its multiple sensors, then leave lunar orbit and travel to 1620 Geographos, a 1.6-mile-long, elongated, stony asteroid. At a distance of 5.3 million miles from Earth, Clementine would fly within 62 miles of the near-Earth asteroid, returning images and data using its.
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Clementine image of the Moon. This image of the Moon, taken on March 21, 1994, is one of thousands captured by Clementine's UVVIS camera as part of its systematic mapping of the lunar surface. It shows an area centered at 67.15°S, 71.84°E at a resolution of 145 meters per pixel. The contrast has been increased slightly to bring out detail.
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Clementine Maps the Moon The Moon has long been a proving ground for spacecraft from its nearby planet. The latest to visit was Clementine, the "smaller, cheaper, faster" mission launched by the Ballistic Missile Defense Organization.Clementine completely mapped the surface of the Moon, and this mosaic was made from the data collected of the Aristarchus plateau.
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Clementine Iron Map of the Moon Image derived from the Clementine global color data (in 750 and 950 nm wavelengths) showing the concentration of iron in the soils of the lunar surface. Note high iron levels of near side maria and elevated iron associated with South Pole-Aitken basin on the far side. Very low iron of north-central far side.
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The Moon's south polar region in a mosaic of images made by the U.S. Clementine spacecraft from lunar orbit in 1994. The mosaic, which is centered on the south pole and combines the illumination received over more than two of the Moon's solar days (each about 29 Earth days), reveals the existence of appreciable permanently shadowed areas where water ice could exist.
Clementine Mission
The highly successful Clementine mission gave scientists their first global look at the Moon. Based on information gathered from this mission combined with data from recent missions, this unique atlas contains 144 maps covering the entire lunar surface, along with colour plates showing the Moon's composition and physical properties.
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The Clementine model, its interstage and solid rocket motor (bottom half) were discarded before insertion into lunar orbit. More than 500,000 people watched as Apollo 17, the last crewed mission.
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Abstract. In the course of 71 days in lunar orbit, from 19 February to 3 May 1994, the Clementine spacecraft acquired just under two million digital images of the moon at visible and infrared wavelengths. These data are enabling the global mapping of the rock types of the lunar crust and the first detailed investigation of the geology of the.
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Farside View of Earth's Moon as Seen by the Clementine Spacecraft. About 50,000 Clementine images were processed to produce the four orthographic views of the Moon. Images PIA00302, PIA00303, PIA00304, and PIA00305 show albedo variations (normalized brightness or reflectivity) of the surface at a wavelength of 750 nm (just longward of visible.