Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55

We report volcanic changes on Io since the last Galileo (2002) and New Horizons (2007) flybys as observed by NASA’s Juno spacecraft, examining Io’s volcanism down to the local scale (<10 km pixel ^−1 ). From 3428 Jovian Infrared Auroral Mapper image frames obtained between 2017 March 21 (PJ5) and...

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Main Authors: Jason E. Perry, Ashley Gerard Davies, David A. Williams, David M. Nelson
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Planetary Science Journal
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Online Access:https://doi.org/10.3847/PSJ/adbae3
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author Jason E. Perry
Ashley Gerard Davies
David A. Williams
David M. Nelson
author_facet Jason E. Perry
Ashley Gerard Davies
David A. Williams
David M. Nelson
author_sort Jason E. Perry
collection DOAJ
description We report volcanic changes on Io since the last Galileo (2002) and New Horizons (2007) flybys as observed by NASA’s Juno spacecraft, examining Io’s volcanism down to the local scale (<10 km pixel ^−1 ). From 3428 Jovian Infrared Auroral Mapper image frames obtained between 2017 March 21 (PJ5) and 2023 October 15 (PJ55), a catalog of 2305 hot spot detections with temperatures >200 K at 325 individual sites of volcanic activity has been generated. Where possible, hot spot color temperature, emitting area, and power output are calculated. Some prominent areas of volcanic activity first identified or better resolved in Juno data (Tonatiuh, Lei-Kung Fluctus, Volund, Guaraci Fluctus, Seth Patera, and others) are described. We examined their appearance, volcanological and geological settings, observed thermal emission, and evolving behavior, and quantified the changes that have taken place. Volcanic activity at Tonatiuh and Guaraci Fluctus, the sites of newly imaged lava flows, are examined in detail. At Tonatiuh, JunoCam data provide important context; at Guaraci Fluctus, the combination of data from multiple assets yields a comprehensive understanding of the evolution of a specific eruption episode. We further examine different types of active paterae, some possibly containing lava lakes. A group of bright eruptions are identified whose spatial and temporal locations suggest regional clustering. Our estimates of volcanic thermal emission are broadly consistent with previous analyses of spacecraft data. All derived products are available from the Io Geographical Information System database at Arizona State University. Appendix A contains newly approved feature names.
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spelling doaj-art-0f1540aed26948c8a402a46a06aabd0d2025-08-20T03:06:43ZengIOP PublishingThe Planetary Science Journal2632-33382025-01-01648410.3847/PSJ/adbae3Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55Jason E. Perry0https://orcid.org/0000-0002-6802-7889Ashley Gerard Davies1https://orcid.org/0000-0003-1747-8142David A. Williams2https://orcid.org/0000-0002-7930-9347David M. Nelson3https://orcid.org/0000-0001-9773-2651Lunar and Planetary Laboratory, University of Arizona , 1629 E University Boulevard, Tucson, AZ 85721, USA ; jeperry1@arizona.eduJet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Drive, Pasadena, CA 91109, USA ; Ashley.Davies@jpl.nasa.govArizona State University , Tempe, AZ, USA ; David.Williams@asu.edu, nelson99@asu.eduArizona State University , Tempe, AZ, USA ; David.Williams@asu.edu, nelson99@asu.eduWe report volcanic changes on Io since the last Galileo (2002) and New Horizons (2007) flybys as observed by NASA’s Juno spacecraft, examining Io’s volcanism down to the local scale (<10 km pixel ^−1 ). From 3428 Jovian Infrared Auroral Mapper image frames obtained between 2017 March 21 (PJ5) and 2023 October 15 (PJ55), a catalog of 2305 hot spot detections with temperatures >200 K at 325 individual sites of volcanic activity has been generated. Where possible, hot spot color temperature, emitting area, and power output are calculated. Some prominent areas of volcanic activity first identified or better resolved in Juno data (Tonatiuh, Lei-Kung Fluctus, Volund, Guaraci Fluctus, Seth Patera, and others) are described. We examined their appearance, volcanological and geological settings, observed thermal emission, and evolving behavior, and quantified the changes that have taken place. Volcanic activity at Tonatiuh and Guaraci Fluctus, the sites of newly imaged lava flows, are examined in detail. At Tonatiuh, JunoCam data provide important context; at Guaraci Fluctus, the combination of data from multiple assets yields a comprehensive understanding of the evolution of a specific eruption episode. We further examine different types of active paterae, some possibly containing lava lakes. A group of bright eruptions are identified whose spatial and temporal locations suggest regional clustering. Our estimates of volcanic thermal emission are broadly consistent with previous analyses of spacecraft data. All derived products are available from the Io Geographical Information System database at Arizona State University. Appendix A contains newly approved feature names.https://doi.org/10.3847/PSJ/adbae3IoGalilean satellitesVolcanism
spellingShingle Jason E. Perry
Ashley Gerard Davies
David A. Williams
David M. Nelson
Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
The Planetary Science Journal
Io
Galilean satellites
Volcanism
title Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
title_full Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
title_fullStr Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
title_full_unstemmed Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
title_short Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
title_sort hot spot detections and volcanic changes on io during the juno epoch orbits pj5 to pj55
topic Io
Galilean satellites
Volcanism
url https://doi.org/10.3847/PSJ/adbae3
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