Kepler-91
star
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Kepler-91
Summary
Kepler-91 is a star[1].
Key Facts
- Kepler-91's instance of is recorded as star[2].
- Kepler-91's instance of is recorded as eclipsing binary star[3].
- Kepler-91's instance of is recorded as red giant branch star[4].
- Kepler-91's instance of is recorded as near-infrared source[5].
- Kepler-91's instance of is recorded as rotating variable star[6].
- Kepler-91's constellation is recorded as Lyra[7].
- Kepler-91's spectral class is recorded as G5[8].
- Kepler-91's child astronomical body is recorded as Kepler-91b[9].
- Kepler-91's catalog code is recorded as 2MASS J19024148+4407002[10].
- Kepler-91's catalog code is recorded as KIC 8219268[11].
- Kepler-91's catalog code is recorded as Gaia DR2 2105909326647414400[12].
- Kepler-91's catalog code is recorded as KOI-2133[13].
- Kepler-91's catalog code is recorded as Kepler-91[14].
- Kepler-91's catalog code is recorded as Gaia DR3 2105909326647414400[15].
- Kepler-91's catalog code is recorded as TIC 352011875[16].
- Kepler-91's type of variable star is recorded as Beta Lyrae variable[17].
- Kepler-91's type of variable star is recorded as rotating variable star[18].
- Kepler-91's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.790'}[19].
- Kepler-91's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.23'}[20].
- Kepler-91's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.136'}[21].
- Kepler-91's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9'}[22].
- Kepler-91's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.467858'}[23].
- Kepler-91's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+16.727634'}[24].
- Kepler-91's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.31'}[25].
- Kepler-91's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+6.308464'}[26].
Body
Definition and Type
Recorded instance of include star[2], eclipsing binary star[3], red giant branch star[4], near-infrared source[5], and rotating variable star[6].