4324 Bickel
"Bickel" orbits the Sun in the central main-belt at a distance of 2.0–3.1 AU once every 4 years and 1 month (1,483 days). Its orbit has an eccentricity of 0.20 and an inclination of 8° with respect to the ecliptic. It was first identified as at Heidelberg Observatory in 1924, extending the body's observation arc by 57 years prior to its official discovery observation at Socorro. "Bickel" has been characterized as a common S-type asteroid. In September 2001, the first ever conducted photometric observation of "Bickel" at the Rozhen Observatory, Bulgaria, rendered a rotational lightcurve with a longer-than-average period of hours and a brightness variation of 0.63 magnitude (). A more refined lightcurve was obtained in October 2005, by astronomers Raymond Poncy, Laurent Bernasconi and Rui Goncalves, which gave a well-defined period of hours with an amplitude of 0.72 magnitude (). According to observations by NASA's space-based Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Bickel" measures 11.7 kilometers in diameter and its surface has an albedo of 0.248, while the "Collaborative Asteroid Lightcurve Link" assumes a standard albedo for stony asteroids of 0.20 and calculates a slightly larger diameter of 12.4 kilometers with an absolute magnitude of 11.9. This minor planet was named in honor of German amateur astronomer Wolf Bickel (born 1942) who began observing minor planets at his private Bergisch Gladbach Observatory in 1995. At the time this minor planet was named, he had discovered more than 540 numbered minor planets. The official naming citation was published by the Minor Planet Center on 22 July 2013 (). Bickel has become Germany's most prolific discoverer of asteroids, ahead of (professional) astronomer Freimut Börngen, the first time in 150 years, that an amateur astronomer is ranking first among the German top discoverers. His total number of discoveries has since increased to more than 600.
Naming
The asteroid was named after amateur astronomer Wolf Bickel.