The article reviews crucial data obtained from remote observations of Io using telescopes like Hubble, JWST, and Keck, outlining their contributions to understanding volcanic emissions, atmospheric conditions, and plasma interactions within the Io-Jupiter system. It discusses the current knowledge on Io's mass loss and the variability of its environment. Looking ahead, the article highlights the potential of advanced telescopes such as the ELT, LAPYUTA, and HWO to further enhance our understanding of Io's dynamics and its role within Jupiter's magnetosphere, addressing existing knowledge gaps.
Remote observations from telescopes like Hubble, JWST, and Keck have provided crucial long-term data on Io's atmosphere, volcanic emissions, and plasma interactions.
Future telescopes such as ELT, LAPYUTA, and HWO will push the boundaries even further, significantly contributing to our understanding of Io and its interactions with Jupiter.
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