218 Bianca
- There is also a moon called Bianca.
![]() A three-dimensional model of 218 Bianca based on its light curve.
|
|
Discovery | |
---|---|
Discovered by | Johann Palisa |
Discovery date | September 4, 1880 |
Designations | |
Main belt | |
Orbital characteristics | |
Epoch 30 January 2005 (JD 2453400.5) | |
Aphelion | 445.878 Gm (2.981 AU) |
Perihelion | 351.958 Gm (2.353 AU) |
398.918 Gm (2.667 AU) | |
Eccentricity | 0.118 |
1590.479 d (4.35 a) | |
Average orbital speed
|
18.24 km/s |
301.767° | |
Inclination | 15.231° |
170.896° | |
60.97° | |
Physical characteristics | |
Dimensions | 56.735[1] km |
6.33717[2] h | |
Albedo | 0.1979 ± 0.0407[1] |
Spectral type
|
S[1] (Tholen) |
8.607[1] | |
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218 Bianca is a sizeable Main belt asteroid. It is an S-type asteroid.
It was discovered by Johann Palisa on September 4, 1880, in Pola and was named after the Austro-Hungarian opera singer Bianca Bianchi (real name Bertha Schwarz). The Vienna newspapers contained several published accounts of the circumstances surrounding the honor extended to the diva in Spring 1882.[3]
In the late 1990s, a network of astronomers worldwide gathered lightcurve data that was ultimately used to derive the spin states and shape models of ten new asteroids, including (218) Bianca. The shape model for this asteroid is asymmetrical.[2][4]
References
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External links
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- ↑ 1.0 1.1 1.2 1.3 Lua error in package.lua at line 80: module 'strict' not found. See Table 4.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
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- ↑ Durech, J.; Kaasalainen, M.; Marciniak, A.; Allen, W. H. et al. “Asteroid brightness and geometry,” Astronomy and Astrophysics, Volume 465, Issue 1, April I 2007, pp. 331-337.