JunoCam Observations of Io

Abstract During multiple Juno encounters with Io in 2023 and 2024, the spacecraft's imaging system, JunoCam, acquired approximately one hundred images of Io. These images have a range of scales down to 1 km per pixel, and covered more than half of Io's surface, including the previously poorly resolved northern and southern polar regions. Some of the highest resolution images were acquired of Io's nightside, illuminated by Jupiter‐shine. Here we provide an overview of the JunoCam Io data set and discuss the peculiarities of JunoCam's “pushframe” imaging. Using JunoCam's high resolution coverage of the northern polar region, we have developed an improved geologic map of this previously poorly resolved area, and estimated the heights of 16 previously unidentified or poorly imaged mountains. In the higher resolution images, 14 new or modified plume deposits were identified, as were at least 20 probable new lava flows. Eight “Prometheus‐type” volcanic plumes were identified, five of which were associated with areas showing flow‐like surface changes.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-09-01
DOI
https://doi.org/10.1029/2024je008924
Citations
3
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
3.46

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article

JunoCam Observations of Io

A. G. Hayes, M. A. Caplinger, M. A. Ravine, Leslie Lipkaman et al.
3 citations
Journal of Geophysical Research Planets
Astro and Planetary Science
3.46
article

JunoCam Observations of Io

A. G. Hayes, M. A. Caplinger, M. A. Ravine, Leslie Lipkaman, D. A. Williams, R. M. C. Lopes, Jason Perry, P. Schenk, Madeline Pettine, J. T. Keane, J. Radebaugh, C. J. Hansen, Daniel Krysak, J. A. Rathbun, S. J. Bolton
article en
3 citations

Abstract

Abstract During multiple Juno encounters with Io in 2023 and 2024, the spacecraft's imaging system, JunoCam, acquired approximately one hundred images of Io. These images have a range of scales down to 1 km per pixel, and covered more than half of Io's surface, including the previously poorly resolved northern and southern polar regions. Some of the highest resolution images were acquired of Io's nightside, illuminated by Jupiter‐shine. Here we provide an overview of the JunoCam Io data set and discuss the peculiarities of JunoCam's “pushframe” imaging. Using JunoCam's high resolution coverage of the northern polar region, we have developed an improved geologic map of this previously poorly resolved area, and estimated the heights of 16 previously unidentified or poorly imaged mountains. In the higher resolution images, 14 new or modified plume deposits were identified, as were at least 20 probable new lava flows. Eight “Prometheus‐type” volcanic plumes were identified, five of which were associated with areas showing flow‐like surface changes.

Journal of Geophysical Research PlanetsVol. 130(9)
Brigham Young University (US), Southwest Research Institute (US), Planetary Science Institute (US), Jet Propulsion Laboratory (US), University of Arizona (US), Cornell University (US), Malin Space Science Systems (United States) (US), Arizona State University (US), Lunar and Planetary Institute (US)
National Aeronautics and Space Administration, California Institute of Technology, Southwest Research Institute, Jet Propulsion Laboratory
Openalex Percentile: Top 7%
Astro and Planetary Science
3.46
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