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Shape, density, and geology of the nucleus of Comet 103P/Hartley 2

Authors :
Thomas, P.C.
A’Hearn, Michael F.
Veverka, Joseph
Belton, Michael J.S.
Kissel, Jochen
Klaasen, Kenneth P.
McFadden, Lucy A.
Melosh, H. Jay
Schultz, Peter H.
Besse, Sébastien
Carcich, Brian T.
Farnham, Tony L.
Groussin, Olivier
Hermalyn, Brendan
Li, Jian-Yang
Lindler, Don J.
Lisse, Carey M.
Meech, Karen
Richardson, James E.
Source :
ICARUS. Feb2013, Vol. 222 Issue 2, p550-558. 9p.
Publication Year :
2013

Abstract

Abstract: Data from the Extrasolar Planet Observation and Deep Impact Extended Investigation (EPOXI) mission show Comet 103P/Hartley 2 is a bi-lobed, elongated, nearly axially symmetric comet 2.33km in length. Surface features are primarily small mounds <40m across, irregularly-shaped smooth areas on the two lobes, and a smooth but variegated region forming a “waist” between the two lobes. Assuming parts of the comet body approach the shape of an equipotential surface, the mean density of Hartley 2 is modeled to be 200–400kgm−3. Such a mean density suggests mass loss per orbit of >1%. The shape may be the evolutionary product of insolation, sublimation, and temporary deposition of materials controlled by the object’s complex rotation. [Copyright &y& Elsevier]

Details

Language :
English
ISSN :
00191035
Volume :
222
Issue :
2
Database :
Academic Search Index
Journal :
ICARUS
Publication Type :
Academic Journal
Accession number :
85405361
Full Text :
https://doi.org/10.1016/j.icarus.2012.05.034