Q90683261
star in the constellation Vela
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Q90683261
Summary
Q90683261 is a star[1].
Key Facts
- Q90683261's instance of is recorded as star[2].
- Q90683261's constellation is recorded as Vela[3].
- Q90683261's spectral class is recorded as A2[4].
- Q90683261's catalog code is recorded as CD-50 5050[5].
- Q90683261's catalog code is recorded as CF 7647[6].
- Q90683261's catalog code is recorded as CPD-50 3345[7].
- Q90683261's catalog code is recorded as GSC 08196-00829[8].
- Q90683261's catalog code is recorded as HD 297978[9].
- Q90683261's catalog code is recorded as TYC 8196-829-1[10].
- Q90683261's catalog code is recorded as Gaia DR1 5358380513932410496[11].
- Q90683261's catalog code is recorded as Gaia DR2 5358380518234453632[12].
- Q90683261's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.89'}[13].
- Q90683261's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.27'}[14].
- Q90683261's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.9277'}[15].
- Q90683261's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.7386'}[16].
- Q90683261's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.92'}[17].
- Q90683261's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+575.1754'}[18].
- Q90683261's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+154.87103372038170'}[19].
- Q90683261's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-51.25548959540890'}[20].
- Q90683261's epoch is recorded as J2000.0[21].
- Q90683261's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.269'}[22].
- Q90683261's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.749'}[23].
Body
Definition and Type
Q90683261's instance of is recorded as star[2].