Q90770158

Summary

Q90770158 is a Mira variable^[1].

Key Facts

• Q90770158's instance of is recorded as Mira variable^[2].
• Q90770158's instance of is recorded as infrared source^[3].
• Q90770158's instance of is recorded as long-period variable star^[4].
• Q90770158's instance of is recorded as near-infrared source^[5].
• Q90770158's constellation is recorded as Hydrus^[6].
• Q90770158's spectral class is recorded as M3e^[7].
• Q90770158's catalog code is recorded as GCRV 51423^[8].
• Q90770158's catalog code is recorded as IRAS 01093-7706^[9].
• Q90770158's catalog code is recorded as ASAS J011028-7650.9^[10].
• Q90770158's catalog code is recorded as 2MASS J01102811-7650557^[11].
• Q90770158's catalog code is recorded as Gaia DR2 4636091882325830272^[12].
• Q90770158's catalog code is recorded as RS Hyi^[13].
• Q90770158's catalog code is recorded as TYC 9347-1318-1^[14].
• Q90770158's catalog code is recorded as TIC 402103933^[15].
• Q90770158's catalog code is recorded as Gaia DR3 4636091882325830272^[16].
• Q90770158's type of variable star is recorded as long-period variable star^[17].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.50'}^[18].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.101'}^[19].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.380'}^[20].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.855'}^[21].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.88'}^[22].
• Q90770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.042273'}^[23].
• Q90770158's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1828'}^[24].
• Q90770158's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.0'}^[25].
• Q90770158's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+17.61698141649'}^[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].