Q82138630
Algol variable in the constellation Cygnus
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Q82138630
Summary
Q82138630 is an eclipsing binary star[1].
Key Facts
- Q82138630's instance of is recorded as eclipsing binary star[2].
- Q82138630's instance of is recorded as star[3].
- Q82138630's instance of is recorded as near-infrared source[4].
- Q82138630's instance of is recorded as eruptive variable star[5].
- Q82138630's constellation is recorded as Cygnus[6].
- Q82138630's spectral class is recorded as F8V[7].
- Q82138630's child astronomical body is recorded as Q85476644[8].
- Q82138630's catalog code is recorded as Gaia DR2 2073715630497465856[9].
- Q82138630's catalog code is recorded as KIC 5031857[10].
- Q82138630's catalog code is recorded as 2MASS J19472307+4008190[11].
- Q82138630's catalog code is recorded as KOI-1573[12].
- Q82138630's catalog code is recorded as Kepler-1755[13].
- Q82138630's catalog code is recorded as UCAC4 651-078297[14].
- Q82138630's catalog code is recorded as Gaia DR3 2073715630497465856[15].
- Q82138630's catalog code is recorded as TIC 239225129[16].
- Q82138630's type of variable star is recorded as rotating variable star[17].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.231'}[18].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.931'}[19].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.91'}[20].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.374312'}[21].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.354'}[22].
- Q82138630's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.544'}[23].
- Q82138630's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.3742259'}[24].
- Q82138630's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.2'}[25].
- Q82138630's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.176'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], near-infrared source[4], and eruptive variable star[5].