511 Davida

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511 Davida
Image:511 davida.jpg
Discovery
Discovered by: R. S. Dugan
Discovery date: May 30, 1903
Orbital characteristics
Epoch October 22, 2004 (JD 2453300.5)
Aphelion561.538 Gm (3.754 AU)
Perihelion: 385.946 Gm (2.580 AU)
Semi-major axis: 473.742 Gm (3.167 AU)
Eccentricity: 0.185
Orbital period: 2058.370 d (5.64 a)
Avg. orbital speed: 16.59 km/s
Mean anomaly: 124.997°
Inclination: 15.936°
Longitude of ascending node: 107.683°
Argument of perihelion: 338.694°
Physical characteristics
Dimensions: 326.1 km
Mass: 3.6×1019 kg
Mean density: 2.0 g/cm³
Equatorial surface gravity: 0.0911 m/s²
Escape velocity: 0.1724 km/s
Rotation period: 0.2137 d 1
Albedo: 0.054–0.066 2
Temperature: ~160 K
Spectral type: C
Absolute magnitude: 6.22

511 Davida (pronounced /dəˈvɪdə/?) is a large main belt asteroid. It was discovered by R. S. Dugan in 1903. It is thought to be the sixth most massive asteroid after Ceres, Vesta, Pallas, Hygiea, and Interamnia, averaging some 326 km in diameter and comprising an estimated 1.3% of the total mass of the asteroid belt. It is a C-type asteroid, which means that it is dark in colouring with a carbonate composition.

Davida is one of the few main belt asteroids whose shape has been determined by ground-based visual observation. In 2002, astronomers at the Keck Observatory used the Keck II telescope, which is fitted with adaptive optics, to photograph Davida. The image revealed a semi-oblong object with at least two flat facets. Its rotation period is about 5 hours.

Davida is named after David Peck Todd, an astronomy professor at Amherst College.

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511 Davida


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