Q86843977
star in the constellation Cygnus
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Q86843977
Summary
Q86843977 is a star[1].
Key Facts
- Q86843977's instance of is recorded as star[2].
- Q86843977's instance of is recorded as rotating variable star[3].
- Q86843977's instance of is recorded as near-infrared source[4].
- Q86843977's constellation is recorded as Cygnus[5].
- Q86843977's spectral class is recorded as F3V[6].
- Q86843977's child astronomical body is recorded as Q28503711[7].
- Q86843977's child astronomical body is recorded as Q28503714[8].
- Q86843977's child astronomical body is recorded as Q28503716[9].
- Q86843977's catalog code is recorded as Gaia DR2 2128268380936413568[10].
- Q86843977's catalog code is recorded as KIC 9590976[11].
- Q86843977's catalog code is recorded as 2MASS J19320905+4616390[12].
- Q86843977's catalog code is recorded as Kepler-217[13].
- Q86843977's catalog code is recorded as KOI-710[14].
- Q86843977's catalog code is recorded as Gaia DR3 2128268380936413568[15].
- Q86843977's catalog code is recorded as TIC 240178935[16].
- Q86843977's catalog code is recorded as SPOCS 3966[17].
- Q86843977's catalog code is recorded as SPOCS 3967[18].
- Q86843977's type of variable star is recorded as rotating variable star[19].
- Q86843977's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.319'}[20].
- Q86843977's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.176'}[21].
- Q86843977's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.103'}[22].
- Q86843977's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.107412'}[23].
- Q86843977's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+5.3672833'}[24].
- Q86843977's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.637516'}[25].
- Q86843977's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9137'}[26].
Body
Definition and Type
Recorded instance of include star[2], rotating variable star[3], and near-infrared source[4].