Gravity field and internal structure of Mercury from MESSENGER.

نویسندگان

  • David E Smith
  • Maria T Zuber
  • Roger J Phillips
  • Sean C Solomon
  • Steven A Hauck
  • Frank G Lemoine
  • Erwan Mazarico
  • Gregory A Neumann
  • Stanton J Peale
  • Jean-Luc Margot
  • Catherine L Johnson
  • Mark H Torrence
  • Mark E Perry
  • David D Rowlands
  • Sander Goossens
  • James W Head
  • Anthony H Taylor
چکیده

Radio tracking of the MESSENGER spacecraft has provided a model of Mercury's gravity field. In the northern hemisphere, several large gravity anomalies, including candidate mass concentrations (mascons), exceed 100 milli-Galileos (mgal). Mercury's northern hemisphere crust is thicker at low latitudes and thinner in the polar region and shows evidence for thinning beneath some impact basins. The low-degree gravity field, combined with planetary spin parameters, yields the moment of inertia C/MR(2) = 0.353 ± 0.017, where M and R are Mercury's mass and radius, and a ratio of the moment of inertia of Mercury's solid outer shell to that of the planet of C(m)/C = 0.452 ± 0.035. A model for Mercury's radial density distribution consistent with these results includes a solid silicate crust and mantle overlying a solid iron-sulfide layer and an iron-rich liquid outer core and perhaps a solid inner core.

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عنوان ژورنال:
  • Science

دوره 336 6078  شماره 

صفحات  -

تاریخ انتشار 2012