Q78414655
star in the constellation Cygnus
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Q78414655
Summary
Q78414655 is a star[1].
Key Facts
- Q78414655's instance of is recorded as star[2].
- Q78414655's constellation is recorded as Cygnus[3].
- Q78414655's spectral class is recorded as K3V[4].
- Q78414655's catalog code is recorded as KIC 8720292[5].
- Q78414655's catalog code is recorded as 2MASS J20055093+4451599[6].
- Q78414655's catalog code is recorded as Gaia DR2 2081927363137896704[7].
- Q78414655's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.995'}[8].
- Q78414655's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.376'}[9].
- Q78414655's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.251'}[10].
- Q78414655's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7121'}[11].
- Q78414655's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.5643'}[12].
- Q78414655's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-58.55'}[13].
- Q78414655's metallicity is recorded as {'unit': '1', 'amount': '-0.08'}[14].
- Q78414655's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+132.1999'}[15].
- Q78414655's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+301.46222060961400'}[16].
- Q78414655's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.86662545235650'}[17].
- Q78414655's epoch is recorded as J2000.0[18].
- Q78414655's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4921'}[19].
- Q78414655's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-20.448'}[20].
- Q78414655's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.101'}[21].
Body
Definition and Type
Q78414655's instance of is recorded as star[2].