Q85834096
variable star in the constellation Cygnus
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Q85834096
Summary
Q85834096 is a rotating variable star[1].
Key Facts
- Q85834096's instance of is recorded as rotating variable star[2].
- Q85834096's instance of is recorded as star[3].
- Q85834096's instance of is recorded as near-infrared source[4].
- Q85834096's instance of is recorded as eruptive variable star[5].
- Q85834096's constellation is recorded as Cygnus[6].
- Q85834096's spectral class is recorded as K4[7].
- Q85834096's child astronomical body is recorded as Q19956325[8].
- Q85834096's catalog code is recorded as SPOCS 3117[9].
- Q85834096's catalog code is recorded as Gaia DR2 2076871091425583232[10].
- Q85834096's catalog code is recorded as KOI-305[11].
- Q85834096's catalog code is recorded as KIC 6063220[12].
- Q85834096's catalog code is recorded as 2MASS J19492496+4118001[13].
- Q85834096's catalog code is recorded as Kepler-99[14].
- Q85834096's catalog code is recorded as Kepler-99B[15].
- Q85834096's catalog code is recorded as UCAC4 657-078340[16].
- Q85834096's catalog code is recorded as Gaia DR3 2076871091425583232[17].
- Q85834096's catalog code is recorded as TIC 169462917[18].
- Q85834096's type of variable star is recorded as rotating variable star[19].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.368'}[20].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.852'}[21].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.757'}[22].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.949096'}[23].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.955'}[24].
- Q85834096's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2'}[25].
- Q85834096's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.2409507'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].