720 Bohlinia
A three-dimensional model of 720 Bohlinia based on its light curve.
|
|
| Discovery | |
|---|---|
| Discovered by | Franz Kaiser |
| Discovery site | Heidelberg |
| Discovery date | October 18, 1911 |
| Designations | |
| 1911 MW | |
| Orbital characteristics | |
| Epoch August 18, 2005 (JDCT 2453600.5) | |
| Aphelion | 2.928 AU |
| Perihelion | 2.848 AU |
| 2.888 AU | |
| Eccentricity | 0.014 |
| 4.908 a | |
| 281.521° | |
| Inclination | 2.359° |
| 35.939° | |
| 103.893° | |
| Physical characteristics | |
| Dimensions | 34.64 ± 1.81[1] km |
| Mass | (5.97 ± 0.80) × 1016[1] kg |
|
Mean density
|
2.74 ± 0.56[1] g/cm3 |
| Albedo | 0.203[2] |
| 9.71[2] | |
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720 Bohlinia is a minor planet orbiting the Sun that was discovered by Franz Kaiser, a German astronomer in 1911. It is named for Swedish astronomer Karl Petrus Theodor Bohlin, to mark his 65th birthday.[3] He had worked on the orbits of asteroids.[4]
It is one of the Koronis family of asteroids. A group of astronomers, including Lucy d’Escoffier Crespo da Silva and Richard P. Binzel, used observations made between 1998 through 2000 to determine the spin-vector alignment of these asteroids. The collaborative work resulted in the creation of 61 new individual rotation lightcurves to augment previous published observations.[5]
Binzel and Schelte Bus further added to the knowledge about this asteroid in a lightwave survey published in 2003. This project was known as Small Main-belt Asteroid Spectroscopic Survey, Phase II or SMASSII, which built on a previous survey of the main-belt asteroids. The visible-wavelength (0.435-0.925 micrometre) spectra data was gathered between August 1993 and March 1999.[6]
References
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This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |
- ↑ 1.0 1.1 1.2 Lua error in package.lua at line 80: module 'strict' not found. See Table 1.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ http://ssd.jpl.nasa.gov/sbdb.cgi#top
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Slivan, S. M., Binzel, R. P., Crespo da Silva, L. D., Kaasalainen, M., Lyndaker, M. M., Krco, M.: “Spin vectors in the Koronis family: comprehensive results from two independent analyses of 213 rotation lightcurves,”Icarus, 162, 2003, pp. 285–307.
- ↑ Bus, S., Binzel, R. P. Small Main-belt Asteroid Spectroscopic Survey, Phase II. EAR-A-I0028-4-SBN0001/SMASSII-V1.0. NASA Planetary Data System, 2003.
