Q91069153
star in the constellation Draco
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Q91069153
Summary
Q91069153 is a star[1].
Key Facts
- Q91069153's instance of is recorded as star[2].
- Q91069153's constellation is recorded as Draco[3].
- Q91069153's spectral class is recorded as F5[4].
- Q91069153's catalog code is recorded as AG+82 539[5].
- Q91069153's catalog code is recorded as BD+82 559[6].
- Q91069153's catalog code is recorded as GSC 04582-01076[7].
- Q91069153's catalog code is recorded as PPM 3267[8].
- Q91069153's catalog code is recorded as SAO 3092[9].
- Q91069153's catalog code is recorded as TYC 4582-1076-1[10].
- Q91069153's catalog code is recorded as Gaia DR1 2296401227988082176[11].
- Q91069153's catalog code is recorded as Gaia DR2 2296401232284566784[12].
- Q91069153's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.91'}[13].
- Q91069153's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.36'}[14].
- Q91069153's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7810'}[15].
- Q91069153's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.4975'}[16].
- Q91069153's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+13.32'}[17].
- Q91069153's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+133.3778'}[18].
- Q91069153's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+279.27741351312020'}[19].
- Q91069153's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+82.31229282990070'}[20].
- Q91069153's epoch is recorded as J2000.0[21].
- Q91069153's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+14.220'}[22].
- Q91069153's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+35.577'}[23].
Body
Definition and Type
Q91069153's instance of is recorded as star[2].