Q87285322
star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q87285322
Summary
Q87285322 is a star[1].
Key Facts
- Q87285322's instance of is recorded as star[2].
- Q87285322's constellation is recorded as Cepheus[3].
- Q87285322's spectral class is recorded as G2[4].
- Q87285322's catalog code is recorded as GSC 03979-01344[5].
- Q87285322's catalog code is recorded as 2MASS J21462913+5957071[6].
- Q87285322's catalog code is recorded as Cl Trumpler 37 1802[7].
- Q87285322's catalog code is recorded as Gaia DR2 2203454807113835648[8].
- Q87285322's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.5'}[9].
- Q87285322's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.343'}[10].
- Q87285322's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.03'}[11].
- Q87285322's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.941'}[12].
- Q87285322's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5045'}[13].
- Q87285322's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1779'}[14].
- Q87285322's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38.56'}[15].
- Q87285322's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+314.6732'}[16].
- Q87285322's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+326.62138181770540'}[17].
- Q87285322's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+59.95192762001690'}[18].
- Q87285322's epoch is recorded as J2000.0[19].
- Q87285322's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.617'}[20].
- Q87285322's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+10.170'}[21].
Body
Definition and Type
Q87285322's instance of is recorded as star[2].