Q85833812
rotating variable star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q85833812
Summary
Q85833812 is a rotating variable star[1].
Key Facts
- Q85833812's instance of is recorded as rotating variable star[2].
- Q85833812's instance of is recorded as star[3].
- Q85833812's instance of is recorded as near-infrared source[4].
- Q85833812's instance of is recorded as eruptive variable star[5].
- Q85833812's constellation is recorded as Lyra[6].
- Q85833812's spectral class is recorded as G5[7].
- Q85833812's child astronomical body is recorded as Q28855648[8].
- Q85833812's catalog code is recorded as Gaia DR2 2106821925598401152[9].
- Q85833812's catalog code is recorded as KOI-323[10].
- Q85833812's catalog code is recorded as KIC 9139084[11].
- Q85833812's catalog code is recorded as 2MASS J18561467+4530246[12].
- Q85833812's catalog code is recorded as Kepler-523[13].
- Q85833812's catalog code is recorded as UCAC4 678-067448[14].
- Q85833812's catalog code is recorded as Gaia DR3 2106821925598401152[15].
- Q85833812's catalog code is recorded as TIC 164654277[16].
- Q85833812's catalog code is recorded as SPOCS 3913[17].
- Q85833812's type of variable star is recorded as rotating variable star[18].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.283'}[19].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.908'}[20].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.827'}[21].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.473321'}[22].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.315'}[23].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4'}[24].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.898'}[25].
- Q85833812's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.629'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].