4.5 Article

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

Journal

ICARUS
Volume 222, Issue 2, Pages 550-558

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2012.05.034

Keywords

Comets; Comets, Nucleus; Geological processes; Geophysics

Funding

  1. NASA [NNM07AA99C]
  2. New Frontiers Program Office

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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 2.33 km in length. Surface features are primarily small mounds <40 m 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 200-400 kg m(-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. (C) 2012 Elsevier Inc. All rights reserved.

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