Q92021401

Summary

Q92021401 is a red supergiant^[1].

Key Facts

• Q92021401's instance of is recorded as red supergiant^[2].
• Q92021401's instance of is recorded as double star^[3].
• Q92021401's instance of is recorded as infrared source^[4].
• Q92021401's instance of is recorded as near-infrared source^[5].
• Q92021401's instance of is recorded as variable star^[6].
• Q92021401's constellation is recorded as Perseus^[7].
• Q92021401's spectral class is recorded as M2Iab^[8].
• Q92021401's catalog code is recorded as 2MASS J03064728+5543593^[9].
• Q92021401's catalog code is recorded as CCDM J03068+5544B^[10].
• Q92021401's catalog code is recorded as IRAS 03030+5532^[11].
• Q92021401's catalog code is recorded as IRC +60110^[12].
• Q92021401's catalog code is recorded as RAFGL 434^[13].
• Q92021401's catalog code is recorded as WDS J03068+5545B^[14].
• Q92021401's catalog code is recorded as Gaia DR2 459552193479656320^[15].
• Q92021401's catalog code is recorded as IO Per^[16].
• Q92021401's catalog code is recorded as TIC 251726060^[17].
• Q92021401's catalog code is recorded as Gaia DR3 459552193479656320^[18].
• Q92021401's type of variable star is recorded as slow irregular variables of late spectral types^[19].
• Q92021401's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.42'}^[20].
• Q92021401's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.03'}^[21].
• Q92021401's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.32'}^[22].
• Q92021401's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.342615'}^[23].
• Q92021401's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.183'}^[24].
• Q92021401's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-31.74'}^[25].
• Q92021401's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+46.69694740557999'}^[26].

Body

Definition and Type

Recorded instance of include red supergiant^[2], double star^[3], infrared source^[4], near-infrared source^[5], and variable star^[6].