Q85834125
rotating variable star in the constellation Cygnus
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Q85834125
Summary
Q85834125 is a rotating variable star[1].
Key Facts
- Q85834125's instance of is recorded as rotating variable star[2].
- Q85834125's instance of is recorded as high proper-motion star[3].
- Q85834125's instance of is recorded as near-infrared source[4].
- Q85834125's instance of is recorded as eruptive variable star[5].
- Q85834125's constellation is recorded as Cygnus[6].
- Q85834125's spectral class is recorded as K2V[7].
- Q85834125's child astronomical body is recorded as Q92692784[8].
- Q85834125's catalog code is recorded as Gaia DR2 2078735519547912832[9].
- Q85834125's catalog code is recorded as KOI-315[10].
- Q85834125's catalog code is recorded as KIC 7700622[11].
- Q85834125's catalog code is recorded as 2MASS J19490525+4319599[12].
- Q85834125's catalog code is recorded as Kepler-1716[13].
- Q85834125's catalog code is recorded as UCAC4 667-079334[14].
- Q85834125's catalog code is recorded as Gaia DR3 2078735519547912832[15].
- Q85834125's catalog code is recorded as TIC 273035189[16].
- Q85834125's catalog code is recorded as SPOCS 3714[17].
- Q85834125's type of variable star is recorded as rotating variable star[18].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.429'}[19].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.897'}[20].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.813'}[21].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.931363'}[22].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.579'}[23].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.833'}[24].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.615'}[25].
- Q85834125's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.242'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], high proper-motion star[3], near-infrared source[4], and eruptive variable star[5].