Q94388504
high proper-motion star in the constellation Perseus
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Q94388504
Summary
Q94388504 is a high proper-motion star[1].
Key Facts
- Q94388504's instance of is recorded as high proper-motion star[2].
- Q94388504's constellation is recorded as Perseus[3].
- Q94388504's spectral class is recorded as G4V[4].
- Q94388504's catalog code is recorded as TYC 3315-962-1[5].
- Q94388504's catalog code is recorded as Koenig 18[6].
- Q94388504's catalog code is recorded as Cl Melotte 20 286[7].
- Q94388504's catalog code is recorded as FBFTA Per II 19[8].
- Q94388504's catalog code is recorded as Gaia DR1 435254700197035008[9].
- Q94388504's catalog code is recorded as Gaia DR2 435254704496153600[10].
- Q94388504's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.85'}[11].
- Q94388504's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.70'}[12].
- Q94388504's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.6969'}[13].
- Q94388504's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.8697'}[14].
- Q94388504's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+27.68'}[15].
- Q94388504's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+112.7434'}[16].
- Q94388504's SIMBAD ID is recorded as Koenig 18[17].
- Q94388504's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.02967022871520'}[18].
- Q94388504's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+47.41610845533640'}[19].
- Q94388504's epoch is recorded as J2000.0[20].
- Q94388504's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-74.477'}[21].
- Q94388504's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+53.774'}[22].
- Q94388504's Gaia ID is recorded as 435254704496153600[23].