19521 Chaos

19521 Chaos
19521 Chaos as imaged by the Hubble Space Telescope in September 2001
Discovery
Discovered byDeep Ecliptic Survey
Discovery date19 November 1998
Designations
(19521) Chaos
Pronunciation/ˈk.ɒs/
Named after
Chaos
1998 WH24
TNO (cubewano)
AdjectivesChaotian /kˈʃən/
Symbol (astrological)
Orbital characteristics
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc5902 days (16.16 yr)
Earliest precovery date17 October 1991
Aphelion50.636 AU (7.5750 Tm)
Perihelion40.957 AU (6.1271 Tm)
45.796 AU (6.8510 Tm)
Eccentricity0.10567
309.92 yr (113199 d)
4.3931 km/s
337.2998°
0° 0m 11.449s / day
Inclination12.0502°
50.0239°
≈ 23 December 2033
±10 days
58.4097°
Known satellitescompact or contact binary
Jupiter MOID35.8 AU (5.36 Tm)
Neptune MOID12.5 AU (1.87 Tm)
TJupiter5.884
Physical characteristics
Dimensions415+83
−30
 km
equivalent
600+140
−130
 km
 
~665 
ca. 0.1
B–V=0.95±0.03 
V–R=0.63±0.03 
V–I=1.25±0.04 
4.8 
5.0 

    19521 Chaos is a cubewano, a Kuiper-belt object not in resonance with any planet. Chaos was discovered in 1998 by the Deep Ecliptic Survey with Kitt Peak's 4 m telescope.

    Occultations suggest it is a compact or contact binary equivalent to a sphere 400 to 500 km in diameter. On 20 November 2020, Chaos occulted a magnitude 16.8 star. Three observers detected the occultation, finding that the object is likely smaller than 600 km in diameter. Another occultation was recorded on 14 January 2022; full results on size, shape, geometric albedo, and the spin-axis orientation have not been released. A further occultation occurred on 28 September 2023, with a shadow crossing most of North America. This occultation was observed by over 30 observers; preliminary analysis suggests that Chaos is a binary (possibly a contact binary).