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The ring system orbits much further out than is typical for other ring systems, calling into question current theories of how ring systems are formed. The ring system is around a dwarf planet, named Quaoar, which is approximately half the size of Pluto and orbits the Sun beyond Neptune.
The discovery, published in Nature, was made by an international team of astronomers led by the University of Sheffield and including researchers at the University of Birmingham.
The detection of this ring involved a large observation effort using different ground-based observatories which includes the 1m Artemis telescope of the SPECULOOS Northern observatory in Tenerife. The University of Birmingham is part of the SPECULOOS project, which is actually a survey to search for Earth-like planets orbiting red dwarf stars, and operates observatories around the Globe.
The rings are too small and faint to see directly in an image. Instead, the researchers made their discovery by observing an occultation, when the light from a background star was blocked by Quaoar as it orbits the Sun. The event lasted less than a minute, but was unexpectedly preceded and followed by two dips in light, indicative of a ring system around Quaoar.
The detection of complex rings like this in the outer solar system teaches us fundamental properties of their formation and fate, which might even be applied beyond our solar system.
Dr Daniel Sebastian, School of Physics and Astronomy, University of Birmingham
Ring systems are relatively rare in the solar system – as well as the well-known rings around the giant planets Saturn, Jupiter, Uranus and Neptune, only two other minor planets possess rings – Chariklo and Haumea. All of the previously known ring systems are able to survive because they orbit close to the parent body, so that tidal forces prevent the ring material from accreting and forming moons.
What makes the ring system around Quaoar remarkable is that it lies at a distance of over seven planetary radii – twice as far out as what was previously thought to be the maximum radius according to the so-called `Roche limit’, which is the outer limit of where ring systems were thought to be able to survive. For comparison, the main rings around Saturn lie within three planetary radii. This discovery has therefore forced a rethink on theories of ring formation.
Professor Vik Dhillon, co-author of the study from the University of Sheffield’s Department of Physics and Astronomy, said: “It was unexpected to discover this new ring system in our solar system, and it was doubly unexpected to find the rings so far out from Quaoar, challenging our previous notions of how such rings form. The use of our high-speed camera – HiPERCAM – was key to this discovery as the event lasted less than one minute and the rings are too small and faint to see in a direct image.
“Everyone learns about Saturn’s magnificent rings when they’re a child, so hopefully this new finding will provide further insight into how they came to be.”
Daniel Sebastian, a researcher in the University of Birmingham’s School of Physics and Astronomy, added: “We are excited to live in a time, which allows us to combine space and ground-based observatories in a way that they allow us such amazing discoveries. The detection of complex rings like this in the outer solar system teaches us fundamental properties of their formation and fate, which might even be applied beyond our solar system.”
The study involved 59 academics from all over the world, led by the Federal University of Rio de Janeiro in Brazil. The research was partly funded by the Science and Technology Facilities Council (STFC), part of UK Research and Innovation (UKRI), and included six UK universities – Sheffield, Edinburgh, St Andrews, Warwick, Birmingham, and the Open University.
