Q93212955
star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q93212955
Summary
Q93212955 is a star[1].
Key Facts
- Q93212955's instance of is recorded as star[2].
- Q93212955's constellation is recorded as Cepheus[3].
- Q93212955's spectral class is recorded as F2[4].
- Q93212955's catalog code is recorded as GSC 03974-01318[5].
- Q93212955's catalog code is recorded as 2MASS J21284082+5650143[6].
- Q93212955's catalog code is recorded as Cl Trumpler 37 130[7].
- Q93212955's catalog code is recorded as Gaia DR2 2178760909826616704[8].
- Q93212955's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.5'}[9].
- Q93212955's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.672'}[10].
- Q93212955's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.461'}[11].
- Q93212955's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.374'}[12].
- Q93212955's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6780'}[13].
- Q93212955's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.8743'}[14].
- Q93212955's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-25.04'}[15].
- Q93212955's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+347.9108'}[16].
- Q93212955's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+322.17004555460430'}[17].
- Q93212955's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+56.83731602225500'}[18].
- Q93212955's epoch is recorded as J2000.0[19].
- Q93212955's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.553'}[20].
- Q93212955's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+6.735'}[21].
Body
Definition and Type
Q93212955's instance of is recorded as star[2].