Q89408954
star in the constellation Perseus
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Q89408954
Summary
Q89408954 is a star[1].
Key Facts
- Q89408954's instance of is recorded as star[2].
- Q89408954's constellation is recorded as Perseus[3].
- Q89408954's spectral class is recorded as F3[4].
- Q89408954 is part of Messier 34[5].
- Q89408954's catalog code is recorded as TYC 2853-716-1[6].
- Q89408954's catalog code is recorded as Cl* NGC 1039 BRU 187[7].
- Q89408954's catalog code is recorded as Cl* NGC 1039 W 1526[8].
- Q89408954's catalog code is recorded as GSC 02853-00716[9].
- Q89408954's catalog code is recorded as Gaia DR1 337132186589839872[10].
- Q89408954's catalog code is recorded as Gaia DR2 337132186589839872[11].
- Q89408954's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.46'}[12].
- Q89408954's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.15'}[13].
- Q89408954's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.7577'}[14].
- Q89408954's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.9560'}[15].
- Q89408954's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-0.22'}[16].
- Q89408954's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+511.2474'}[17].
- Q89408954's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+41.12564832544870'}[18].
- Q89408954's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+42.89208764717600'}[19].
- Q89408954's epoch is recorded as J2000.0[20].
- Q89408954's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.686'}[21].
- Q89408954's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.600'}[22].
Body
Definition and Type
Q89408954's instance of is recorded as star[2].
Use and Application
Q89408954 is part of Messier 34[5].