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5357 Sekiguchi

5357 Sekiguchi
Discovery 
Discovered by T. Fujii
K. Watanabe
Discovery site Kitami Obs.
Discovery date 2 March 1992
Designations
MPC designation (5357) Sekiguchi
Named after
Tomohiko Sekiguch
(astronomer)
1992 EL · 1969 TB4
1971 BE3 · 1981 BH
1990 VJ4 · 1990 WU13
main-belt · (outer)
Orbital characteristics
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 65.89 yr (24,066 days)
Aphelion 3.2971 AU
Perihelion 2.6793 AU
2.9882 AU
Eccentricity 0.1034
5.17 yr (1,887 days)
37.449°
0° 11m 26.88s / day
Inclination 9.0837°
301.97°
116.81°
Physical characteristics
Dimensions 13.948±0.118
14.281±0.193 km
14.52±0.65 km
15.19±1.13 km
25.44 km (calculated)
5.4048±0.0011 h
5.4100±0.0011 h
5.41±0.01 h
0.057 (assumed)
0.192±0.032
0.334±0.052
0.3829±0.0259
C
11.7 · 10.9 · 11.60 · 11.66±0.17 · 11.719±0.003 (R) · 11.624±0.002 (R)

5357 Sekiguchi, provisional designation 1992 EL, is an asteroid from the outer region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 2 March 1992, by Japanese amateur astronomers Tetsuya Fujii and Kazuro Watanabe at the Kitami Observatory in eastern Hokkaidō, Japan.

The asteroid orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 2 months (1,887 days). Its orbit has an eccentricity of 0.10 and an inclination of 9° with respect to the ecliptic. The first precovery was obtained at Goethe Link Observatory in 1950, extending the asteroid's observation arc by 42 years prior to its discovery.

A rotational light-curve of this asteroid was obtained by French astronomers René Roy and Laurent Bernasconi from photometric observations made in October 2005. It showed a rotation period of 5.41±0.01 hours with a brightness variation of 0.72 in magnitude (U=3). In October 2010 and November 2011, two more light-curves were obtained at the U.S. Palomar Transient Factory, rendering a period of 5.4048 and 5.4100 hours with an amplitude of 0.58 and 0.27 in magnitude, respectively (U=2/2).


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