Matches in DBpedia 2016-04 for { ?s ?p "3873 Roddy (1984 WB) is a Mars-crossing asteroid discovered on November 21, 1984 by C. Shoemaker at Palomar. It is a member of the Hungaria family and is a probable binary system. Photometric observations of the asteroid during 2005 at the Palmer Divide Observatory in Colorado Springs, Colorado, were used to generate a light-curve with a period of 7000247820000000000♠2.4782±0.0002 hours and a variation in brightness of 0.09 ± 0.02 magnitude."@en }
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- 3873_Roddy abstract "3873 Roddy (1984 WB) is a Mars-crossing asteroid discovered on November 21, 1984 by C. Shoemaker at Palomar. It is a member of the Hungaria family and is a probable binary system. Photometric observations of the asteroid during 2005 at the Palmer Divide Observatory in Colorado Springs, Colorado, were used to generate a light-curve with a period of 7000247820000000000♠2.4782±0.0002 hours and a variation in brightness of 0.09 ± 0.02 magnitude.".
- Q639165 abstract "3873 Roddy (1984 WB) is a Mars-crossing asteroid discovered on November 21, 1984 by C. Shoemaker at Palomar. It is a member of the Hungaria family and is a probable binary system. Photometric observations of the asteroid during 2005 at the Palmer Divide Observatory in Colorado Springs, Colorado, were used to generate a light-curve with a period of 7000247820000000000♠2.4782±0.0002 hours and a variation in brightness of 0.09 ± 0.02 magnitude.".
- 3873_Roddy comment "3873 Roddy (1984 WB) is a Mars-crossing asteroid discovered on November 21, 1984 by C. Shoemaker at Palomar. It is a member of the Hungaria family and is a probable binary system. Photometric observations of the asteroid during 2005 at the Palmer Divide Observatory in Colorado Springs, Colorado, were used to generate a light-curve with a period of 7000247820000000000♠2.4782±0.0002 hours and a variation in brightness of 0.09 ± 0.02 magnitude.".
- Q639165 comment "3873 Roddy (1984 WB) is a Mars-crossing asteroid discovered on November 21, 1984 by C. Shoemaker at Palomar. It is a member of the Hungaria family and is a probable binary system. Photometric observations of the asteroid during 2005 at the Palmer Divide Observatory in Colorado Springs, Colorado, were used to generate a light-curve with a period of 7000247820000000000♠2.4782±0.0002 hours and a variation in brightness of 0.09 ± 0.02 magnitude.".