Discovery
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Discovered by | Johann Palisa |
Discovery date | September 4, 1880 |
Designations
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Minor planet category |
Main belt |
Epoch 30 January, 2005 (JD 2453400.5) | |
Aphelion | 445.878 Gm (2.981 AU) |
Perihelion | 351.958 Gm (2.353 AU) |
Semi-major axis | 398.918 Gm (2.667 AU) |
Eccentricity | 0.118 |
Orbital period | 1590.479 d (4.35 a) |
Average orbital speed | 18.24 km/s |
Mean anomaly | 301.767° |
Inclination | 15.231° |
Longitude of ascending node | 170.896° |
Argument of perihelion | 60.97° |
Physical characteristics
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Dimensions | 61.0 km |
Mass | unknown |
Mean density | unknown |
Equatorial surface gravity | unknown |
Escape velocity | unknown |
Rotation period | 6.337 h |
Albedo | 0.174 |
Temperature | unknown |
Spectral type | S |
Absolute magnitude (H) | 8.6 |
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.[1]
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.[2][3]
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