Q86844187
rotating variable star in the constellation Cygnus
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Q86844187
Summary
Q86844187 is a rotating variable star[1].
Key Facts
- Q86844187's instance of is recorded as rotating variable star[2].
- Q86844187's instance of is recorded as star[3].
- Q86844187's instance of is recorded as near-infrared source[4].
- Q86844187's constellation is recorded as Cygnus[5].
- Q86844187's spectral class is recorded as G9[6].
- Q86844187's child astronomical body is recorded as Q86029040[7].
- Q86844187's child astronomical body is recorded as Q28503087[8].
- Q86844187's child astronomical body is recorded as Q28503084[9].
- Q86844187's catalog code is recorded as Gaia DR2 2126648731589350272[10].
- Q86844187's catalog code is recorded as KIC 9020160[11].
- Q86844187's catalog code is recorded as 2MASS J19244401+4519234[12].
- Q86844187's catalog code is recorded as Kepler-191[13].
- Q86844187's catalog code is recorded as KOI-582[14].
- Q86844187's catalog code is recorded as Gaia DR3 2126648731589350272[15].
- Q86844187's catalog code is recorded as TIC 159647213[16].
- Q86844187's catalog code is recorded as SPOCS 3889[17].
- Q86844187's type of variable star is recorded as rotating variable star[18].
- Q86844187's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.96'}[19].
- Q86844187's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.88'}[20].
- Q86844187's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.420'}[21].
- Q86844187's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.767342'}[22].
- Q86844187's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.36190927'}[23].
- Q86844187's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.85'}[24].
- Q86844187's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.7691126'}[25].
- Q86844187's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6695'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], and near-infrared source[4].