Q87016444
star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q87016444
Summary
Q87016444 is a star[1].
Key Facts
- Q87016444's instance of is recorded as star[2].
- Q87016444's constellation is recorded as Cepheus[3].
- Q87016444's spectral class is recorded as F8[4].
- Q87016444's catalog code is recorded as GSC 04262-02098[5].
- Q87016444's catalog code is recorded as 2MASS J21471444+6031422[6].
- Q87016444's catalog code is recorded as Cl Trumpler 37 2051[7].
- Q87016444's catalog code is recorded as Gaia DR2 2203624922179708928[8].
- Q87016444's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.6'}[9].
- Q87016444's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.833'}[10].
- Q87016444's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.54'}[11].
- Q87016444's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.455'}[12].
- Q87016444's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.8076'}[13].
- Q87016444's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1480'}[14].
- Q87016444's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.23'}[15].
- Q87016444's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+317.6620'}[16].
- Q87016444's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+326.81016544808080'}[17].
- Q87016444's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+60.52841010296350'}[18].
- Q87016444's epoch is recorded as J2000.0[19].
- Q87016444's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.567'}[20].
- Q87016444's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+9.010'}[21].
Body
Definition and Type
Q87016444's instance of is recorded as star[2].