Q93718548
star in the constellation Cygnus
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Q93718548
Summary
Q93718548 is a star[1].
Key Facts
- Q93718548's instance of is recorded as star[2].
- Q93718548's constellation is recorded as Cygnus[3].
- Q93718548's spectral class is recorded as G4V[4].
- Q93718548's catalog code is recorded as Gaia DR2 2130082884357681152[5].
- Q93718548's catalog code is recorded as KIC 11812936[6].
- Q93718548's catalog code is recorded as 2MASS J19251183+5004277[7].
- Q93718548's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6180'}[8].
- Q93718548's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.537'}[9].
- Q93718548's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.235'}[10].
- Q93718548's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.192'}[11].
- Q93718548's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6464'}[12].
- Q93718548's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.7'}[13].
- Q93718548's metallicity is recorded as {'unit': '1', 'amount': '+0.14'}[14].
- Q93718548's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+607.386'}[15].
- Q93718548's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.29932199013166'}[16].
- Q93718548's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.07435512904583'}[17].
- Q93718548's epoch is recorded as J2000.0[18].
- Q93718548's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5743'}[19].
- Q93718548's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.660'}[20].
- Q93718548's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+10.076'}[21].
Body
Definition and Type
Q93718548's instance of is recorded as star[2].