Q76926603
star in the constellation Ursa Major
Press Enter · cited answer in seconds
0 sources
Q76926603
Summary
Q76926603 is a star[1].
Key Facts
- Q76926603's instance of is recorded as star[2].
- Q76926603's constellation is recorded as Ursa Major[3].
- Q76926603's spectral class is recorded as F8[4].
- Q76926603's catalog code is recorded as BSD 55-422[5].
- Q76926603's catalog code is recorded as GSC 02523-00252[6].
- Q76926603's catalog code is recorded as 2MASS J11284938+3012435[7].
- Q76926603's catalog code is recorded as Gaia DR2 4022670668696237696[8].
- Q76926603's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8'}[9].
- Q76926603's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.386'}[10].
- Q76926603's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.097'}[11].
- Q76926603's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.061'}[12].
- Q76926603's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.2980'}[13].
- Q76926603's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5799'}[14].
- Q76926603's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.77'}[15].
- Q76926603's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+387.6119'}[16].
- Q76926603's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+172.20576119301830'}[17].
- Q76926603's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+30.21218367859010'}[18].
- Q76926603's epoch is recorded as J2000.0[19].
- Q76926603's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-20.856'}[20].
- Q76926603's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+14.911'}[21].
Body
Definition and Type
Q76926603's instance of is recorded as star[2].