01.08.19
Volcanic Plumes on Jupiter’s Moon Io
SAN ANTONIO — Dec. 31, 2018 — A team of space scientists has captured new images of a volcanic plume on Jupiter’s moon Io during the Juno mission’s 17th flyby of the gas giant. On Dec. 21, during winter solstice, four of Juno’s cameras captured images of the Jovian moon Io, the most volcanic body in our solar system. JunoCam, the Stellar Reference Unit (SRU), the Jovian Infrared Auroral Mapper (JIRAM) and the Ultraviolet Imaging Spectrograph (UVS) observed Io for over an hour, providing a glimpse of the moon’s polar regions as well as evidence of an active eruption.
“We knew we were breaking new ground with a multi-spectral campaign to view Io’s polar region, but no one expected we would get so lucky as to see an active volcanic plume shooting material off the moon’s surface,” said Scott Bolton, principal investigator of the Juno mission and an associate vice president of Southwest Research Institute’s Space Science and Engineering Division. “This is quite a New Year’s present showing us that Juno has the ability to clearly see plumes.”
JunoCam acquired the first images on Dec. 21 at 12:00, 12:15 and 12:20 coordinated universal time (UTC) before Io entered Jupiter’s shadow. The Images show the moon half-illuminated with a bright spot seen just beyond the terminator, the day-night boundary.
“The ground is already in shadow, but the height of the plume allows it to reflect sunlight, much like the way mountaintops or clouds on the Earth continue to be lit after the sun has set,” explained Candice Hansen-Koharcheck, the JunoCam lead from the Planetary Science Institute.
At 12:40 UTC, after Io had passed into the darkness of total eclipse behind Jupiter, sunlight reflecting off nearby moon Europa helped to illuminate Io and its plume. SRU images released by SwRI depict Io softly illuminated by moonlight from Europa. The brightest feature on Io in the image is thought to be a penetrating radiation signature, a reminder of this satellite’s role in feeding Jupiter’s radiation belts, while other features show the glow of activity from several volcanoes. “As a low-light camera designed to track the stars, the SRU can only observe Io under very dimly lit conditions. Dec. 21 gave us a unique opportunity to observe Io’s volcanic activity with the SRU using only Europa’s moonlight as our lightbulb,” said Heidi Becker, lead of Juno’s Radiation Monitoring Investigation, at NASA’s Jet Propulsion Laboratory.
Sensing heat at long wavelengths, the JIRAM instrument detects hotspots in the daylight and at night.
“Though Jupiter’s moons are not JIRAM’s primary objectives, every time we pass close enough to one of them, we take advantage of the opportunity for an observation,” said Alberto Adriani, a researcher at Italy’s National Institute of Astrophysics. “The instrument is sensitive to infrared wavelengths, which are perfect to study the volcanism of Io. This is one of the best images of Io that JIRAM has been able to collect so far.”
The latest images can lead to new insights into the gas giant’s interactions with its five moons, causing phenomena such as Io’s volcanic activity or freezing of the moon’s atmosphere during eclipse, added Bolton. JIRAM recently documented Io’s volcanic activity before and after eclipse. Io’s volcanoes were discovered by NASA’s Voyager spacecraft in 1979. Io’s gravitational interaction with Jupiter drives the moon’s volcanoes, which emit umbrella-like plumes of SO2 gas and produce extensive basaltic lava fields.
The recent Io images were captured at the halfway point of the mission, which is scheduled to complete a map of Jupiter in July 2021. Launched in 2011, Juno arrived at Jupiter in 2016. The spacecraft orbits Jupiter every 53 days, studying its auroras, atmosphere and magnetosphere.
The solar-powered Juno features eight scientific instruments designed to study Jupiter’s interior structure, atmosphere and magnetosphere. NASA’s Jet Propulsion Laboratory manages the Juno mission for Bolton. Juno is part of the New Frontiers Program, which is managed at Marshall Space Flight Center in Huntsville, Alabama, for NASA’s Science Mission Directorate. Lockheed Martin Space built the spacecraft, and SwRI provided two Juno instruments to study the massive Jovian aurora.
For more information, visit https://www.swri.org/industries/space-science.
About SwRI:
SwRI is an independent, nonprofit, applied research and development organization based in San Antonio, Texas, with nearly 2,600 employees and an annual research volume of more than $583 million. Southwest Research Institute and SwRI are registered marks in the U.S. Patent and Trademark Office. For more information, please visit newsroom.swri.org or www.swri.org.
“We knew we were breaking new ground with a multi-spectral campaign to view Io’s polar region, but no one expected we would get so lucky as to see an active volcanic plume shooting material off the moon’s surface,” said Scott Bolton, principal investigator of the Juno mission and an associate vice president of Southwest Research Institute’s Space Science and Engineering Division. “This is quite a New Year’s present showing us that Juno has the ability to clearly see plumes.”
JunoCam acquired the first images on Dec. 21 at 12:00, 12:15 and 12:20 coordinated universal time (UTC) before Io entered Jupiter’s shadow. The Images show the moon half-illuminated with a bright spot seen just beyond the terminator, the day-night boundary.
“The ground is already in shadow, but the height of the plume allows it to reflect sunlight, much like the way mountaintops or clouds on the Earth continue to be lit after the sun has set,” explained Candice Hansen-Koharcheck, the JunoCam lead from the Planetary Science Institute.
At 12:40 UTC, after Io had passed into the darkness of total eclipse behind Jupiter, sunlight reflecting off nearby moon Europa helped to illuminate Io and its plume. SRU images released by SwRI depict Io softly illuminated by moonlight from Europa. The brightest feature on Io in the image is thought to be a penetrating radiation signature, a reminder of this satellite’s role in feeding Jupiter’s radiation belts, while other features show the glow of activity from several volcanoes. “As a low-light camera designed to track the stars, the SRU can only observe Io under very dimly lit conditions. Dec. 21 gave us a unique opportunity to observe Io’s volcanic activity with the SRU using only Europa’s moonlight as our lightbulb,” said Heidi Becker, lead of Juno’s Radiation Monitoring Investigation, at NASA’s Jet Propulsion Laboratory.
Sensing heat at long wavelengths, the JIRAM instrument detects hotspots in the daylight and at night.
“Though Jupiter’s moons are not JIRAM’s primary objectives, every time we pass close enough to one of them, we take advantage of the opportunity for an observation,” said Alberto Adriani, a researcher at Italy’s National Institute of Astrophysics. “The instrument is sensitive to infrared wavelengths, which are perfect to study the volcanism of Io. This is one of the best images of Io that JIRAM has been able to collect so far.”
The latest images can lead to new insights into the gas giant’s interactions with its five moons, causing phenomena such as Io’s volcanic activity or freezing of the moon’s atmosphere during eclipse, added Bolton. JIRAM recently documented Io’s volcanic activity before and after eclipse. Io’s volcanoes were discovered by NASA’s Voyager spacecraft in 1979. Io’s gravitational interaction with Jupiter drives the moon’s volcanoes, which emit umbrella-like plumes of SO2 gas and produce extensive basaltic lava fields.
The recent Io images were captured at the halfway point of the mission, which is scheduled to complete a map of Jupiter in July 2021. Launched in 2011, Juno arrived at Jupiter in 2016. The spacecraft orbits Jupiter every 53 days, studying its auroras, atmosphere and magnetosphere.
The solar-powered Juno features eight scientific instruments designed to study Jupiter’s interior structure, atmosphere and magnetosphere. NASA’s Jet Propulsion Laboratory manages the Juno mission for Bolton. Juno is part of the New Frontiers Program, which is managed at Marshall Space Flight Center in Huntsville, Alabama, for NASA’s Science Mission Directorate. Lockheed Martin Space built the spacecraft, and SwRI provided two Juno instruments to study the massive Jovian aurora.
For more information, visit https://www.swri.org/industries/space-science.
About SwRI:
SwRI is an independent, nonprofit, applied research and development organization based in San Antonio, Texas, with nearly 2,600 employees and an annual research volume of more than $583 million. Southwest Research Institute and SwRI are registered marks in the U.S. Patent and Trademark Office. For more information, please visit newsroom.swri.org or www.swri.org.
JunoCam acquired three images of Io prior to when it entered eclipse, all showing a volcanic plume illuminated beyond the terminator. The image shown here, reconstructed from red, blue and green filter images, was acquired at 12:20 (UTC) on Dec. 21, 2018. The Juno spacecraft was approximately 300,000 km from Io.
Credit: Image Courtesy of NASA/SwRI/MSSS
Credit: Image Courtesy of NASA/SwRI/MSSS
Juno’s Radiation Monitoring Investigation collected this image of Jupiter’s moon Io with Juno’s Stellar Reference Unit (SRU) star camera shortly after Io was eclipsed by Jupiter at 12:40:29 (UTC) Dec. 21, 2018. Io is softly illuminated by moonlight from another of Jupiter’s moons, Europa. The brightest feature on Io is suspected to be a penetrating radiation signature. The glow of activity from several of Io’s volcanos is seen, including a plume circled in the image.
Credit: Image Courtesy of NASA/JPL-Caltech/SwRI
Credit: Image Courtesy of NASA/JPL-Caltech/SwRI
The Jovian Infrared Auroral Mapper (JIRAM) image was acquired at 12:30 (UTC) on Dec. 21, 2018. The instrument reveals very high temperatures at the location of a volcanic eruption on Io. This observation was taken during the same fully eclipsed period of images from the JunoCam and Stellar Reference Unit.
Credit: Image Courtesy of NASA/JPL-Caltech/SwRI/INAF
Credit: Image Courtesy of NASA/JPL-Caltech/SwRI/INAF