Q93399600
star in the constellation Cygnus
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Q93399600
Summary
Q93399600 is a star[1].
Key Facts
- Q93399600's instance of is recorded as star[2].
- Q93399600's constellation is recorded as Cygnus[3].
- Q93399600's spectral class is recorded as K4III[4].
- Q93399600's catalog code is recorded as Gaia DR2 2129504124628100480[5].
- Q93399600's catalog code is recorded as KIC 10917950[6].
- Q93399600's catalog code is recorded as 2MASS J19225902+4821143[7].
- Q93399600's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3655'}[8].
- Q93399600's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.632'}[9].
- Q93399600's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.071'}[10].
- Q93399600's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.922'}[11].
- Q93399600's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4955'}[12].
- Q93399600's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-63.34'}[13].
- Q93399600's metallicity is recorded as {'unit': '1', 'amount': '-0.12'}[14].
- Q93399600's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2018.16'}[15].
- Q93399600's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+290.74595386402797'}[16].
- Q93399600's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.35396924772389'}[17].
- Q93399600's epoch is recorded as J2000.0[18].
- Q93399600's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4463'}[19].
- Q93399600's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.287'}[20].
- Q93399600's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.606'}[21].
Body
Definition and Type
Q93399600's instance of is recorded as star[2].