Q66611704
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Q66611704
Summary
Q66611704 is a high proper-motion star[1].
Key Facts
- Q66611704's instance of is recorded as high proper-motion star[2].
- Q66611704's spectral class is recorded as F2III/IV[3].
- Q66611704's catalog code is recorded as HD 115693[4].
- Q66611704's catalog code is recorded as GSC 05550-01031[5].
- Q66611704's catalog code is recorded as HIC 64971[6].
- Q66611704's catalog code is recorded as HIP 64971[7].
- Q66611704's catalog code is recorded as 2MASS J13185865-1238530[8].
- Q66611704's catalog code is recorded as PPM 227105[9].
- Q66611704's catalog code is recorded as SAO 157849[10].
- Q66611704's catalog code is recorded as TD1 16763[11].
- Q66611704's catalog code is recorded as uvby98 100115693[12].
- Q66611704's catalog code is recorded as YZ V11 4753[13].
- Q66611704's catalog code is recorded as BD-11 3487[14].
- Q66611704's catalog code is recorded as TYC 5550-1031-1[15].
- Q66611704's catalog code is recorded as Gaia DR1 3609552672325635456[16].
- Q66611704's catalog code is recorded as Gaia DR2 3609552676621081088[17].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.72'}[18].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.34'}[19].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.2436'}[20].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.585'}[21].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.447'}[22].
- Q66611704's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.366'}[23].
- Q66611704's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.3695'}[24].
- Q66611704's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-22.20'}[25].
- Q66611704's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+106.7293'}[26].
Body
Definition and Type
Q66611704's instance of is recorded as high proper-motion star[2].