Q113709726
eclipsing binary star in the constellation Cygnus
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Q113709726
Summary
Q113709726 is an eclipsing binary star[1].
Key Facts
- Q113709726's instance of is recorded as eclipsing binary star[2].
- Q113709726's instance of is recorded as near-infrared source[3].
- Q113709726's instance of is recorded as eruptive variable star[4].
- Q113709726's constellation is recorded as Cygnus[5].
- Q113709726's spectral class is recorded as K3V[6].
- Q113709726's child astronomical body is recorded as Q82443659[7].
- Q113709726's child astronomical body is recorded as Q92357172[8].
- Q113709726's child astronomical body is recorded as Q92357280[9].
- Q113709726's child astronomical body is recorded as Q92357164[10].
- Q113709726's catalog code is recorded as KOI-1358[11].
- Q113709726's catalog code is recorded as Kepler-1987[12].
- Q113709726's catalog code is recorded as UCAC4 665-079405[13].
- Q113709726's catalog code is recorded as Gaia DR3 2078000289864478976[14].
- Q113709726's catalog code is recorded as TIC 271958892[15].
- Q113709726's catalog code is recorded as Gaia DR2 2078000289864478976[16].
- Q113709726's catalog code is recorded as 2MASS J19431812+4256362[17].
- Q113709726's catalog code is recorded as KIC 7376983[18].
- Q113709726's type of variable star is recorded as rotating variable star[19].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.49125'}[20].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.842'}[21].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.154'}[22].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.321'}[23].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.545'}[24].
- Q113709726's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.47'}[25].
- Q113709726's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.95'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], near-infrared source[3], and eruptive variable star[4].