Q81510767
high proper-motion star in the constellation Canes Venatici
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Q81510767
Summary
Q81510767 is a high proper-motion star[1].
Key Facts
- Q81510767's instance of is recorded as high proper-motion star[2].
- Q81510767's constellation is recorded as Canes Venatici[3].
- Q81510767's spectral class is recorded as G5V:[4].
- Q81510767's spectral class is recorded as G5V[5].
- Q81510767's catalog code is recorded as AG+48 1021[6].
- Q81510767's catalog code is recorded as BD+49 2156[7].
- Q81510767's catalog code is recorded as GSC 03456-00079[8].
- Q81510767's catalog code is recorded as HIC 62059[9].
- Q81510767's catalog code is recorded as HIP 62059[10].
- Q81510767's catalog code is recorded as NGP 49 104[11].
- Q81510767's catalog code is recorded as PPM 53148[12].
- Q81510767's catalog code is recorded as SAO 44299[13].
- Q81510767's catalog code is recorded as TYC 3456-79-1[14].
- Q81510767's catalog code is recorded as 2MASS J12431078+4825076[15].
- Q81510767's catalog code is recorded as Gaia DR1 1543486760850380416[16].
- Q81510767's catalog code is recorded as Gaia DR2 1543486760850380416[17].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.316'}[18].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.009'}[19].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.963'}[20].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.50'}[21].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.22'}[22].
- Q81510767's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3740'}[23].
- Q81510767's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.7720'}[24].
- Q81510767's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.10'}[25].
- Q81510767's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+113.9991'}[26].
Body
Definition and Type
Q81510767's instance of is recorded as high proper-motion star[2].