Q66492189
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Q66492189
Summary
Q66492189 is a high proper-motion star[1].
Key Facts
- Q66492189's instance of is recorded as high proper-motion star[2].
- Q66492189's spectral class is recorded as G0V[3].
- Q66492189's catalog code is recorded as HD 68346[4].
- Q66492189's catalog code is recorded as CPC 0 5460[5].
- Q66492189's catalog code is recorded as GSC 08148-00002[6].
- Q66492189's catalog code is recorded as HIC 39947[7].
- Q66492189's catalog code is recorded as HIP 39947[8].
- Q66492189's catalog code is recorded as IRAS 08081-5141[9].
- Q66492189's catalog code is recorded as 2MASS J08093009-5150338[10].
- Q66492189's catalog code is recorded as PPM 336691[11].
- Q66492189's catalog code is recorded as SAO 235781[12].
- Q66492189's catalog code is recorded as UBV M 14060[13].
- Q66492189's catalog code is recorded as uvby98 100068346[14].
- Q66492189's catalog code is recorded as TYC 8148-2-1[15].
- Q66492189's catalog code is recorded as Gaia DR1 5513068365298444544[16].
- Q66492189's catalog code is recorded as Gaia DR2 5513068369598665984[17].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.123'}[18].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.526'}[19].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.3772'}[20].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.451'}[21].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.225'}[22].
- Q66492189's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.094'}[23].
- Q66492189's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+17.3493'}[24].
- Q66492189's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.38'}[25].
- Q66492189's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+57.6392'}[26].
Body
Definition and Type
Q66492189's instance of is recorded as high proper-motion star[2].