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The Clementine mission —A 10-year perspective

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Abstract

Clementine was a technology demonstration mission jointly sponsored by the Department of Defense (DOD) and NASA that was launched on January 25th, 1994. Its principal objective was to use the Moon, a near-Earth asteroid, and the spacecraft’s Interstage Adapter as targets to demonstrate lightweight sensor performance and several innovative spacecraft systems and technologies. The design, development, and operation of the Clementine spacecraft and ground system was performed by the Naval Research Laboratory. For over two months Clementine mapped the Moon, producing the first multispectral global digital map of the Moon, the first global topographic map, and contributing several other important scientific discoveries, including the possibility of ice at the lunar South Pole. New experiments or schedule modifications were made with minimal constraints, maximizing science return, thus creating a new paradigm for mission operations. Clementine was the first mission known to conduct an in-flight autonomous operations experiment. After leaving the Moon, Clementine suffered an onboard failure that caused cancellation of the asteroid rendezvous. Despite this setback, NASA and the DOD applied the lessons learned from the Clementine mission to later missions. Clementine set the standard against which new small spacecraft missions are commonly measured. More than any other mission, Clementine has the most influence (scientifically, technically, and operationally) on the lunar missions being planned for the next decade.

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References

  • Bussey D B J, Spudis P D and Robinson M S 1999 Illu- mination Conditions at the Lunar South Pole;Geophys. Res. Lett. 26(9) 1187.

    Article  Google Scholar 

  • Bussey D B J, Robinson M R, Fristad K and Spudis P D 2004 Permanent Sunlight at the Lunar North Pole;Lunar Planet. Sci. XXXV CD-ROM 1387.

    Google Scholar 

  • Carraway J, Henry P, Herman M, Kissel G, Price H, Staehle R and Underwood M 1994 Lessons Learned from Clementine on the Way to Pluto; Proceedings of the AIAA/USU Conference on Small Satellites AIAA Washington DC.

  • COMPLEX (Committee on Planetary and Lunar Explo- ration; Space Studies Board; Commission on Physical Sci- ences Mathematics and Applications; National Research Council) 1997 Lessons Learned From The Clementine Mission;National Academy of Science, Washington DC. Duxbury T 1997 Personal Communication (July).

  • Feldman W C, Maurice S, Lawrence D J, Little R C, Lawson S L, Gasnault O, Wiens R C, Barraclough B L, Elphic R C, Prettyman T H, Steinberg J T and Binder A B 2001 Evidence for Water Ice Near the Lunar Poles;J. Geophys. Res. 106 E10 23,231–23,251.

    Article  Google Scholar 

  • Gillis J J and Spudis P D 2000 Geology of the Smythii and Marginis Region of the Moon Using Integrated Remotely Sensed Data;J. Geophys. Res. 105 E2 4217–4233.

    Article  Google Scholar 

  • Horan D M and Regeon P A 1995 Clementine - A Mission to the Moon and Beyond;1995 NRL Review, Naval Research Laboratory, Washington DC, pp. 45–57.

    Google Scholar 

  • Jolliff B L, Gillis J, Haskin L, Korotev R and Wieczorek M 2000 Major Lunar Crustal Terranes: Surface Expressions and Crust-Mantle Origins;J. Geophys. Res. 105 E2 4197–4216.

    Article  Google Scholar 

  • Kaufman B, Middour J and Richon K 1995 Mission Design of the Clementine Space Experiment; AAS Paper 95-124Spaceflight Mechanics 1995 Advances in the Astronautical Sciences 89(1) 407–422.

    Google Scholar 

  • Lucey P G, Spudis P D, Zuber M, Smith D and Malaret E 1994 Topographic-Compositional Units on the Moon and the Early Evolution of the Lunar Crust;Science 266 1855–1858.

    Article  Google Scholar 

  • Lucey P G, Taylor G J and Malaret E 1995 Abundance and Distribution of Iron on the Moon;Science 268 1150–1153.

    Article  Google Scholar 

  • Lucey P G, Taylor G J, Hawke B R and Spudis P D 1998 FeO and TiO2 Concentrations in the South Pole-Aitken Basin: Implications for Mantle Composition and Basin Formation;J. Geophys. Res. 103 E2 3701–3708.

    Article  Google Scholar 

  • Lucey P G, Blewett D and Jolliff B 2000 Lunar Iron and Titanium Abundance Algorithms Based on Final Processing of Clementine UV-Vis Images;J. Geophys. Res. 105 E8 20, 297–20, 305.

    Google Scholar 

  • Nozette Set al 1994 The Clementine Mission to the Moon: Scientific Overview;Science 266 1835–1839.

    Article  Google Scholar 

  • Nozette S, Lichtenburg C, Spudis P D, Bonner R, Ort W, Malaret E, Robinson M and Shoemaker E M 1996 The Clementine Bistatic Radar Experiment;Science 274 1495–1498.

    Article  Google Scholar 

  • Nozette S, Spudis P D, Robinson M, Bussey D B J, Lichtenberg C and Bonner R 2001 Integration of Lunar Polar Remote-Sensing Data Sets: Evidence for Ice at the Lunar South Pole;J. Geophys. Res. 106 E19 23,253–23,266.

    Article  Google Scholar 

  • NRC Space Studies Board 2003 New Frontiers in the Solar System: An Integrated Exploration Strategy; National Research Council, Washington DC, pp. 54–60.

    Google Scholar 

  • Pieters C M, Head J W, Gaddis L, Jolliff B and Duke M 2001 Rock Types of the South Pole-Aitken Basin and the Extent of Volcanism;J. Geophys. Res. 106 E11 28,001–28,022.

    Article  Google Scholar 

  • Rajmon D and Spudis P 2004 Distribution and Stratigra- phy of Basaltic Units in Maria Tranquillitatis and Fecun-ditatis: A Clementine Perspective;Meteor. Planet. Sci. 39(10) 1699–1720.

    Article  Google Scholar 

  • Regeon P A and Chapman R J 1994 CLEMENTINE: New Directions and Perspectives for One-of-a-Kind Spacecraft Missions; Proceedings of the AIAA/USU Conference on Small Satellites AIAA Washington DC.

  • Regeon P A, Chapman R J and Baugh R 1994 CLEMEN- TINE — The Deep Space Program Science Experiment, International Academy of Astronautics, Paper IAA-L- 0501 Low Cost Planetary Missions Conference, Laurel MD.

  • Robinson M S 2005 Clementine: A Scientific Summary;International Lunar Conference 6, Udaipur, India.

  • Robinson M S and Jolliff B 2002 Apollo 17 Landing Site: Topography Photometric Corrections and Heterogeneity of the Surrounding Highland Massifs;J. Geophys. Res. 107 E11 doi:101029/2001JE001614.

    Google Scholar 

  • Rustan Lt Col P L 1994 CLEMENTINE: An Experi- ment to Flight Qualify Lightweight Space Technologies;EOS Transactions American Geophysical Union 75(15) 161–165.

    Article  Google Scholar 

  • Shoemaker E 1995 Personal Communication (February).

  • Simpson R A and Tyler G L 1999 Reanalysis of Clementine Bistatic Radar Data from the Lunar South Pole;J. Geo-phys. Res. 104 E2 3845–3862.

    Article  Google Scholar 

  • Sorensen T C 1995 Global Mapping by the Clemen- tine Spacecraft; AAS Paper 95-127Spaceflight Mechan- ics 1995, Advances in the Astronautical Sciences 89(1) 457–476.

    Google Scholar 

  • Sorensen T Cet al 1995a Effective Science Mission Planning and Operations — TheClementine Approach Paper RALGS31 1st Annual Reducing the Cost of Space Ground Systems and Operations Symposium; Rutherford-Appleton Laboratories.

  • Sorensen T C, Oswald D C, Shook R M and Van Gaas- beck J 1995b Spacecraft Autonomous Operations Exper- iment Performed During the Clementine Lunar Mission;J. Spacecraft and Rockets 32(6) 1049–1053.

    Article  Google Scholar 

  • Spudis P D 1993The Geology of Multi-ring Basins: The Moon and Other Planets (New York and Cambridge: Cambridge University Press) 263 pp.

    Google Scholar 

  • Spudis P D, Reisse R A and Gillis J J 1994 Ancient Multi- Ring Basins on the Moon Revealed by Clementine Laser Altimetry;Science 266 1848–1851.

    Article  Google Scholar 

  • Spudis P D, Stockstill K R, Ockels W J and Kruiff M 1995 Physical Environment of the Lunar South Pole from Clementine Data: Implications for Future Exploration of the Moon;Lunar Planet. Sci. XXVI 1339–1340.

    Google Scholar 

  • Spudis P D, Bussey D B J, Lichtenberg C, Marinelli B and Nozette S 2005 Mini-SAR: An Imaging Radar for the Chandrayaan 1 Mission to the Moon;Lunar Planet. Sci. XXXVI CD ROM 1153.

    Google Scholar 

  • Stacy N J S, Campbell D B and Ford P G 1997 Arecibo Radar Mapping of the Lunar Poles: A Search for Ice Deposits;Science 276 1527–1530.

    Article  Google Scholar 

  • Stone E 2000 Personal Communication (November).

  • Wilhelms D E 1987 The Geologic History of the Moon; US Geol. Survey Prof. Paper 1347, 300 pp.

  • Wilson R 1994 Personal Communication (June).

  • Worden Col S P 1992 The Strategic Defense Initiative Organization CLEMENTINE Mission; Proceedings of the Near-Earth-Object Interception Workshop Jan 14–16 1992.

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Sorensen, T.C., Spudis, P.D. The Clementine mission —A 10-year perspective. J Earth Syst Sci 114, 645–668 (2005). https://doi.org/10.1007/BF02715950

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