By Larry W. Esposito, Ellen R. Stofan, Thomas E. Cravens
Published through the yank Geophysical Union as a part of the Geophysical Monograph Series.
With the hunt for extra-solar planets in complete apparatus, it has turn into necessary to achieve a extra special realizing of the evolution of the opposite earth-like planets in our personal sunlight process. house missions to Venus, together with the Soviet Veneras, Pioneer Venus, and Magellan, supplied a wealth of data approximately this planet' enigmatic floor and surroundings, yet left many basic questions on its starting place and evolution unanswered.
This booklet discusses how the learn of Venus will reduction our knowing of terrestrial and extra-solar planet evolution, with specific connection with floor and inside methods, atmospheric circulate, chemistry, and aeronomy. Incorporating effects from the hot eu Venus show undertaking, Exploring Venus as a Terrestrial Planet examines the open questions and relates them to Earth and different terrestrial planets. The aim is to stimulate brooding about these broader matters because the new Venus facts arrive.
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Additional resources for Exploring Venus as a Terrestrial Planet
M. Khazins, Impact cratering on Venus: Physical and mechanical midels, J. Geophys. , 97, 16,167-16,181, 1992. Ivanov, M. A. and J. W. Head, Tessera terrain on Venus: A survey of the global distribution, characteristics, and relation to surrounding units from Magellan data, J. Geophys. , 101, 14861–14908, 1996. Ivanov, M. A. and J. W. Head, Geology of Venus: Mapping of a global geotraverse at 30 oN latitude, J. Geophys. , 106, 17515–17566, 2001. Ivanov, M. , and J. W. S. Geological Survey. Geologic Investigation Series Map I-2792, 2004a.
J. C. Aubele, D. A. Senske, S. T. Keddie, K. P. Magee, and J. W. Head, Volcanoes and centers of volcanism on Venus, in Venus II. Geology, Geophysics, Atmosphere, and Solar Wind Environment, edited by S. W. , pp. 757–793, Univ. of Arizona Press, Tucson, 1997. 41 De Witt, M. , and L. D. Aswal, Greenstone Belts (Oxford Monographs on Geology and Geophysics), pp. 840, Oxford University Press, USA, 1997. Donahue, T. , and J. B. Pollack, Origin and evolution of the atmosphere of Venus, in Venus, edited by D.
39 • What was the mechanism of tessera formation (deformation resulted from upwelling or downwelling) and how long was the tessera-forming phase? • How did the folded mountain ranges surrounding Lakshmi Planum form? • W hat caused the deformation typical of densely fractured plains, ridge belts and wrinkle ridges; in particular, how can we explain the stresses necessary to form areally extensive coherent arrays of wrinkle ridges? • Is Venus still volcanically and tectonically active? • A re coronae manifestations of mantle plumes?
Exploring Venus as a Terrestrial Planet by Larry W. Esposito, Ellen R. Stofan, Thomas E. Cravens