Q86166537

Summary

Q86166537 is a long-period variable star^[1].

Key Facts

• Q86166537's instance of is recorded as long-period variable star^[2].
• Q86166537's instance of is recorded as infrared source^[3].
• Q86166537's instance of is recorded as near-infrared source^[4].
• Q86166537's constellation is recorded as Eridanus^[5].
• Q86166537's spectral class is recorded as M5/6^[6].
• Q86166537's catalog code is recorded as 2MASS J04565186-0632084^[7].
• Q86166537's catalog code is recorded as GSC 04749-00626^[8].
• Q86166537's catalog code is recorded as IRAS 04544-0636^[9].
• Q86166537's catalog code is recorded as NSV 1781^[10].
• Q86166537's catalog code is recorded as UCAC2 29397307^[11].
• Q86166537's catalog code is recorded as Gaia DR2 3187378827605051648^[12].
• Q86166537's catalog code is recorded as KR Eri^[13].
• Q86166537's catalog code is recorded as TYC 4749-626-1^[14].
• Q86166537's catalog code is recorded as TIC 138798148^[15].
• Q86166537's catalog code is recorded as Gaia DR3 3187378827605051648^[16].
• Q86166537's type of variable star is recorded as SRb semi-regular variable star^[17].
• Q86166537's type of variable star is recorded as long-period variable star^[18].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.341'}^[19].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.497'}^[20].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.81'}^[21].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.13'}^[22].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.014'}^[23].
• Q86166537's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.101122'}^[24].
• Q86166537's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.708'}^[25].
• Q86166537's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1412.429'}^[26].

Body

Definition and Type

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