Q93212630
star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q93212630
Summary
Q93212630 is a star[1].
Key Facts
- Q93212630's instance of is recorded as star[2].
- Q93212630's constellation is recorded as Cepheus[3].
- Q93212630's spectral class is recorded as F8[4].
- Q93212630's catalog code is recorded as GSC 03978-01079[5].
- Q93212630's catalog code is recorded as 2MASS J21292978+5831322[6].
- Q93212630's catalog code is recorded as Cl Trumpler 37 969[7].
- Q93212630's catalog code is recorded as Gaia DR2 2179481223074692224[8].
- Q93212630's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.0'}[9].
- Q93212630's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.902'}[10].
- Q93212630's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.643'}[11].
- Q93212630's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.565'}[12].
- Q93212630's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.0033'}[13].
- Q93212630's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2239'}[14].
- Q93212630's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-64.93'}[15].
- Q93212630's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+449.6605'}[16].
- Q93212630's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+322.37408453114860'}[17].
- Q93212630's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+58.52560553317650'}[18].
- Q93212630's epoch is recorded as J2000.0[19].
- Q93212630's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-15.525'}[20].
- Q93212630's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.942'}[21].
Body
Definition and Type
Q93212630's instance of is recorded as star[2].