Q90676177
star in the constellation Gemini
Press Enter · cited answer in seconds
0 sources
Q90676177
Summary
Q90676177 is a star[1].
Key Facts
- Q90676177's instance of is recorded as star[2].
- Q90676177's constellation is recorded as Gemini[3].
- Q90676177's spectral class is recorded as F5[4].
- Q90676177's catalog code is recorded as AG+27 817[5].
- Q90676177's catalog code is recorded as BD+27 1405[6].
- Q90676177's catalog code is recorded as GSC 01919-02016[7].
- Q90676177's catalog code is recorded as HD 59668[8].
- Q90676177's catalog code is recorded as PPM 97631[9].
- Q90676177's catalog code is recorded as SAO 79478[10].
- Q90676177's catalog code is recorded as TYC 1919-2016-1[11].
- Q90676177's catalog code is recorded as YZ 27 4018[12].
- Q90676177's catalog code is recorded as 2MASS J07320637+2706524[13].
- Q90676177's catalog code is recorded as Gaia DR1 872370117663561344[14].
- Q90676177's catalog code is recorded as Gaia DR2 872370121960936064[15].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.64'}[16].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.98'}[17].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.969'}[18].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.812'}[19].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.781'}[20].
- Q90676177's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5810'}[21].
- Q90676177's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.4868'}[22].
- Q90676177's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.25'}[23].
- Q90676177's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+133.5684'}[24].
- Q90676177's SIMBAD ID is recorded as HD 59668[25].
- Q90676177's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+113.02651599910190'}[26].