(79983) 1999 DF9

Trans-Neptunian object of the Kuiper belt From Wikipedia, the free encyclopedia

(79983) 1999 DF9 (provisional designation 1999 DF9) is a trans-Neptunian object of the Kuiper belt, classified as a non-resonant cubewano, that measures approximately 270 kilometers in diameter.

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(79983) 1999 DF9
Discovery[1]
Discovered byJ. X. Luu
C. Trujillo
D. C. Jewitt
Discovery siteKitt Peak National Obs.
Discovery date20 February 1999
Designations
(79983) 1999 DF9
1999 DF9
TNO[1] · cubewano[2][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 2
Observation arc17.06 yr (6,231 days)
Aphelion53.567 AU
Perihelion39.830 AU
46.698 AU
Eccentricity0.1471
319.12 yr (116,560 days)
19.489°
0° 0m 11.16s / day
Inclination9.8105°
334.84°
178.63°
Physical characteristics
Dimensions265 km (calculated)[4]
306 km[3]
6.65 h[5]
0.10 (assumed)[4]
B–V = 0.920±0.060[6]
V–R = 0.710±0.050[6]
V–I = 1.360±0.060[6]
5.797±0.110 (R)[7] · 6.0[1][4]
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    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.[8] As no precoveries were taken, the minor planet's observation arc begins with its discovery observation in 1999.[8]

    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.[1] 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 6.65 hours with a brightness variation of 0.40 magnitude (U=2).[5]

    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,[4] while the Johnston's archive give a diameter of 306 kilometers for an albedo of 0.09.[3]

    Numbering and naming

    This minor planet was numbered by the Minor Planet Center on 4 May 2004.[9] As of 2018, it has not been named.[8]

    References

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