Matches in DBpedia 2016-04 for { ?s ?p "1101 Clematis is a minor planet orbiting the Sun that was discovered by German astronomer Karl Wilhelm Reinmuth on September 22, 1928, in Heidelberg. Initially it received the designation 1928 SJ. It was named for the clematis flower.Photometric observations made in 2003 at the Santana Observatory in Rancho Cucamonga, California, give a synodic rotation period of 12.68 ± 0.01 hours. The light curve shows a brightness variation of 0.40 ± 0.05 in magnitude.This object is the namesake of a dynamic family of 5–16 asteroids that share similar spectral properties and orbital elements; hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination."@en }
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- 1101_Clematis abstract "1101 Clematis is a minor planet orbiting the Sun that was discovered by German astronomer Karl Wilhelm Reinmuth on September 22, 1928, in Heidelberg. Initially it received the designation 1928 SJ. It was named for the clematis flower.Photometric observations made in 2003 at the Santana Observatory in Rancho Cucamonga, California, give a synodic rotation period of 12.68 ± 0.01 hours. The light curve shows a brightness variation of 0.40 ± 0.05 in magnitude.This object is the namesake of a dynamic family of 5–16 asteroids that share similar spectral properties and orbital elements; hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination.".
- Q135934 abstract "1101 Clematis is a minor planet orbiting the Sun that was discovered by German astronomer Karl Wilhelm Reinmuth on September 22, 1928, in Heidelberg. Initially it received the designation 1928 SJ. It was named for the clematis flower.Photometric observations made in 2003 at the Santana Observatory in Rancho Cucamonga, California, give a synodic rotation period of 12.68 ± 0.01 hours. The light curve shows a brightness variation of 0.40 ± 0.05 in magnitude.This object is the namesake of a dynamic family of 5–16 asteroids that share similar spectral properties and orbital elements; hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination.".