Q97052869
eclipsing binary star
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Q97052869
Summary
Q97052869 is an eclipsing binary star[1].
Key Facts
- Q97052869's instance of is recorded as eclipsing binary star[2].
- Q97052869's constellation is recorded as Lyra[3].
- Q97052869's catalog code is recorded as MDV 805[4].
- Q97052869's catalog code is recorded as 2MASS J18263306+3332413[5].
- Q97052869's catalog code is recorded as UCAC4 618-062757[6].
- Q97052869's catalog code is recorded as Gaia DR2 4592496207629668224[7].
- Q97052869's type of variable star is recorded as Algol variable[8].
- Q97052869's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.248'}[9].
- Q97052869's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.345'}[10].
- Q97052869's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.656'}[11].
- Q97052869's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.83'}[12].
- Q97052869's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8060'}[13].
- Q97052869's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0790'}[14].
- Q97052869's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+55.86'}[15].
- Q97052869's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+926.784'}[16].
- Q97052869's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+276.63773323358123'}[17].
- Q97052869's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+33.54483483271250'}[18].
- Q97052869's epoch is recorded as J2000.0[19].
- Q97052869's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-10.088'}[20].
- Q97052869's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.021'}[21].
Body
Definition and Type
Q97052869's instance of is recorded as eclipsing binary star[2].