Q76745813
star in the constellation Cygnus
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Q76745813
Summary
Q76745813 is a star[1].
Key Facts
- Q76745813's instance of is recorded as star[2].
- Q76745813's constellation is recorded as Cygnus[3].
- Q76745813's spectral class is recorded as G5V:[4].
- Q76745813's catalog code is recorded as Gaia DR2 2079448381039027200[5].
- Q76745813's catalog code is recorded as KIC 9362728[6].
- Q76745813's catalog code is recorded as 2MASS J19544763+4552399[7].
- Q76745813's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7516'}[8].
- Q76745813's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.844'}[9].
- Q76745813's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.281'}[10].
- Q76745813's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.145'}[11].
- Q76745813's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4224'}[12].
- Q76745813's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-119.97'}[13].
- Q76745813's metallicity is recorded as {'unit': '1', 'amount': '-0.48'}[14].
- Q76745813's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2367.42'}[15].
- Q76745813's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.69846382759334'}[16].
- Q76745813's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.87776865636250'}[17].
- Q76745813's epoch is recorded as J2000.0[18].
- Q76745813's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4941'}[19].
- Q76745813's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+5.548'}[20].
- Q76745813's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+7.173'}[21].
Body
Definition and Type
Q76745813's instance of is recorded as star[2].