CALL FOR PROPOSALS:

ORGANIZERS

  • Harvey Thorleifson, Chair
    Minnesota Geological Survey
  • Carrie Jennings, Vice Chair
    Minnesota Geological Survey
  • David Bush, Technical Program Chair
    University of West Georgia
  • Jim Miller, Field Trip Chair
    University of Minnesota Duluth
  • Curtis M. Hudak, Sponsorship Chair
    Foth Infrastructure & Environment, LLC

 

Paper No. 2
Presentation Time: 1:45 PM

THE GEOPHYSICS OF MERCURY: MESSENGER's VIEW FROM ORBIT


HAUCK II, Steven A.1, ZUBER, Maria T.2, SMITH, David E.2, JOHNSON, Catherine L.3, PHILLIPS, Roger J.4, LEMOINE, Frank G.5, MARGOT, Jean-Luc6, NEUMANN, Gregory A.5, PEALE, Stanton J.7 and SOLOMON, Sean C.8, (1)Department of Geological Sciences, Case Western Reserve University, 10900 Euclid Avenue, AW Smith 112, Cleveland, OH 44106-7216, (2)Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307, (3)Department of Earth and Ocean Sciences, University of British Columbia, 6339 Stores Road, Vancouver, BC V6T 1Z4, Canada, (4)Planetary Science Directorate, Southwest Research Institute, 1050 Walnut St, Suite 300, Boulder, CO 80302, (5)Planetary Geodynamics Laboratory, NASA Goddard Space Flight Center, Mail Code 698, Greenbelt, MD 20771, (6)Department of Earth and Space Sciences, University of California, Los Angeles, 595 Charles Young Drive East, Los Angeles, CA 90095, (7)Department of Physics, University of California Santa Barbara, Broida Hall, Mail Code 9530, Santa Barbara, CA 93106, (8)Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Rd. NW, Washington, DC 20015, hauck@case.edu

On March 18, 2011, MESSENGER entered an elliptical, near-polar orbit about Mercury, becoming the first spacecraft to orbit that planet. As part of MESSENGER’s geophysics investigation, the Mercury Laser Altimeter (MLA) is ranging to the surface of Mercury when the spacecraft slant range is less than 1500 km, largely over the northern hemisphere. MLA profiles have sampled a variety of landforms, including volcanic plains, tectonic structures, and impact craters and basins as well as longer-wavelength variations in topography. MLA has also profiled several polar impact craters previously identified by Earth-based observations as hosting radar-bright deposits in their interiors. Tracking of radio signal transmissions from MESSENGER’s low- and high-gain antennas is yielding new information on the gravity field of Mercury. Regional variations in Mercury’s gravity field, together with topographic information, provide important constraints on mechanisms of topographic compensation. Importantly, MESSENGER is also improving estimates of the second-degree spherical harmonic gravity-field coefficients C20 and C22. Prior to MESSENGER orbital operations, C20 was the least constrained parameter necessary for determining the size of Mercury’s core. Ultimately, the determination of the planet’s normalized polar moment of inertia (C/MR2), where M and R are Mercury’s mass and radius, and the ratio of the polar moment of inertia of the mantle and crust to the planet’s polar moment of inertia (Cm/C) provide crucial constraints on Mercury’s internal structure. Observations by MESSENGER’s Magnetometer indicate a dipole-dominated planetary magnetic field, centered on the spin axis, with a tilt of less than 3° and a northward displacement along its axis of 0.2 R. These observations are consistent with a core dynamo as the origin for Mercury’s internal magnetic field, albeit one with an unusual geometry or boundary conditions.
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