Q66492078
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Q66492078
Summary
Q66492078 is a high proper-motion star[1].
Key Facts
- Q66492078's instance of is recorded as high proper-motion star[2].
- Q66492078's spectral class is recorded as F6V[3].
- Q66492078's catalog code is recorded as HD 43382[4].
- Q66492078's catalog code is recorded as GSC 02428-00379[5].
- Q66492078's catalog code is recorded as HIC 29882[6].
- Q66492078's catalog code is recorded as HIP 29882[7].
- Q66492078's catalog code is recorded as 2MASS J06173373+3508570[8].
- Q66492078's catalog code is recorded as PPM 71459[9].
- Q66492078's catalog code is recorded as SAO 58944[10].
- Q66492078's catalog code is recorded as TD1 6555[11].
- Q66492078's catalog code is recorded as uvby98 100043382[12].
- Q66492078's catalog code is recorded as AG+35 627[13].
- Q66492078's catalog code is recorded as BD+35 1375[14].
- Q66492078's catalog code is recorded as TYC 2428-379-1[15].
- Q66492078's catalog code is recorded as Gaia DR2 3452686417838855168[16].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.080'}[17].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.110'}[18].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.700'}[19].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.5537'}[20].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.779'}[21].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.613'}[22].
- Q66492078's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.534'}[23].
- Q66492078's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+21.8480'}[24].
- Q66492078's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.12'}[25].
- Q66492078's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+45.7708'}[26].
Body
Definition and Type
Q66492078's instance of is recorded as high proper-motion star[2].