Q93759766
rotating variable star in the constellation Cygnus
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Q93759766
Summary
Q93759766 is a rotating variable star[1].
Key Facts
- Q93759766's instance of is recorded as rotating variable star[2].
- Q93759766's instance of is recorded as star[3].
- Q93759766's instance of is recorded as near-infrared source[4].
- Q93759766's constellation is recorded as Cygnus[5].
- Q93759766's child astronomical body is recorded as Q28857323[6].
- Q93759766's has part is recorded as Q118392951[7].
- Q93759766's catalog code is recorded as KIC 11455181[8].
- Q93759766's catalog code is recorded as 2MASS J19272758+4919333[9].
- Q93759766's catalog code is recorded as UCAC4 697-066332[10].
- Q93759766's catalog code is recorded as TIC 26541175[11].
- Q93759766's catalog code is recorded as KOI-3131[12].
- Q93759766's catalog code is recorded as Kepler-1437[13].
- Q93759766's type of variable star is recorded as rotating variable star[14].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.400'}[15].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.027'}[16].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.917'}[17].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.71'}[18].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.11'}[19].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.82'}[20].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.62'}[21].
- Q93759766's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.71'}[22].
- Q93759766's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.93'}[23].
- Q93759766's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.9'}[24].
- Q93759766's metallicity is recorded as {'unit': '1', 'amount': '+0.02'}[25].
- Q93759766's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1182.0'}[26].