Fundamental physics and absolute positioning metrology with the MAGIA lunar orbiter

被引:0
|
作者
Simone Dell’Agnello
Caterina Lops
Giovanni O. Delle Monache
Douglas G. Currie
Manuele Martini
Roberto Vittori
Angioletta Coradini
Cesare Dionisio
Marco Garattini
Alessandro Boni
Claudio Cantone
Riccardo March
Giovanni Bellettini
Roberto Tauraso
Mauro Maiello
Luca Porcelli
Simone Berardi
Nicola Intaglietta
机构
[1] INFN—Laboratori Nazionali di Frascati (LNF),Department of Physics
[2] University of Maryland (UMD),INFN—LNF and Department of Mathematics
[3] Aeronautica Militare Italiana,undefined
[4] INAF—Istituto di Fisica dello Spazio Interplanetario (IFSI),undefined
[5] Rheinmetall Italia S.p.A.,undefined
[6] INFN—LNF and CNR-Istituto per le Applicazioni del Calcolo (IAC),undefined
[7] University of Rome “Tor Vergata”,undefined
来源
Experimental Astronomy | 2011年 / 32卷
关键词
LLR; SLR; Gravitational redshift; Lunar science; ILN; Tests of general relativity;
D O I
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中图分类号
学科分类号
摘要
MAGIA is a mission approved by the Italian Space Agency (ASI) for Phase A study. Using a single large-diameter laser retroreflector, a large laser retroreflector array and an atomic clock onboard MAGIA we propose to perform several fundamental physics and absolute positioning metrology experiments: VESPUCCI, an improved test of the gravitational redshift in the Earth–Moon system predicted by General Relativity; MoonLIGHT-P, a precursor test of a second generation Lunar Laser Ranging (LLR) payload for precision gravity and lunar science measurements under development for NASA, ASI and robotic missions of the proposed International Lunar Network (ILN); Selenocenter (the center of mass of the Moon), the determination of the position of the Moon center of mass with respect to the International Terrestrial Reference Frame/System (ITRF/ITRS); this will be compared to the one from Apollo and Lunokhod retroreflectors on the surface; MapRef, the absolute referencing of MAGIA’s lunar altimetry, gravity and geochemical maps with respect to the ITRF/ITRS. The absolute positioning of MAGIA will be achieved thanks to: (1) the laboratory characterization of the retroreflector performance at INFN-LNF; (2) the precision tracking by the International Laser Ranging Service (ILRS), which gives two fundamental contributions to the ITRF/ITRS, i.e. the metrological definition of the geocenter (the Earth center of mass) and of the scale of length; (3) the radio science and accelerometer payloads; (4) support by the ASI Space Geodesy Center in Matera, Italy. Future ILN geodetic nodes equipped with MoonLIGHT and the Apollo/Lunokhod retroreflectors will become the first realization of the International Moon Reference Frame (IMRF), the lunar analog of the ITRF.
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页码:19 / 35
页数:16
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