Q78311930
high proper-motion star in the constellation Canes Venatici
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Q78311930
Summary
Q78311930 is a high proper-motion star[1].
Key Facts
- Q78311930's instance of is recorded as high proper-motion star[2].
- Q78311930's constellation is recorded as Canes Venatici[3].
- Q78311930's spectral class is recorded as G0[4].
- Q78311930's catalog code is recorded as AG+52 896[5].
- Q78311930's catalog code is recorded as BD+52 1632[6].
- Q78311930's catalog code is recorded as GSC 03458-01609[7].
- Q78311930's catalog code is recorded as HD 233950[8].
- Q78311930's catalog code is recorded as HIC 61002[9].
- Q78311930's catalog code is recorded as HIP 61002[10].
- Q78311930's catalog code is recorded as PPM 33588[11].
- Q78311930's catalog code is recorded as SAO 28409[12].
- Q78311930's catalog code is recorded as TYC 3458-1609-1[13].
- Q78311930's catalog code is recorded as YZ 52 4090[14].
- Q78311930's catalog code is recorded as 2MASS J12300998+5201521[15].
- Q78311930's catalog code is recorded as Gaia DR1 1568885754330084608[16].
- Q78311930's catalog code is recorded as Gaia DR2 1568885758626753664[17].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.854'}[18].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.637'}[19].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.553'}[20].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.80'}[21].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.33'}[22].
- Q78311930's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7036'}[23].
- Q78311930's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.3554'}[24].
- Q78311930's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-13.07'}[25].
- Q78311930's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+186.7274'}[26].
Body
Definition and Type
Q78311930's instance of is recorded as high proper-motion star[2].