Q88441024

Summary

Q88441024 is a double star^[1].

Key Facts

• Q88441024's instance of is recorded as double star^[2].
• Q88441024's constellation is recorded as Grus^[3].
• Q88441024's spectral class is recorded as G5^[4].
• Q88441024 comprises Q83771297^[5].
• Q88441024 comprises Q85370300^[6].
• Q88441024's catalog code is recorded as Gaia DR2 6511282506499054592^[7].
• Q88441024's catalog code is recorded as WISE J222114.01-510805.8^[8].
• Q88441024's catalog code is recorded as UCAC4 195-197242^[9].
• Q88441024's catalog code is recorded as WDS J22212-5108AB^[10].
• Q88441024's catalog code is recorded as CD-51 13245^[11].
• Q88441024's catalog code is recorded as CF 19878^[12].
• Q88441024's catalog code is recorded as CPD-51 11804^[13].
• Q88441024's catalog code is recorded as GSC 08445-01014^[14].
• Q88441024's catalog code is recorded as 2MASS J22211387-5108054^[15].
• Q88441024's catalog code is recorded as RAVE J222113.9-510805^[16].
• Q88441024's catalog code is recorded as Gaia DR1 6511282502202977024^[17].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.7910'}^[18].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.34'}^[19].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.48'}^[20].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.92'}^[21].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.61'}^[22].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.23'}^[23].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.15'}^[24].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.638'}^[25].
• Q88441024's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.309'}^[26].

Body

Definition and Type

Q88441024's instance of is recorded as double star^[2].

Use and Application

Components include Q83771297^[5], a high proper-motion star^[27] and Q85370300^[6], a high proper-motion star^[28].