EGU25-7099, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-7099
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 01 May, 11:30–11:40 (CEST)
 
Room 0.94/95
Observations of Io from Juno's close flybys
Alessandro Mura1, Francesca Zambon1, Federico Tosi1, Rosaly Lopes2, Peter Mouginis-Mark3, Scott Bolton4, Jani Radebaugh5, Julie Rathbun6, Melissa Mirino1, Matteo Paris1, Christina Plainaki7, Davide Grassi1, Alberto Adriani1, Roberto Sordini1, Giuseppe Piccioni1, GIuseppe Sindoni7, Raffaella Noschese1, and Andrea Cicchetti1
Alessandro Mura et al.
  • 1INAF, IAPS, Rome, Italy (alessandro.mura@inaf.it)
  • 2JPL-CalTech, Pasadena, CA, USA
  • 3Hawaii Univ., HI, USA
  • 4SwRI, San Antonio, TX, USA
  • 5B. Young Univ., UT, USA
  • 6Cornell Univ., Itacha, NY, USA
  • 7ASI, Rome, Italy

JIRAM (Jovian Infrared Auroral Mapper) is an imager/spectrometer
onboard Juno, primarily designed for studying Jupiter's atmosphere and
auroral emissions. During its mission, JIRAM also obtained extensive
data on Io, the most volcanically active body in the solar system. The
instrument combines imaging and spectroscopy in a single device. The
imager operates in two bands: the "L" band (~3.3 to 3.6  µm), which primarily
detects surface albedo, and the "M" band (~4.5 to 5 µm), optimized for
mapping thermal structures. The spectrometer covers a range of 2 to 5
µm with a spectral resolution of 9 µm. With an angular resolution of
0.01°/pixel, JIRAM achieved a spatial resolution of up to 300 m during
close flybys of Io.
This work summarizes JIRAM’s observations of Io during the first 62
Juno orbits, and in particular the last ones, where the observation
conditions were more favourable. Detailed thermal maps reveal a
multitude of volcanic hotspots, including ring-shaped near-infrared
emissions from numerous lava lakes. The evolution of Loki Patera, the
largest and most active lava lake on Io, was monitored over nearly two
years, providing new insights into its thermal characteristics. These
observations contribute significantly to our understanding of Io’s
dynamic volcanism and thermal processes

How to cite: Mura, A., Zambon, F., Tosi, F., Lopes, R., Mouginis-Mark, P., Bolton, S., Radebaugh, J., Rathbun, J., Mirino, M., Paris, M., Plainaki, C., Grassi, D., Adriani, A., Sordini, R., Piccioni, G., Sindoni, G., Noschese, R., and Cicchetti, A.: Observations of Io from Juno's close flybys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7099, https://doi.org/10.5194/egusphere-egu25-7099, 2025.