Icarus 156, 76–106 (2002) doi:10.1006/icar.2001.6758, available online at http://www.idealibrary.com on Photochemistry of a Volcanically Driven Atmosphere on Io: Sulfur and Oxygen Species from a Pele-Type Eruption Julianne I. Moses Lunar and Planetary Institute, 3600 Bay Area Blvd., Houston, Texas 77058-1113 E-mail:
[email protected] Mikhail Yu. Zolotov Department of Earth and Planetary Sciences, Washington University CB1169, One Brookings Drive, St. Louis, Missouri 63130-4899 and Bruce Fegley, Jr. Department of Earth and Planetary Sciences, Planetary Chemistry Laboratory, McDonnell Center for the Space Sciences, Washington University CB1169, One Brookings Drive, St. Louis, Missouri 63130-4899 Received November 15, 2000; revised September 17, 2001 polar regions might also affect the surface spectral properties. We To determine how active volcanism might affect the standard predict that the S/O ratio in the torus and neutral clouds might picture of sulfur dioxide photochemistry on Io, we have developed be correlated with volcanic activity—during periods when volcanic a one-dimensional atmospheric model in which a variety of sulfur-, outgassing of S2 (or other molecular sulfur vapors) is prevalent, we oxygen-, sodium-, potassium-, and chlorine-bearing volatiles are would expect the escape of sulfur to be enhanced relative to that of volcanically outgassed at Io’s surface and then evolve due to photol- oxygen, and the S/O ratio in the torus and neutral clouds could be ysis, chemical kinetics, and diffusion. Thermochemical equilibrium correspondingly increased. c 2002 Elsevier Science (USA) calculations in combination with recent observations of gases in the Key Words: Io; photochemistry; atmospheres, composition; vol- Pele plume are used to help constrain the composition and physi- canism; geochemistry.