TOKYO: Ringed celestial bodies may be more common within our solar system than previously thought, say scientists who have discovered how rings form around minor planets known as centaurs.
Centaurs are minor planets that orbit between Jupiter and Neptune, their current or past orbits crossing those of the giant planets. It is estimated that there are around 44,000 centaurs with diameters larger than one kilometre.
Until recently it was thought that the four giants such as Saturn and Jupiter were the only ringed celestial bodies within our solar system.
However, in 2014 observations of stellar occultation, an event that occurs when light from a star is blocked from the observer by a celestial body, by multiple telescopes showed that rings exist around the centaur Chariklo.
Soon after this, scientists discovered that rings likely exist around another centaur, Chiron, but the origin of the rings around these minor planets remained a mystery.
The team from Kobe University in Japan began by estimating
the probability that these centaurs passed close enough to the
giant planets to be destroyed by their tidal pull.
The study showed that about 10 per cent of centaurs would
experience that level of close encounter.
Researchers used computer simulations to study the
disruption caused by tidal pull when the centaurs passed close
by the giant planets.
The outcome of such encounters was found to vary
depending on parameters such as the initial spin of the
passing centaur, the size of its core and the distance of its
closest approach to a giant planet.
They found that if the passing centaur is differentiated
and has a silicate core covered by an icy mantle, fragments of
the partially-destroyed centaur will often spread out around
the largest remnant body in a disc shape, from which rings are
expected to form.
The simulations suggest that the existence of rings around
centaurs would be much more common than previously thought.
It is highly likely that other centaurs with rings or
small moons exist, awaiting discovery by future observations,
The findings appear in the Astrophysical Journal Letters.