(248835) 2006 SX368

(248835) 2006 SX368
Discovery[1]
Discovered by A. C. Becker
A. W. Puckett
J. M. Kubica
Discovery site APO
Discovery date 16 September 2006
Designations
MPC designation (145451) 2005 RM43
centaur[1][2]
Orbital characteristics [1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc 2160 days (5.91 yr)
Aphelion 32.098 AU (4.8018 Tm)
Perihelion 11.956 AU (1.7886 Tm)
22.027 AU (3.2952 Tm)
Eccentricity 0.45720
103.38 yr (37760.8 d)
0.00949
19.679°
0° 0m 34.321s / day
Inclination 36.299°
280.05°
70.625°
Earth MOID 11.1304 AU (1.66508 Tm)
Jupiter MOID 8.07021 AU (1.207286 Tm)
Jupiter Tisserand parameter 3.186
Physical characteristics
Dimensions 75 ± 5 km[3]
Mass 2×1018 kg
Mean density
 1 g/cm3 (assumed)
0.05–0.06[3]
Temperature 80 K
9.5[1]

    (248835) 2006 SX368 /əˈkɪroʊ.iː/, also known as 2006 SX368, is a centaur orbiting in the outer Solar System between Saturn and Neptune. It was discovered on September 16, 2006 by Andrew Becker, Andrew Puckett and Jeremy Kubica at Apache Point Observatory in Sunspot, New Mexico.

    Orbit

    Centaurs have short dynamical lives due to strong interactions with the giant planets. The orbit of (248835) 2006 SX368 is unusually eccentric — near the perihelion it comes under influence of Uranus, while at the aphelion it travels slightly beyond the orbit of Neptune.[3]

    Physical characteristics

    In 2010, thermal flux from (248835) 2006 SX368 in the far-infrared was measured by the Herschel Space Telescope. As a result, its equivalent size was estimated to lie within a range from 70 kilometres (43 mi) to 80 kilometres (50 mi).[3]

    See also

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 2006 SX368" (2012-08-15 last obs). Retrieved 7 April 2016.
    2. ↑ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2008-10-16.
    3. 1 2 3 4 Muller, T.G.; Lellouch, E.; Stansberry, J.; et al. (2010). ""TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)". Astronomy and Astrophysics 518: L146. arXiv:1005.2923. Bibcode:2010A&A...518L.146M. doi:10.1051/0004-6361/201014683.

    External links


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