6235 Burney
6235 Burney, provisional designation, is a Florian or background asteroid from the inner regions of the asteroid belt, approximately in diameter. It was discovered on 14 November 1987, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at the Kushiro Observatory on Hokkaido, Japan. The likely elongated L-type asteroid has a rotation period of 15.5 hours. It was named for Venetia Burney, who first proposed 's name.
Orbit and classification
Burney is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. In the HCM assessment by Zappala and based on osculating Keplerian orbital elements, the asteroid has also been classified as a member of the Flora family, a giant asteroid family and the largest family of stony asteroids in the main-belt.It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 4 months. Its orbit has an eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. The body's observation arc begins with its first observation as at Goethe Link Observatory in October 1950, more than 37 years prior to its official discovery observation at Kushiro.
Physical characteristics
Burney has been characterized as an L-type asteroid by Pan-STARRS survey and in the SDSS-based taxonomy. It is also an assumed S-type.Rotation period
In December 2004, a rotational lightcurve of Burney was obtained from photometric observations by Donald Pray at the Carbuncle Hill Observatory. Lightcurve analysis gave a well-defined rotation period of 15.515 hours with a brightness variation of 0.60 magnitude. The Wide-field Infrared Survey Explorer also measured a high amplitude 0.71 and 0.95 magnitude, which indicates that asteroid has an elongated shape.Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Burney measures between 3.64 and 4.083 kilometers in diameter and its surface has an albedo between 0.29 and 0.36.The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family – and calculates a diameter of 4.50 kilometers based on an absolute magnitude of 13.9.