3255 Tholen
3255 Tholen, provisional designation "", is a stony asteroid, Mars-crosser and relatively fast rotator, that measures approximately in diameter. It was discovered on 2 September 1980, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona. The S-type asteroid has a rotation period of 2.95 hours. It was later named after American astronomer David Tholen. Orbit and classification. "Tholen" is a Mars-crossing asteroid, crossing the orbit of Mars at 1.666 AU. Members of this dynamically unstable group are located between the main belt and near-Earth populations. It orbits the Sun at  a distance of 1.5–3.2 AU once every 3 years and 8 months (1,334 days; semi-major axis of 2.37 AU). Its orbit has an eccentricity of 0.36 and an inclination of 21° with respect to the ecliptic. In September 1969, it was first observed as "" at the Argentinian El Leoncito site, extending the body's observation arc by 11 years prior to its official discovery observation at Anderson Mesa. Naming. This minor planet was named after David J. Tholen (born 1955), a discoverer of minor planets and planetary scientist at the Institute for Astronomy of the University of Hawaii , known for his eight-color taxonomic scheme on minor planets. The official naming citation was published by the Minor Planet Center on 14 April 1987 (). Physical characteristics. In the SMASS classification, as well as in the Bus–DeMeo classification, "Tholen" is a common S-type asteroid. Diameter and albedo. According to the space-based survey carried out by the Japanese Akari satellite and NASA's NEOWISE mission, the asteroid measures between 4.0 and 6.8 kilometers in diameter, and its surface has an albedo of 0.14 and 0.34, respectively, while the "Collaborative Asteroid Lightcurve Link" assumes a standard albedo for stony  asteroids of 0.20 and derives a diameter of 5.1 kilometers with an absolute magnitude of 13.84. Rotation period. Several rotational lightcurves were obtained for this asteroid from photometric observations. In September 2013, Italian astronomer Andrea Ferrero at the Bigmuskie Observatory in Mombercelli, Italy, derived a rotation period of hours with a brightness variation of 0.11 in magnitude (), while two month later, in November 2013, astronomer Brian A. Skiff obtained two lightcurves that both gave a period of 2.95 and an amplitude of 0.24 and 0.28 in magnitude, respectively (). The results supersede two older lightcurves from 1991 and 2002, that gave  a period of and 6 hours, respectively ().