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— CH. 1 · DISCOVERY AND NAMING HISTORY —

2060 Chiron

~5 min read · Ch. 1 of 6
6 sections
  • On the 1st of November 1977, astronomer Charles Kowal spotted a faint object moving against the background stars. He captured images of this object on the 18th of October at Palomar Observatory. The discovery made headlines because Chiron was then the most distant known minor planet. Some newspapers even claimed it was the tenth planet in our solar system. This excitement faded as astronomers realized it belonged to a new class of objects called centaurs. These bodies orbit between Saturn and Uranus rather than within the asteroid belt. The Minor Planet Center officially published its name on the 1st of April 1978. They chose the name Chiron after a half-human, half-horse figure from Greek mythology. This centaur was known for being wise and just among all his kin. He served as an instructor to many famous Greek heroes. Other similar objects would later be named after different centaurs from that same mythological tradition.

  • Chiron follows a highly eccentric path around the Sun with an orbital eccentricity of 0.37. Its closest approach brings it inside Saturn's orbit while its farthest point extends beyond Uranus. In May 720, the object will make its nearest modern pass to Saturn. During that encounter, Saturn's gravity will reduce Chiron's semi-major axis from 14 AU to 13.7 AU. The object does not cross paths with Uranus but remains trapped between these two giant planets. Centaurs like Chiron do not maintain stable orbits over long periods. Gravitational tugs from the outer planets eventually eject them or send them into new trajectories. Scientists believe Chiron originated in the Kuiper belt before drifting inward. It may transform into a short-period comet within approximately one million years. The object reached perihelion in 1996 and arrived at aphelion in May 2021. This unique position makes it a Saturn-Uranus object by definition.

  • The James Webb Space Telescope revealed gas emissions and diverse ices on Chiron's surface between 0.97 and 5.27 micrometers. Absorption bands showed carbon dioxide, carbon monoxide, ethane, propane, and acetylene alongside amorphous water ice. Fluorescent methane emissions provided the first evidence of a gas coma rich in this compound. Gaseous carbon dioxide emission appeared in the fundamental stretching band at 4.27 micrometers. Researchers argue that methane desorption results from a density phase transition of amorphous water ice at low temperatures near 61 Kelvin. Irradiation products included both reducing compounds like ethane and oxidizing forms such as CO3. Complex carbon-bearing molecules did not appear in the spectrum despite expectations. This absence suggests physical or temporal separation between methane and carbon dioxide reservoirs. Visible light spectra resemble C-type asteroids while infrared data matches Halley's Comet nucleus characteristics. Water ice remains absent from visible and near-infrared observations but dominates other spectral ranges.

  • In February 1988, Chiron brightened by 75 percent while located 12 AU from the Sun. This behavior mimics comets rather than typical asteroids. Observations in April 1989 confirmed the development of a cometary coma around the object. A tail became detectable in 1993 during further study. Carbon monoxide was identified in very small amounts in 1995 with production rates sufficient to explain the observed coma. Cyanide also appeared in the spectrum recorded in 1991. Unlike most comets, water does not form a major component of Chiron's coma due to its distance from the Sun. The object reached perihelion in 1996 when conditions favored activity. Earlier observations near aphelion failed to reveal any cometary features. Scientists suggest Chiron has not occupied its current orbit for long enough to exhaust all volatiles. It measures approximately 220 kilometers in diameter making it unusually large for a comet nucleus. Official designations now include both 2060 Chiron as a minor planet and 95P/Chiron as a comet.

  • Unexpected stellar occultation events on the 7th of November 1993 led astronomers to propose ring structures around Chiron. Additional data from the 9th of March 1994 and the 29th of November 2011 refined these initial findings. The rings span roughly 280 kilometers in radius and appear sharply defined against space. Their changing appearance at different viewing angles explains long-term brightness variations in the object. Water ice within the rings accounts for fluctuations in infrared absorption bands including their disappearance in 2001 when viewed edge-on. Independent observations on the 28th of November 2018 showed less material than seen in 2011 but hinted at developing partial third ring formation. By December 2022, more material existed than either prior event with the third ring fully developed. J.L. Ortiz speculated that extra material came from an outburst observed in 2021 which bolstered generation of the new ring. This cyclical process maintains the overall structure despite constant evolution. Both Chiron and Chariklo share similar ring widths separations and optical depths until recent changes occurred.

  • The Chiron Orbiter Mission was proposed for NASA's New Frontiers program or Flagship program in May 2010. Launch dates could range from as early as 2023 to as late as 2025 depending on budget constraints and propulsion technology available. Another mission concept called Centaurus formed part of the Discovery Program if approved for funding. That proposal would have launched between 2026 and 2029 to conduct a flyby of 2060 Chiron plus one other centaur object sometime during the 2030s. No missions have been officially selected yet despite these detailed proposals. Scientists continue studying how best to approach such distant targets given current technological limitations. The complexity of reaching Chiron requires advanced propulsion systems capable of handling long-duration travel times. Budget allocations remain uncertain for future deep space exploration initiatives involving centaurs.

Common questions

When was 2060 Chiron discovered and by whom?

Astronomer Charles Kowal spotted 2060 Chiron on the 1st of November 1977. He captured images of this object on the 18th of October at Palomar Observatory before its official naming.

What is the orbital path of 2060 Chiron around the Sun?

2060 Chiron follows a highly eccentric path with an orbital eccentricity of 0.37 that extends between Saturn and Uranus. Its closest approach brings it inside Saturn's orbit while its farthest point reaches beyond Uranus.

How did James Webb Space Telescope observations change understanding of 2060 Chiron?

The James Webb Space Telescope revealed gas emissions and diverse ices on 2060 Chiron's surface between 0.97 and 5.27 micrometers. Fluorescent methane emissions provided the first evidence of a gas coma rich in this compound alongside carbon dioxide and other volatiles.

Why does 2060 Chiron have rings and when were they confirmed?

Unexpected stellar occultation events on the 7th of November 1993 led astronomers to propose ring structures around 2060 Chiron. Additional data from the 9th of March 1994 and the 29th of November 2011 refined these findings showing rings spanning roughly 280 kilometers in radius.

What are the proposed future missions to study 2060 Chiron?

The Chiron Orbiter Mission was proposed for NASA's New Frontiers program or Flagship program in May 2010 with launch dates ranging from 2023 to 2025. Another mission concept called Centaurus formed part of the Discovery Program if approved for funding to conduct a flyby during the 2030s.