Q90085628
high proper-motion star in the constellation Hercules
Press Enter · cited answer in seconds
0 sources
Q90085628
Summary
Q90085628 is a high proper-motion star[1].
Key Facts
- Q90085628's instance of is recorded as high proper-motion star[2].
- Q90085628's constellation is recorded as Hercules[3].
- Q90085628's spectral class is recorded as G0[4].
- Q90085628's catalog code is recorded as AG+33 1564[5].
- Q90085628's catalog code is recorded as BD+33 2960[6].
- Q90085628's catalog code is recorded as GSC 02615-00936[7].
- Q90085628's catalog code is recorded as HD 162197[8].
- Q90085628's catalog code is recorded as HIC 87152[9].
- Q90085628's catalog code is recorded as HIP 87152[10].
- Q90085628's catalog code is recorded as PPM 80600[11].
- Q90085628's catalog code is recorded as SAO 66345[12].
- Q90085628's catalog code is recorded as TYC 2615-936-1[13].
- Q90085628's catalog code is recorded as 2MASS J17482032+3348011[14].
- Q90085628's catalog code is recorded as uvby98 100162197[15].
- Q90085628's catalog code is recorded as Gaia DR1 4607307831848465920[16].
- Q90085628's catalog code is recorded as Gaia DR2 4607307836143102208[17].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.20'}[18].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.937'}[19].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.625'}[20].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.555'}[21].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.81'}[22].
- Q90085628's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.0495'}[23].
- Q90085628's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+17.7919'}[24].
- Q90085628's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+21.17'}[25].
- Q90085628's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+56.2054'}[26].