Q80399076
rotating variable star in the constellation Cygnus
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Q80399076
Summary
Q80399076 is a rotating variable star[1].
Key Facts
- Q80399076's instance of is recorded as rotating variable star[2].
- Q80399076's instance of is recorded as star[3].
- Q80399076's instance of is recorded as near-infrared source[4].
- Q80399076's constellation is recorded as Cygnus[5].
- Q80399076's spectral class is recorded as G2V[6].
- Q80399076 is part of Q1348576[7].
- Q80399076's child astronomical body is recorded as Q97051873[8].
- Q80399076's catalog code is recorded as Gaia DR2 2081880913079644288[9].
- Q80399076's catalog code is recorded as KIC 8331612[10].
- Q80399076's catalog code is recorded as 2MASS J20050688+4415019[11].
- Q80399076's catalog code is recorded as Kepler-1915[12].
- Q80399076's catalog code is recorded as Gaia DR3 2081880913079644288[13].
- Q80399076's catalog code is recorded as TIC 185184560[14].
- Q80399076's catalog code is recorded as KOI-3318[15].
- Q80399076's catalog code is recorded as Kepler-1915A[16].
- Q80399076's type of variable star is recorded as rotating variable star[17].
- Q80399076's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.521'}[18].
- Q80399076's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.175'}[19].
- Q80399076's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.039'}[20].
- Q80399076's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.827951'}[21].
- Q80399076's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.90023607'}[22].
- Q80399076's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.03'}[23].
- Q80399076's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.084'}[24].
- Q80399076's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6688'}[25].
- Q80399076's metallicity is recorded as {'unit': '1', 'amount': '+0.06'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], and near-infrared source[4].
Use and Application
Q80399076 is part of Q1348576[7].