Q93284980

Summary

Q93284980 is a Mira variable^[1].

Key Facts

• Q93284980's instance of is recorded as Mira variable^[2].
• Q93284980's instance of is recorded as infrared source^[3].
• Q93284980's instance of is recorded as long-period variable star^[4].
• Q93284980's instance of is recorded as near-infrared source^[5].
• Q93284980's constellation is recorded as Cepheus^[6].
• Q93284980's spectral class is recorded as M3^[7].
• Q93284980's catalog code is recorded as IRAS 20379+5921^[8].
• Q93284980's catalog code is recorded as IRC +60296^[9].
• Q93284980's catalog code is recorded as RAFGL 5530^[10].
• Q93284980's catalog code is recorded as RAFGL 5530S^[11].
• Q93284980's catalog code is recorded as 2MASS J20390533+5932207^[12].
• Q93284980's catalog code is recorded as Gaia DR2 2193763574181648512^[13].
• Q93284980's catalog code is recorded as UU Cep^[14].
• Q93284980's catalog code is recorded as TIC 276986802^[15].
• Q93284980's catalog code is recorded as Gaia DR3 2193763574181648512^[16].
• Q93284980's type of variable star is recorded as SRa semi-regular variable star^[17].
• Q93284980's type of variable star is recorded as long-period variable star^[18].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.85'}^[19].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.85'}^[20].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.25'}^[21].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.15'}^[22].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.18'}^[23].
• Q93284980's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.920792'}^[24].
• Q93284980's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6575'}^[25].
• Q93284980's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1520.913'}^[26].

Body

Definition and Type

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