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— CH. 1 · INTRODUCTION —

2060 Chiron

~7 min read · Ch. 1 of 7
7 sections
  • 2060 Chiron started its modern life as a small smudge on photographic plates taken at Palomar Observatory on the 18th of October 1977. Charles Kowal spotted it on the 1st of November that year. He had found something nobody had seen before in that part of the Solar System, and at the time, the press even floated the idea that it might be the tenth planet.

    It was not a planet. It was not quite an asteroid either. And as the decades passed and the instruments grew more powerful, Chiron revealed itself to be stranger and stranger. What exactly is it? Where does it come from? And why does a body barely 200 kilometers across have rings?

  • Palomar Observatory gave Kowal the images he needed, but Chiron itself had been crossing the sky long before anyone noticed. Once researchers went looking through archival plates, they traced it back to April 1895, a full eighty-two years before the official discovery. That April image was taken just one month after Chiron had passed perihelion in March 1895, its closest point to the Sun. A perihelion passage also occurred in 1945, but no one caught it then. Searches at the time were not sensitive enough to pick up slow-moving objects at that distance.

    At the moment Kowal found it, Chiron was near aphelion, the far end of its orbit, making it the most distant known minor planet at the time. Its official designation came quickly: 2060 Chiron. The name was published by the Minor Planet Center on the 1st of April 1978, drawn from Greek mythology. Chiron was the son of the Titan Cronus and the nymph Philyra, half-human and half-horse, and regarded as the wisest and most just of all centaurs, serving as a teacher to the Greek heroes. The name also carried a practical suggestion: that future objects found in similar orbits should be named after other centaurs from mythology.

    A symbol was later devised for Chiron by Al H. Morrison. It is used mostly in astrology rather than astronomy, shaped like a key and also readable as an OK monogram standing for Object Kowal.

  • Chiron travels a highly eccentric path, with an eccentricity of 0.37. Its perihelion falls just inside Saturn's orbit, while its aphelion reaches just outside the perihelion of Uranus, though it never closes in on Uranus's average distance from the Sun. This places it squarely in a zone controlled by two of the Solar System's giants.

    The consequences of that position are significant. Centaurs, as a class, do not hold stable orbits. The gravitational influence of the giant planets will eventually pull Chiron away from its current path, either shifting it into a new orbit or ejecting it from the Solar System altogether, over a period of millions of years. The best current estimate is that Chiron likely originated in the Kuiper belt and will probably evolve into a short-period comet in roughly a million years.

    Chiron's closest recorded approach to Saturn in modern times occurred around May of the year 720, when it came within 30.5 million kilometers of the planet. Saturn's gravity during that passage shrank Chiron's semi-major axis from 14.55 AU to 13.7 AU. Chiron reached perihelion in 1996 and swung out to aphelion in May 2021.

  • In February 1988, while Chiron sat 12 AU from the Sun, it abruptly brightened by 75 percent. Asteroids do not do that. Comets do. Follow-up observations in April 1989 confirmed what astronomers had begun to suspect: Chiron had developed a cometary coma, a cloud of gas and dust surrounding its nucleus. A tail was detected in 1993.

    What drives Chiron's activity is not water. The body sits too far from the Sun for water ice to sublimate. Instead, in 1995, carbon monoxide was detected in very small amounts, and the derived production rate was calculated to be sufficient to explain the observed coma. Cyanide had also turned up in Chiron's spectrum in 1991. The James Webb Space Telescope later revealed a rich inventory: absorption bands of carbon dioxide, carbon monoxide, ethane, propane, and acetylene, along with water ice in its amorphous state. A key finding was fluorescent methane emissions, providing what the authors described as the first evidence of a gas coma rich in methane. Methane desorption was linked to a density phase transition of amorphous water ice at 61 Kelvin, a process previously studied in the laboratory.

    Chiron is officially classified as both a minor planet and a comet, carrying the cometary designation 95P/Chiron alongside 2060 Chiron. The term proto-comet has also been applied. At roughly 220 kilometers in diameter, it is unusually large for a comet nucleus. Its dual classification reflects a genuine ambiguity in how astronomers draw the line between the two categories of object. Chiron was the first member of what is now recognized as the family of Chiron-type comets, a grouping that also includes 39P/Oterma, 165P/LINEAR, 166P/NEAT, and 167P/CINEOS.

  • On the 7th of November 1993 and the 9th of March 1994, astronomers watching Chiron pass in front of background stars noticed unexpected dips in starlight that no one could immediately explain. A third such event on the 29th of November 2011 added weight to the puzzle. These signals had initially been attributed to jets from Chiron's comet-like activity. A re-analysis proposed something more surprising: Chiron has rings, proposed to sit at a radius of 324 units, sharply defined.

    Once the ring hypothesis was taken seriously, a lot of earlier puzzles fell into place. The long-term variation in Chiron's brightness, which had complicated size and albedo estimates for decades, could be largely explained by the changing viewing angle of the rings. The disappearance of infrared water-ice absorption bands in 2001 matched the moment when the rings were edge-on to observers on Earth.

    Further occultations on the 28th of November 2018 and the 15th of December 2022 showed that the rings are not static. In 2018, there was less material than in 2011, but signs of a partial third ring beginning to develop. By 2022, there was more material than in either earlier observation, and the third ring had become fully formed. J.L. Ortiz speculated that an outburst observed in 2021 may have fed material into orbit around Chiron, driving the third ring's growth. The ring structure is expected to continue cycling in this way.

    Chiron's rings share a striking resemblance to those of 10199 Chariklo. Until the 2018 observation, the width, separation, and optical depth of the two ring systems were nearly identical, suggesting a common structural origin. Both ring systems also sit within their respective Roche limits, the zone inside which tidal forces prevent material from clumping into a moon. Chiron's newly developed third ring may reach outside that boundary, depending on its density.

  • Pinning down Chiron's size has proved surprisingly difficult. In 1984, Larry Lebofsky estimated a diameter of around 180 kilometers. Estimates through the 1990s came in closer to 150 kilometers. The Spitzer Space Telescope in 2007 suggested a figure of 233 kilometers, and the Herschel Space Observatory weighed in at 218 kilometers in 2013. A 2023 study by Sickafoose returned to 196 kilometers. The uncertainty is not just a matter of measurement precision; Chiron's highly variable cometary activity makes it hard to determine its nucleus's true absolute magnitude, which in turn affects every size calculation.

    Four rotational light curves taken between 1989 and 1997 produced a well-defined rotation period of 5.918 hours. The brightness variation was small, between 0.05 and 0.09 magnitudes, suggesting the body is close to spheroidal rather than elongated or irregular.

    Chiron's visible and near-infrared spectrum is neutral, similar to C-type asteroids and the nucleus of Halley's Comet. Near-infrared observations show no water ice on its surface, though the James Webb Space Telescope found water ice in its amorphous form in the coma. Complex carbon-bearing molecules resulting from the combined irradiation of CH and CO groups were not detected, which researchers suggest may point to a physical or temporal separation between Chiron's methane and carbon dioxide reservoirs.

  • The Chiron Orbiter Mission was published in May 2010 as a proposal for NASA's New Frontiers or Flagship program. It outlined an orbiter mission to Chiron with a potential launch window stretching from 2023 at the earliest to 2025 at the latest, depending on budget and choice of propulsion.

    A separate proposal emerged under the Discovery Program, named Centaurus. If approved, it would have launched between 2026 and 2029 and conducted a flyby of 2060 Chiron and one other centaur in the 2030s. Neither mission has been selected as of the time of this documentary, but the evolving ring structure documented through the 2022 occultation gives any future mission a dynamic and changing target to study.

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Common questions

Who discovered 2060 Chiron and when was it found?

2060 Chiron was discovered by Charles Kowal on the 1st of November 1977, using images taken on the 18th of October at Palomar Observatory. It was the most distant known minor planet at the time of its discovery.

Why is 2060 Chiron classified as both a minor planet and a comet?

In February 1988, Chiron brightened by 75 percent at 12 AU from the Sun, behavior typical of comets. A cometary coma was confirmed in 1989 and a tail was detected in 1993. It now carries both the minor planet designation 2060 Chiron and the cometary designation 95P/Chiron.

Does 2060 Chiron have rings?

Yes, Chiron has rings, making it one of four known minor planets with ring systems, alongside 10199 Chariklo, Haumea, and Quaoar. It is the only known comet to have rings. Occultation observations in 1993, 1994, 2011, 2018, and 2022 revealed the rings, including a third ring that fully developed by the December 2022 event.

What is 2060 Chiron made of?

James Webb Space Telescope observations detected carbon dioxide, carbon monoxide, ethane, propane, acetylene, and amorphous water ice in Chiron's coma. Fluorescent methane emissions were also detected, providing the first evidence of a gas coma rich in methane. Cyanide was identified in Chiron's spectrum as early as 1991.

How big is 2060 Chiron?

Size estimates for Chiron range from roughly 166 to 271 kilometers in diameter across different studies. A 2023 study by Sickafoose placed it at 196 kilometers. The uncertainty stems partly from Chiron's variable cometary activity, which makes its nucleus's absolute magnitude difficult to determine.

What is the rotation period of 2060 Chiron?

Chiron has a rotation period of 5.918 hours, derived from four rotational light curves taken between 1989 and 1997. The small brightness variation of 0.05 to 0.09 magnitudes indicates the body is roughly spheroidal in shape.

All sources

48 references cited across the entry

  1. 1journalChironAl H. Morrison — 1977
  2. 3journalMaterial around the Centaur (2060) Chiron from the 2018 November 28 UT Stellar OccultationAmanda A. Sickafoose et al. — 1 November 2023
  3. 6bookDictionary of Minor Planet Names – (2060) ChironLutz D. Schmadel — Springer Berlin Heidelberg — 2007
  4. 8webChiron Fact Sheet20 August 2014
  5. 9bookDictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)Lutz D. Schmadel — Springer Berlin Heidelberg — 2009
  6. 10webAstDys (2060) Chiron EphemeridesDepartment of Mathematics, University of Pisa, Italy
  7. 12journalDetection of CN Emission from (2060) ChironSchelte J. Bus et al. — 15 February 1991
  8. 13webThe Structure of the Inner Coma of Comet Chiron: Imaging The ExopauseKaren J. Meech — Institute for Astronomy, University of Hawaii — 19 February 1994
  9. 15newsA second minor planet may possess Saturn-like ringsSpace Daily — 17 March 2015
  10. 16journalThe discovery and orbit of /2060/ ChironCharles T. Kowal et al. — December 1978
  11. 17journalThe color temperature of (2060) Chiron: A warm and small nucleusHumberto Campins et al. — December 1994
  12. 18journalThe effect on the Edgeworth-Kuiper Belt of a large distant tenth planetSimon J. Collander-Brown et al. — 2000
  13. 20journalSimulations of the Population of Centaurs II: Individual ObjectsJonathan M. Horner et al. — 2004
  14. 21bookSolar System Update: Topical and Timely Reviews in Solar System SciencesDavid C. Jewitt et al. — Springer-Praxis Ed. — 2006
  15. 22journalProperties of the nuclei of Centaurs Chiron and CharikloOlivier Groussin et al. — January 2004
  16. 23arxivPhysical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space TelescopeJohn Stansberry et al. — November 2007
  17. 24journal2060 Chiron - Colorimetry and cometary behaviorWilliam K. Hartmann et al. — January 1990
  18. 25journal(2060) ChironKaren J. Meech et al. — April 1989
  19. 26journalThe Atmosphere of 2060 ChironKaren J. Meech et al. — October 1990
  20. 29webA second ringed centaur? Centaurs with rings could be commonEmily Lakdawalla — Planetary Society — 2015-01-27
  21. 30journalPossible ring material around centaur (2060) ChironJosé Luis Ortiz Moreno et al. — 2015
  22. 31conferenceObservations of Carbon Monoxide in (2060) ChironMaria Womack et al. — 1999
  23. 32journalWater Ice in 2060 Chiron and Its Implications for Centaurs and Kuiper Belt ObjectsJane X. Luu et al. — March 2000
  24. 33journalUnveiling the ice and gas nature of active centaur (2060) Chiron using the James Webb Space TelescopeNoemi Pinilla-Alonso et al. — December 2024
  25. 34journalLaboratory experiments on the sublimation of methane through ice dust layers and applications to cometary activityCarla Tamai et al. — July 2023
  26. 35journalTNOs are Cool: A survey of the trans-Neptunian region. VIII. Combined Herschel PACS and SPIRE observations of nine bright targets at 70-500 mumSonia Fornasier et al. — July 2013
  27. 36journal2060 Chiron - CCD and electronographic photometrySchelte J. Bus et al. — February 1989
  28. 37journalCometary activity in 2060 ChironJane X. Luu et al. — September 1990
  29. 38journalCCD photometry of 2060 Chiron in 1985 and 1991Robert L. Marcialis et al. — August 1993
  30. 39journalPhotometric monitoring of 2060 Chiron's brightness at perihelionDaniela Lazzaro et al. — December 1997
  31. 40journalVisible and Infrared Photometry of Six CentaursJohn K. Davies et al. — August 1998
  32. 41journalPolarimetry of Centaurs (2060) Chiron, (5145) Pholus and (10199) CharikloIrina N. Belskaya et al. — November 2010
  33. 42journalUpdated taxonomy of trans-Neptunian objects and centaurs: Influence of albedoIrina N. Belskaya et al. — April 2015
  34. 43journalThe bimodal colors of Centaurs and small Kuiper belt objectsNuno Peixinho et al. — October 2012
  35. 44journalAbsolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary resultsPeter Veres et al. — November 2015
  36. 45journalThe changing material around (2060) Chiron from an occultation on 2022 December 15J. L. Ortiz et al. — 7 August 2023