Q85262839
high proper-motion star in the constellation Serpens
Press Enter · cited answer in seconds
0 sources
Q85262839
Summary
Q85262839 is a high proper-motion star[1].
Key Facts
- Q85262839's instance of is recorded as high proper-motion star[2].
- Q85262839's constellation is recorded as Serpens[3].
- Q85262839's spectral class is recorded as F3/5V[4].
- Q85262839's catalog code is recorded as AG+04 1895[5].
- Q85262839's catalog code is recorded as BD+04 3028[6].
- Q85262839's catalog code is recorded as GSC 00358-00788[7].
- Q85262839's catalog code is recorded as HD 138714[8].
- Q85262839's catalog code is recorded as HIC 76187[9].
- Q85262839's catalog code is recorded as HIP 76187[10].
- Q85262839's catalog code is recorded as PPM 161688[11].
- Q85262839's catalog code is recorded as SAO 121059[12].
- Q85262839's catalog code is recorded as TYC 358-788-1[13].
- Q85262839's catalog code is recorded as YZ 4 5235[14].
- Q85262839's catalog code is recorded as 2MASS J15334105+0413282[15].
- Q85262839's catalog code is recorded as Gaia DR1 4427566577244065024[16].
- Q85262839's catalog code is recorded as Gaia DR2 4427566581540330496[17].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.961'}[18].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.749'}[19].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.696'}[20].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.89'}[21].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.31'}[22].
- Q85262839's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7739'}[23].
- Q85262839's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.2578'}[24].
- Q85262839's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+23.70'}[25].
- Q85262839's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+190.1936'}[26].