Matches in DBpedia 2016-04 for { ?s ?p "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude."@en }
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- (5119)_1988_RA1 abstract "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude.".
- Q1412976 abstract "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude.".
- (5119)_1988_RA1 comment "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude.".
- Q1412976 comment "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude.".