Io’s Atmospheric Collapse observed during Eclipse

An artist’s rendering depicts Io’s volcanic plumes creating the atmosphere in sunlight. Credit: Image courtesy of Southwest Research Institute

Research reveals freezing effects of Jupiter’s shadow on moon’s volcanic gases. A study led by SwRI’s Constantine Tsang concluded that Io’s thin atmosphere, which consists primarily of sulfur dioxide (SO2) gas emitted from volcanoes, collapses as the SO2 freezes onto the surface as ice when Io is shaded by Jupiter. When the moon moves out of eclipse and ice warms, the atmosphere reforms through sublimation, where ice converts directly to gas. “This research is the first time scientists have observed this phenomenon directly, improving our understanding of this geologically active moon,” said Tsang, SwRI’s Space Science and Engineering Division.

The team used the 8meter Gemini North telescope in Hawaii and the Texas Echelon Cross Echelle Spectrograph (TEXES). Data showed that Io’s atmosphere begins to “deflate” when the temperatures drop from -235F in sunlight to -270F during eclipse. Eclipse occurs 2 hours of every Io day (1.7 Earth days). In full eclipse, the atmosphere collapses as most SO2 gas settles as frost on the moon’s surface. The atmosphere redevelops as the surface warms once the moon returns to full sunlight.

John Spencer said “Though Io’s hyperactive volcanoes are the ultimate source of the SO2, sunlight controls the atmospheric pressure on a daily basis by controlling the temperature of the ice on the surface. We’ve long suspected this, but can finally watch it happen.” Prior to the study, no direct observations of Io’s atmosphere in eclipse had been possible because Io’s atmosphere is difficult to observe in the darkness of Jupiter’s shadow. This breakthrough was possible because TEXES measures the atmosphere using heat radiation, not sunlight, and the giant Gemini telescope can sense the faint heat signature of Io’s collapsing atmosphere.

Tsang and Spencer’s observations occurred over 2 nights in November 2013, when Io was more than 420 million miles from Earth. On both occasions, Io was observed moving in and out of Jupiter’s shadow, for ~40 minutes before and after eclipse. Io is the most volcanically active object in the solar system. Tidal heating, the result of Io’s gravitational interaction with Jupiter, drives the moon’s volcanic activity. Io’s volcanoes emit umbrella-like plumes of SO2 gas extending up to 300 miles above the moon’s surface and produce extensive basaltic lava fields that can flow for hundreds of miles.

This study is also timely given that NASA’s Juno spacecraft entered Jupiter orbit on July 4. “Io spews out gases that eventually fill the Jupiter system, ultimately seeding some of the auroral features seen at Jupiter’s poles,” Tsang said. “Understanding how these emissions from Io are controlled will help paint a better picture of the Jupiter system.” http://www.swri.org/9what/releases/2016/io-atmosphere-collapse-eclipse.htm.V6Cn9k3NZYg