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
xsd:integer
36008648
xsd:integer
1063250567
<astronomicalUnit>
131.0
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
xsd:double
4.51
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