Q88486009
star in the constellation Cygnus
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Q88486009
Summary
Q88486009 is a star[1].
Key Facts
- Q88486009's instance of is recorded as star[2].
- Q88486009's constellation is recorded as Cygnus[3].
- Q88486009's spectral class is recorded as F5V[4].
- Q88486009's catalog code is recorded as GSC 03150-03005[5].
- Q88486009's catalog code is recorded as LF 3b +38 329[6].
- Q88486009's catalog code is recorded as TYC 3150-3005-1[7].
- Q88486009's catalog code is recorded as 2MASS J20083258+3839499[8].
- Q88486009's catalog code is recorded as Gaia DR1 2061853167032757760[9].
- Q88486009's catalog code is recorded as Gaia DR2 2061853171361323392[10].
- Q88486009's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.17'}[11].
- Q88486009's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.860'}[12].
- Q88486009's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.77'}[13].
- Q88486009's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.1566'}[14].
- Q88486009's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3388'}[15].
- Q88486009's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.22'}[16].
- Q88486009's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+746.9376'}[17].
- Q88486009's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+302.13577569867130'}[18].
- Q88486009's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.66384127203490'}[19].
- Q88486009's epoch is recorded as J2000.0[20].
- Q88486009's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.951'}[21].
- Q88486009's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.449'}[22].
Body
Definition and Type
Q88486009's instance of is recorded as star[2].