Q78310620
high proper-motion star in the constellation Canes Venatici
Press Enter · cited answer in seconds
0 sources
Q78310620
Summary
Q78310620 is a high proper-motion star[1].
Key Facts
- Q78310620's instance of is recorded as high proper-motion star[2].
- Q78310620's constellation is recorded as Canes Venatici[3].
- Q78310620's spectral class is recorded as G5[4].
- Q78310620's catalog code is recorded as AG+50 961[5].
- Q78310620's catalog code is recorded as AGKR 11362[6].
- Q78310620's catalog code is recorded as BD+51 1777[7].
- Q78310620's catalog code is recorded as GSC 03458-01939[8].
- Q78310620's catalog code is recorded as HD 110391[9].
- Q78310620's catalog code is recorded as HIC 61913[10].
- Q78310620's catalog code is recorded as HIP 61913[11].
- Q78310620's catalog code is recorded as PPM 33680[12].
- Q78310620's catalog code is recorded as SAO 28477[13].
- Q78310620's catalog code is recorded as TYC 3458-1939-1[14].
- Q78310620's catalog code is recorded as YZ 50 4121[15].
- Q78310620's catalog code is recorded as 2MASS J12412064+5024574[16].
- Q78310620's catalog code is recorded as Gaia DR1 1567767310486725248[17].
- Q78310620's catalog code is recorded as Gaia DR2 1567767314783448576[18].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.371'}[19].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.129'}[20].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.139'}[21].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.33'}[22].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.84'}[23].
- Q78310620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2196'}[24].
- Q78310620's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.2373'}[25].
- Q78310620's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+7.93'}[26].
Body
Definition and Type
Q78310620's instance of is recorded as high proper-motion star[2].