Q87741076

Summary

Q87741076 is a red supergiant^[1].

Key Facts

• Q87741076's instance of is recorded as red supergiant^[2].
• Q87741076's instance of is recorded as infrared source^[3].
• Q87741076's instance of is recorded as long-period variable star^[4].
• Q87741076's instance of is recorded as near-infrared source^[5].
• Q87741076's constellation is recorded as Tucana^[6].
• Q87741076's spectral class is recorded as M5e^[7].
• Q87741076's catalog code is recorded as ASAS J005300-6953.2^[8].
• Q87741076's catalog code is recorded as 2MASS J00525975-6953102^[9].
• Q87741076's catalog code is recorded as GCRV 50812^[10].
• Q87741076's catalog code is recorded as IRAS 00511-7009^[11].
• Q87741076's catalog code is recorded as Gaia DR2 4691925392020685696^[12].
• Q87741076's catalog code is recorded as TZ Tuc^[13].
• Q87741076's catalog code is recorded as TYC 9135-1647-1^[14].
• Q87741076's catalog code is recorded as AAVSO 0049-70^[15].
• Q87741076's catalog code is recorded as TIC 39071244^[16].
• Q87741076's catalog code is recorded as Gaia DR3 4691925392020685696^[17].
• Q87741076's type of variable star is recorded as long-period variable star^[18].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.10'}^[19].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.07'}^[20].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.397'}^[21].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.65'}^[22].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.154'}^[23].
• Q87741076's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.268827'}^[24].
• Q87741076's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.426'}^[25].
• Q87741076's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+197.0'}^[26].

Body

Definition and Type

Recorded instance of include red supergiant^[2], infrared source^[3], long-period variable star^[4], and near-infrared source^[5].