Q66492448
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Q66492448
Summary
Q66492448 is a high proper-motion star[1].
Key Facts
- Q66492448's instance of is recorded as high proper-motion star[2].
- Q66492448's spectral class is recorded as G0V[3].
- Q66492448's catalog code is recorded as HD 106742[4].
- Q66492448's catalog code is recorded as CPC 20.1 3535[5].
- Q66492448's catalog code is recorded as GSC 08978-05551[6].
- Q66492448's catalog code is recorded as HIC 59865[7].
- Q66492448's catalog code is recorded as HIP 59865[8].
- Q66492448's catalog code is recorded as 2MASS J12163826-6311526[9].
- Q66492448's catalog code is recorded as PPM 359300[10].
- Q66492448's catalog code is recorded as SAO 251825[11].
- Q66492448's catalog code is recorded as UBV 11017[12].
- Q66492448's catalog code is recorded as UBV M 17985[13].
- Q66492448's catalog code is recorded as uvby98 100106742[14].
- Q66492448's catalog code is recorded as Gaia DR1 6054216927290622336[15].
- Q66492448's catalog code is recorded as TYC 8978-5551-1[16].
- Q66492448's catalog code is recorded as Gaia DR2 6054216931644194304[17].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.555'}[18].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.975'}[19].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.8221'}[20].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.916'}[21].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.657'}[22].
- Q66492448's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.610'}[23].
- Q66492448's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.5097'}[24].
- Q66492448's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.93'}[25].
- Q66492448's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+68.9194'}[26].
Body
Definition and Type
Q66492448's instance of is recorded as high proper-motion star[2].