(10115) 1992 SK

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(10115) 1992 SK
Discovery [1]
Discovered by E. F. Helin
J. Alu
Discovery site Palomar Obs.
Discovery date 24 September 1992
Designations
MPC designation (10115) 1992 SK
1992 SK · 1985 SD
1985 TO2
Apollo · NEO · PHA
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 60.22 yr (21,996 days)
Aphelion 1.6537 AU
Perihelion 0.8430 AU
1.2483 AU
Eccentricity 0.3247
1.39 yr (509 days)
124.84°
Inclination 15.321°
8.9261°
233.62°
Earth MOID 0.0465 AU
Physical characteristics
Dimensions 0.90±0.20 km[2]
1.000±0.085 km[3]
0.938±0.294 km[4]
1.18 km (calculated)[5]
7.328±0.002 h[lower-alpha 1]
7.31832 h[6]
7.31±0.02 h[7]
7.323±0.005 h[8]
7.319 h[5]
0.34±0.25[2]
0.38±0.24[9]
0.2799±0.1397[3]
0.318±0.214[4]
0.20 (assumed)[5]
SMASS = S[1]
S[5] · S/Sq [10]
17.0[1][3][4][5]
17.4[lower-alpha 1]

(10115) 1992 SK, is an eccentric stony asteroid, classified as near-Earth object and potentially hazardous asteroid. It belongs to the group of Apollo asteroids and measures approximately 1 kilometer in diameter. It was discovered by American astronomers Eleanor Helin and Jeff T. Alu at the U.S. Palomar Observatory, California, on 24 September 1992.[11]

The S-type asteroid orbits the Sun at a distance of 0.8–1.7 AU once every 17 months (509 days). Its orbit has a high eccentricity of 0.32 and an inclination of 15° with respect to the ecliptic. Its Earth minimum orbit intersection distance is Lua error in Module:Convert at line 1851: attempt to index local 'en_value' (a nil value).. This makes the body a potentially hazardous asteroid, because its MOID is less than 0.05 AU and its diameter is greater than 150 meters.[1] The first precovery was obtained at Palomar Observatory in 1953, extending the asteroid's observation arc by 39 years prior to its discovery.[11]

Several rotational light-curves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a light-curve, that rendered a rotation period of 7.328±0.002 hours and a brightness variation of 0.72 in magnitude (U=n/a).[lower-alpha 1] In March 2006, observations by astronomer David Polishook from the ground-based Wise Observatory, Israel, gave a rotation period of 7.31±0.02 and amplitude of 0.70 mag (U=2),[7] and in November 2011, American astronomer Brian Warner at the Palmer Divide Observatory, Colorado, obtained the first well-defined period of 7.323±0.005 hours with an amplitude of 0.50 mag (U=3).[8]

According to the surveys carried out by NASA's space-based Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures 1.0 and 0.94 kilometers in diameter and its surface has an albedo of 0.28 ot 0.32, respectively.[3][4] The ExploreNEOs project finds an albedo of 0.34, with an diameter of 0.9 kilometers,[2] and the Collaborative Asteroid Lightcurve Link calculates a diameter of 1.18 kilometers based on an assumed standard albedo for stony asteroids of 0.20.[5]

References

  1. 1.0 1.1 1.2 Pravec (1999) web: rotation period 7.328±0.002 hours with a brightness amplitude of 0.72 mag. Two more light-curves rendered similar periods. No quality rating by CALL. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (10115)
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External links


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