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Rings of Chariklo information


Apparent brightness measurement by JWST during Chariklo's occultation in 2022

The minor planet and centaur 10199 Chariklo, with a diameter of about 250 kilometres (160 mi), is the second-smallest celestial object with confirmed rings (with 2060 Chiron being the smallest[1]) and the fifth ringed celestial object discovered in the Solar System, after the gas giants and ice giants.[2] Orbiting Chariklo is a bright ring system consisting of two narrow and dense bands, 6–7 km (4 mi) and 2–4 km (2 mi) wide, separated by a gap of 9 kilometres (6 mi).[2][3] The rings orbit at distances of about 400 kilometres (250 mi) from the centre of Chariklo, a thousandth the distance between Earth and the Moon. The discovery was made by a team of astronomers using ten telescopes at various locations in Argentina, Brazil, Chile and Uruguay in South America during observation of a stellar occultation on 3 June 2013, and was announced on 26 March 2014.[2]

The existence of a ring system around a minor planet was unexpected because it had been thought that rings could only be stable around much more massive bodies. Ring systems around minor bodies had not previously been discovered despite the search for them through direct imaging and stellar occultation techniques.[2] Chariklo's rings should disperse over a period of at most a few million years, so either they are very young, or they are actively contained by shepherd moons with a mass comparable to that of the rings.[2][4][5] The team nicknamed the rings Oiapoque (the inner, more substantial ring) and Chuí (the outer ring), after the two rivers that form the northern and southern coastal borders of Brazil. A request for formal names will be submitted to the IAU at a later date.[4]

  1. ^ Cite error: The named reference Ortiz2015 was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference nature_paper was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference Reuters was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference ESO ring was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference nature_news was invoked but never defined (see the help page).

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Rings of Chariklo

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centaur 10199 Chariklo, with a diameter of about 250 kilometres (160 mi), is the second-smallest celestial object with confirmed rings (with 2060 Chiron...

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10199 Chariklo

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period of rotation. Infrared observations of Chariklo indicate the presence of water ice, which may in fact be located in its rings. Chariklo was discovered...

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detect any dust rings around Pluto. 10199 Chariklo, a centaur, was the first minor planet discovered to have rings. It has two rings, perhaps due to a...

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2060 Chiron

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of Chariklo's rings until the 2018 observation, indicating that the same type of structure had been responsible for both. Moreover, both their rings are...

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coast to coast." Rings of Chariklo, one of which is named "Oiapoque" after the river. List of rivers of French Guiana List of rivers of the Americas by...

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Shepherd moon

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in mass to the rings. Chiron is also thought to have rings similar in form to those of Chariklo. A major gap in the large ring system of the V1400 Centauri...

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Quaoar

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confinement of rings to the 1:3 spin-orbit resonance may be common among ringed small Solar System bodies, as it has been previously seen in Chariklo and Haumea...

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Montalto, M. (July 2016). "Photometry of Centaurs and trans-Neptunian objects: 2060 Chiron (1977 UB), 10199 Chariklo (1997 CU26), 38628 Huya (2000 EB173)...

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