Q80535296
star in the constellation Cygnus
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Q80535296
Summary
Q80535296 is a star[1].
Key Facts
- Q80535296's instance of is recorded as star[2].
- Q80535296's constellation is recorded as Cygnus[3].
- Q80535296's spectral class is recorded as K0V[4].
- Q80535296's catalog code is recorded as Gaia DR2 2049077048080736000[5].
- Q80535296's catalog code is recorded as KIC 2593780[6].
- Q80535296's catalog code is recorded as 2MASS J19404653+3750214[7].
- Q80535296's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.4877'}[8].
- Q80535296's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.131'}[9].
- Q80535296's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.710'}[10].
- Q80535296's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.612'}[11].
- Q80535296's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2266'}[12].
- Q80535296's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+7.2'}[13].
- Q80535296's metallicity is recorded as {'unit': '1', 'amount': '+0.01'}[14].
- Q80535296's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+449.115'}[15].
- Q80535296's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.19390992559880'}[16].
- Q80535296's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.83927040641084'}[17].
- Q80535296's epoch is recorded as J2000.0[18].
- Q80535296's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5225'}[19].
- Q80535296's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.172'}[20].
- Q80535296's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.428'}[21].
Body
Definition and Type
Q80535296's instance of is recorded as star[2].