The rings of (2060) Chiron: Evidence of an evolving system
C. L. Pereira, F. Braga-Ribas, B. Sicardy, R. Leiva, M. Assafin, B. E. Morgado, J. L. Ortiz, P. Santos-Sanz, J. I. B. Camargo, G. Margoti, Y. Kilic, G. Benedetti-Rossi, R. Vieira-Martins, T. F. L. L. Pinheiro, R. Sfair, F. L. Rommel, A. R. Gomes-Júnior, R. C. Boufleur, R. Duffard, J. Desmars, D. Souami, N. Morales, F. Arrese, K. Barkaoui, A. Burdanov, C. A. Colazo, C. A. Domingues, H. Dutra, R. C. Gargalhone, C. Jacques, F. Jablonski, L. Liberato, R. Melia, J. C. Oliveira, M. Sardiña, J. Spagnotto, T. Speranza, A. Wilberger, M. A. Zorzan, L. S. Brito, J. P. Cavalcante, T. Q. Costa, M. Emilio, E. Garcia-Migani, M. Gillon, E. Gradovski, E. Jehin, V. Lattari, M. Malacarne, L. A. Mammana, M. Melita, W. Melo, A. J. Ortiz, P. Quitral-Manosalva, G. Ramon, I. Rodrigues, L. Vanzi
TL;DR
The paper investigates the emergence and evolution of a ring system around the small body (2060) Chiron by analyzing a 2023 multi-chord stellar occultation. It contrasts an equatorial-disk representation with a spherical-shell model, deriving three co-planar rings at roughly $r \,\approx\, 273$, 325, and 438 km, plus an outer feature near 1380 km, embedded in a broad disk whose mean ring-plane orientation is $\lambda \\approx\,151°$ and $\beta \\approx\,20°$. The total ring mass is estimated near $m_{ring} \\approx 10^{11}$ kg, with a ring-to-Chiron mass ratio $\\mu \\approx 3.5\\times 10^{-8}$, and the inner rings lie close to the 1/2 and 1/3 spin-orbit resonances at radii $a_{1/2} \\approx 238±45$ km and $a_{1/3} \\approx 312±59$ km. Overall, the findings support ongoing ring formation around Chiron, offering valuable constraints on the processes that generate and confine rings around small bodies and informing models of circum-object disk evolution and episodic activity in the outer Solar System.
Abstract
The centaur (2060) Chiron has long been a candidate for hosting material in orbit, based on occultation and photometric and spectroscopic data. Here, we present a multichord stellar occultation observed on 2023 September 10 UT that reveals new and complex structures surrounding Chiron. High-cadence light curves show multiple secondary events that are best explained (when compared with a multishell interpretation) with a system of three confined rings located at average radii of 273, 325, and 438 km, the outermost of which lies beyond Chiron's Roche limit. The rings appear coplanar, with a mean pole orientation of λ = 151° +/- 4° and \b{eta} = 20° +/- 6°. A broader, disklike structure extends from about 200 to 800 km, and a newly detected faint feature is observed at ~1380 km. Chiron thus appears as the fourth small solar system body known for hosting a ring system. Comparisons with previous occultation events that have occurred since 1994 show that these features are not permanent. With these observations, we may witness for the first time the ongoing formation and evolution of a ring system.
