NASA’s Juno probe takes a close look at lava lakes on Jupiter’s moon Io

New findings from NASA’s Juno probe provide a more complete picture of the extent of lava lakes on Jupiter’s moon Io and include information for the first time about the volcanic processes at work there. These results come from Juno’s Jovian Infrared Auroral Mapper (JIRAM) instrument, provided by the Italian Space Agency, which “sees” in infrared light. Researchers published a paper on Juno’s most recent volcanic discoveries in Earth and Environment Communications.

Io has intrigued astronomers since 1610, when Galileo Galilei first discovered the Jovian moon, which is slightly larger than Earth. Some 369 years later, NASA’s Voyager 1 space probe captured a volcanic eruption on the Moon. Subsequent missions to Jupiter, with more flybys of Io, discovered additional plumes, as well as lava lakes. Scientists now believe that Io, which is stretched and compressed like an accordion by neighboring moons and Jupiter itself, is the most volcanically active world in the solar system. But while there are many theories about the types of volcanic eruptions on the Moon’s surface, there is little data to support them.

In May and October 2023, Juno flew by Io, being approximately 21,700 miles (35,000 kilometers) and 8,100 miles (13,000 kilometers) away, respectively. Among Juno’s instruments that got a close look at the alluring moon was JIRAM.

Designed to capture infrared light (invisible to the naked eye) that emerges from Jupiter’s depths, JIRAM probes the weather layer up to 50 to 70 kilometers below the gas giant’s cloud tops. But during Juno’s extended mission, the mission team also used the instrument to study the moons Io, Europa, Ganymede and Callisto. Images from JIRAM Io showed the presence of bright rings surrounding the ground of many hot spots.

“The high spatial resolution of JIRAM’s infrared images, combined with Juno’s favorable position during flybys, revealed that the entire surface of Io is covered in lava lakes contained in caldera-like formations,” said Alessandro Mura, Juno’s co-investigator. from the National Institute of Astrophysics in Rome. “In the region of Io’s surface where we have the most complete data, we estimate that about 3% of it is covered by one of these molten lava lakes.” (A caldera is a large depression formed when a volcano erupts and collapses.)

Fire-breathing lakes

Data from JIRAM’s flyby of Io not only highlights the moon’s abundant lava reserves, but also provides insight into what might be happening beneath the surface. Infrared images of several lava lakes on Io show a thin circle of lava at the boundary, between the central crust that covers most of the lava lake and the lake walls. Recycling of the melt is implied by the absence of lava flows on and beyond the lake edge, indicating that there is a balance between the melt that has spouted into the lava lakes and the melt that is returned to the underground system.

“We now have an idea of ​​what is the most common type of volcanism on Io: huge lava lakes where magma rises and falls,” Mura explained. “The lava crust is forced to break against the lake walls, forming the typical lava ring seen in Hawaiian lava lakes. The walls are likely hundreds of meters high, which explains why no observed generally no magma escaping from the pegs”—bowl-shaped features created by volcanism—“and moving across the surface of the moon.”

JIRAM data suggest that most of the surface area of ​​these Io hotspots is composed of rocky crust that rises and falls cyclically as a contiguous surface due to central upwelling of magma. In this hypothesis, as the crust touches the walls of the lake, friction prevents it from sliding, deforming it and eventually breaking apart, exposing the lava just below the surface.

An alternative hypothesis remains in play: Magma wells up in the middle of the lake, expands, and forms a crust that sinks along the lake’s edge, exposing the lava.

“We are just starting to look at the JIRAM results from close flybys of Io in December 2023 and February 2024,” said Scott Bolton, principal investigator for Juno at the Southwest Research Institute in San Antonio. “The observations show fascinating new insights into Io’s volcanic processes. Combining these new results with Juno’s longer-term campaign to monitor and map Io’s never-before-seen north and south pole volcanoes, JIRAM proves to be one of the most valuable tools for learning how this tortured world works.

Juno made its 62nd flyby of Jupiter, which included a flyby of Io at an altitude of about 18,175 miles (29,250 kilometers), on June 13. The 63rd flyby of the gas giant is scheduled for July 16.