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Titel: Farside explorer
Type: Journal articleJournal article
Person(er):
Forfatter:  Mimoun, David
Univ Toulouse, ISAE

Forfatter:  Wieczorek, Mark A.
Univ Paris Diderot, Inst Phys Globe Paris

Forfatter:  Alkalai, Leon
CALTECH, Jet Prop Lab.

Forfatter:  Banerdt, W. Bruce
CALTECH, Jet Prop Lab.

Forfatter:  Baratoux, David
CNRS, IRAP

Forfatter:  Bougeret, Jean-Louis
Observ Paris, CNRS

Forfatter:  Bouley, Sylvain
Observ Paris, Inst Mecan Celeste & Calcul Ephemerides

Forfatter:  Cecconi, Baptiste
Observ Paris, CNRS

Forfatter:  Falcke, Heino
MPIfR

Forfatter:  Flohrer, Joachim
German Aerosp Ctr DLR

Forfatter:  Garcia, Raphael F.
CNRS, IRAP

Forfatter:  Grimm, Robert
SW Res Inst, Boulder

Forfatter:  Grott, Matthias
German Aerosp Ctr DLR

Forfatter:  Gurvits, Leonid
Delft Univ Technol, Dept Astrodynam & Space Missions

Forfatter:  Jaumann, Ralf
German Aerosp Ctr DLR

Forfatter:  Johnson, Catherine L.
Planetary Sci Inst, Tucson

Forfatter:  Knapmeyer, Martin
German Aerosp Ctr DLR

Forfatter:  Kobayashi, Naoki
ISAS JAXA

Forfatter:  Konovalenko, Alexander
Inst Radio Astron

Forfatter:  Lawrence, David
Johns Hopkins Univ, Appl Phys Lab.

Forfatter:  Le Feuvre, Mathieu
Univ Nantes, Lab Planetol & Geodynam

Forfatter:  Lognonne, Philippe
Univ Paris Diderot, Inst Phys Globe Paris

Forfatter:  Neal, Clive
Univ Notre Dame, Notre Dame

Forfatter:  Oberst, Juergen
German Aerosp Ctr DLR

Forfatter:  Olsen, Nils (Cwisno: 38306)
Tech Univ Denmark, Copenhagen, Denmark
Email:

Forfatter:  Rottgering, Huub
Leiden Univ, Leiden Observ

Forfatter:  Spohn, Tilman
German Aerosp Ctr DLR

Forfatter:  Vennerstrøm, Susanne (Cwisno: 38320)
Technical University of Denmark
Email:

Forfatter:  Woan, Graham
Univ Glasgow, Sch Phys & Astron, Scotland

Forfatter:  Zarka, Philippe
Univ Paris Diderot, UPMC, CNRS, LESIA,Observ Paris
Uddrag: Farside Explorer is a proposed Cosmic Vision medium-size mission to the farside of the Moon consisting of two landers and an instrumented relay satellite. The farside of the Moon is a unique scientific platform in that it is shielded from terrestrial radio-frequency interference, it recorded the primary differentiation and evolution of the Moon, it can be continuously monitored from the Earth-Moon L2 Lagrange point, and there is a complete lack of reflected solar illumination from the Earth. Farside Explorer will exploit these properties and make the first radio-astronomy measurements from the most radio-quiet region of near-Earth space, determine the internal structure and thermal evolution of the Moon, from crust to core, and quantify impact hazards in near-Earth space by the measurement of flashes generated by impact events. The Farside Explorer flight system includes two identical solar-powered landers and a science/telecommunications relay satellite to be placed in a halo orbit about the Earth-Moon L2 Lagrange point. One lander would explore the largest and oldest recognized impact basin in the Solar System- the South Pole-Aitken basin-and the other would investigate the primordial highlands crust. Radio astronomy, geophysical, and geochemical instruments would be deployed on the surface, and the relay satellite would continuously monitor the surface for impact events.
Publiceret: in journal: Experimental Astronomy (ISSN: 0922-6435) (DOI: http://dx.doi.org/10.1007/s10686-011-9252-3), vol: 33, issue: 2-3, pages: 529-585, 2012
DOI:
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