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  • Unknown author (Lunar and Planetary Institute, 1994)
    Information about the scientific investigations funded by the NASA Venus Data Analysis Program (VDAP) during fiscal year 1993. The VDAP Directory consists of summary sheets from the proposals that were selected by NASA ...
  • Treiman, Allan H.; https://orcid.org/0000-0002-8073-2839 (Lunar and Planetary Institute, 2009)
    The workshop has several objectives: to assess current knowledge of Venus’ geochemistry; to consider Earth-based investigations (laboratory and theoretical) that will enhance understanding of current data and enable future ...
  • Wood, Charles A.; Francis, Peter W. (Lunar and Planetary Institute, 1988)
    Observations of electrical noise and sulfur dioxide variations by the Pioneer Venus spacecraft have been interpreted as evidence for ongoing volcanic activity (Scarf and Russell, 1983; Esposito, 1984). Recently this ...
  • Balcerski, Jeff; Steffes, P. G. (Paul Gregory), 1955-; Arney, Giada Nicole (Lunar and Planetary Institute, 2017)
    The objectives of this workshop were to discuss (1) the status of modeling of Venus’ exosphere, atmosphere, surface, and interior; and (2) the factors that are currently limiting the ability of investigators to advance ...
  • Santos, Alison R.; Filiberto, Justin; https://orcid.org/0000-0001-5058-1905; Ganesh, Indujaa; Gilmore, Martha S.; Lewis, Jonathan A.; Treiman, Allan H.; https://orcid.org/0000-0002-8073-2839 (2020)
    We encourage the Decadal Panel to continue its emphasis on the surface of Venus as a spacecraft target and to promote the continued development of technologies that can collect petrologic data in Venus’ challenging environment.
  • Kremic, Tibor; Singh, Upendra N.; Baines, Kevin Hays; https://orcid.org/0000-0002-5544-9986 (Lunar and Planetary Institute, 2015)
    The objectives of this two-day workshop are to (1) present, discuss, and document the status of the instrument technologies and the definition of new instruments; and (2) present, discuss, and document the status and needs ...
  • Fegley, Bruce; Treiman, Allan H.; Sharpton, Virgil L. (Lunar and Planetary Institute, 1992)
    We utilize Earth-based, Earth-orbital, and spacecraft observations of the atmosphere and surface of Venus, thermodynamic models of atmosphere-lithosphere interactions, and where available kinetic data on relevant gas-solid ...
  • McGovern, Patrick J. (Geophysicist); https://orcid.org/0000-0001-9647-3096 (2020)
    Here I identify the next steps that would unleash the potential of the vast range of volcanic phenomena recorded at the surface of Venus to inform, or perhaps transform, studies of Venus’ evolution and the volcanic expressions ...
  • Binzel, Richard P.; Schenk, Paul M. (Lunar and Planetary Institute, 2014)
    The scope of this workshop, the first dedicated to Vesta as a planetary body, includes dynamics, impact mechanics and impactor flux, internal and surface composition, shape and internal structure, formation and geologic ...
  • Mouginis-Mark, Peter J. (Lunar and Planetary Institute, 1981)
    This slide set is intended to show that although Hawaiian volcanos are small when compared to those found on the other planets, we can learn a considerable amount about how the extraterrestrial features were formed. Through ...
  • 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.
  • Simonds, Charles H.; Phinney, William C.; McGee, Patricia E.; Cochran, Ann (Pergamon Press, 1978)
    A field study at the 30 km diameter West Clearwater impact crater was carried out during the summer of 1977 to identify the nature of the flow of impact melt and less shocked debris during the excavation stage of the ...
  • Simonds, Charles H.; Phinney, William C.; McGee, Patricia E.; Cochran, Ann (Pergamon Press, 1978)
    Impactites lining the base of the crater at West Clearwater Lake consist of a 0 to 20 m thickness of fragmental breccia overlain by about 18 m of clast-rich melt rock which in turn is overlain by at least 85 m of clast-poor ...
  • Bogard, Donald D.; Rutherford, Malcolm J.; Schmidt, Greg; Shearer, Charles K. (Lunar and Planetary Institute, 2011)
    The purpose of this workshop is to bring together members of the planetary science community to discuss and integrate mission observations, laboratory measurements, and theoretical models for the volatile behavior and ...
  • Rivera-Valentín, Edgard G.; Rathbun, Julie; Keane, James Tuttle; Lynch, Kennda; Richey, Christina; Diniega, Serina; Vertesi, Janet (2020)
    In order to identify trends in underrepresentation in planetary science and related fields and to inform diversity initiatives, we conducted a demographic analysis using the American Astronomical Society’s Division of ...
  • Whalen, Michael T.; Lowery, Christopher M.; Bralower, Timothy J.; Gulick, Sean P. S.; Morgan, Joanna V.; Grice, Kliti; Schaefer, Bettina; Smit, Jan; Ormö, Jens; Wittmann, Axel 1971-; Kring, David A. (David Allen); Lyons, Shelby; Goderis, Steven; IODP-ICDP Expedition 364 Scientists (Elsevier, 2020-12)
    The upper suevite, Transitional Unit, and overlying green marlstone on the peak ring of the Chicxulub impact structure at Site M0077 appear to record a complete transition from resurge deposits into post-impact sediments. ...
  • 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.
  • Ciarletti, Valérie; Clifford, Stephen Mark, 1952- (Mary Ann Liebert, Inc., 2017-07-01)
    The search for evidence of past or present life on Mars is the principal objective of the 2020 ESA-Roscosmos ExoMars Rover mission. If such evidence is to be found anywhere, it will most likely be in the subsurface, where ...
  • Ashwal, Lewis D.; Card, K. D. (Lunar and Planetary Institute, 1983)
    Various topics relevant to crustal genesis, especially the relationship between Archean low - and high-grade terrains, were discussed. The central Superior Province of the Canadian Shield was studied.
  • Appleby, J., (John F.) (Lunar and Planetary Institute, 1993)
    The planetary science community described instrumentation needed for missions that may go into development during the next 5 to 10 years. Then the DoD community to informed their counterparts in planetary science about ...

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