Q85612492
high proper-motion star in the constellation Aquarius
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Q85612492
Summary
Q85612492 is a high proper-motion star[1].
Key Facts
- Q85612492's instance of is recorded as high proper-motion star[2].
- Q85612492's constellation is recorded as Aquarius[3].
- Q85612492's spectral class is recorded as K5V[4].
- Q85612492's catalog code is recorded as L 789-1[5].
- Q85612492's catalog code is recorded as LHS 6409[6].
- Q85612492's catalog code is recorded as LP 820-73[7].
- Q85612492's catalog code is recorded as NLTT 54647[8].
- Q85612492's catalog code is recorded as TYC 5818-538-1[9].
- Q85612492's catalog code is recorded as G 156-41[10].
- Q85612492's catalog code is recorded as LTT 9162[11].
- Q85612492's catalog code is recorded as TYC 5818-1313-1[12].
- Q85612492's catalog code is recorded as PPM 723173[13].
- Q85612492's catalog code is recorded as UCAC4 378-174159[14].
- Q85612492's catalog code is recorded as StKM 2-1643[15].
- Q85612492's catalog code is recorded as Gaia DR1 2597253413511536896[16].
- Q85612492's catalog code is recorded as Gaia DR2 2597253417806816768[17].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.20'}[18].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.888'}[19].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.572'}[20].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.525'}[21].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.371'}[22].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.877'}[23].
- Q85612492's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.4373'}[24].
- Q85612492's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+21.0319'}[25].
- Q85612492's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.25'}[26].
Body
Definition and Type
Q85612492's instance of is recorded as high proper-motion star[2].