Analysis and interpretation of the surface topography and gravitational potential of Venus

Journal of Geophysical Research: Planets

Volumn 101, Issue E2, 1996, Pages 4711-4724

  Arkani Hamed, Jafar ^a  

^a MCGILL UNIVERSITY   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

EARTH GRAVITY; GRAVITATIONAL POTENTIAL; ISOSTATIC COMPENSATION; MANTLE DYNAMICS; MOHO; PLANETARY STRUCTURE; SPHERICAL HARMONICS; SURFACE TOPOGRAPHY;

EARTH; VENUS;

EID: 19844365892     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/95JE03390     Document Type: Article

References (5)

1. Arkani-Hamed, J., Viscosity of the Moon, Moon, 6, 100-111, 1973.
2. Arkani-Hamed, J., Implications of the long-wavelength components of the gravity and surface topography of Venus, Proc. Lunar Planet. Sci. Conf. 21st, 13-26, 1991.
3. Arkani-Hamed, J., On the thermal evolution of Venus, J. Geophys. Res., 99, 2019-2033, 1994.
4. Arkani-Hamed, J., and M.N. Toksoz, Thermal evolution of Venus, Phys. Earth Planet. Inter., 34, 232-250, 1984.
5. Basilevsky, A.T., G.V. Nikolaeva, and C.M. Weitz, Geology of the Venera 8 landing site region from Magellan data: Morphology and geochemical considerations, J. Geophys. Res., 97, 16,315-16,335, 1992.