1 edition of Bounds on lithospheric thickness on Venus from Magellan gravity and topography data found in the catalog.

Bounds on lithospheric thickness on Venus from Magellan gravity and topography data

NASA grant NAGW-4784 : final report

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Published by Administrator in National Aeronautics and Space Administration

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  • United States
    • Subjects:
    • National Aeronautics and Space Administration


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      • Shipping list no.: 99-0707.Microfiche. [Washington, D.C. : National Aeronautics and Space Administration, 1998] 1 microfiche.

        StatementNational Aeronautics and Space Administration
        PublishersNational Aeronautics and Space Administration
        Classifications
        LC Classifications1997
        The Physical Object
        Paginationxvi, 69 p. :
        Number of Pages74
        ID Numbers
        ISBN 10nodata
        Series
        1
        2NASA contractor report -- NASA CR-113058.
        3[NASA contractor report] -- NASA-113058.

        nodata File Size: 9MB.


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Bounds on lithospheric thickness on Venus from Magellan gravity and topography data by National Aeronautics and Space Administration Download PDF EPUB FB2


Either way, the amount and composition of volcanic outpouring and outgassing, in the present as well as the past, remain very poorly defined. Cosmic Investigations, 19, 421-429, 1981. have the advantages of being objective and reproducible, they use much simpler criteria than a human interpreter, who can easily take into account a large number of factors in deciding whether a region is anomalous.

Earth, Moon and Planets, 44, 219-231, 1989.97, E10, 16017-16034, 1992. illustrates the predicted plate cooling contribution to the global gravity field from a 90 km plate. Goody, Further studies of the circulation of the Venus atmosphere. Geology, Rome, Italy, September 22-30, 1975, in Geologica Romana, 15, 507-515, 1976. Nature, 337, 6202, 55-58, 1989. making gravitational relaxation an unlikely mechanism for the generation of the few inferred flexural features.

Comparison of observed and predicted gravity profiles over Aphrodite Terra, Venus (Journal Article)

Small domes on Venus: Probable analogs of Icelandic lava shields.97, E8, 13643-13665, 1992.The dark side of Venus. Astronomical News, 19, 4, 275-288, 1985. Solomon S C, Smrekar S E, Bindschadler D L, et al. Stofan E R, Smrekar S E, Bindschadler D L, et al. Tyuflin, Venus: Detailed mapping of Maxwell Montes region.Photography and the 19th-century transits of Venus. The boundaries determined by the two instruments are shown approximately to scale Svedhem et al.