Detection of CN emission from (2060) Chiron

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Spectroscopy, Chiron, Cyanogen, Emission Spectra, Carbon Dioxide, Carbon Monoxide, Cometary Atmospheres, Comets, Outgassing, Asteroids, Chiron, Emissions, Cyanide, Comets, Spectra, Outgassing, Carbon Dioxide, Flux, Comet Nuclei, Surface, Chemistry, Spectroscopy, Spectrophotometry, Photometry, Earth-Based Observations, Ccd Methods, Procedure, Astronomy, Sublimation, Carbon Monoxide, Ice, Parameters, Parent Molecules, Models, Cn Radical

Scientific paper

The detection of CN emission the spectrum of (2060) Chiron not only underscores its cometary nature, but represents, at a heliocentric distance in excess of 11 AU, the most distantly detected instance of a cometary gas species. These observations are noted to be consistent with a driving of Chiron's outgassing by isolated outbursts of CO2 from a small fraction of Chiron's surface. If dusty particles or icy grains are dragged out by the gas with unit dust-to-gas mass ratio, outbursts need occur only once every several months. Such small-surface outgassings appear to characterize comets which have made many passages close to the sun.

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