HAT-P-27

http://dbpedia.org/resource/HAT-P-27 an entity of type: Thing

HAT-P-27, also known as WASP-40, is the primary of a binary star system about 650 light-years away. It is a G-type main-sequence star. The star's age is similar to the Sun's at 4.4 billion years. HAT-P-27 is enriched in heavy elements, having a 195% concentration of iron compared to the Sun. The very dim stellar companion was detected in 2015 at a projected separation of 0.656″ and proven to be physically bound to the system in 2016. rdf:langString
HAT-P-27 — звезда, которая находится в созвездии Девы на расстоянии около 665 световых лет от нас. Вокруг звезды обращается как минимум одна планета. rdf:langString
rdf:langString HAT-P-27
rdf:langString HAT-P-27
rdf:langString HAT-P-27
rdf:langString HAT-P-27 B
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xsd:integer 1063250567
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xsd:double 4.4
xsd:double 12.214
xsd:double 0.656
rdf:langString G8
xsd:double 0.078
rdf:langString J2000
rdf:langString b
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xsd:integer 85
xsd:double 0.57
xsd:double 0.66 0.945
xsd:double 0.29
xsd:double 0.036
xsd:double 4.9922
xsd:double 3.039586
rdf:langString HAT-P-27
xsd:double -2.757
xsd:double -28.621
xsd:double -15.901
xsd:double 0.898 1.038
xsd:double 0.4
xsd:double 0.6
xsd:double 0.0403
xsd:integer 5300
rdf:langString HAT-P-27, also known as WASP-40, is the primary of a binary star system about 650 light-years away. It is a G-type main-sequence star. The star's age is similar to the Sun's at 4.4 billion years. HAT-P-27 is enriched in heavy elements, having a 195% concentration of iron compared to the Sun. The very dim stellar companion was detected in 2015 at a projected separation of 0.656″ and proven to be physically bound to the system in 2016.
rdf:langString HAT-P-27 — звезда, которая находится в созвездии Девы на расстоянии около 665 световых лет от нас. Вокруг звезды обращается как минимум одна планета.
xsd:nonNegativeInteger 7061

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