Matches in DBpedia 2016-04 for { ?s ?p "19763 Klimesh, provisional designation 2000 MC, is a stony asteroid and slow rotator from the inner regions of the asteroid belt, about 7 kilometers in diameter. It was discovered on 18 June 2000, by NASA's and JPL's Near-Earth Asteroid Tracking program (NEAT) with the Maui Space Surveillance System (MSSS) at the U.S. Haleakala Observatory site on the island of Maui, Hawaii.The S-type asteroid is a member of the Phocaea family, a group of asteroids with similar orbital characteristics. It orbits the Sun at a distance of 1.9–2.9 AU once every 3 years and 8 months (1,350 days). Its orbit shows an eccentricity of 0.20 and an inclination of 23 degrees from the plane of the ecliptic.It has a very long rotation period of 101 hours with a brightness amplitude of 6999670000000000000♠0.67 in magnitude, as observed by Czech astronomer Petr Pravec at the Ondřejov Observatory during the body's 2011-opposition. At the same time an alternative analysis of a fragmentary light-curve analysis by Italian astronomer Silvano Casulli, however, only gave a period of 4.4 hours with an amplitude of 0.12. The body is possibly a \"tumbler\", that is, it might undergo a non-principal axis rotation. According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid has a diameter of 7.3 kilometers with an albedo of 0.18 and 0.16, based on two different data sets.The minor planet was named after JPL researcher Matthew Klimesh (b. 1968) who developed the efficient data compressor for archiving the voluminous NEAT data. He has been with the Communications Systems and Research Section at Caltech’s Jet Propulsion Laboratory since 1996. His research interests include data compression, rate-distortion theory and channel coding."@en }
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- 19763_Klimesh abstract "19763 Klimesh, provisional designation 2000 MC, is a stony asteroid and slow rotator from the inner regions of the asteroid belt, about 7 kilometers in diameter. It was discovered on 18 June 2000, by NASA's and JPL's Near-Earth Asteroid Tracking program (NEAT) with the Maui Space Surveillance System (MSSS) at the U.S. Haleakala Observatory site on the island of Maui, Hawaii.The S-type asteroid is a member of the Phocaea family, a group of asteroids with similar orbital characteristics. It orbits the Sun at a distance of 1.9–2.9 AU once every 3 years and 8 months (1,350 days). Its orbit shows an eccentricity of 0.20 and an inclination of 23 degrees from the plane of the ecliptic.It has a very long rotation period of 101 hours with a brightness amplitude of 6999670000000000000♠0.67 in magnitude, as observed by Czech astronomer Petr Pravec at the Ondřejov Observatory during the body's 2011-opposition. At the same time an alternative analysis of a fragmentary light-curve analysis by Italian astronomer Silvano Casulli, however, only gave a period of 4.4 hours with an amplitude of 0.12. The body is possibly a \"tumbler\", that is, it might undergo a non-principal axis rotation. According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid has a diameter of 7.3 kilometers with an albedo of 0.18 and 0.16, based on two different data sets.The minor planet was named after JPL researcher Matthew Klimesh (b. 1968) who developed the efficient data compressor for archiving the voluminous NEAT data. He has been with the Communications Systems and Research Section at Caltech’s Jet Propulsion Laboratory since 1996. His research interests include data compression, rate-distortion theory and channel coding.".