• Title of article

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

  • Author/Authors

    Thomas، نويسنده , , P.C. and A’Hearn، نويسنده , , Michael F. and Veverka، نويسنده , , Joseph and Belton، نويسنده , , Michael J.S. and Kissel، نويسنده , , Jochen and Klaasen، نويسنده , , Kenneth P. and McFadden، نويسنده , , Lucy A. and Melosh، نويسنده , , H. Jay and Schultz، نويسنده , , Peter H. and Besse، نويسنده , , Sébastien and Carcich، نويسنده , , Brian T. and Farnham، نويسنده , , Tony L. and، نويسنده ,

  • Issue Information
    روزنامه با شماره پیاپی سال 2013
  • Pages
    9
  • From page
    550
  • To page
    558
  • 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 2.33 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.
  • Keywords
    Nucleus , comets , comets , geological processes , geophysics
  • Journal title
    Icarus
  • Serial Year
    2013
  • Journal title
    Icarus
  • Record number

    2379595