Matches in DBpedia 2015-10 for { ?s ?p "131 Vala is an inner main-belt asteroid. It was discovered by C. H. F. Peters on May 24, 1873, and named after Völva, a prophetess in Norse mythology. One observation of an occultation of a star by Vala is from Italy (May 26, 2002). 10-µm radiometric data collected from Kitt Peak in 1975 gave a diameter estimate of 34 km.In the Tholen classification system, it is categorized as an SU-type asteroid, while the Bus asteroid taxonomy system lists it as an K-type asteroid. Photometric observations of this asteroid during 2007 at the Organ Mesa Observatory in Las Cruces, New Mexico were used to create a "nearly symmetric bimodal" light curve plot. This showed a rotation period of 10.359 ± 0.001 hours and a brightness variation of 0.09 ± 0.02 magnitude during each cycle. The result is double the 5.18 hour period reported in the JPL Small-Body Database.On 2028-Apr-05, Vala will pass 0.0276 AU (4,130,000 km; 2,570,000 mi) from asteroid 2 Pallas."@en }
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- 131_Vala abstract "131 Vala is an inner main-belt asteroid. It was discovered by C. H. F. Peters on May 24, 1873, and named after Völva, a prophetess in Norse mythology. One observation of an occultation of a star by Vala is from Italy (May 26, 2002). 10-µm radiometric data collected from Kitt Peak in 1975 gave a diameter estimate of 34 km.In the Tholen classification system, it is categorized as an SU-type asteroid, while the Bus asteroid taxonomy system lists it as an K-type asteroid. Photometric observations of this asteroid during 2007 at the Organ Mesa Observatory in Las Cruces, New Mexico were used to create a "nearly symmetric bimodal" light curve plot. This showed a rotation period of 10.359 ± 0.001 hours and a brightness variation of 0.09 ± 0.02 magnitude during each cycle. The result is double the 5.18 hour period reported in the JPL Small-Body Database.On 2028-Apr-05, Vala will pass 0.0276 AU (4,130,000 km; 2,570,000 mi) from asteroid 2 Pallas.".