MOA-2010-BLG-477L

http://dbpedia.org/resource/MOA-2010-BLG-477L an entity of type: Thing

MOA-2010-BLG-477L is a star whose existence was detected when it caused a microlensing event in August, 2010. The microlensing event also revealed the existence of a planet orbiting the star. At first the star was thought to be about 0.67 times the mass of the Sun, in the main-sequence phase of its stellar evolution. But by the time the star should have been separated enough in the sky from the source star of the microlensing event it was not detected, implying that it is actually a dim white dwarf star. rdf:langString
rdf:langString MOA-2010-BLG-477L
rdf:langString MOA-2010-BLG-477L
xsd:integer 36021396
xsd:integer 1112382682
xsd:integer 7500
rdf:langString K
xsd:integer 2300
rdf:langString J2000
rdf:langString b
xsd:double 0.53 1.5
xsd:integer 2
rdf:langString MOA+2010-BLG-477
rdf:langString MOA+2010-BLG-477+b
rdf:langString The star
rdf:langString planet b
rdf:langString unknown
rdf:langString MOA-2010-BLG-477L is a star whose existence was detected when it caused a microlensing event in August, 2010. The microlensing event also revealed the existence of a planet orbiting the star. At first the star was thought to be about 0.67 times the mass of the Sun, in the main-sequence phase of its stellar evolution. But by the time the star should have been separated enough in the sky from the source star of the microlensing event it was not detected, implying that it is actually a dim white dwarf star.
xsd:nonNegativeInteger 5957

data from the linked data cloud