3401 Vanphilos
3401 Vanphilos, provisional designation, is a stony, eccentric asteroid and sizeable Mars-crosser, approximately 7 kilometers in diameter. It was discovered on 1 August 1981, by and at Harvard's Oak Ridge Observatory in Massachusetts, United States.
Orbit and classification
Vanphilos orbits the Sun in the inner main-belt at a distance of 1.5–3.2 AU once every 3 years and 8 months. Its orbit has an eccentricity of 0.36 and an inclination of 22° with respect to the ecliptic. In 1946, it was first identified as at the Finnish Turku Observatory, extending the body's observation arc by 35 years prior to its official discovery at Harvard.Physical characteristics
In the SMASS taxonomy, Vanphilos is characterized as a common S-type asteroid.Rotation period
In February and March 2008, three rotational lightcurves of Vanphilos were obtained from photometric observations by astronomers Petr Pravec, James W. Brinsfield and Robert Stephens. Light-curve analysis gave a well defined rotation period of 4.225 and 4.226 hours, respectively, with a change in brightness between 0.50 and 0.54 magnitude.In August 2014, astronomer Brian Warner derived a concurring period of 4.227 hours with an amplitude of 0.62 magnitude from his observations taken at the Palmer Divide Station in Colorado. Light-curve plots were published on-line by the Ondřejov Observatory and the Center for Solar System Studies.