Q66647918
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Q66647918
Summary
Q66647918 is a high proper-motion star[1].
Key Facts
- Q66647918's instance of is recorded as high proper-motion star[2].
- Q66647918's spectral class is recorded as K0III+F/G[3].
- Q66647918's catalog code is recorded as HD 213066[4].
- Q66647918's catalog code is recorded as GSC 05811-00350[5].
- Q66647918's catalog code is recorded as HIC 110979[6].
- Q66647918's catalog code is recorded as HIP 110979[7].
- Q66647918's catalog code is recorded as 2MASS J22290491-0944282[8].
- Q66647918's catalog code is recorded as PPM 206410[9].
- Q66647918's catalog code is recorded as SAO 146111[10].
- Q66647918's catalog code is recorded as SRS 17445[11].
- Q66647918's catalog code is recorded as uvby98 100213066[12].
- Q66647918's catalog code is recorded as YZ 99 7937[13].
- Q66647918's catalog code is recorded as BD-10 5925[14].
- Q66647918's catalog code is recorded as TYC 5811-350-1[15].
- Q66647918's catalog code is recorded as Gaia DR1 2615081513519419392[16].
- Q66647918's catalog code is recorded as Gaia DR2 2615081517814569984[17].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.34'}[18].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.70'}[19].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.5486'}[20].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.598'}[21].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.333'}[22].
- Q66647918's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.250'}[23].
- Q66647918's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+12.7871'}[24].
- Q66647918's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38.93'}[25].
- Q66647918's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+78.2038'}[26].
Body
Definition and Type
Q66647918's instance of is recorded as high proper-motion star[2].