Q85833810
rotating variable star in the constellation Lyra
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Q85833810
Summary
Q85833810 is a rotating variable star[1].
Key Facts
- Q85833810's instance of is recorded as rotating variable star[2].
- Q85833810's instance of is recorded as star[3].
- Q85833810's instance of is recorded as near-infrared source[4].
- Q85833810's instance of is recorded as eruptive variable star[5].
- Q85833810's constellation is recorded as Lyra[6].
- Q85833810's spectral class is recorded as G5V[7].
- Q85833810's child astronomical body is recorded as Q92692961[8].
- Q85833810's catalog code is recorded as SPOCS 3072[9].
- Q85833810's catalog code is recorded as Gaia DR2 2051808789021826432[10].
- Q85833810's catalog code is recorded as KOI-103[11].
- Q85833810's catalog code is recorded as KIC 2444412[12].
- Q85833810's catalog code is recorded as 2MASS J19264400+3745057[13].
- Q85833810's catalog code is recorded as Kepler-1710[14].
- Q85833810's catalog code is recorded as UCAC4 639-067491[15].
- Q85833810's catalog code is recorded as Gaia DR3 2051808789021826432[16].
- Q85833810's catalog code is recorded as TIC 137316027[17].
- Q85833810's type of variable star is recorded as rotating variable star[18].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.078'}[19].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.047'}[20].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.551563'}[21].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.344'}[22].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.536'}[23].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.03'}[24].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.729'}[25].
- Q85833810's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.47'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].