Q90478221

Summary

Q90478221 is a long-period variable star^[1].

Key Facts

• Q90478221's instance of is recorded as long-period variable star^[2].
• Q90478221's constellation is recorded as Taurus^[3].
• Q90478221's spectral class is recorded as M:^[4].
• Q90478221 is part of Pleiades^[5].
• Q90478221's catalog code is recorded as Cl* Melotte 22 MT 97^[6].
• Q90478221's catalog code is recorded as [KSP2003] G165.8790-22.1098^[7].
• Q90478221's catalog code is recorded as SV* HV 6191^[8].
• Q90478221's catalog code is recorded as NSV 1343^[9].
• Q90478221's catalog code is recorded as [KSP2003] J034906.26+253523.3^[10].
• Q90478221's catalog code is recorded as TYC 1804-662-1^[11].
• Q90478221's catalog code is recorded as GSC 01804-00662^[12].
• Q90478221's catalog code is recorded as UCAC2 40807695^[13].
• Q90478221's catalog code is recorded as 2MASS J03490631+2535230^[14].
• Q90478221's catalog code is recorded as HAT 260-00303^[15].
• Q90478221's catalog code is recorded as Gaia DR1 69958110944431232^[16].
• Q90478221's catalog code is recorded as Gaia DR2 69958115241943808^[17].
• Q90478221's catalog code is recorded as V1244 Tau^[18].
• Q90478221's type of variable star is recorded as SRb semi-regular variable star^[19].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.27'}^[20].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.68'}^[21].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.093'}^[22].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.23'}^[23].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.944'}^[24].
• Q90478221's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8723'}^[25].
• Q90478221's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3202'}^[26].

Body

Definition and Type

Q90478221's instance of is recorded as long-period variable star^[2].

Use and Application

Q90478221 is part of Pleiades^[5].