Q89122729
W Ursae Majoris variable star in the constellation Serpens
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Q89122729
Summary
Q89122729 is an eclipsing binary star[1].
Key Facts
- Q89122729's instance of is recorded as eclipsing binary star[2].
- Q89122729's instance of is recorded as near-infrared source[3].
- Q89122729's instance of is recorded as astrophysical X-ray source[4].
- Q89122729's constellation is recorded as Serpens[5].
- Q89122729's spectral class is recorded as G4V[6].
- Q89122729's catalog code is recorded as GSC 01502-01762[7].
- Q89122729's catalog code is recorded as 1RXS J155650.6+221602[8].
- Q89122729's catalog code is recorded as SBC9 2991[9].
- Q89122729's catalog code is recorded as UCAC2 39680325[10].
- Q89122729's catalog code is recorded as UCAC3 225-122835[11].
- Q89122729's catalog code is recorded as 2MASS J15564947+2216016[12].
- Q89122729's catalog code is recorded as Gaia DR1 1218233800966950016[13].
- Q89122729's catalog code is recorded as Gaia DR2 1218233805261820288[14].
- Q89122729's catalog code is recorded as AU Ser[15].
- Q89122729's catalog code is recorded as TYC 1502-1762-1[16].
- Q89122729's catalog code is recorded as ASAS J155649+2216.0[17].
- Q89122729's catalog code is recorded as TIC 229555752[18].
- Q89122729's catalog code is recorded as Gaia DR3 1218233805261820288[19].
- Q89122729's type of variable star is recorded as W Ursae Majoris variable[20].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.04'}[21].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.76'}[22].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.311'}[23].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.945'}[24].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.802'}[25].
- Q89122729's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.913328'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], near-infrared source[3], and astrophysical X-ray source[4].