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EnVision: taking the pulse of our twin planet.

Authors :
Ghail, Richard
Wilson, Colin
Galand, Marina
Hall, David
Cochrane, Chris
Mason, Philippa
Helbert, Joern
MontMessin, Franck
Limaye, Sanjay
Patel, Manish
Bowles, Neil
Stam, Daphne
Wahlund, Jan-Erik
Rocca, Fabio
Waltham, David
Mather, Tamsin
Biggs, Juliet
Genge, Matthew
Paillou, Philippe
Mitchell, Karl
Source :
Experimental Astronomy; Apr2012, Vol. 33 Issue 2/3, p337-363, 27p
Publication Year :
2012

Abstract

EnVision is an ambitious but low-risk response to ESA's call for a medium-size mission opportunity for a launch in 2022. Venus is the planet most similar to Earth in mass, bulk properties and orbital distance, but has evolved to become extremely hostile to life. EnVision's 5-year mission objectives are to determine the nature of and rate of change caused by geological and atmospheric processes, to distinguish between competing theories about its evolution and to help predict the habitability of extrasolar planets. Three instrument suites will address specific surface, atmosphere and ionosphere science goals. The Surface Science Suite consists of a 2.2 m radar antenna with Interferometer, Radiometer and Altimeter operating modes, supported by a complementary IR surface emissivity mapper and an advanced accelerometer for orbit control and gravity mapping. This suite will determine topographic changes caused by volcanic, tectonic and atmospheric processes at rates as low as 1 mm a. The Atmosphere Science Suite consists of a Doppler LIDAR for cloud top altitude, wind speed and mesospheric structure mapping, complemented by IR and UV spectrometers and a spectrophotopolarimeter, all designed to map the dynamic features and compositions of the clouds and middle atmosphere to identify the effects of volcanic and solar processes. The Ionosphere Science Suite uses a double Langmiur probe and vector magnetometer to understand the behaviour and long-term evolution of the ionosphere and induced magnetosphere. The suite also includes an interplanetary particle analyser to determine the delivery rate of water and other components to the atmosphere. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
09226435
Volume :
33
Issue :
2/3
Database :
Complementary Index
Journal :
Experimental Astronomy
Publication Type :
Academic Journal
Accession number :
74550759
Full Text :
https://doi.org/10.1007/s10686-011-9244-3