USRA Houston Repository

Browsing LPI Contributions by Subject "QB641"

Browsing LPI Contributions by Subject "QB641"

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  • Bristow, Thomas F.; Craig, Patricia I.; https://orcid.org/0000-0003-4080-4997; Treiman, Allan H.; https://orcid.org/0000-0002-8073-2839 (American Association for the Advancement of Science, 2018-06-06)
    Clay minerals provide indicators of the evolution of aqueous conditions and possible habitats for life on ancient Mars. Analyses by the Mars Science Laboratory rover Curiosity show that ~3.5–billion year (Ga) fluvio-lacustrine ...
  • George, Jeffrey A.; Stoker, Carol R.; Clifford, Stephen Mark, 1952-; https://orcid.org/0000-0003-0771-1713 (Lunar and Planetary Institute, 2001)
    The primary goal of the conference is to identify the most direct, unambiguous, and cost-effective approach to assessing the three-dimensional distribution and state of water within the martian crust — at a resolution ...
  • Zimbelman, James R.; Solomon, Sean C.; Sharpton, Virgil L.; https://orcid.org/0000-0002-0420-8453 (Lunar and Planetary Institute, 1991)
    Mars has been the target of a number of ambitious spacecraft missions, including the American Viking orbiters and landers in the late 1970s and, more recently, the Soviet Phobos spacecraft in 1989. Soon after the Viking ...
  • Unknown author (Lunar and Planetary Institute, 2017)
    Escape to the Red Planet and interact with a 3D model of Mars. Observe the transition from a wet planet early in its history to the dry world we see today. View locations of past landing sites and the top three targets for ...
  • Howard, Alan D.; Moore, J. (Jeff); Rice, J. W. (James W.) (Lunar and Planetary Institute, 2001)
  • Bish, David L.; Treiman, Allan H.; https://orcid.org/0000-0002-8073-2839 (International Union of Crystallography, 2014-11)
    The Mars Science Laboratory landed in Gale crater on Mars in August 2012, and the Curiosity rover then began field studies on its drive toward Mount Sharp, a central peak made of ancient sediments. CheMin is one of ten ...
  • Bedford, Candice; https://orcid.org/0000-0002-0783-1064; Schwenzer, Susanne Petra; Bridges, John C.; Banham, Steven; Wiens, Roger; Gasnault, Olivier M.; Rampe, Elizabeth; Frydenvang, Jens; Gasda, Patrick J.; https://orcid.org/0000-0002-9608-0759 (Elsevier, 2020-05)
    A ChemCam geochemical study of the ancient aeolian Stimson formation in Gale crater. The geochemical effect of mineral sorting in the ancient dunes has been preserved. The Stimson dunes were transported SW-NE, opposite to ...
  • Udry, Arya; Filiberto, Justin; https://orcid.org/0000-0001-5058-1905; Gross, Juliane; Schmidt, Mariek E.; Rogers, Deanne; Hausrath, Libby; Wiens, Roger; Lanza, Nina (2020-07)
    This white paper summarizes the scientific importance of studying igneous compositions in meteorites, surface samples, and through orbital analyses to better constrain the geology of Mars as a whole and better understand ...
  • Burt, Donald M. (Lunar and Planetary Institute, 1989)
    Although direct evidence is lacking, indirect evidence suggests that iron-rich clay minerals or poorly ordered chemical equivalents ("palagonite") are widespread on the martian surface. Such clays (or other Fe and OH-bearing ...
  • Newman, Claire E.; Kahanpää, H.; Richardson, M. I.; Martínez, Germán M.; Vicente‐Retortillo, Álvaro; Lemmon, Mark T.; https://orcid.org/0000-0002-4553-7624; https://orcid.org/0000-0001-5885-236X (AGU, 2019-11-15)
    The daytime Martian atmosphere produces convective vortices called "dust devils" when they are dust‐filled. Vortices produce rapid pressure drops, which have been detected in Gale Crater by Mars Science Laboratory instruments. ...
  • Guzewich, Scott; Abshire, James B.; Baker, M. M. (Mariah M.); Martínez, Germán M.; https://orcid.org/0000-0001-5885-236X (2020-07-15)
    Wind is the process that connects Mars' climate system. Measurements of Mars atmospheric winds from orbit would dramatically advance our understanding of Mars and help prepare for human exploration of the Red Planet. ...
  • Kiefer, Walter S.; Clifford, Stephen Mark, 1952-; Treiman, Allan H.; https://orcid.org/0000-0002-8073-2839; https://orcid.org/0000-0001-6741-5460; https://orcid.org/0000-0003-0771-1713 (Lunar and Planetary Institute, 1997)
    An overview of Mars, including its volcanoes, the Valles Marineris canyon system, features formed by running water, the SNC meteorites, and its two small moons, Phobos and Deimos. This is the second edition, revised in ...
  • Smith, Isaac; Calvin, Wendy; https://orcid.org/0000-0002-6097-9586 (Lunar and Planetary Institute, 2016)
    The conference is designed to pull together the current state of Mars polar research from many fields, including geology, atmospheric, and climate sciences.
  • Barlow, Nadine G.; Sharpton, Virgil L.; https://orcid.org/0000-0002-5588-294X (Planetary Image Center/Lunar and Planetary Institute, 1987)
    Illustrates the diversity of Martian impact craters and demonstrates their role in understanding the geological evolution of Mars
  • Zimbelman, James R.; https://orcid.org/0000-0002-0420-8453 (Center for Information and Research Services, Lunar and Planetary Institute, 1987)
    Illustrates various geologic features on Mars, including some of the best examples of Viking Orbiter images that include constructional volcanic landforms.
  • Williams, Steven H. (Center for Information and Research Services, Lunar and Planetary Institute, 1990)
    An overview of the types of aeolian activity and landforms found on Mars. Includes a glossary of Martian place names and terms and a short reference list.

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