Matches in DBpedia 2016-04 for { ?s ?p "1235 Schorria, provisional designation 1931 UJ, is an asteroid from the innermost region of the asteroid belt, about 9 kilometers in diameter. The Mars-crosser is one of the slowest rotating asteroids known to exist. It was discovered on 18 October 1931, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany.The asteroid is classified as both, C-type and X-type on the Tholen scheme. It is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. The body orbits the Sun at a distance of 1.6–2.2 AU once every 2 years and 8 months (964 days). Its orbit is tilted by 25 degrees to the plane of the ecliptic and shows an eccentricity of 0.15. Contrary to the expected low albedo for dark, carbonaceous CX-type asteroids, the Collaborative Asteroid Lightcurve Link (CALL) assumes a high albedo of 0.40 for the body. This is rather typical for the descendants of the E-belt, a hypothesized population of primordial asteroids, from which the E-type Hungarian asteroids with high inclinations and a semi-major axis of 1.9 AU are thought to have originated.Based on light-curve observations conducted at the U.S. Palmer Divide Observatory in Colorado during February through April 2009, it has an outstandingly long rotation period of 7003126500000000000♠1265±80 hours, or about 52 days, with a high brightness amplitude of 7000139999999999999♠1.40 in magnitude. This makes the asteroid among the slowest rotators known. The body was also a suspected \"tumbler\". However, no significant evidence of such a non-principal axis rotation could be found.It was named after Richard Schorr (1867–1951), astronomer at Bergedorf Observatory, Hamburg, who discovered the minor planets 869 Mellena and 1240 Centenaria. The lunar crater Schorr is also named in his honour."@en }
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- 1235_Schorria abstract "1235 Schorria, provisional designation 1931 UJ, is an asteroid from the innermost region of the asteroid belt, about 9 kilometers in diameter. The Mars-crosser is one of the slowest rotating asteroids known to exist. It was discovered on 18 October 1931, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany.The asteroid is classified as both, C-type and X-type on the Tholen scheme. It is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. The body orbits the Sun at a distance of 1.6–2.2 AU once every 2 years and 8 months (964 days). Its orbit is tilted by 25 degrees to the plane of the ecliptic and shows an eccentricity of 0.15. Contrary to the expected low albedo for dark, carbonaceous CX-type asteroids, the Collaborative Asteroid Lightcurve Link (CALL) assumes a high albedo of 0.40 for the body. This is rather typical for the descendants of the E-belt, a hypothesized population of primordial asteroids, from which the E-type Hungarian asteroids with high inclinations and a semi-major axis of 1.9 AU are thought to have originated.Based on light-curve observations conducted at the U.S. Palmer Divide Observatory in Colorado during February through April 2009, it has an outstandingly long rotation period of 7003126500000000000♠1265±80 hours, or about 52 days, with a high brightness amplitude of 7000139999999999999♠1.40 in magnitude. This makes the asteroid among the slowest rotators known. The body was also a suspected \"tumbler\". However, no significant evidence of such a non-principal axis rotation could be found.It was named after Richard Schorr (1867–1951), astronomer at Bergedorf Observatory, Hamburg, who discovered the minor planets 869 Mellena and 1240 Centenaria. The lunar crater Schorr is also named in his honour.".