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