MIDAS – The Micro-Imaging Dust Analysis System for the Rosetta Mission

被引：0
|
作者：
W. Riedler
K. Torkar
H. Jeszenszky
J. Romstedt
H. St. C. Alleyne
H. Arends
W. Barth
J. V. D. Biezen
B. Butler
P. Ehrenfreund
M. Fehringer
G. Fremuth
J. Gavira
O. Havnes
E. K. Jessberger
R. Kassing
W. Klöck
C. Koeberl
A. C. Levasseur-Regourd
M. Maurette
F. Rüdenauer
R. Schmidt
G. Stangl
M. Steller
I. Weber
机构：
[1] Österreichische Akademie der Wissenschaften,Institut für Weltraumforschung
[2] Science Directorate,Institut für Technische Physik
[3] ESA/ESTEC,Institut für Planetologie
[4] ARC Seibersdorf Research GmbH,Auroral Observatory
[5] Universität Gesamthochschule Kassel,Center for Earth Sciences
[6] Westfälische Wilhelms-Universität Münster,Institut für Sensor
[7] Sterrewacht Leiden, und Aktuatorsysteme
[8] Université Paris 6/Aéronomie CNRS,undefined
[9] Astrophysique du Solide,undefined
[10] C.S.N.S.M.,undefined
[11] University of Tromsø,undefined
[12] Röntgenanalytik Messtechnik GmbH,undefined
[13] Universität Wien,undefined
[14] University of Sheffield,undefined
[15] Technische Universität Wien,undefined
来源：
Space Science Reviews | 2007年 / 128卷
关键词：
Rosetta; atomic force microscope; comet; coma; dust; 67P/Churyumov-Gerasimenko;
D O I：
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中图分类号：
学科分类号：
摘要：
The International Rosetta Mission is set for a rendezvous with Comet 67 P/Churyumov-Gerasimenko in 2014. On its 10 year journey to the comet, the spacecraft will also perform a fly-by of the two asteroids Stein and Lutetia in 2008 and 2010, respectively. The mission goal is to study the origin of comets, the relationship between cometary and interstellar material and its implications with regard to the origin of the Solar System. Measurements will be performed that shed light into the development of cometary activity and the processes in the surface layer of the nucleus and the inner coma.
引用
收藏
页码：869 / 904
页数：35
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