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(79983) 1999 DF9
Trans-Neptunian object of the Kuiper belt
Trans-Neptunian object of the Kuiper belt
| Field | Value |
|---|---|
| minorplanet | yes |
| name | |
| background | #C2E0FF |
| discovery_ref | |
| discovered | 20 February 1999 |
| discoverer | J. X. Luu |
| C. Trujillo | |
| D. C. Jewitt | |
| discovery_site | Kitt Peak National Obs. |
| mpc_name | |
| alt_names | |
| mp_category | TNOcubewano |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 2 |
| observation_arc | 17.06 yr (6,231 days) |
| aphelion | 53.567 AU |
| perihelion | 39.830 AU |
| semimajor | 46.698 AU |
| eccentricity | 0.1471 |
| period | 319.12 yr (116,560 days) |
| mean_anomaly | 19.489° |
| mean_motion | / day |
| inclination | 9.8105° |
| asc_node | 334.84° |
| arg_peri | 178.63° |
| satellites | 0 |
| dimensions | 265 km (calculated) |
| 306 km | |
| rotation | h |
| albedo | 0.10 (assumed) |
| spectral_type | B–V = |
| V–R = | |
| V–I = | |
| abs_magnitude | (R)6.0 |
C. Trujillo D. C. Jewitt 306 km V–R = V–I =
**** (provisional designation ****) is a trans-Neptunian object of the Kuiper belt, classified as a non-resonant cubewano, that measures approximately 270 kilometers in diameter.
Discovery
It was discovered on 20 February 1999, by American and British astronomers Jane Luu, Chad Trujillo and David C. Jewitt at the U.S. Kitt Peak National Observatory in Arizona. As no precoveries were taken, the minor planet's observation arc begins with its discovery observation in 1999.
Classification and orbit
The minor planet is a classical Kuiper belt object or "cubewano", which are not in an orbital resonance with Neptune and do not cross the giant planet's orbit. It orbits the Sun at a distance of 39.8–53.6 AU once every 319 years and 1 month (116,560 days). Its orbit has an eccentricity of 0.15 and an inclination of 10° with respect to the ecliptic. This makes it a relatively eccentric body for a classical Kuiper belt object, which typically have low-eccentricities of 0.10 or less.
Physical characteristics
In February 2001, a rotational lightcurve was published for this minor planet from photometric observations by Portuguese astronomer Pedro Lacerda and the discovering astronomer Jane Luu. Lightcurve analysis gave a relatively short rotation period of hours with a brightness variation of 0.40 magnitude ().
The Collaborative Asteroid Lightcurve Link assumes a low albedo of 0.10 and calculates a mean-diameter of 265 kilometers, based on an absolute magnitude of 6.0, while Johnston's Archive give a diameter of 306 kilometers for an albedo of 0.09.
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 4 May 2004. As of 2025, it has not been named.
References
|access-date= 12 November 2018}}
|author-link=Marc W. Buie
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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