Q85239329
star in the constellation Lacerta
Press Enter · cited answer in seconds
0 sources
Q85239329
Summary
Q85239329 is a star[1].
Key Facts
- Q85239329's instance of is recorded as star[2].
- Q85239329's constellation is recorded as Lacerta[3].
- Q85239329's spectral class is recorded as G5:[4].
- Q85239329's catalog code is recorded as GSC 03987-00386[5].
- Q85239329's catalog code is recorded as LF 4 +54 1089[6].
- Q85239329's catalog code is recorded as 2MASS J22364332+5514398[7].
- Q85239329's catalog code is recorded as Gaia DR2 2006496712253312640[8].
- Q85239329's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.6'}[9].
- Q85239329's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.968'}[10].
- Q85239329's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.72'}[11].
- Q85239329's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.635'}[12].
- Q85239329's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.0247'}[13].
- Q85239329's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.9899'}[14].
- Q85239329's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.22'}[15].
- Q85239329's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+334.4593'}[16].
- Q85239329's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+339.18051324262960'}[17].
- Q85239329's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.24443749750250'}[18].
- Q85239329's epoch is recorded as J2000.0[19].
- Q85239329's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.079'}[20].
- Q85239329's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+11.864'}[21].
Body
Definition and Type
Q85239329's instance of is recorded as star[2].