Q90560315
rotating variable star in the constellation Cygnus
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Q90560315
Summary
Q90560315 is a rotating variable star[1].
Key Facts
- Q90560315's instance of is recorded as rotating variable star[2].
- Q90560315's instance of is recorded as star[3].
- Q90560315's instance of is recorded as near-infrared source[4].
- Q90560315's constellation is recorded as Cygnus[5].
- Q90560315's spectral class is recorded as G7V[6].
- Q90560315's child astronomical body is recorded as Q82443614[7].
- Q90560315's catalog code is recorded as Gaia DR2 2086847785054193792[8].
- Q90560315's catalog code is recorded as KOI-2620[9].
- Q90560315's catalog code is recorded as KIC 11465950[10].
- Q90560315's catalog code is recorded as 2MASS J19470081+4922411[11].
- Q90560315's catalog code is recorded as Kepler-1862[12].
- Q90560315's catalog code is recorded as Gaia DR3 2086847785054193792[13].
- Q90560315's catalog code is recorded as TIC 27913951[14].
- Q90560315's type of variable star is recorded as rotating variable star[15].
- Q90560315's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.196'}[16].
- Q90560315's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.827127'}[17].
- Q90560315's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.847'}[18].
- Q90560315's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.5824638'}[19].
- Q90560315's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.94'}[20].
- Q90560315's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.895'}[21].
- Q90560315's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.761'}[22].
- Q90560315's metallicity is recorded as {'unit': '1', 'amount': '+0.22'}[23].
- Q90560315's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1314.06'}[24].
- Q90560315's SIMBAD ID is recorded as Kepler-1862[25].
- Q90560315's NASA Exoplanet Archive ID is recorded as Kepler-1862[26].