Q81119107
star in the constellation Draco
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Q81119107
Summary
Q81119107 is a star[1].
Key Facts
- Q81119107's instance of is recorded as star[2].
- Q81119107's constellation is recorded as Draco[3].
- Q81119107's spectral class is recorded as F8[4].
- Q81119107's catalog code is recorded as AG+83 529[5].
- Q81119107's catalog code is recorded as BD+83 590[6].
- Q81119107's catalog code is recorded as GSC 04649-02227[7].
- Q81119107's catalog code is recorded as PPM 3606[8].
- Q81119107's catalog code is recorded as SAO 3425[9].
- Q81119107's catalog code is recorded as TYC 4649-2227-1[10].
- Q81119107's catalog code is recorded as Gaia DR1 2301967849201423232[11].
- Q81119107's catalog code is recorded as Gaia DR2 2301967853498150912[12].
- Q81119107's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.96'}[13].
- Q81119107's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.56'}[14].
- Q81119107's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8509'}[15].
- Q81119107's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.5611'}[16].
- Q81119107's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-73.97'}[17].
- Q81119107's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+219.2454'}[18].
- Q81119107's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+307.81107321674160'}[19].
- Q81119107's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.62826588317030'}[20].
- Q81119107's epoch is recorded as J2000.0[21].
- Q81119107's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+8.496'}[22].
- Q81119107's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+31.807'}[23].
Body
Definition and Type
Q81119107's instance of is recorded as star[2].