Thickness of the crust of Mercury from geoid‐to‐topography ratios
Open Access
- 8 January 2015
- journal article
- research article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 42 (4), 1029-1038
- https://doi.org/10.1002/2014gl062487
Abstract
No abstract availableFunding Information
- MESSENGER Participating Scientist Program (NNX09AR45G)
- UCLA Division of Physical Sciences
- DFG (T0704/1-1)
- Helmholtz Gemeinschaft (VH-NG-1017)
- NASA Discovery Program (NAS5-97271)
This publication has 55 references indexed in Scilit:
- Gravity Field and Internal Structure of Mercury from MESSENGERScience, 2012
- Topography of the Northern Hemisphere of Mercury from MESSENGER Laser AltimetryScience, 2012
- Finite volume discretization for dynamic viscosities on Voronoi gridsPhysics of the Earth and Planetary Interiors, 2008
- Does mantle convection currently exist on Mercury?Physics of the Earth and Planetary Interiors, 2007
- Thickness of the Martian crust: Improved constraints from geoid‐to‐topography ratiosJournal of Geophysical Research, 2004
- Depth of faulting on Mercury: Implications for heat flux and crustal and effective elastic thicknessGeophysical Research Letters, 2004
- The mechanical and thermal structure of Mercury's early lithosphereGeophysical Research Letters, 2002
- Constraining the crustal thickness on Mercury from viscous topographic relaxationGeophysical Research Letters, 2002
- The structure and compensation of the lunar highland crustJournal of Geophysical Research, 1997
- Gravitational and topographic isotropy of the Earth, Moon, Mars, and VenusJournal of Geophysical Research, 1995