Jupiter’s largest moon, Ganymede, was closely examined by NASA’s Juno mission in June 2021 for signs of magnetic reconnection.
As the magnetic field lines of Jupiter and Ganymede fused, snapped, and reoriented heating and accelerating the charged particles in the vicinity, a team led by Southwest Research Institute used Juno data to investigate the electron and ion particles and magnetic fields.
“Ganymede is the only moon in our solar system with its own magnetic field,” said Juno Principal Investigator Dr. Scott Bolton of SwRI. “The snapping and reconnecting of Ganymede’s magnetic field lines with Jupiter’s create the magnetospheric fireworks.”
The magnetic energy that has been accumulated is transformed into kinetic energy and heat during the explosive physical process of magnetic reconnection. In the magnetopause, which separates the two zones, Ganymede’s tiny magnetosphere interacts with Jupiter’s enormous magnetosphere.
“We interpreted the presence of accelerated electrons traveling along the magnetic field at Ganymede’s magnetopause as evidence that magnetic reconnection was occurring there during the Juno flyby,” said Dr. Robert Ebert, lead author of a Geophysical Research Letters paper describing the findings.
“These observations further support the notion that magnetic reconnection at Ganymede’s magnetopause can be a driver of dynamic processes in the local space environment around this moon of Jupiter.”
Nothing is simple or small when you have the biggest planet in the solar system as your neighbor. This was the first measurement of this complicated interaction at Ganymede. This gives us a very early tantalizing taste of the information we expect to learn from ESA’s JUICE mission.
Thomas Greathouse
Increased electron fluxes, including accelerated, magnetic field-aligned electrons, were seen by Juno’s SwRI-developed Jovian Auroral Distributions Experiment (JADE). Reconnection as observed by Juno is thought to be related to the generation of Ganymede’s aurora.
“The accelerated electrons observed by JADE are similar to those observed by NASA’s Magnetospheric Multiscale (MSS) spacecraft during reconnection at the Earth’s magnetopause,” said Dr. Stephen Fuselier, a co-author of the paper. “That’s one of the exciting results from the Ganymede flyby: Despite the vast differences between Ganymede and Earth, we find commonality in the universal process of magnetic reconnection.”
During the Juno flyby, the SwRI-led Ultraviolet Spectrograph (UVS) observed Ganymede’s auroral emissions, which are expected to be produced by electrons accelerated via magnetic reconnection.
SwRI has built two additional UVS instruments to operate in Jupiter orbit aboard ESA’s JUpiter ICy moons Explorer (JUICE) spacecraft and NASA’s Europa Clipper. The European Space Agency’s JUICE mission is scheduled to launch in April 2023 and arrive at Jupiter in 2031. NASA’s Europa Clipper is scheduled to launch in October 2024 and arrive at Jupiter in 2030.
“Nothing is simple or small when you have the biggest planet in the solar system as your neighbor,” said Thomas Greathouse, a Juno scientist from SwRI. “This was the first measurement of this complicated interaction at Ganymede. This gives us a very early tantalizing taste of the information we expect to learn from ESA’s JUICE mission.”
