Extensive Surface Changes on Io Seen in High-Resolution LBT/SHARK Visible Wavelength Imagery in Early 2025
Extensive Surface Changes on Io Seen in High-Resolution LBT/SHARK Visible Wavelength Imagery in Early 2025
Ashley Gerard Davies1, Gianluca Li Causi2, Jason Perry3, Stuart Jefferies4, Fernando Pedichini2, Dino Mesa5, David A Williams6, Imke De Pater7, David M Nelson6, Fabian Baron8, Albert Conrad9, Katherine de Kleer10, Simone Antoniucci2, Douglas Hope11, Maria Bergomi5, Francesco D'Alessio5, Simone Filomeno2, Tania Gomes Machado5, Fulvio Laudisio5, Luca Marafatto12, Ester Marini13, Roberto Piazzesi5, Davide Ricci5, Vincenzo Testa13, Piero Vaccari5 and Daniele Vassallo5, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy, (3)University of Arizona, Tucson, AZ, United States, (4)Georgia State University, Atlanta, GA, United States, (5)INAF-Osservatorio Astronomico di Padova, Padova, Italy, (6)Arizona State University, Tempe, AZ, United States, (7)Univ California Berkeley, Berkeley, United States, (8)Georgia State University, Atlanta, United States, (9)University of Arizona, LBTO, Tucson, AZ, United States, (10)California Institute of Technology, Geological and Planetary Sciences, Pasadena, United States, (11)Georgia Tech Research Institute, Atlanta, United States, (12)5INAF-Osservatorio Astronomico di Padova, Padova, Italy, (13)2INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy