(511) Davida

from Wikipedia, the free encyclopedia
Asteroid
(511) Davida
Image through the Keck telescope
Image through the Keck telescope
Properties of the orbit ( animation )
Orbit type Outer main belt
Major semi-axis 3.166  AU
eccentricity 0.186
Perihelion - aphelion 2.576 AU - 3.756 AU
Inclination of the orbit plane 15.9 °
Length of the ascending node 107.6 °
Argument of the periapsis 338.2 °
Time of passage of the perihelion June 23, 2008
Sidereal period 5 a 232 d
Mean orbital velocity 16.6 km / s
Physical Properties
Medium diameter (270.327 ± 1.045) km
Albedo 0.0540
Rotation period 5 h 8 min
Absolute brightness 6.22 mag
Spectral class
(according to Tholen)
C.
Spectral class
(according to SMASSII)
C.
history
Explorer R. S. Dugan
Date of discovery May 30, 1903
Another name 1903 LU
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items.

(511) Davida is an asteroid of the main outer asteroid belt discovered by Raymond Smith Dugan on May 30, 1903 . The asteroid is named after the American astronomer David Peck Todd .

Davida moves at a distance of 2.58 ( perihelion ) to 3.76 ( aphelion ) astronomical units around the sun in 5.638 years . The orbit is inclined 15.94 ° to the ecliptic , the orbital eccentricity is 0.186.

With a mean diameter of around 270 km, Davida is one of the largest asteroids in the main belt. The asteroid has a dark carbonaceous surface with an albedo of 0.054. It rotates around its own axis in around 5 hours and 8 minutes.

In 2002, images of Davida at the Keck Observatory were made using adaptive optics that show an irregular body.

A series of images of the asteroid (511) Davida over a period of just over an hour (December 26, 2002, Keck Observatory )

See also

Web links

Commons : 511 Davida  - Collection of images, videos and audio files