GeminiFocus 2014 Year in Review | Page 11

Figure 1. Detection of the three outbursts. Panels a-c are observations at the W.M. Keck Observatory; the image in panel d was captured at Gemini N. Figure adapted from de Pater et al., 2014, and de Kleer et al., 2014. During this time, volcanic activity was both widespread and vigorous on all the terrestrial planets and many smaller bodies; ancient volcanic features on their surfaces preserve records of this activity. As the Solar System aged and cooled, active volcanism died out on most of these bodies, while on planets such as Earth, where it still takes place today, the activity has vastly diminished in intensity. An exception to this trend is Jupiter’s moon Io, which hosts hundreds of active volcanoes over a surface area smaller than the continent of Asia. The most energetic eruptions on Io dwarf anything we see on Earth today — in temperature, power, and spatial extent. Io’s blasts can produce sulfurous plumes that reach hundreds of miles above the moon’s surface. The moon’s extreme volcanism is powered by tidal heating: Io is locked in an orbital resonance with the neighboring moons Europa and Ganymede, meaning that it encounters these moons at the same position in each orbit. This leads to a coherent gravitational pull that forces Io into an eccentric path around January 2015 Jupiter. The changing distance from Jupiter over the course of each orbit — a mere 1.77 days — causes the moon’s surface to bulge by varying amounts, which generates the intense internal friction that heats Io’s interior and powers its volcanic activity. Although Io is the only of Jupiter’s moons to display active surface volcanism, the gravitational interaction that heats its interior also acts on Europa and Ganymede, keeping their interiors warm enough to host subsurface oceans of liquid water. Though the heating processes in these moons are hidden from view by their icy surfaces, the insight we gain into heat dissipation in Io’s interior is directly applicable to Europa and Ganymede, and can help us understand the formation and history of their hidden oceans. Observing Volcanoes from a Volcano On the night of August 15, 2013, Imke de Pater (University of California Berkeley), a member of our team, used the W.M. Keck 2014 Year in Review GeminiFocus 9