1575 Winifred
Discovery [1] | |
---|---|
Discovered by | R. C. Cameron (Indiana University) |
Discovery site | Goethe Link Obs. |
Discovery date | 20 April 1950 |
Designations | |
MPC designation | 1575 Winifred |
Named after
|
Winifred Sawtelle (staff member at USNO)[2] |
1950 HH · 1928 HG 1939 GK · 1950 HD1 1977 UH1 |
|
main-belt · Phocaea [3] | |
Orbital characteristics [1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 87.84 yr (32,083 days) |
Aphelion | 2.7996 AU |
Perihelion | 1.9488 AU |
2.3742 AU | |
Eccentricity | 0.1791 |
3.66 yr (1,336 days) | |
356.93° | |
Inclination | 24.825° |
206.84° | |
348.33° | |
Physical characteristics | |
Dimensions | 9.3 km[1] 9.31±1.0 km (IRAS)[4] 9.441±0.131 km[5] 10.66±0.43 km[6] 9.45 km (derived)[3] |
125±2 h[7] 129 h[8] |
|
0.2452±0.064[4] 0.2388±0.0311[5] 0.247±0.034[6] 0.3134 (derived)[3] |
|
S [3] | |
12.0[1][3][6] 12.3[5] 11.36±1.19[9] |
|
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1575 Winifred, provisional designation 1950 HH, is a stony Phocaea asteroid and slow rotator from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 20 April 1950, by astronomer R. C. Cameron of Indiana University at the U.S. Goethe Link Observatory, Indiana.[10]
The stony S-type asteroid is a member of the Phocaea family, a group of asteroids with similar orbital characteristics, named after the family's namesake 25 Phocaea. It orbits the Sun at a distance of 1.9–2.8 AU once every 3 years and 8 months (1,336 days). Its orbit has an eccentricity of 0.18 and an inclination of 25° with respect to the ecliptic.[1] The first precovery was taken at Johannesburg Observatory in 1928, extending the asteroid's observation arc by 22 years prior to its discovery.[10]
In July 2009, a rotational light-curve was obtained for this asteroid from photometric observations made by American astronomer Brian Warner at the U.S. Palmer Divide Observatory in Colorado. The well-defined light-curve rendered a long rotation period of 125±2 hours with an exceptionally high brightness amplitude of 1.20 in magnitude (U=3), and no sign of a non-principal axis rotation (NPAR).[7] The result superseded a previous observation by French astronomer Laurent Bernasconi in May 2005, that gave a similar, yet less accurate period of 129 hours, with a smaller amplitude of 0.51 in magnitude (U=1).[8]
According to the surveys carried out by the Infrared Astronomical Satellite, IRAS, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid has an albedo of 0.24 to 0.25 and a diameter between 9.3 and 10.7 kilometers,[4][5][6] while the Collaborative Asteroid Lightcurve Link derives a much higher albedo of 0.31 and a diameter of 9.5 kilometers.[3]
The minor planet was named for a staff member of the United States Naval Observatory in Washington D.C., Miss Winifred Sawtelle. The naming was proposed by the discovering astronomer.[2] Naming citation was published before November 1977 (M.P.C. 844).[11]
See also
References
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External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1575 Winifred at the JPL Small-Body Database
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