Matches in DBpedia 2016-04 for { ?s ?p "(9992) 1997 TG19 is an unnamed, stony asteroid, classified as an eccentric Mars-crosser, that measures between 3 and 4 kilometers in diameter. It was discovered on 8 October 1997, by Japanese astronomers Tetsuo Kagawa and Takeshi Urata at Gekko Observatory near Shizuoka, Japan.The stony S-type asteroid orbits the Sun at a distance of 1.5–2.8 AU once every 3 years and 2 months (1,169 days). Its orbit shows a typically high eccentricity of 0.29 and an inclination of 3 degrees from the plane of the ecliptic.Between 2006 and 2013, three photometric light-curve analysis at the Hunters Hill Observatory, Australia, the Ondřejov Observatory, Czechia, and the U.S. Palomar Transient Factory, California, rendered a well-defined, concurring rotation period of 7000574020000000000♠5.7402±0.0005 hours (best result) with a brightness amplitude of 0.42, 0.40 and 0.27 in magnitude, respectively.According to the survey carried out by the Japanese Akari satellite, the asteroid's surface has an albedo of 0.13, which is untypically low for stony asteroids, and determines a diameter of 4.75 kilometers. The Collaborative Asteroid Lightcurve Link assumes a higher albedo of 0.20 and calculates a corresponding diameter of 3.1 kilometers, as the higher the body's reflectivity (albedo), the shorter its diameter, for a given absolute brightness (magnitude)."@en }
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- (9992)_1997_TG19 abstract "(9992) 1997 TG19 is an unnamed, stony asteroid, classified as an eccentric Mars-crosser, that measures between 3 and 4 kilometers in diameter. It was discovered on 8 October 1997, by Japanese astronomers Tetsuo Kagawa and Takeshi Urata at Gekko Observatory near Shizuoka, Japan.The stony S-type asteroid orbits the Sun at a distance of 1.5–2.8 AU once every 3 years and 2 months (1,169 days). Its orbit shows a typically high eccentricity of 0.29 and an inclination of 3 degrees from the plane of the ecliptic.Between 2006 and 2013, three photometric light-curve analysis at the Hunters Hill Observatory, Australia, the Ondřejov Observatory, Czechia, and the U.S. Palomar Transient Factory, California, rendered a well-defined, concurring rotation period of 7000574020000000000♠5.7402±0.0005 hours (best result) with a brightness amplitude of 0.42, 0.40 and 0.27 in magnitude, respectively.According to the survey carried out by the Japanese Akari satellite, the asteroid's surface has an albedo of 0.13, which is untypically low for stony asteroids, and determines a diameter of 4.75 kilometers. The Collaborative Asteroid Lightcurve Link assumes a higher albedo of 0.20 and calculates a corresponding diameter of 3.1 kilometers, as the higher the body's reflectivity (albedo), the shorter its diameter, for a given absolute brightness (magnitude).".
- Q711603 abstract "(9992) 1997 TG19 is an unnamed, stony asteroid, classified as an eccentric Mars-crosser, that measures between 3 and 4 kilometers in diameter. It was discovered on 8 October 1997, by Japanese astronomers Tetsuo Kagawa and Takeshi Urata at Gekko Observatory near Shizuoka, Japan.The stony S-type asteroid orbits the Sun at a distance of 1.5–2.8 AU once every 3 years and 2 months (1,169 days). Its orbit shows a typically high eccentricity of 0.29 and an inclination of 3 degrees from the plane of the ecliptic.Between 2006 and 2013, three photometric light-curve analysis at the Hunters Hill Observatory, Australia, the Ondřejov Observatory, Czechia, and the U.S. Palomar Transient Factory, California, rendered a well-defined, concurring rotation period of 7000574020000000000♠5.7402±0.0005 hours (best result) with a brightness amplitude of 0.42, 0.40 and 0.27 in magnitude, respectively.According to the survey carried out by the Japanese Akari satellite, the asteroid's surface has an albedo of 0.13, which is untypically low for stony asteroids, and determines a diameter of 4.75 kilometers. The Collaborative Asteroid Lightcurve Link assumes a higher albedo of 0.20 and calculates a corresponding diameter of 3.1 kilometers, as the higher the body's reflectivity (albedo), the shorter its diameter, for a given absolute brightness (magnitude).".