Q80541206
star in the constellation Cygnus
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Q80541206
Summary
Q80541206 is a star[1].
Key Facts
- Q80541206's instance of is recorded as star[2].
- Q80541206's constellation is recorded as Cygnus[3].
- Q80541206's spectral class is recorded as G9II-III[4].
- Q80541206's catalog code is recorded as Gaia DR2 2073281014168612992[5].
- Q80541206's catalog code is recorded as KIC 4179377[6].
- Q80541206's catalog code is recorded as 2MASS J19452624+3917419[7].
- Q80541206's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3239'}[8].
- Q80541206's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.570'}[9].
- Q80541206's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.050'}[10].
- Q80541206's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.912'}[11].
- Q80541206's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1674'}[12].
- Q80541206's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.72'}[13].
- Q80541206's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[14].
- Q80541206's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+296.35935396875163'}[15].
- Q80541206's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.29498982452750'}[16].
- Q80541206's epoch is recorded as J2000.0[17].
- Q80541206's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4961'}[18].
- Q80541206's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+440'}[19].
- Q80541206's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.969'}[20].
- Q80541206's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.296'}[21].
Body
Definition and Type
Q80541206's instance of is recorded as star[2].