Workshop on Oxygen in Asteroids and MeteoritesContents include the following: Constraints on the detection of solar nebula's oxidation state through asteroid observation. Oxidation/Reduction Processes in Primitive Achondrites. Low-Temperature Chemical Processing on Asteroids. On the Formation Location of Asteroids and Meteorites. The Spectral Properties of Angritic Basalts. Correlation Between Chemical and Oxygen Isotopic Compositions in Chondrites. Effect of In-Situ Aqueous Alteration on Thermal Model Heat Budgets. Oxidation-Reduction in Meteorites: The Case of High-Ni Irons. Ureilite Atmospherics: Coming up for Air on a Parent Body. High Temperature Effects Including Oxygen Fugacity, in Pre-Planetary and Planetary Meteorites and Asteroids. Oxygen Isotopic Variation of Asteroidal Materials. High-Temperature Chemical Processing on Asteroids: An Oxygen Isotope Perspective. Oxygen Isotopes and Origin of Opaque Assemblages from the Ningqiang Carbonaceous Chondrite. Water Distribution in the Asteroid Belt. Comparative Planetary Mineralogy: V Systematics in Planetary Pyroxenes and fo 2 Estimates for Basalts from Vesta.
IDRelationTitle20050202048WorkCorrelations of (Delta)O-17 with Chemical Characteristics Among Chondrite Groups20050202072WorkWhat is the Water (OH) Content of the E Asteroids?20050202069WorkA Chemical Model of Micrometeorite Impact into Olivine20050202048WorkCorrelations of (Delta)O-17 with Chemical Characteristics Among Chondrite Groups20050202052WorkConstraints on the Detection of the Solar Nebula's Oxidation State Through Asteroid Observations20050202060WorkCompetitive Oxidation and Hydration During Aqueous Alteration of Asteroids20050202069WorkA Chemical Model of Micrometeorite Impact into Olivine20050202072WorkWhat is the Water (OH) Content of the E Asteroids?20050202052WorkConstraints on the Detection of the Solar Nebula's Oxidation State Through Asteroid Observations20050202060WorkCompetitive Oxidation and Hydration During Aqueous Alteration of Asteroids