Q76738492
star in the constellation Cygnus
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Q76738492
Summary
Q76738492 is a star[1].
Key Facts
- Q76738492's instance of is recorded as star[2].
- Q76738492's constellation is recorded as Cygnus[3].
- Q76738492's spectral class is recorded as F2IV[4].
- Q76738492's catalog code is recorded as Gaia DR2 2082815429242179328[5].
- Q76738492's catalog code is recorded as KIC 10177111[6].
- Q76738492's catalog code is recorded as 2MASS J20105101+4711138[7].
- Q76738492's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.0443'}[8].
- Q76738492's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.138'}[9].
- Q76738492's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.930'}[10].
- Q76738492's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.829'}[11].
- Q76738492's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7165'}[12].
- Q76738492's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-34.2'}[13].
- Q76738492's metallicity is recorded as {'unit': '1', 'amount': '+0.06'}[14].
- Q76738492's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1395.67'}[15].
- Q76738492's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+302.71256672428717'}[16].
- Q76738492's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+47.18719571614277'}[17].
- Q76738492's epoch is recorded as J2000.0[18].
- Q76738492's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6846'}[19].
- Q76738492's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.831'}[20].
- Q76738492's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.226'}[21].
Body
Definition and Type
Q76738492's instance of is recorded as star[2].