Q90316285

Summary

Q90316285 is a long-period variable star^[1].

Key Facts

• Q90316285's instance of is recorded as long-period variable star^[2].
• Q90316285's constellation is recorded as Serpens^[3].
• Q90316285's spectral class is recorded as M2^[4].
• Q90316285's catalog code is recorded as AG+18 1384^[5].
• Q90316285's catalog code is recorded as BD+18 2989^[6].
• Q90316285's catalog code is recorded as GSC 01489-00919^[7].
• Q90316285's catalog code is recorded as HIC 74642^[8].
• Q90316285's catalog code is recorded as HIP 74642^[9].
• Q90316285's catalog code is recorded as IRAS 15127+1813^[10].
• Q90316285's catalog code is recorded as PPM 131255^[11].
• Q90316285's catalog code is recorded as TYC 1489-919-1^[12].
• Q90316285's catalog code is recorded as 2MASS J15150303+1802524^[13].
• Q90316285's catalog code is recorded as Gaia DR1 1211649856620225280^[14].
• Q90316285's catalog code is recorded as Gaia DR2 1211649860916344960^[15].
• Q90316285's catalog code is recorded as OS Ser^[16].
• Q90316285's type of variable star is recorded as SRb semi-regular variable star^[17].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.69'}^[18].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.965'}^[19].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.36'}^[20].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.967'}^[21].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.674'}^[22].
• Q90316285's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.8514'}^[23].
• Q90316285's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3465'}^[24].
• Q90316285's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+742.6662'}^[25].
• Q90316285's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+228.76272769867140'}^[26].

Body

Definition and Type

Q90316285's instance of is recorded as long-period variable star^[2].