Q66491804
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Q66491804
Summary
Q66491804 is a high proper-motion star[1].
Key Facts
- Q66491804's instance of is recorded as high proper-motion star[2].
- Q66491804's spectral class is recorded as F8/G0V[3].
- Q66491804's catalog code is recorded as HD 12951[4].
- Q66491804's catalog code is recorded as CPC 21.3 211[5].
- Q66491804's catalog code is recorded as GSC 09357-00696[6].
- Q66491804's catalog code is recorded as HIC 9414[7].
- Q66491804's catalog code is recorded as HIP 9414[8].
- Q66491804's catalog code is recorded as IRAS 02012-7906[9].
- Q66491804's catalog code is recorded as 2MASS J02005716-7852130[10].
- Q66491804's catalog code is recorded as PPM 367501[11].
- Q66491804's catalog code is recorded as SAO 255839[12].
- Q66491804's catalog code is recorded as TD1 1228[13].
- Q66491804's catalog code is recorded as uvby98 100012951[14].
- Q66491804's catalog code is recorded as TYC 9357-696-1[15].
- Q66491804's catalog code is recorded as Gaia DR1 4633220915730158592[16].
- Q66491804's catalog code is recorded as Gaia DR2 4633220920027104896[17].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.39'}[18].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.84'}[19].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.6952'}[20].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.816'}[21].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.586'}[22].
- Q66491804's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.466'}[23].
- Q66491804's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+21.5035'}[24].
- Q66491804's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+30.62'}[25].
- Q66491804's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+46.5041'}[26].
Body
Definition and Type
Q66491804's instance of is recorded as high proper-motion star[2].