U22B:
The New Jupiter as Revealed by Juno


Note: Abstract submissions to Union sessions are by invitation only.


Session ID#: 49705

Session Description:
NASA's Juno mission to Jupiter launched in 2011 and arrived at Jupiter on July 4, 2016.  The results of Juno have revolutionized our understanding of Jupiter and giant planets throughout our solar system and beyond.   As the largest and most massive planet in our solar system, Jupiter offers unique insight in the history of our solar system and how planetary systems in general form and evolve.  Juno's multidisciplinary study of Jupiter constrains the interior structure and atmospheric composition, investigates Jupiter's deep atmospheric dynamics, and provides the first in-situ investigation of Jupiter's polar magnetosphere and aurorae.  This session provides key results from Juno's discoveries as well as context with respect to current theory and models of Jupiter's formation and evolution.
OSPA Liaison:  Fran Bagenal, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Primary Convener:  Scott J Bolton, Southwest Research Institute, San Antonio, United States
Conveners:  Jonathan I Lunine, Cornell University, Department of Astronomy, Ithaca, NY, United States, Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States and Fran Bagenal, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Primary Liaison:  Scott J Bolton, Southwest Research Institute, San Antonio, United States
Chairs:  Scott J Bolton, Southwest Research Institute, San Antonio, United States and Jonathan I Lunine, Cornell University, Department of Astronomy, Ithaca, NY, United States

Cross-Listed:
  • A - Atmospheric Sciences
  • P - Planetary Sciences
  • SH - SPA-Solar and Heliospheric Physics
  • SM - SPA-Magnetospheric Physics
Index Terms:

5704 Atmospheres [PLANETARY SCIENCES: FLUID PLANETS]
5706 Aurorae [PLANETARY SCIENCES: FLUID PLANETS]
5724 Interiors [PLANETARY SCIENCES: FLUID PLANETS]
6220 Jupiter [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

David J Stevenson, California Institute of Technology, Pasadena, United States
Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States
Barry Mauk1, Scott J Bolton2, Steven Levin3, Alberto Adriani4, Frederic Allegrini2, Fran Bagenal5, Heidi N Becker6, John E P Connerney7, Randy Gladstone2 and William S Kurth8, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Jet Propulsion Laboratory, Pasadena, United States, (4)INAF-IAPS, Rome, Italy, (5)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (7)Space Research Corporation, Annapolis, United States, (8)University of Iowa, Iowa City, IA, United States
Candice J Hansen1, Alberto Adriani2, Heidi N Becker3, Randy Gladstone4, Glenn Orton5, G. Eichstädt6, M. A. Caplinger7, Michael A Ravine7, John Rogers8 and Scott J Bolton4, (1)Planetary Science Institute Tucson, Tucson, AZ, United States, (2)INAF-IAPS, Rome, Italy, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (6)Independent scholar, Stuttgart, Germany, (7)Malin Space Science Systems, San Diego, CA, United States, (8)British Astronomical Association, London, United Kingdom

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