Q90590152
star in the constellation Draco
Press Enter · cited answer in seconds
0 sources
Q90590152
Summary
Q90590152 is a star[1].
Key Facts
- Q90590152's instance of is recorded as star[2].
- Q90590152's constellation is recorded as Draco[3].
- Q90590152's spectral class is recorded as F8[4].
- Q90590152's catalog code is recorded as AG+53 1154[5].
- Q90590152's catalog code is recorded as BD+53 2119[6].
- Q90590152's catalog code is recorded as GSC 03918-00879[7].
- Q90590152's catalog code is recorded as HD 234692[8].
- Q90590152's catalog code is recorded as PPM 36772[9].
- Q90590152's catalog code is recorded as SAO 31108[10].
- Q90590152's catalog code is recorded as TYC 3918-879-1[11].
- Q90590152's catalog code is recorded as YZ 53 5698[12].
- Q90590152's catalog code is recorded as 2MASS J18412715+5350125[13].
- Q90590152's catalog code is recorded as Gaia DR1 2147159910545643520[14].
- Q90590152's catalog code is recorded as Gaia DR2 2147159914842615296[15].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.60'}[16].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.746'}[17].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.547'}[18].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.506'}[19].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.03'}[20].
- Q90590152's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4812'}[21].
- Q90590152's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.2059'}[22].
- Q90590152's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-24.83'}[23].
- Q90590152's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+237.7612'}[24].
- Q90590152's SIMBAD ID is recorded as HD 234692[25].
- Q90590152's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+280.36311025031690'}[26].