Q66639492
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Q66639492
Summary
Q66639492 is an infrared source[1].
Key Facts
- Q66639492's instance of is recorded as infrared source[2].
- Q66639492's instance of is recorded as high proper-motion star[3].
- Q66639492's spectral class is recorded as G3/5V[4].
- Q66639492's catalog code is recorded as HD 146817[5].
- Q66639492's catalog code is recorded as CPC 0 14602[6].
- Q66639492's catalog code is recorded as GSC 07856-00827[7].
- Q66639492's catalog code is recorded as HIC 80013[8].
- Q66639492's catalog code is recorded as HIP 80013[9].
- Q66639492's catalog code is recorded as 2MASS J16195959-4049053[10].
- Q66639492's catalog code is recorded as PPM 321600[11].
- Q66639492's catalog code is recorded as SAO 226665[12].
- Q66639492's catalog code is recorded as uvby98 100146817[13].
- Q66639492's catalog code is recorded as Gaia DR1 5993794880692365312[14].
- Q66639492's catalog code is recorded as TYC 7856-827-1[15].
- Q66639492's catalog code is recorded as Gaia DR2 5993794885009577600[16].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.39'}[17].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.71'}[18].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.5470'}[19].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.482'}[20].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.198'}[21].
- Q66639492's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.134'}[22].
- Q66639492's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+20.4547'}[23].
- Q66639492's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+31.25'}[24].
- Q66639492's metallicity is recorded as {'unit': '1', 'amount': '-0.09'}[25].
- Q66639492's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+48.8885'}[26].
Body
Definition and Type
Recorded instance of include infrared source[2] and high proper-motion star[3].