Lunar and Planetary Science XXXVI, Part 5Topics discussed include: Automation Recognition oF Crater-Like Structures in Terrestrial and Plantary Images; Condensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites; Tomographic Location of Potential Melt-Bearing Phenocrysts in Lunar Glass Spherules; Source and Evolution of Vapor Due to Impacts into Layered Carbonates and Silicates; Noble Gases and I-Xe Ages of the Zag Meteorite; The MArs Hand Lens Imager (MAHLI) for the 209 Mars Science Laboratory; The Sedimentary Rocks of Meridiani Planum, in Context; Three-System Isotopic of Lunar Norite 78238: Rb-Sr Results; Constraints on the Role of Curium-247 as a Source of Fission Xenon in the Early Solar System; New Features in the ADS Abstract Service; Cassini RADAR's First Look at Titan; Volcanism and Volatile Recycling on Venus from Lithospheric Delamination; The Fate of Water in the Martian Magma Ocean and the Formation of an Early Atmosphere; Mars Odyssey Neutron Spectrometer Water-Equivalent Hydrogen: Comparison with Glacial; Landforms on Tharsis; Using Models of Permanent Shadow to Constrain Lunar Polar Water Ice Abundances; Martian Radiative Transfer Modeling Using the Optimal Spectral Sampling Method; Petrological and Geochemical Consideration on the Tuserkanite Meteorite; and Mineralogy of Asteroids from Observations with the Spitzer Space Telescope.
Sponsors: NASA Johnson Space Center, Lunar and Planetary Inst.
Funding Number(s)
CONTRACT_GRANT: NCC5-679
Distribution Limits
Public
Copyright
Public Use Permitted.
Available Downloads
There are no available downloads for this record.
Related Records
IDRelationTitle20050166876WorkA Gas-Poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Consequences for the Atmosphere of Titan20050166890WorkThermal Emission Variability of Zamama, Culann and Tupan on Io Using Galileo Near-Infrared Mapping Spectrometer (NIMS) Data20050166873WorkCondensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites20050166880WorkThree-System Isotopic of Lunar Norite 78238: Rb-Sr Results20050166870WorkTomographic Location of Potential Melt-Bearing Phenocrysts in Lunar Glass Spherules20050166888WorkMineralogy of Asteroids from Observations with the Spitzer Space Telescope20050166892WorkThe 2004 Opposition of Ceres Observed with Adaptive Optics on the VLT20050166883WorkCassini RADAR's First Look at Titan20050166886WorkMartian Radiative Transfer Modeling Using the Optimal Spectral Sampling Method20050166884WorkVolcanism and Volatile Recycling on Venus from Lithospheric Delamination20050166874WorkThe Mars Hand Lens Imager (MAHLI) for the 209 Mars Science Laboratory20050166882WorkNew Features in the ADS Abstract Service20050166893WorkThe Saturn System as Observed by Cassini's Ultraviolet Imaging Spectrograph20050166870WorkTomographic Location of Potential Melt-Bearing Phenocrysts in Lunar Glass Spherules20050166873WorkCondensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites20050166874WorkThe Mars Hand Lens Imager (MAHLI) for the 209 Mars Science Laboratory20050166876WorkA Gas-Poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Consequences for the Atmosphere of Titan20050166880WorkThree-System Isotopic of Lunar Norite 78238: Rb-Sr Results20050166882WorkNew Features in the ADS Abstract Service20050166883WorkCassini RADAR's First Look at Titan20050166884WorkVolcanism and Volatile Recycling on Venus from Lithospheric Delamination20050166886WorkMartian Radiative Transfer Modeling Using the Optimal Spectral Sampling Method20050166888WorkMineralogy of Asteroids from Observations with the Spitzer Space Telescope20050166890WorkThermal Emission Variability of Zamama, Culann and Tupan on Io Using Galileo Near-Infrared Mapping Spectrometer (NIMS) Data20050166892WorkThe 2004 Opposition of Ceres Observed with Adaptive Optics on the VLT20050166893WorkThe Saturn System as Observed by Cassini's Ultraviolet Imaging Spectrograph