Q86581983
high proper-motion star in the constellation Phoenix
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Q86581983
Summary
Q86581983 is a high proper-motion star[1].
Key Facts
- Q86581983's instance of is recorded as high proper-motion star[2].
- Q86581983's constellation is recorded as Phoenix[3].
- Q86581983's spectral class is recorded as G8V[4].
- Q86581983's catalog code is recorded as Gaia DR1 6523572499580457856[5].
- Q86581983's catalog code is recorded as CD-50 14083[6].
- Q86581983's catalog code is recorded as CPC 0 20770[7].
- Q86581983's catalog code is recorded as CPD-50 11884[8].
- Q86581983's catalog code is recorded as GSC 08463-00657[9].
- Q86581983's catalog code is recorded as HD 224287[10].
- Q86581983's catalog code is recorded as HIC 118040[11].
- Q86581983's catalog code is recorded as HIP 118040[12].
- Q86581983's catalog code is recorded as PPM 351514[13].
- Q86581983's catalog code is recorded as SAO 248071[14].
- Q86581983's catalog code is recorded as TYC 8463-657-1[15].
- Q86581983's catalog code is recorded as 2MASS J23563549-5018133[16].
- Q86581983's catalog code is recorded as Gaia DR2 6523572499581919872[17].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.12'}[18].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.30'}[19].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.951'}[20].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.600'}[21].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.498'}[22].
- Q86581983's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1329'}[23].
- Q86581983's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+18.4859'}[24].
- Q86581983's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+44.37'}[25].
- Q86581983's metallicity is recorded as {'unit': '1', 'amount': '-0.32'}[26].
Body
Definition and Type
Q86581983's instance of is recorded as high proper-motion star[2].