1373 Cincinnati
From Infogalactic: the planetary knowledge core
Discovery [1][2] | |
---|---|
Discovered by | E. Hubble |
Discovery site | Mount Wilson Obs. |
Discovery date | 30 August 1935 |
Designations | |
MPC designation | 1373 Cincinnati |
Named after
|
Cincinnati Obs.[3] |
1935 QN | |
main-belt (outer) | |
Orbital characteristics [1][4] | |
Epoch 27 June 2015 (JD 2457200.5) | |
Uncertainty parameter 0 | |
Observation arc | 79.83 yr (29,159 days) |
Aphelion | 4.4969 AU |
Perihelion | 2.3451 AU |
3.4210 AU | |
Eccentricity | 0.3145 |
6.33 yr (2311.2 days) | |
239.90° | |
Inclination | 38.936° |
297.47° | |
99.314° | |
Earth MOID | 1.6332 AU |
Physical characteristics | |
5.28 h | |
Temperature | ~151 K[citation needed] |
SMASS = Xk | |
11.6 | |
1373 Cincinnati, provisional designation 1935 QN, is an asteroid of the outer main-belt, discovered by the famous American astronomer Edwin Hubble at Mount Wilson Observatory on August 30, 1935. It was his only asteroid discovery.
The X-type asteroid has an extremely inclined, cometary-like orbit of 39 degrees to the ecliptic.[1][5] Cincinnati is similar to the Cybele asteroids.[6]
Recommended by the Minor Planet Center, the asteroid is named after the Cincinnati Observatory, whose staff provided most of the orbit computations.[1]
References
- ↑ 1.0 1.1 1.2 1.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ http://www.minorplanetcenter.net/iau/lists/NumberedMPs.html
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ The Asteroid Orbital Elements Database
- ↑ Spectral properties of asteroids in cometary orbits
- ↑ Dynamical evolution of the Cybele asteroids, V. Carruba, D. Nesvorny, M. E. Huaman, (2015)
External links
- Lua error in package.lua at line 80: module 'strict' not found.
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