Matches in DBpedia 2016-04 for { ?s ?p "(6491) 1991 OA is a highly eccentric, stony asteroid, classified as near-Earth object and potentially hazardous asteroid, about half a kilometer in diameter. It was discovered on 16 July 1991, by American astronomer Henry E. Holt at the U.S. Palomar Observatory in California.The asteroid is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. Its Earth Minimum orbit intersection distance (MOID) is 0.0429 AU, and on 1 August 2086, it will make a close approach and pass by Earth at a distance of 0.09 AU (13,000,000 km).The S-type asteroid orbits the Sun at a distance of 1.0–4.0 AU once every 3 years and 12 months (1,445 days). Its orbit shows an very high eccentricity of 0.59 and an inclination of 6 degrees from the plane of the ecliptic. A photometric light-curve analysis rendered a rotation period of 2.69 hours with an brightness amplitude of 0.08 in magnitude. The Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.20 and derives a diameter of 0.53 kilometers."@en }
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- (6491)_1991_OA abstract "(6491) 1991 OA is a highly eccentric, stony asteroid, classified as near-Earth object and potentially hazardous asteroid, about half a kilometer in diameter. It was discovered on 16 July 1991, by American astronomer Henry E. Holt at the U.S. Palomar Observatory in California.The asteroid is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. Its Earth Minimum orbit intersection distance (MOID) is 0.0429 AU, and on 1 August 2086, it will make a close approach and pass by Earth at a distance of 0.09 AU (13,000,000 km).The S-type asteroid orbits the Sun at a distance of 1.0–4.0 AU once every 3 years and 12 months (1,445 days). Its orbit shows an very high eccentricity of 0.59 and an inclination of 6 degrees from the plane of the ecliptic. A photometric light-curve analysis rendered a rotation period of 2.69 hours with an brightness amplitude of 0.08 in magnitude. The Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.20 and derives a diameter of 0.53 kilometers.".
- Q619748 abstract "(6491) 1991 OA is a highly eccentric, stony asteroid, classified as near-Earth object and potentially hazardous asteroid, about half a kilometer in diameter. It was discovered on 16 July 1991, by American astronomer Henry E. Holt at the U.S. Palomar Observatory in California.The asteroid is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. Its Earth Minimum orbit intersection distance (MOID) is 0.0429 AU, and on 1 August 2086, it will make a close approach and pass by Earth at a distance of 0.09 AU (13,000,000 km).The S-type asteroid orbits the Sun at a distance of 1.0–4.0 AU once every 3 years and 12 months (1,445 days). Its orbit shows an very high eccentricity of 0.59 and an inclination of 6 degrees from the plane of the ecliptic. A photometric light-curve analysis rendered a rotation period of 2.69 hours with an brightness amplitude of 0.08 in magnitude. The Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.20 and derives a diameter of 0.53 kilometers.".