Q85023421
W Ursae Majoris variable star in the constellation Cetus
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Q85023421
Summary
Q85023421 is a RR Lyrae variable[1].
Key Facts
- Q85023421's instance of is recorded as RR Lyrae variable[2].
- Q85023421's instance of is recorded as eclipsing binary star[3].
- Q85023421's instance of is recorded as near-infrared source[4].
- Q85023421's instance of is recorded as blue object[5].
- Q85023421's constellation is recorded as Cetus[6].
- Q85023421's spectral class is recorded as F0[7].
- Q85023421's catalog code is recorded as 2MASS J02204424-1423228[8].
- Q85023421's catalog code is recorded as RAVE J022044.3-142323[9].
- Q85023421's catalog code is recorded as Gaia DR1 5146911614355920512[10].
- Q85023421's catalog code is recorded as Gaia DR2 5146911614355920512[11].
- Q85023421's catalog code is recorded as TY Cet[12].
- Q85023421's catalog code is recorded as ASAS J022044-1423.4[13].
- Q85023421's catalog code is recorded as TYC 5284-1862-1[14].
- Q85023421's catalog code is recorded as TIC 302515557[15].
- Q85023421's catalog code is recorded as Gaia DR3 5146911614355920512[16].
- Q85023421's type of variable star is recorded as W Ursae Majoris variable[17].
- Q85023421's type of variable star is recorded as RR Lyrae variables with nearly symmetric light curves[18].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.44'}[19].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.87'}[20].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.000'}[21].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.858'}[22].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.785'}[23].
- Q85023421's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.615091'}[24].
- Q85023421's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6385'}[25].
- Q85023421's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-89.22'}[26].