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Autor Williams, Jean-Pierre |
Documentos disponibles escritos por este autor (16)
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Ruiz Pérez, Javier ; Williams, Jean-Pierre ; Dohm, James M. ; Fernández, Carlos ; López, Valle | Rosen Pub. Group | 2009Heat flow calculations based on geological and/or geophysical indicators can help to constrain the thickness, and potentially the geochemical stratification, of the martian crust. Here we analyze the Warrego rise region, part of the ancient moun[...]texto impreso
Dohm, James M. ; Anderson, Robert C. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; McGuire, Patrick C. ; Buczkowski, Debra L. ; Wang, Ruye ; Scharenbroich, Lucas ; Hare, Trent M. ; Connerney, J.E.P. ; Baker, Victor R. ; Wheelock, Shawn J. ; Ferris, Justin C. ; Miyamoto, Hirdy | Elsevier Science Publishers | 2009Claritas rise is a prominent ancient (Noachian) center of tectonism identified through investigation of comprehensive paleotectonic information of the western hemisphere of Mars. This center is interpreted to be the result of magmatic-driven act[...]texto impreso
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Depth of faulting and ancien theat flows in the Kuiper region of Mercuryfrom lobate scarp topography
Egea González, Isabel ; Ruiz Pérez, Javier ; Fernández Rodríguez, Carlos ; Williams, Jean-Pierre ; Márquez González, Álvaro ; Lara López, Luisa M. | Elsevier B.V. | 2012Mercurian lobate scarp sare interpreted to be the surface expressions of thrust faults formed by planetary cooling and contraction, which deformed the crust downto the brittle–ductile transition (BDT) dep that the time of faulting. In this work[...]texto impreso
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Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Rosenburg, Margaret A. ; Aharonson, Oded ; Phillips, Roger J | American Geophysical Union | 2011Mercury’s coupled 3:2 spin?orbit resonance in conjunction with its relatively high eccentricity of ?0.2 and near?zero obliquity results in both a latitudinal and longitudinal variation in annual average solar insolation and thus equatorial hot a[...]texto impreso
Kim, Kyeong J. ; Dohm, James M. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Yu, B.H. ; Hare, Trent M. ; Hasebe, Nobuyuki ; Yamashita, N. ; Karouji, Yuzuru ; Kobayashi, Shingo ; Hareyama, Makoto ; Shibamura, Eido ; Kobayashi, Masanori ; Uston, Claude d' ; Gasnault, Olivier ; Forni, Olivier ; Reedy, R.C. | United States. National Aeronautics and Space Administration. | 2010texto impreso
Ruiz Pérez, Javier ; Williams, Jean-Pierre ; Dohm, James M. ; Fernández, Carlos ; López, Valle | Elsevier Science B.V., Amsterdam | 2013Heat flow is a very important parameter for constraining the thermal evolution of a planetary body. Several procedures for calculating heat flows for Mars from geophysical or geological proxies have been used, which are valid for the time when t[...]texto impreso
Dohm, James M. ; Williams, Jean-Pierre ; Anderson, Robert C. ; Ruiz Pérez, Javier ; McGuire, Patrick C. ; Komatsu, Goro ; Davila, Alfonso F. ; Ferris, Justin C. ; Baker, Victor R. ; Boynton, William V. ; Fairén, Alberto G. ; Hare, Trent M. ; Miyamoto, Hirdy ; Tanaka, Kennth L. ; Wheelock, Shawn J. | Elsevier Science Publishers | 2009In this paper, we show that the complex geological evolution of Valles Marineris, Mars, has been highly influenced by the manifestation of magmatism (e.g., possible plume activity). This is based on a diversity of evidence, reported here, for th[...]texto impreso
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Kim, Kyeong J. ; Dohm, James M. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Yu, Byeong-Hyeok ; Hare, Trent M. ; Hasebe, Nobuyuki ; Yamashita, Naoyuki ; Karouji, Yuzuru ; Kobayashi, Shingo ; Hareyama, Makoto ; Shibamura, Eido ; Kobayashi, Masanori ; Uston, Claude d' ; Gasnault, Olivier ; Forni, Olivier ; Reedy, R.C. | 2011texto impreso
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King, Kyeong Ja ; Dohm, James M. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Hare, Trent M. ; Hasebe, Nobuyuki ; Karouji, Yuzuru ; Kobayashi, Shingo ; Hareyama, Makoto ; Shibamura, Eido ; Kobayashi, Masanori ; Uston, Claude d' ; Gasnault, Olivier ; Forni, Olivier ; Maurice, Sylvestre | Elsevier | 2012Using Geographic Information Systems (GIS), we performed comparative analysis among stratigraphic information and the Kaguya (SELENE) GRS data of the 2500-km-diameter South Pole-Aitken (SPA) basin and its surroundings. Results indicate chat the [...]