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- P41B-05: HST+JWST - Juno Io Campaign 2024-2025: Connecting Volcanos to the Plasma Environment
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Kurt Retherford, Southwest Research Institute (First Author, Presenting Author)
Fran Bagenal, University of Colorado Boulder
Tracy Becker, Southwest Research Institute
Matthew Burger, STScI
Nathaniel Cunningham, Nebraska Wesleyan University
Vincent Dols, University of Colorado Boulder
Lori Feaga, University of Maryland
Amanda Hendrix, Planetary Science Institute
Vincent Hue, Laboratoire d'Astrophysique de Marseille
Kandis Lea Jessup, Southwest Research Inst
Joshua Kammer, Southwest Research Institute
Katherine de Kleer, California Institute of Technology
Emmanuel Lellouch, LESIA, Observatoire de Paris
Melissa McGrath, SETI Institute Mountain View
Zachariah Milby, University of Colorado
Philippa Molyneux, Southwest Research Institute
Edward Nerney, University of Colorado Boulder
Jonathan Nichols, University of Leicester
Lorenz Roth, KTH Royal Institute of Technology
Joachim Saur, University of Cologne
Carl Schmidt, Boston University
H. Smith, Johns Hopkins University Applied Physics Laboratory
John Spencer, Southwest Research Institute
Samantha Trumbo, University of California San Diego
Michael Velez, University of Texas at San Antonio
Shawn Brueshaber, Michigan Technological University
Simon Mendenhall, University of Texas at San Antonio
Randy Gladstone, Southwest Research Institute
Thomas Greathouse, Southwest Research Institute
Thomas Momary, NASA Jet Propulsion Laboratory
Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology
Alessandro Mura, IAPS-INAF
Joey Mukherjee, Southwest Research Inst
Steven Ybarra, Southwest Research Institute
Umer Salman, Southwest Research Institute
We have acquired numerous Hubble Space Telescope observations of Jupiter's moon Io during the era where the Juno spacecraft flew past or encountered Io. Several instruments and modes observed Io in different ways, targeting its surface volcanoes on up toward the region of gas that escaped Io's gravity, which is an important supplier of material to the Jovian magnetosphere. An additional supporting observation of Io with the James Webb Space Telescope complements this campaign. Roughly 40% of the large program observations are in hand at the time of the abstract submission, with the majority of remaining observations planned for the time of the presentation.
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