Q88736748
eclipsing binary star
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Q88736748
Summary
Q88736748 is an eclipsing binary star[1].
Key Facts
- Q88736748's instance of is recorded as eclipsing binary star[2].
- Q88736748's constellation is recorded as Cygnus[3].
- Q88736748's spectral class is recorded as K2[4].
- Q88736748's catalog code is recorded as BD+45 3047[5].
- Q88736748's catalog code is recorded as GSC 03559-00102[6].
- Q88736748's catalog code is recorded as HD 190585[7].
- Q88736748's catalog code is recorded as TYC 3559-102-1[8].
- Q88736748's catalog code is recorded as 2MASS J20034832+4536148[9].
- Q88736748's catalog code is recorded as KIC 9246715[10].
- Q88736748's catalog code is recorded as Gaia DR1 2082288140396700672[11].
- Q88736748's catalog code is recorded as KOI-7601[12].
- Q88736748's catalog code is recorded as Gaia DR2 2082288144698194944[13].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.679'}[14].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.208'}[15].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.085'}[16].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.65'}[17].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.74'}[18].
- Q88736748's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2779'}[19].
- Q88736748's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6238'}[20].
- Q88736748's metallicity is recorded as {'unit': '1', 'amount': '+0.05'}[21].
- Q88736748's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+615.8394'}[22].
- Q88736748's SIMBAD ID is recorded as HD 190585[23].
- Q88736748's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+300.95133790686180'}[24].
- Q88736748's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.60411208879640'}[25].
- Q88736748's epoch is recorded as J2000.0[26].