Titlebook: Io: A New View of Jupiter’s Moon ; Rosaly M. C. Lopes,Katherine de Kleer,James Tuttle Book 2023Latest edition The Editor(s) (if applicable

Infraction

Alfred S. McEwen,Amanda F. Haapala,Laszlo P. Keszthelyi,Kathleen E. Mandtn connection with common-pool resources. While initial interpretations of the commons emphasized their implicit vulnerabilities and thus revealed rather tragic notions, especially Ostrom’s insights on self-organized governance instead propose ways in which collective groups that jointly provide comm

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endocardium

Setting the Stage: Formation and Earliest Evolution of Io, in Jupiter’s equatorial plane. As such they must have formed from a dissipative disk of gas and/or solids in orbit around Jupiter. The ice-rich compositions of Europa and, especially, Ganymede and Callisto, indicate that this circumplanetary disk must have been cool enough for water ice stability.

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Panacea

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sundowning

The Composition of Io,xamines the many different, but frustratingly indirect, constraints we have on the bulk composition of this restless moon. A detailed consideration of Io’s lavas is used to illustrate how decades of research have bounded, but not pinned down, the chemistry of Io. A self-consistent model for the core

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The Plumes and Atmosphere of Io,source of Io’s atmosphere is sublimation of SO. frost, at times and/or locally volcanoes have a substantial effect on the atmosphere (and sometimes dominate), as shown both via observations and model simulations. The effect of sputtering is less clear, but may be important at high latitudes, and per

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Space Environment of Io,act of magnetospheric ions on Io’s atmosphere supplies clouds of escaping neutral atoms that populate a substantial fraction of its orbit. At the same time, ionization of atoms in the neutral cloud is the primary source of magnetospheric plasma. The stability of this feedback loop depends on the pla

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