Geophysical Research Letters (Jun 2024)

Observation of Io's Resurfacing via Plume Deposition Using Ground‐Based Adaptive Optics at Visible Wavelengths With LBT SHARK‐VIS

  • Al Conrad,
  • Fernando Pedichini,
  • Gianluca Li Causi,
  • Simone Antoniucci,
  • Imke dePater,
  • Ashley Gerard Davies,
  • Katherine deKleer,
  • Roberto Piazzesi,
  • Vincenzo Testa,
  • Piero Vaccari,
  • Martina Vicinanza,
  • Jennifer Power,
  • Steve Ertel,
  • Joseph C. Shields,
  • Sam Ragland,
  • Fabrizio Giorgi,
  • Stuart M. Jefferies,
  • Douglas Hope,
  • Jason Perry,
  • David A. Williams,
  • David M. Nelson

DOI
https://doi.org/10.1029/2024GL108609
Journal volume & issue
Vol. 51, no. 11
pp. n/a – n/a

Abstract

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Abstract Since volcanic activity was first discovered on Io from Voyager images in 1979, changes on Io's surface have been monitored from both spacecraft and ground‐based telescopes. Here, we present the highest spatial resolution images of Io ever obtained from a ground‐based telescope. These images, acquired by the SHARK‐VIS instrument on the Large Binocular Telescope, show evidence of a major resurfacing event on Io's trailing hemisphere. When compared to the most recent spacecraft images, the SHARK‐VIS images show that a plume deposit from a powerful eruption at Pillan Patera has covered part of the long‐lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth‐based telescopes. The SHARK‐VIS instrument ushers in a new era of high resolution imaging of Io's surface using adaptive optics at visible wavelengths.

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