Q88603979
high proper-motion star in the constellation Eridanus
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Q88603979
Summary
Q88603979 is a high proper-motion star[1].
Key Facts
- Q88603979's instance of is recorded as high proper-motion star[2].
- Q88603979's constellation is recorded as Eridanus[3].
- Q88603979's spectral class is recorded as K4Vk:[4].
- Q88603979's spectral class is recorded as K4V (k)[5].
- Q88603979's catalog code is recorded as 2MASS J04201424-0902134[6].
- Q88603979's catalog code is recorded as BD-09 872[7].
- Q88603979's catalog code is recorded as GEN# -0.00900872[8].
- Q88603979's catalog code is recorded as GSC 05313-02344[9].
- Q88603979's catalog code is recorded as HERZ 589[10].
- Q88603979's catalog code is recorded as HIC 20240[11].
- Q88603979's catalog code is recorded as HIP 20240[12].
- Q88603979's catalog code is recorded as PPM 186808[13].
- Q88603979's catalog code is recorded as TYC 5313-2344-1[14].
- Q88603979's catalog code is recorded as UGP 80[15].
- Q88603979's catalog code is recorded as Gaia DR1 3192532754001087616[16].
- Q88603979's catalog code is recorded as Gaia DR2 3192532758297814656[17].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.81'}[18].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0'}[19].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.815'}[20].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.273'}[21].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.126'}[22].
- Q88603979's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4183'}[23].
- Q88603979's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+29.3920'}[24].
- Q88603979's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-7.131'}[25].
- Q88603979's metallicity is recorded as {'unit': '1', 'amount': '-0.22'}[26].
Body
Definition and Type
Q88603979's instance of is recorded as high proper-motion star[2].