(523683) 2014 CP23, provisional designation 2014 CP23, is a trans-Neptunian object from the scattered disc located in the outermost region of the Solar System It was discovered on 29 October 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States.[1] The dwarf planet candidate measures approximately 267 kilometers (170 miles) in diameter.
Discovery[1] | |
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Discovered by | Pan-STARRS 1 |
Discovery site | Haleakalā Obs. |
Discovery date | 29 October 2011 |
Designations | |
MPC designation | (523683) 2014 CP23 |
Alternative designations | 2014 CP23 |
Minor planet category | TNO[2] · SDO[3] p-DP[4] · distant[1] |
Orbital characteristics[2] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 2 | |
Observation arc | 15.10 yr (5,517 d) |
Aphelion | 66.519 AU |
Perihelion | 38.119 AU |
Semi-major axis | 52.319 AU |
Eccentricity | 0.2714 |
Orbital period (sidereal) | 378.44 yr (138,225 d) |
Mean anomaly | 356.73° |
Mean motion | 0° 0m 9.36s / day |
Inclination | 28.510° |
Longitude of ascending node | 145.86° |
Argument of perihelion | 22.015° |
Physical characteristics | |
Mean diameter | 266 km (est.)[4] 267 km (est.)[3] |
Geometric albedo | 0.08 (assumed)[4] 0.09 (assumed)[3] |
Absolute magnitude (H) | 6.1[1][2] |
2014 CP23 orbits the Sun at a distance of 38.1–66.5 AU once every 378 years and 5 months (138,225 days; semi-major axis of 52.32 AU). Its orbit has an eccentricity of 0.27 and an inclination of 29° with respect to the ecliptic.[2] It is a scattered-disc object on a moderately eccentric orbit that never comes closer than 8 AU to the orbit of Neptune.
The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in January 2003, or more than 8 years prior to its official discovery observation at Haleakala Observatory.[1]
This minor planet was numbered by the Minor Planet Center on 25 September 2018 and received the number 523683 in the minor planet catalog (M.P.C. 111779).[5] As of 2018, it has not been named.[1]
According to American astronomer Michael Brown and the Johnston's archive, 2014 CP23 measures 266 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively.[3][4] On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system.[4] As of 2018, no spectral type and color indices, nor a rotational lightcurve have been obtained from spectroscopic and photometric observations. The body's color, rotation period, pole and shape remain unknown.[2][6]
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Trans-Neptunian objects | |
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Dwarf planets (moons) | |
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