P33D:
The Solar System Collapsing Disk: Evidence from Comets, Meteorites, and Giant Planet Atmospheres Posters

Wednesday, 17 December 2014: 1:40 PM-6:00 PM
Primary Convener:  Kathleen Mandt, Southwest Research Institute San Antonio, San Antonio, TX, United States
Co-Convener:  Olivier Mousis, Besançon Astronomical Observatory, Besançon Cedex, France

Abstracts Submitted to this Session:

4044
 
Cometary Nitrogen-Noble gases and the Origin of the Oceans: Waiting for ROSINA-Rosetta Data
Bernard Marty1, Ursina Calmonte2, Kathrin Altwegg2, Hans R Balsiger2, Akiva Bar-Nun3, Jean-Jacques Berthelier4, Andre Michel Bieler5, Frederik Dhooghe6, Björn Fiethe7, Urs A. Mall8, Olivier Mousis9, Tobias C Owen10 and Martin Rubin2, (1)CRPG-CNRS,Université de Lorraine, Vandoeuvre les Nancy, France, (2)University of Bern, Bern, Switzerland, (3)Tel Aviv University, Tel Aviv, Israel, (4)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (5)University of Michigan, Ann Arbor, MI, United States, (6)Belgian Institute for Space Aeronomy, Brussels, Belgium, (7)Technische Universitat Braunschweig, Braunschweig, Germany, (8)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (9)University of Franche-Comté, Besançon, France, (10)Univ Hawaii, Honolulu, HI, United States
4045
 
Exploring the Origin of Volatiles in Terrestrial Worlds
Edwin Anthony Bergin1, Geoffrey Blake2, Fred Ciesla3 and L. Ilsedore Cleeves1, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)California Institute of Technology, Pasadena, CA, United States, (3)University of Chicago, Chicago, IL, United States
4046
 
Origin and Evolution of the Cometary Reservoirs
Luke Dones, Southwest Research Inst, Boulder, CO, United States, Nathan A Kaib, University of Oklahoma Norman Campus, Norman, OK, United States and Ramon Brasser, Tokyo Institute of Technology, Tokyo, Japan
4047
 
An Investigation of the Streamline Geometry of Photoevaporative Winds from Planet-Forming Disks
Lynsey Schroeder, Embry-Riddle Aeronautical University, Daytona Beach, FL, United States and Uma Gorti, SETI Institute Mountain View, Mountain View, CA, United States; NASA Ames Research Center, Moffett Field, CA, United States
4048
 
Modeling Oxygen Isotopes in the Nascent Solar Nebula for Material to be measured with Rosetta at Comet 67P/Churyumov-Gerasimenko
Claudia J Alexander1, Dogacan Su Ozturk2, Valeriy Tenishev2 and Tamas I Gombosi3, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Michigan Ann Arbor, AOSS, Ann Arbor, MI, United States, (3)Univ of Michigan, Ann Arbor, MI, United States
4049
 
Argon Measurement Capabilities at Comet 67P with ROSINA/DFMS
Myrtha Hässig1, Stephen Fuselier1, Kathrin Altwegg2, Hans Balsiger2, Jean-Jacques Berthelier3, Ursina Calmonte2, Johan MSJ De Keyser4, Björn Fiethe5, Tamas I Gombosi6, Andre Michel Bieler6, Annette Jäckel2, Lena Le Roy2, Urs A. Mall7, Peter Wurz2, Sébastien Gasc2, Martin Rubin2, Chia-yu Tzou2 and Henri Reme8, (1)Southwest Research Institute San Antonio, San Antonio, TX, United States, (2)University of Bern, Bern, Switzerland, (3)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (4)Belgian Institute for Space Aeronomy, Brussels, Belgium, (5)Technical University of Braunschweig, Braunschweig, Germany, (6)Univ of Michigan, Ann Arbor, MI, United States, (7)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (8)IRAP, Toulouse, France
4050
 
Explaining the Noble Gas Content of the Planets: Theoretical Models for Argon-Trapping by Amorphous Ices in the Solar Nebula
Cecilia Brooke Sanders and Fred Ciesla, University of Chicago, Chicago, IL, United States
4051
 
Expected constraints on the outer solar system formation conditions from the Rosetta-ROSINA measurements
Olivier Mousis1, Kathrin Altwegg2, Hans R Balsiger2, Akiva Bar-Nun3, Jean-Loup Bertaux4, Jean-Jacques Berthelier5, Andre Michel Bieler6, Peter A Bochsler2, Christelle Briois7, Ursina Calmonte2, Michael R Combi8, Johan De Keyser9, Frederik Dhooghe9, Björn Fiethe10, Stephen Fuselier11, Sébastien Gasc2, Fritz Gliem10, Tamas I Gombosi12, Myrtha Hässig11, Annette Jäckel2, Ernest Kopp2, Axel Korth13, Lena Le Roy2, Urs A. Mall13, Bernard Marty14, Henri Rème15, Martin Rubin2, Jean-Andre Sauvaud16, Jack H Waite Jr11 and Peter Wurz2, (1)University of Franche-Comté, Besançon, France, (2)University of Bern, Bern, Switzerland, (3)Tel Aviv University, Tel Aviv, Israel, (4)University of Versailles Saint-Quentin en Yvelines, Versailles, France, (5)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (6)University of Michigan, Ann Arbor, MI, United States, (7)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, LPC2E, Orléans Cedex 2, France, (8)Univ Michigan, Ann Arbor, MI, United States, (9)Belgian Institute for Space Aeronomy, Brussels, Belgium, (10)Technische Universitat Braunschweig, Braunschweig, Germany, (11)Southwest Research Institute San Antonio, San Antonio, TX, United States, (12)Univ of Michigan, Ann Arbor, MI, United States, (13)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (14)CRPG Centre de Recherches Pétrographiques et Géochimiques, Vandoeuvre-Les-Nancy, France, (15)IRAP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (16)IRAP/CNRS, Toulouse, France
4052
 
Upper limits to the fractionation of isotopes due to atmospheric escape: Implications for potential 14N/15N in Pluto’s atmosphere
Kathleen Mandt, Southwest Research Institute San Antonio, San Antonio, TX, United States and Olivier Mousis, University of Franche-Comté, Besançon, France
4053
 
Oxygen and Nitrogen Isotopes in the Sun and Solar Nebula
James R Lyons, Arizona State University, Tempe, AZ, United States
 
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