Ring discovered around dwarf planet Quaoar confounds theories
Astronomers have spotted a ring around a Pluto-sized dwarf planet called Quaoar in the outer reaches of the solar system.
The observations, by a powerful telescope on La Palma, reveal the ring to be much further away from the planet than is typical, calling into question how such systems form.
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Astronomers have spotted a ring around a Pluto-sized dwarf planet called Quaoar in the outer reaches of the solar system.
The observations, by a powerful telescope on La Palma, reveal the ring to be much further away from the planet than is typical, calling into question how such systems form.
Prof Vik Dhillon, of the University of Sheffields department of physics and astronomy, and his co-authors, said: The ring came as a real surprise and doubly surprising was where it was, well outside the theoretical maximum for where a ring can survive according to classical theory. These are the most unusual rings weve seen.
https://www.theguardian.com/science/2023/feb/08/ring-discovered-around-dwarf-planet-quaoar-confounds-theories
A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
Abstract
Planetary rings are observed not only around giant planets1, but also around small bodies such as the Centaur Chariklo2 and the dwarf planet Haumea3. Up to now, all known dense rings were located close enough to their parent bodies, being inside the Roche limit, where tidal forces prevent material with reasonable densities from aggregating into a satellite. Here we report observations of an inhomogeneous ring around the trans-Neptunian body (50000) Quaoar. This trans-Neptunian object has an estimated radius4 of 555?km and possesses a roughly 80-km satellite5 (Weywot) that orbits at 24 Quaoar radii6,7. The detected ring orbits at 7.4?radii from the central body, which is well outside Quaoars classical Roche limit, thus indicating that this limit does not always determine where ring material can survive. Our local collisional simulations show that elastic collisions, based on laboratory experiments8, can maintain a ring far away from the body. Moreover, Quaoars ring orbits close to the 1/3 spinorbit resonance9 with Quaoar, a property shared by Chariklos2,10,11 and Haumeas3 rings, suggesting that this resonance plays a key role in ring confinement for small bodies.
https://www.nature.com/articles/s41586-022-05629-6
(Quaoar is not an official dwarf planet yet, according to the IAU, though it seems to qualify. Having its own ring must surely give it a boost)