IAU Colloquium 168
Cometary Nuclei in Space and Time
Nanjing,
China
May 18-22, 1998
Electronically-submitted Abstracts of Participants
THE IN-SITU ANALYSIS OF WIRTANEN NUCLEUS BY THE ROSETTA LANDER PAYLOAD
J-P. Bibring (1), H-U. Auster (2), W. Kofman (3), D. Mühlmann (4), S.
Mottola (5), C. Pillinger (6), R. Rieder (7), H. Rosenbauer (8), T. Spohn
(9)
(1) IAS, Institut d'Astrophysique Spatiale, 91405 Orsay Campus,
France, (2) MPI für EP, Berlin, (3)
CEPHAG, Grenoble, (4) DLR, Köln, (5) DLR, Berlin,
(6) Open University, Milton Keynes, (7) MPI für Chemie, Mainz,
(8) MPIA, Lindau, (9) Inst. für Planet., Münster
The Rosetta Lander is designed to land a payload of about 20 kg on the
nucleus of comet Wirtanen in 2012 at 3 AU from the Sun, to perform a highly
complex and integrated program of measurements immediately after landing,
then following the comet evolution as it will approach perihelion. 9 sets
of instruments are dedicated to analyse the elemental, isotopic, molecular
& mineralogical composition of surface and sub-surface samples, to image
the drilled samples and the landing site, to characterize the physical
properties of the surface material, to measure the plasma around the comet
and to sound its interior. The Lander and its payload are developped as an
integrated international venture.
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