Q85465216
high proper-motion star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q85465216
Summary
Q85465216 is a high proper-motion star[1].
Key Facts
- Q85465216's instance of is recorded as high proper-motion star[2].
- Q85465216's constellation is recorded as Cepheus[3].
- Q85465216's spectral class is recorded as G0[4].
- Q85465216's catalog code is recorded as AG+75 933[5].
- Q85465216's catalog code is recorded as BD+74 952[6].
- Q85465216's catalog code is recorded as GSC 04600-02096[7].
- Q85465216's catalog code is recorded as HD 210476[8].
- Q85465216's catalog code is recorded as PPM 11074[9].
- Q85465216's catalog code is recorded as SAO 10250[10].
- Q85465216's catalog code is recorded as TYC 4600-2096-1[11].
- Q85465216's catalog code is recorded as uvby98 100210476[12].
- Q85465216's catalog code is recorded as 2MASS J22064289+7527200[13].
- Q85465216's catalog code is recorded as Gaia DR1 2280154088262218240[14].
- Q85465216's catalog code is recorded as GEN# +1.00210476[15].
- Q85465216's catalog code is recorded as Gaia DR2 2280154092559184128[16].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.36'}[17].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.385'}[18].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.139'}[19].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.096'}[20].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.89'}[21].
- Q85465216's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.2293'}[22].
- Q85465216's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.5630'}[23].
- Q85465216's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-0.98'}[24].
- Q85465216's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+73.7300'}[25].
- Q85465216's SIMBAD ID is recorded as HD 210476[26].