Q93759962
rotating variable star in the constellation Lyra
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Q93759962
Summary
Q93759962 is a rotating variable star[1].
Key Facts
- Q93759962's instance of is recorded as rotating variable star[2].
- Q93759962's instance of is recorded as star[3].
- Q93759962's instance of is recorded as near-infrared source[4].
- Q93759962's constellation is recorded as Lyra[5].
- Q93759962's spectral class is recorded as M0V[6].
- Q93759962's child astronomical body is recorded as Q28857201[7].
- Q93759962's catalog code is recorded as Gaia DR2 2104065209429419520[8].
- Q93759962's catalog code is recorded as KIC 6186964[9].
- Q93759962's catalog code is recorded as KOI-2839[10].
- Q93759962's catalog code is recorded as 2MASS J19001557+4133175[11].
- Q93759962's catalog code is recorded as Kepler-1366[12].
- Q93759962's catalog code is recorded as Gaia DR3 2104065209430717568[13].
- Q93759962's catalog code is recorded as TIC 120421638[14].
- Q93759962's type of variable star is recorded as rotating variable star[15].
- Q93759962's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.772'}[16].
- Q93759962's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.099'}[17].
- Q93759962's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.961'}[18].
- Q93759962's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.87936'}[19].
- Q93759962's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.62'}[20].
- Q93759962's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.6'}[21].
- Q93759962's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.1401'}[22].
- Q93759962's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}[23].
- Q93759962's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+806000'}[24].
- Q93759962's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+467.268'}[25].
- Q93759962's SIMBAD ID is recorded as Kepler-1366[26].