1600 Vyssotsky
Discovery [1] | |
---|---|
Discovered by | C. A. Wirtanen |
Discovery site | Lick Observatory |
Discovery date | 22 October 1947 |
Designations | |
MPC designation | 1600 Vyssotsky |
Named after
|
Alexander Vyssotsky (astronomer)[2] |
1947 UC | |
main-belt (inner) · Hungaria [3] | |
Orbital characteristics [1] | |
Epoch 27 June 2015 (JD 2457200.5) | |
Uncertainty parameter 0 | |
Observation arc | 68.00 yr (24,836 days) |
Aphelion | 1.9179 AU |
Perihelion | 1.7799 AU |
1.8489 AU | |
Eccentricity | 0.0373 |
2.51 yr (918 days) | |
245.76° | |
Inclination | 21.169° |
60.614° | |
50.558° | |
Earth MOID | 0.8144 AU |
Physical characteristics | |
Dimensions | 7.50±0.50 km[4] 7.41±0.06 km[5] 7.67 km (calculated)[3] |
3.2011 h[6] 3.2±0.01 h[7] 3.20144±0.00002 h[8] 3.201±0.001 h[9] 3.20116±0.00004 h[10] 3.201264±0.00001 h[11] 3.201±0.001 h[12] 3.201±0.001 h[13] 3.205±0.005 h[14] 3.20124±0.00004 h[8] 3.201±0.005 h[15] 3.205±0.003 h[16] |
|
0.506±0.187[17] 0.547±0.076[4] 0.321±0.059[5] 0.3 (assumed)[3] |
|
SMASS = A A [3] |
|
12.6 | |
1600 Vyssotsky, provisional designation 1947 UC, is a reddish asteroid from the inner regions of the asteroid belt, about 8 kilometers in diameter. It was discovered on October 22, 1947 by American astronomer Carl Wirtanen at Lick Observatory on the summit of Mount Hamilton, California.[18]
The asteroid is a member of the Hungaria family, that form the last, innermost dense concentration of asteroids in the Solar System. Contrary to most members of this family, Vyssotsky has a very rare A-type spectra. It orbits the Sun at a distance of 1.8–1.9 AU once every two and a half years (918 days). Its orbit is of low-eccentricity and heavily tilted towards the plane of the ecliptic. Its geometric albedo lies between 0.03 and 0.06.[4][5][17]
Photometric observations at the Palmer Divide Observatory (see video in § External links) in the U.S. state of Colorado in 1999 were used to build a light curve for this object. The asteroid displayed a rotation period of 3.201±0.001 hours and a brightness variation of 0.19±0.01 in magnitude.[13] A repeated observation in 2014 gave a period of 3.205±0.003 hours.[16]
It was named in honor of Russian–American astronomer Alexander Vyssotsky (1888–1973) who joined the faculty of the University of Virginia in 1923 and stayed at the McCormick Observatory on Mount Jefferson, Virginia, for 35 years. He was active in the fields of photometry, astrometry and spectral classification.[2]
References
- ↑ 1.0 1.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 3.2 3.3 Lua error in package.lua at line 80: module 'strict' not found.
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- ↑ 5.0 5.1 5.2 Lua error in package.lua at line 80: module 'strict' not found.
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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 Geneve, Raoul Behrend
- The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.)
- 1600 Vyssotsky at the JPL Small-Body Database