Q92198940
star in the constellation Cygnus
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Q92198940
Summary
Q92198940 is a star[1].
Key Facts
- Q92198940's instance of is recorded as star[2].
- Q92198940's constellation is recorded as Cygnus[3].
- Q92198940's spectral class is recorded as K2III[4].
- Q92198940's catalog code is recorded as Gaia DR2 2078339317402996224[5].
- Q92198940's catalog code is recorded as KIC 8438344[6].
- Q92198940's catalog code is recorded as 2MASS J19383257+4429424[7].
- Q92198940's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.0280'}[8].
- Q92198940's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.243'}[9].
- Q92198940's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.674'}[10].
- Q92198940's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.540'}[11].
- Q92198940's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3149'}[12].
- Q92198940's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-68.18'}[13].
- Q92198940's metallicity is recorded as {'unit': '1', 'amount': '+0.04'}[14].
- Q92198940's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3175.61'}[15].
- Q92198940's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+294.63574392173877'}[16].
- Q92198940's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.49509449164333'}[17].
- Q92198940's epoch is recorded as J2000.0[18].
- Q92198940's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4583'}[19].
- Q92198940's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.036'}[20].
- Q92198940's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.151'}[21].
Body
Definition and Type
Q92198940's instance of is recorded as star[2].