P51G:
Planetary Atmospheres and Their Evolution I
Session ID#: 1521
Friday, 19 December 2014: 8:00 AM-10:00 AM
2009 (Moscone West)
Chairs: Feng Tian, Tsinghua University, Beijing, China, Sanjay S Limaye, University of Wisconsin Madison, Madison, WI, United States and Yongyun Hu, Peking University, Department of Atmospheric and Oceanic Sciences, School of Physics, Beijing, China
Primary Convener: Feng Tian, Tsinghua University, Beijing, China
Co-Convener: Eric Chassefiere, University of Paris-Sud 11, Orsay, France
OSPA Liaison: Feng Tian, Tsinghua University, Beijing, China
Co-Sponsor(s):
Virtual Option?: Yes
Swirl Theme: Comparative Planetology and Habitability
Abstracts Submitted to this Session:
Habitable Planets in Venus' Orbit and with Modern Venus' Slow Rotation (11859)
Jun Yang, Peking University, Department of Atmospheric and Oceanic Sciences, School of Physics, Beijing, China and Dorian S Abbot, University of Chicago, Geophysical Sciences, Chicago, IL, United States
Evaporating Atmospheres Around Close-in Exoplanets. (Invited) (6085)
James Owen1, Alan Jackson2, Yanqin Wu1 and Fred Adams3, (1)University of Toronto, Toronto, ON, Canada, (2)Towson University, Towson, United States, (3)University of Michigan, Ann Arbor, United States
Electrodynamics in Giant Planet Atmospheres (Invited) (11185)
Tommi Koskinen, University of Arizona, Tucson, United States, Roger V Yelle, University of Arizona, Lunar and Planetary Laboratory, Tucson, United States, Panayotis Lavvas, University of Reims, Reims, France and James Cho, Queen Mary, University of London, London, United Kingdom
Formation and Evolution of the Atmosphere on Early Titan (6383)
Nadejda Marounina1, Gabriel Tobie2, Sabrina Carpy3, Julien Monteux1,4, Benjamin Charnay5 and Olivier Grasset1, (1)LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France, (2)Nantes Université, Univ Angers, Le Mans Université, CNRS, Laboratoire de Planétologie et Géosciences, LPG UMR 6112, Nantes, France, (3)LPGN Laboratoire de Planétologie et Géodynamique, Nantes, France, (4)Laboratoire Magmas et Volcans, Clermont-Ferrand Cedex, France, (5)Paris Observatory, LESIA, Paris, France
New evidence for chemical depletion of ammonia in the 1 to 2 bar region of Jupiter's atmosphere (Invited) (10858)
Michael H. Wong1,2, Sushil K Atreya1, Paul N Romani3, Imke De Pater4, William R Kuhn1 and Konstantinos S. Kalogerakis5, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of California, Berkeley, United States, (3)NASA - GSFC, Greenbelt, MD, United States, (4)University of California Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States, (5)SRI International, Center for Geospace Studies, Menlo Park, United States
Can Water Be Frozen on the Nightside of Tidal-locking Exoplanets? (24078)
Yongyun Hu1, Jun Yang1, Yonggang Liu2 and Dorian S Abbot3, (1)Peking University, Department of Atmospheric and Oceanic Sciences, School of Physics, Beijing, China, (2)Peking University, Beijing, China, (3)University of Chicago, Geophysical Sciences, Chicago, IL, United States
The Formation of Haze During the Rise of Oxygen in the Atmosphere of the Early Earth (30622)
Sarah M Horst, Johns Hopkins University, Department of Earth and Planetary Sciences, Baltimore, MD, United States, Mark Jellinek, University of British Columbia, Vancouver, BC, Canada, Raymond Pierrehumbert, Univ of Chicago, Chicago, IL, United States and Margaret A Tolbert, University of Colorado at Boulder, Boulder, CO, United States
