Q80546536
star in the constellation Cygnus
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Q80546536
Summary
Q80546536 is a star[1].
Key Facts
- Q80546536's instance of is recorded as star[2].
- Q80546536's constellation is recorded as Cygnus[3].
- Q80546536's spectral class is recorded as K2V[4].
- Q80546536's catalog code is recorded as Gaia DR2 2052348992830446464[5].
- Q80546536's catalog code is recorded as KIC 3857834[6].
- Q80546536's catalog code is recorded as 2MASS J19334559+3856581[7].
- Q80546536's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4744'}[8].
- Q80546536's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.075'}[9].
- Q80546536's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.598'}[10].
- Q80546536's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.489'}[11].
- Q80546536's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.1601'}[12].
- Q80546536's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-71.19'}[13].
- Q80546536's metallicity is recorded as {'unit': '1', 'amount': '+0.07'}[14].
- Q80546536's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+193.795'}[15].
- Q80546536's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.43997156885460'}[16].
- Q80546536's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.94946503508471'}[17].
- Q80546536's epoch is recorded as J2000.0[18].
- Q80546536's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5083'}[19].
- Q80546536's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-30.834'}[20].
- Q80546536's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.252'}[21].
Body
Definition and Type
Q80546536's instance of is recorded as star[2].