Matches in DBpedia 2016-04 for { ?s ?p "ADS 16402 is a binary star system, composed of two sun-like stars located 450 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831. The two stars are separated by 1500 AUs. The star system is estimated to be 3.6 billion years old. The secondary star ADS 16402 B is also designated HAT-P-1."@en }
Showing triples 1 to 4 of
4
with 100 triples per page.
- ADS_16402 abstract "ADS 16402 is a binary star system, composed of two sun-like stars located 450 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831. The two stars are separated by 1500 AUs. The star system is estimated to be 3.6 billion years old. The secondary star ADS 16402 B is also designated HAT-P-1.".
- Q290674 abstract "ADS 16402 is a binary star system, composed of two sun-like stars located 450 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831. The two stars are separated by 1500 AUs. The star system is estimated to be 3.6 billion years old. The secondary star ADS 16402 B is also designated HAT-P-1.".
- ADS_16402 comment "ADS 16402 is a binary star system, composed of two sun-like stars located 450 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831. The two stars are separated by 1500 AUs. The star system is estimated to be 3.6 billion years old. The secondary star ADS 16402 B is also designated HAT-P-1.".
- Q290674 comment "ADS 16402 is a binary star system, composed of two sun-like stars located 450 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831. The two stars are separated by 1500 AUs. The star system is estimated to be 3.6 billion years old. The secondary star ADS 16402 B is also designated HAT-P-1.".