Q87706427
Algol variable in the constellation Cygnus
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Q87706427
Summary
Q87706427 is an eclipsing binary star[1].
Key Facts
- Q87706427's instance of is recorded as eclipsing binary star[2].
- Q87706427's instance of is recorded as star[3].
- Q87706427's instance of is recorded as near-infrared source[4].
- Q87706427's instance of is recorded as eruptive variable star[5].
- Q87706427's constellation is recorded as Cygnus[6].
- Q87706427's child astronomical body is recorded as Q28504011[7].
- Q87706427's child astronomical body is recorded as Q28504014[8].
- Q87706427's catalog code is recorded as Gaia DR2 2073691303802278784[9].
- Q87706427's catalog code is recorded as 2MASS J19511083+4025037[10].
- Q87706427's catalog code is recorded as KIC 5299459[11].
- Q87706427's catalog code is recorded as KOI-1576[12].
- Q87706427's catalog code is recorded as UCAC4 653-081323[13].
- Q87706427's catalog code is recorded as Gaia DR3 2073691303802278784[14].
- Q87706427's catalog code is recorded as TIC 169930145[15].
- Q87706427's catalog code is recorded as SPOCS 3454[16].
- Q87706427's catalog code is recorded as Kepler-307[17].
- Q87706427's type of variable star is recorded as rotating variable star[18].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.833'}[19].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.452'}[20].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.321'}[21].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.043186'}[22].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.299'}[23].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.092'}[24].
- Q87706427's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.082'}[25].
- Q87706427's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.95'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], near-infrared source[4], and eruptive variable star[5].