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About: Kepler-38     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatPlanetaryTransitVariables, within Data Space : dbpedia.org associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatBinaryStarsyago:BinaryStar109221070yago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930yago:WikicatKeplerObjectsOfIntereststaryago:Star109444100yago:Thing100002452yago:Variable109468959yago:Whole100003553yago:WikicatPlanetaryTransitVariables New Facet based on Instances of this Class

Kepler-38 is a binary star system in the constellation Lyra. These stars, called Kepler-38A and Kepler-38B have masses of 95% and 25% solar masses respectively. The brighter star is spectral class G while the secondary has spectral class M. They are separated by 0.147 AU, and complete an eccentric orbit around a common center of mass every 18.8 days.