A Lancaster University PhD student has measured the optical depth of Saturn’s rings using a new method based on how much sunlight reached the Cassini spacecraft while it was in the shadow of the rings. The optical depth is connected to the transparency of an object and a measure of how far light can travel through that object before it gets absorbed or scattered.
The research, led by Lancaster University in collaboration with the Swedish Institute of Space Physics, is published in the Monthly Notices of the Royal Astronomical Society.
The NASA-ESA Cassini spacecraft was launched in 1997 and reached Saturn in 2004, carrying out the most extensive survey of the planet and its moons to date. The mission ended in 2017 when Cassini plunged into the Saturnian atmosphere, after diving 22 times between the planet and its rings.
Video of the Cassini spacecraft moving through the plane of Saturn’s ring system, created by George Xystouris using NASA Eyes. Credit: NASA/JPL
Lancaster University PhD student George Xystouris, under the supervision of Dr Chris Arridge, analysed historic data from the Langmuir Probe on board Cassini, an instrument that was measuring the cold plasma, i.e. low energy ions and electrons, in the magnetosphere of Saturn.
For their study they focused on solar eclipses of the spacecraft: periods where Cassini was in the shadow of Saturn or the main rings. During each eclipse, the Langmuir Probe recorded dramatic changes in the data.
George said: “As the probe is metallic, whenever it is sunlit, the sunlight can give enough energy to the probe to release electrons. This is the photoelectric effect, and the electrons that are released are so-called ‘photoelectrons’. They can create problems though, as they have the same properties as the electrons in the cold plasma around Saturn and there is not an easy way to separate the two.”
“Focusing on the data variations we realised that they were connected with how much sunlight each ring would allow to pass. Eventually, using the properties of the material that the Langmuir Probe was made of, and how bright the Sun was in Saturn’s neighbourhood, we managed to calculate the change in the photoelectrons number for each ring, and calculate Saturn’s rings optical depth.
“This was a novel and exciting result! We used an instrument that is mainly used for plasma measurements to measure a planetary feature, which is a unique use of the Langmuir Probe, and our results agreed with studies that used high-resolution imagers to measure the transparency of the rings.”
Τhe main rings, which extend up to 140,000 km from the planet, but have a maximum thickness of only 1km, are to disappear from view from Earth by 2025. In that year the rings will be tilted edge-on to Earth, making it almost impossible to view them. They will tilt back towards Earth during the next phase of Saturn's 29-year orbit, and will continue to become more visible and brighter until 2032.
Professor Mike Edmunds, the President of the Royal Astronomical Society, added: "It is always good to see a postgraduate student involved in using space probe instrumentation in an unusual and inventive way. Innovation of this kind is just what is needed in astronomical research - and an approach which many former students who are in a variety of careers are applying to help address the world's problems".
Media contacts
Gillian Whitworth
Lancaster University
gillian.whitworth@lancaster.ac.uk
Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877699
press@ras.ac.uk
Science contacts
George Xystouris
Lancaster University
g.xystouris@lancaster.ac.uk
Dr Chris Arridge
Lancaster University
c.arridge@lancaster.ac.uk
Image and video
Artist’s impression of Cassini in orbit around Saturn. Credit: NASA / JPL – Caltech
Movie of the Cassini spacecraft moving through the plane of Saturn’s ring system, created using the NASA’s Eyes tool. Credit: George Xystouris / NASA / JPL
Further information
The new work appears in: “Estimating the optical depth of Saturn’s main rings using the Cassini Langmuir Probe”, Georgios Xystouris, Christopher S Arridge, Michiko M Morooka and Jan-Erik Wahlund, Monthly Notices of the Royal Astronomical Society, Volume 526, Issue 4, December 2023, Pages 5839–5860.
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