Q76740230
star in the constellation Cygnus
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Q76740230
Summary
Q76740230 is a star[1].
Key Facts
- Q76740230's instance of is recorded as star[2].
- Q76740230's constellation is recorded as Cygnus[3].
- Q76740230's spectral class is recorded as F5V[4].
- Q76740230's catalog code is recorded as Gaia DR2 2085797407855158144[5].
- Q76740230's catalog code is recorded as KIC 10498878[6].
- Q76740230's catalog code is recorded as 2MASS J20040268+4736188[7].
- Q76740230's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2516'}[8].
- Q76740230's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.876'}[9].
- Q76740230's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.575'}[10].
- Q76740230's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.476'}[11].
- Q76740230's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3820'}[12].
- Q76740230's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.3'}[13].
- Q76740230's metallicity is recorded as {'unit': '1', 'amount': '-0.11'}[14].
- Q76740230's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2617.8'}[15].
- Q76740230's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+301.01118365762330'}[16].
- Q76740230's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+47.60522243490778'}[17].
- Q76740230's epoch is recorded as J2000.0[18].
- Q76740230's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6298'}[19].
- Q76740230's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.609'}[20].
- Q76740230's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.215'}[21].
Body
Definition and Type
Q76740230's instance of is recorded as star[2].