Observations at many sites in South America, including ESO�s La Silla Observatory, have made the surprise discovery that the remote asteroid Chariklo is surrounded by two dense and narrow rings. This is the smallest object by far found to have rings and only the fifth body in the Solar System � after the much larger planets Jupiter, Saturn, Uranus and Neptune � to have this feature. The origin of these rings remains a mystery, but they may be the result of a collision that created a disc of debris. This artist�s impression shows a close-up of what the rings might look like. L. Calcada/M. Kornmesser/Nick Risinger/ESO
Rings have been discovered around an asteroid for the first time to the surprise of astronomers who didn't think asteroids could have rings.
The asteroid Chariklo, which is also considered a minor planet, appears to be encircled by two narrow rings, reported an international team of scientists in a paper published online Wednesday in the journal Nature.
"We weren't looking for a ring and didn't think small bodies like Chariklo had them at all," said Felipe Braga-Ribas of the Observatório Nacional/MCTI in Rio de Janeiro, Brazil, lead author of the report, in a statement.
"So the discovery — and the amazing amount of detail we saw in the system — came as a complete surprise!"
Chariklo is the largest of the Centaurs, a group of asteroids orbiting between Saturn and Uranus. Its diameter is about 250 kilometres. In comparison, Lake Ontario is 310 kilometres long and Prince Edward Island is 224 kilometres long.
Chariklo is named after a nymph who was the wife of the centaur Chiron in Greek mythology.
Chariklo's rings were discovered when it passed in front of a star called UCAC4 on June 3, 2013, as viewed from South America. During such an event, called an occultation, the light from the star is temporarily blocked by an object passing in front of it. As researchers viewed the event from seven different telescopes around South America, they noticed two short dips in the star's brightness before and after the occultation.
A comparison of the data from the different telescopes and some calculations revealed that the dips were caused by two rings, one seven and one three kilometres wide, with a nine-kilometre gap in-between. They have been nicknamed Oiapoque and Chuí, two rivers near the northern and southern ends of Brazil
The rings sit 1,000 times closer to Chariklo than the moon does to Earth, said study co-author Uffe Grae Jorgensen of the University of Copenhagen, in a news release from the European Southern Observatory. The ESO runs two of the telescopes used in the study.
The researchers think the rings formed from debris left over from a collision of an object with Chariklo or between two objects orbiting it. That debris was shaped into rings by one or more undiscovered small "shepherd" moons — about a kilometre across — embedded in the rings themselves.
"What we are witnessing is perhaps the unveiling of an object that is in the middle of the same stage of development as the Earth and the moon 4.5 billion years ago, when there was a giant collision between Earth and another planet," Jorgensen said in a news release from the University of Copenhagen.
He added that if the rings eventually gather up into a single moon, it will be about two kilometres in diameter.
Only four other objects in the solar system are known to have rings: The giant planets Jupiter, Saturn, Uranus and Neptune.
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