Scientists observe Io’s atmospheric collapse during eclipse

Research reveals freezing effects of Jupiter’s shadow on moon’s volcanic gases

2 August 2016

Joint Release

WASHINGTON, DC — A team of scientists has documented atmospheric changes on Io, Jupiter’s volcanically active satellite, as the giant planet casts its shadow over the moon’s surface during daily eclipses.

A new study concludes that Io’s thin atmosphere, which consists primarily of sulfur dioxide gas emitted from volcanoes, collapses as the sulfur dioxide 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 Constantine Tsang, a senior research scientist in Southwest Research Institute’s Space Science and Engineering Division in Boulder, Colorado, and lead author of the new study.

Jupiter IO Artistic Concept FINAL

The findings were published in a new study in the Journal of Geophysical Research-Planets, a publication of the American Geophysical Union. The team used the eight-meter Gemini North telescope in Hawaii and the Texas Echelon Cross Echelle Spectrograph (TEXES) for this research.

Data showed that Io’s atmosphere begins to “deflate” when the temperatures drop from -235 degrees Fahrenheit in sunlight to -270 degrees Fahrenheit during eclipse. Eclipse occurs 2 hours of every Io day (1.7 Earth days). In full eclipse, the atmosphere effectively collapses as most of the sulfur dioxide gas settles as frost on the moon’s surface. The atmosphere redevelops as the surface warms once the moon returns to full sunlight.

“This confirms that Io’s atmosphere is in a constant state of collapse and repair, and shows that a large fraction of the atmosphere is supported by sublimation of sulfur dioxide ice,” said John Spencer, an SwRI scientist who also participated in the study. “Though Io’s hyperactive volcanoes are the ultimate source of the sulfur dioxide, 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 two 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 a period about 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 sulfur dioxide 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.”

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Title

“The Collapse of Io’s Primary Atmosphere in Jupiter Eclipse”

Authors:
Constantine C.C. Tsang: Southwest Research Institute, Department of Space Studies, Boulder, CO, USA;

John R. Spencer: Southwest Research Institute, Department of Space Studies, Boulder, CO, USA;

Emmanuel Lellouch: Observatoire de Meudon, LEISA, Meudon F-92195, France;

Miguel Lopez Valverde: Instituto de Astrofisica de Andalucia/CSIC, Glorieta de la Astronomia s/n, Granada, Spain;

Matthew J. Richter: University of California at Davis, Department of Physics, Davis, CA, USA.

Contact Information for the Authors:
Constantine Tsang: +1 (720) 208-7202, con@boulder.swri.edu


AGU Contact:

Lauren Lipuma
+1 (202) 777-7396
llipuma@agu.org

 
SwRI Contact:
Robert Crowe
+1 (210) 522-4630
robert.crowe@swri.org