Q87556669
high proper-motion star in the constellation Scorpius
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Q87556669
Summary
Q87556669 is a high proper-motion star[1].
Key Facts
- Q87556669's instance of is recorded as high proper-motion star[2].
- Q87556669's constellation is recorded as Scorpius[3].
- Q87556669's spectral class is recorded as G0V[4].
- Q87556669's catalog code is recorded as Gaia DR1 5992780821733093248[5].
- Q87556669's catalog code is recorded as CD-41 10675[6].
- Q87556669's catalog code is recorded as CPC 0 14814[7].
- Q87556669's catalog code is recorded as CPD-41 7489[8].
- Q87556669's catalog code is recorded as GSC 07861-00937[9].
- Q87556669's catalog code is recorded as HD 148371[10].
- Q87556669's catalog code is recorded as HIC 80759[11].
- Q87556669's catalog code is recorded as HIP 80759[12].
- Q87556669's catalog code is recorded as PPM 321784[13].
- Q87556669's catalog code is recorded as SAO 226811[14].
- Q87556669's catalog code is recorded as TYC 7861-937-1[15].
- Q87556669's catalog code is recorded as 2MASS J16292061-4202002[16].
- Q87556669's catalog code is recorded as Gaia DR2 5992780826052542080[17].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.275'}[18].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.042'}[19].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.961'}[20].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.27'}[21].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.81'}[22].
- Q87556669's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1428'}[23].
- Q87556669's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.6055'}[24].
- Q87556669's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-37.16'}[25].
- Q87556669's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[26].
Body
Definition and Type
Q87556669's instance of is recorded as high proper-motion star[2].