511 Davida

Physical characteristics

Davida is approximately 270–310 km in diameter and comprises an estimated 1.5% of the total mass of the asteroid belt. It is a C-type asteroid, which means that it is dark in colouring with a carbonaceous chondrite composition.

From 2002 to 2007, astronomers at the Keck Observatory used the Keck II telescope, which is fitted with adaptive optics, to photograph Davida. The asteroid is not a dwarf planet: there are at least two promontories and at least one flat facet with 15-km deviations from a best-fit ellipsoid. The facet is presumably a 150-km global-scale crater like the ones seen on 253 Mathilde. Conrad et al. (2007) show that craters of this size "can be expected from the impactor size distribution, without likelihood of catastrophic disruption of Davida."

Mass

In 2001, Michalak estimated Davida to have a mass of (6.64±0.56)×10¹⁹ kg. In 2007, Baer and Chesley estimated Davida to have a mass of (5.9±0.6)×10¹⁹ kg. As of 2010, Baer suggests Davida has a mass of (3.84±0.20)×10¹⁹ kg. This most recent estimate by Baer indicates that Davida is approximately tied with 704 Interamnia as the fifth-most-massive asteroid, though the error bars of Interamnia are large.

Composition

Davida's ore content is calculated to be large, and tops other asteroids in calculated worth, with 16 Psyche coming second with a large difference in hypothetical worth.