Q91451397
star in the constellation Hercules
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Q91451397
Summary
Q91451397 is a star[1].
Key Facts
- Q91451397's instance of is recorded as star[2].
- Q91451397's constellation is recorded as Hercules[3].
- Q91451397's spectral class is recorded as F2[4].
- Q91451397's catalog code is recorded as BD+14 3696[5].
- Q91451397's catalog code is recorded as GSC 01051-00825[6].
- Q91451397's catalog code is recorded as HD 229941[7].
- Q91451397's catalog code is recorded as 2MASS J18534248+1419220[8].
- Q91451397's catalog code is recorded as Gaia DR2 4507147927489053056[9].
- Q91451397's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0'}[10].
- Q91451397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.686'}[11].
- Q91451397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.515'}[12].
- Q91451397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.430'}[13].
- Q91451397's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.7159'}[14].
- Q91451397's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5129'}[15].
- Q91451397's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.93'}[16].
- Q91451397's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+660.9822'}[17].
- Q91451397's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+283.42702654809340'}[18].
- Q91451397's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+14.32278547506740'}[19].
- Q91451397's epoch is recorded as J2000.0[20].
- Q91451397's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.795'}[21].
- Q91451397's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.425'}[22].
Body
Definition and Type
Q91451397's instance of is recorded as star[2].