Q76742557
star in the constellation Cygnus
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Q76742557
Summary
Q76742557 is a star[1].
Key Facts
- Q76742557's instance of is recorded as star[2].
- Q76742557's constellation is recorded as Cygnus[3].
- Q76742557's spectral class is recorded as F3V[4].
- Q76742557's spectral class is recorded as F5Vawvar[5].
- Q76742557's catalog code is recorded as KIC 11667623[6].
- Q76742557's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-76.4'}[7].
- Q76742557's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-7.0'}[8].
- Q76742557's metallicity is recorded as {'unit': '1', 'amount': '-0.15'}[9].
- Q76742557's metallicity is recorded as {'unit': '1', 'amount': '-0.30'}[10].
- Q76742557's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+354'}[11].
- Q76742557's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+294.7974200'}[12].
- Q76742557's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.7904820'}[13].
- Q76742557's epoch is recorded as J2000.0[14].
- Q76742557's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6579'}[15].
- Q76742557's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6713'}[16].
- Q76742557's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+11200'}[17].
- Q76742557's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+13500'}[18].
- Q76742557's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-26.0'}[19].
- Q76742557's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-22.0'}[20].
Body
Definition and Type
Q76742557's instance of is recorded as star[2].