Q66612017
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Q66612017
Summary
Q66612017 is a high proper-motion star[1].
Key Facts
- Q66612017's instance of is recorded as high proper-motion star[2].
- Q66612017's spectral class is recorded as F7/8V[3].
- Q66612017's catalog code is recorded as HD 188007[4].
- Q66612017's catalog code is recorded as GSC 05155-01736[5].
- Q66612017's catalog code is recorded as HIC 97866[6].
- Q66612017's catalog code is recorded as HIP 97866[7].
- Q66612017's catalog code is recorded as 2MASS J19531373-0532249[8].
- Q66612017's catalog code is recorded as PPM 203400[9].
- Q66612017's catalog code is recorded as SAO 143880[10].
- Q66612017's catalog code is recorded as uvby98 100188007[11].
- Q66612017's catalog code is recorded as YZ 0 4066[12].
- Q66612017's catalog code is recorded as YZ 95 6961[13].
- Q66612017's catalog code is recorded as BD-05 5096[14].
- Q66612017's catalog code is recorded as TYC 5155-1736-1[15].
- Q66612017's catalog code is recorded as Gaia DR1 4197231673047273856[16].
- Q66612017's catalog code is recorded as Gaia DR2 4197231677351639296[17].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.94'}[18].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.41'}[19].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.2881'}[20].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.415'}[21].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.174'}[22].
- Q66612017's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.134'}[23].
- Q66612017's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.0779'}[24].
- Q66612017's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.90'}[25].
- Q66612017's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+71.0333'}[26].
Body
Definition and Type
Q66612017's instance of is recorded as high proper-motion star[2].