Farside explorer: Unique science from a mission to the farside of the moon

Farside Explorer is a proposed Cosmic Vision medium-size mission to the farside of theMoon 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 prim...

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Published in:Experimental Astronomy
Main Authors: Mimoun, D. (author), Wieczorek, M.A. (author), Gurvits, L. (author)
Format: Article in Journal/Newspaper
Language:English
Published: Springer-Verlag 2012
Subjects:
Online Access:https://doi.org/10.1007/s10686-011-9252-3
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spelling fttudelft:oai:tudelft.nl:uuid:ec0be8cd-acfe-4c30-b17a-95430a4ce057 2023-07-30T04:06:54+02:00 Farside explorer: Unique science from a mission to the farside of the moon Mimoun, D. (author) Wieczorek, M.A. (author) Gurvits, L. (author) 2012-04-01 https://doi.org/10.1007/s10686-011-9252-3 http://resolver.tudelft.nl/uuid:ec0be8cd-acfe-4c30-b17a-95430a4ce057 en eng Springer-Verlag Experimental Astronomy, 33(2-3)2012--1572-9508 http://link.springer.com/article/10.1007/s10686-011-9252-3 https://doi.org/10.1007/s10686-011-9252-3 http://resolver.tudelft.nl/uuid:ec0be8cd-acfe-4c30-b17a-95430a4ce057 (c)2012 The Authors and Springer moon Farside radio astronomy geophysics impact flux ESA's Cosmic Vision Program journal article Text 2012 fttudelft https://doi.org/10.1007/s10686-011-9252-3 2023-07-08T20:26:22Z Farside Explorer is a proposed Cosmic Vision medium-size mission to the farside of theMoon 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 solarpowered 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. Space Engineering Aerospace Engineering Article in Journal/Newspaper South pole Delft University of Technology: Institutional Repository Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) Lagrange ENVELOPE(-62.597,-62.597,-64.529,-64.529) South Pole Experimental Astronomy 33 2-3 529 585
institution Open Polar
collection Delft University of Technology: Institutional Repository
op_collection_id fttudelft
language English
topic moon
Farside
radio astronomy
geophysics
impact flux
ESA's Cosmic Vision Program
spellingShingle moon
Farside
radio astronomy
geophysics
impact flux
ESA's Cosmic Vision Program
Mimoun, D. (author)
Wieczorek, M.A. (author)
Gurvits, L. (author)
Farside explorer: Unique science from a mission to the farside of the moon
topic_facet moon
Farside
radio astronomy
geophysics
impact flux
ESA's Cosmic Vision Program
description Farside Explorer is a proposed Cosmic Vision medium-size mission to the farside of theMoon 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 solarpowered 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. Space Engineering Aerospace Engineering
format Article in Journal/Newspaper
author Mimoun, D. (author)
Wieczorek, M.A. (author)
Gurvits, L. (author)
author_facet Mimoun, D. (author)
Wieczorek, M.A. (author)
Gurvits, L. (author)
author_sort Mimoun, D. (author)
title Farside explorer: Unique science from a mission to the farside of the moon
title_short Farside explorer: Unique science from a mission to the farside of the moon
title_full Farside explorer: Unique science from a mission to the farside of the moon
title_fullStr Farside explorer: Unique science from a mission to the farside of the moon
title_full_unstemmed Farside explorer: Unique science from a mission to the farside of the moon
title_sort farside explorer: unique science from a mission to the farside of the moon
publisher Springer-Verlag
publishDate 2012
url https://doi.org/10.1007/s10686-011-9252-3
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long_lat ENVELOPE(-44.516,-44.516,-60.733,-60.733)
ENVELOPE(-62.597,-62.597,-64.529,-64.529)
geographic Aitken
Lagrange
South Pole
geographic_facet Aitken
Lagrange
South Pole
genre South pole
genre_facet South pole
op_relation Experimental Astronomy, 33(2-3)2012--1572-9508
http://link.springer.com/article/10.1007/s10686-011-9252-3
https://doi.org/10.1007/s10686-011-9252-3
http://resolver.tudelft.nl/uuid:ec0be8cd-acfe-4c30-b17a-95430a4ce057
op_rights (c)2012 The Authors and Springer
op_doi https://doi.org/10.1007/s10686-011-9252-3
container_title Experimental Astronomy
container_volume 33
container_issue 2-3
container_start_page 529
op_container_end_page 585
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