5692 Shirao, provisional designation 1992 FR, is a stony Eunomia asteroid from the middle region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 23 March 1992, by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory, Hokkaidō, Japan.[10] The asteroid was later named for Japanese geologist and astrophotographer Motomaro Shirao.[2]
Discovery [1] | |
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Discovered by | K. Endate K. Watanabe |
Discovery site | Kitami Obs. |
Discovery date | 23 March 1992 |
Designations | |
MPC designation | (5692) Shirao |
Named after | Motomaro Shirao (geologist, photographer)[2] |
Alternative designations | 1992 FR · 1949 KK 1966 FO · 1966 FS 1970 CH · 1976 SN2 1979 HT2 · 1979 HV1 1985 UW2 · 1989 SO9 |
Minor planet category | main-belt · Eunomia [3] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 67.83 yr (24,776 days) |
Aphelion | 3.1373 AU |
Perihelion | 2.1723 AU |
Semi-major axis | 2.6548 AU |
Eccentricity | 0.1818 |
Orbital period (sidereal) | 4.33 yr (1,580 days) |
Mean anomaly | 287.13° |
Mean motion | 0° 13m 40.44s / day |
Inclination | 11.931° |
Longitude of ascending node | 181.78° |
Argument of perihelion | 44.251° |
Physical characteristics | |
Dimensions | 9.17 km (calculated)[3] 9.548±0.155[4] 9.75±0.30 km[5] 9.811±0.063 km[6] |
Synodic rotation period | 2.886±0.002 h[7] 2.8878±0.0004 h[lower-alpha 1] 2.90±0.02 h (ii)[8] |
Geometric albedo | 0.21 (assumed)[3] 0.2218±0.0290[6] 0.223±0.030[4][5] |
Spectral type | S [3][9] |
Absolute magnitude (H) | 12.3[5][6] · 12.47±0.25[9] · 12.5[1][3] |
Shirao is a member of the Eunomia family, a large group of stony asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in the central main-belt at a distance of 2.2–3.1 AU once every 4 years and 4 months (1,580 days). Its orbit has an eccentricity of 0.18 and an inclination of 12° with respect to the ecliptic.[1]
In 1949, it was first identified as 1949 KK at Goethe Link Observatory. The body's observation arc begins in 1955, with a precovery at Palomar Observatory, 37 years prior to its official discovery observation at Kitami.[10]
In June 2014, a rotational lightcurve of Shirao was obtained from photometric observations made by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. It gave a well-defined rotation period of 2.8878 hours with a brightness variation of 0.16 magnitude (U=3).[lower-alpha 1]
Previous lightcurves were obtained by French astronomer René Roy (2.90 hours, Δ 0.13 mag, U=2) in June 2001,[8] by American astronomer Donald P. Pray (2.886 hours, Δ 0.12 mag, U=2) in March 2005,[7] and by astronomers Dominique Suys, Hugo Riemis and Jan Vantomme (2.90 hours, Δ 0.15 mag, U=2+) in September 2006.[3][8]
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, Shirao measures between 9.5 and 9.8 kilometers in diameter and its surface has an albedo of 0.22,[4][5][6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.21 – derived from 15 Eunomia, the largest member and namesake of this asteroid family – and calculates a diameter of 9.2 kilometers.[3]
This minor planet was named after Motomaro Shirao (born 1953), a Japanese geologist and astrophotographer, who is known for his photographs of volcanoes and lunar geological features.[2] The official naming citation was published by the Minor Planet Center on 4 April 1996 (M.P.C. 26930).[11]
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