Search Results - "PRETTYMAN, T. H"
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Extensive water ice within Ceres’ aqueously altered regolith: Evidence from nuclear spectroscopy
Published in Science (American Association for the Advancement of Science) (06-01-2017)“…The surface elemental composition of dwarf planet Ceres constrains its regolith ice content, aqueous alteration processes, and interior evolution. Using…”
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Elemental composition of the lunar surface: Analysis of gamma ray spectroscopy data from Lunar Prospector
Published in Journal of Geophysical Research - Planets (01-12-2006)“…Gamma ray spectroscopy data acquired by Lunar Prospector are used to determine global maps of the elemental composition of the lunar surface. Maps of the…”
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Dawn arrives at Ceres: Exploration of a small, volatile-rich world
Published in Science (American Association for the Advancement of Science) (02-09-2016)“…On 6 March 2015, Dawn arrived at Ceres to find a dark, desiccated surface punctuated by small, bright areas. Parts of Ceres' surface are heavily cratered, but…”
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Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution
Published in Geophysical research letters (16-07-2017)“…Prior to the arrival of the Dawn spacecraft at Ceres, the dwarf planet was anticipated to be ice‐rich. Searches for morphological features related to ice have…”
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Dawn at Vesta: Testing the Protoplanetary Paradigm
Published in Science (American Association for the Advancement of Science) (11-05-2012)“…The Dawn spacecraft targeted 4 Vesta, believed to be a remnant intact protoplanet from the earliest epoch of solar system formation, based on analyses of…”
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Global Distribution of Neutrons from Mars: Results from Mars Odyssey
Published in Science (American Association for the Advancement of Science) (05-07-2002)“…Global distributions of thermal, epithermal, and fast neutron fluxes have been mapped during late southern summer/northern winter using the Mars Odyssey…”
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Global distribution of near-surface hydrogen on Mars
Published in Journal of Geophysical Research - Planets (01-09-2004)“…Neutron data observed using the Neutron Spectrometer aboard 2001 Mars Odyssey provide a lower limit to the global inventory of Martian water‐equivalent…”
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Journal Article Conference Proceeding -
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Impact-driven mobilization of deep crustal brines on dwarf planet Ceres
Published in Nature astronomy (01-08-2020)“…Ceres, the only dwarf planet in the inner Solar System, appears to be a relict ocean world. Data collected by NASA's Dawn spacecraft provided evidence that…”
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Chondritic models of 4 Vesta: Implications for geochemical and geophysical properties
Published in Meteoritics & planetary science (01-11-2013)“…Simple mass‐balance and thermodynamic constraints are used to illustrate the potential geochemical and geophysical diversity of a fully differentiated…”
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Distribution of Hydrogen in the near Surface of Mars: Evidence for Subsurface Ice Deposits
Published in Science (American Association for the Advancement of Science) (05-07-2002)“…Using the Gamma-Ray Spectrometer on the Mars Odyssey, we have identified two regions near the poles that are enriched in hydrogen. The data indicate the…”
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Vesta's Shape and Morphology
Published in Science (American Association for the Advancement of Science) (11-05-2012)“…Vesta's surface is characterized by abundant impact craters, some with preserved ejecta blankets, large troughs extending around the equatorial region,…”
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MCNPX benchmark for cosmic ray interactions with the Moon
Published in Journal of Geophysical Research - Planets (01-06-2006)“…The MCNPX radiation transport code is used to simulate cosmic ray interactions within the Moon. Accurate source, geometric, and physics models are developed to…”
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Evidence for water ice near the lunar poles
Published in Journal of Geophysical Research (25-10-2001)“…Improved versions of Lunar Prospector thermal and epithermal neutron data were studied to help discriminate between potential delivery and retention mechanisms…”
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Journal Article Conference Proceeding -
14
Vesta, vestoids, and the HED meteorites: Interconnections and differences based on Dawn Framing Camera observations
Published in Journal of geophysical research. Planets (01-10-2013)“…The Framing Camera (FC) on the Dawn spacecraft provided the first view of 4 Vesta at sufficiently high spatial resolution to enable a detailed correlation of…”
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Small-area thorium features on the lunar surface
Published in Journal of Geophysical Research - Planets (01-09-2003)“…Using an improved understanding of the Lunar Prospector Gamma‐Ray Spectrometer (LP‐GRS) spatial footprint, we have derived a new map of global thorium…”
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Distribution of iron on Vesta
Published in Meteoritics & planetary science (01-11-2013)“…We have completed a mapping study of 7.6 MeV gamma rays produced by neutron capture by Fe at the surface of the main belt asteroid 4 Vesta as measured by the…”
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A Probabilistic Approach to Determination of Ceres' Average Surface Composition From Dawn Visible‐Infrared Mapping Spectrometer and Gamma Ray and Neutron Detector Data
Published in Journal of geophysical research. Planets (01-12-2020)“…The Visible‐Infrared Mapping Spectrometer (VIR) on board the Dawn spacecraft revealed that aqueous secondary minerals—Mg‐phyllosilicates, NH4‐bearing phases,…”
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Improved modeling of Lunar Prospector neutron spectrometer data: Implications for hydrogen deposits at the lunar poles
Published in Journal of Geophysical Research - Planets (01-08-2006)“…New models have been computed for the Lunar Prospector (LP) thermal and epithermal neutron counting rates using the particle transport code MCNPX. This work…”
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Global spatial deconvolution of Lunar Prospector Th abundances
Published in Geophysical research letters (01-02-2007)“…We have completed the first global spatial deconvolution analysis of planetary gamma‐ray data for lunar Th abundances as measured by the Lunar Prospector…”
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Dawn completes its mission at 4 Vesta
Published in Meteoritics & planetary science (01-11-2013)“…The Dawn mission was designed to test our hypothesis about the origin and evolution of the early solar system by visiting the largest differentiated basaltic…”
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