Q88984550
rotating variable star in the constellation Lyra
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Q88984550
Summary
Q88984550 is a rotating variable star[1].
Key Facts
- Q88984550's instance of is recorded as rotating variable star[2].
- Q88984550's instance of is recorded as star[3].
- Q88984550's instance of is recorded as near-infrared source[4].
- Q88984550's constellation is recorded as Lyra[5].
- Q88984550's spectral class is recorded as M1V[6].
- Q88984550's child astronomical body is recorded as Q97051905[7].
- Q88984550's catalog code is recorded as KIC 6592335[8].
- Q88984550's catalog code is recorded as KOI-4777[9].
- Q88984550's catalog code is recorded as 2MASS J19090291+4201563[10].
- Q88984550's catalog code is recorded as Gaia DR2 2102436351673656704[11].
- Q88984550's catalog code is recorded as Kepler-1971[12].
- Q88984550's catalog code is recorded as Gaia DR3 2102436351673656704[13].
- Q88984550's catalog code is recorded as TIC 158427808[14].
- Q88984550's type of variable star is recorded as rotating variable star[15].
- Q88984550's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.221'}[16].
- Q88984550's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.671'}[17].
- Q88984550's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.449'}[18].
- Q88984550's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.0'}[19].
- Q88984550's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.830034'}[20].
- Q88984550's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.41'}[21].
- Q88984550's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.4'}[22].
- Q88984550's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.8323'}[23].
- Q88984550's metallicity is recorded as {'unit': '1', 'amount': '+0.1'}[24].
- Q88984550's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+170.66'}[25].
- Q88984550's SIMBAD ID is recorded as Kepler-1971[26].