Q89409008
star in the constellation Perseus
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Q89409008
Summary
Q89409008 is a star[1].
Key Facts
- Q89409008's instance of is recorded as star[2].
- Q89409008's constellation is recorded as Perseus[3].
- Q89409008's spectral class is recorded as G0[4].
- Q89409008 is part of Messier 34[5].
- Q89409008's catalog code is recorded as TYC 2857-996-1[6].
- Q89409008's catalog code is recorded as GSC 02857-00996[7].
- Q89409008's catalog code is recorded as Cl* NGC 1039 W 1410[8].
- Q89409008's catalog code is recorded as Cl* NGC 1039 BRU 128[9].
- Q89409008's catalog code is recorded as Gaia DR1 337203586126216832[10].
- Q89409008's catalog code is recorded as Gaia DR2 337203586126216832[11].
- Q89409008's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.57'}[12].
- Q89409008's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.31'}[13].
- Q89409008's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5832'}[14].
- Q89409008's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6759'}[15].
- Q89409008's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+6.25'}[16].
- Q89409008's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+596.6943'}[17].
- Q89409008's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.62162013854000'}[18].
- Q89409008's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.21432036510800'}[19].
- Q89409008's epoch is recorded as J2000.0[20].
- Q89409008's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.105'}[21].
- Q89409008's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.717'}[22].
Body
Definition and Type
Q89409008's instance of is recorded as star[2].
Use and Application
Q89409008 is part of Messier 34[5].