Q66630969

Summary

Q66630969 is an eruptive variable star^[1].

Key Facts

• Q66630969's instance of is recorded as eruptive variable star^[2].
• Q66630969's instance of is recorded as red giant branch star^[3].
• Q66630969's instance of is recorded as infrared source^[4].
• Q66630969's spectral class is recorded as G9III^[5].
• Q66630969's catalog code is recorded as HD 184498^[6].
• Q66630969's catalog code is recorded as GSC 03556-01708^[7].
• Q66630969's catalog code is recorded as HIC 96129^[8].
• Q66630969's catalog code is recorded as HIP 96129^[9].
• Q66630969's catalog code is recorded as KIC 9652494^[10].
• Q66630969's catalog code is recorded as 2MASS J19324423+4618381^[11].
• Q66630969's catalog code is recorded as PPM 58484^[12].
• Q66630969's catalog code is recorded as SAO 48573^[13].
• Q66630969's catalog code is recorded as AG+46 1478^[14].
• Q66630969's catalog code is recorded as BD+46 2716^[15].
• Q66630969's catalog code is recorded as TYC 3556-1708-1^[16].
• Q66630969's catalog code is recorded as Gaia DR1 2128082490450457216^[17].
• Q66630969's catalog code is recorded as Gaia DR2 2128082494753251840^[18].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.6619'}^[19].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.124'}^[20].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.669'}^[21].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.552'}^[22].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.95'}^[23].
• Q66630969's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.95'}^[24].
• Q66630969's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.6056'}^[25].
• Q66630969's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-19.25'}^[26].

Body

Definition and Type

Recorded instance of include eruptive variable star^[2], red giant branch star^[3], and infrared source^[4].