Solar System lightshows to be probed by Leicester astronomers
An artistic representation of how the northern infrared aurora on Uranus would have looked like in 2006. Credit to NASA, ESA and M. Showalter (SETI Institute) for the background image of Uranus, as was observed by the Hubble Space Telescope (in the visible spectrum) in August 2005.
A team of astronomers at the University of Leicester will be searching for explanations for the some of the spectacular light shows seen in the atmospheres of planets in our solar system.
They have been awarded observation time with the James Webb Space Telescope (JWST) by the Space Telescope Science Institute (STScI) for two programmes that will focus on the mysterious aurorae of the gas giants Saturn and Uranus. Their successful proposals were among 1,931 submissions for the James Webb Space Telescope (JWST) Cycle 3 General Observer Program.
The team, led by Dr Henrik Melin from the University of Leicester School of Physics and Astronomy, will be trying to unravel the mysteries of the aurorae on two of our solar system’s most distant and largest planets.
Both planets show auroral emissions, caused by highly energetic charged particles, which are funnelled down and collide with a planet's atmosphere via the planet's magnetic field lines. On Earth, the most famous results of this process are the spectacles of the Northern and Southern Lights.
The first project that Dr Melin’s team will use the JWST for will observe the aurora of Uranus, of which very little is known. The conduit of the auroral currents is the magnetic field, which at Uranus is full of strange complexity.
The project will capture images over the course of a single Uranian day, or one full rotation of the planet, in the early months of 2025. This way, the team will be able to map the auroral emissions across a whole rotation Uranus’s magnetic field to answer their key question: are the emissions produced via the interaction with the solar wind (like the Earth), or are there internal sources within the system (like Jupiter), or somewhere in-between (like Saturn)?
Credit: NASA, ESA, CSA, STScI, M. Tiscareno (SETI Institute), M. Hedman (University of Idaho), M. El Moutamid (Cornell University), M. Showalter (SETI Institute), L. Fletcher (University of Leicester), H. Hammel (AURA); image processing by J. DePasquale (STScI).
For the second project, led by Luke Moore at the Boston University Center for Space Physics, the astronomers will observe Saturn’s northern auroral region through an entire Saturnian day, 10.6 hours in length, to observe the changing temperature of this region as the planet rotates. In revealing the atmospheric auroral energies for the first time we can hunt for a source of Saturn’s atmospherically driven aurora, and thus contextualize this new process more widely, allowing us to understand whether the process is important at Earth, other planets in the solar system, and within astrophysical objects across the universe.
Both projects will use the JWST NIRSpec instrument.
Dr Henrik Melin from the University of Leicester School of Physics and Astronomy said: “JWST is already changing how we perceive the Universe, from the Solar System, our very own cosmic backyard, to the first galaxies formed at the beginning of time. I am thrilled to have been awarded time on this remarkable observatory, and this data will fundamentally shape our understanding of both Saturn and Uranus.”