Q66640437

Summary

Q66640437 is a high proper-motion star^[1].

Key Facts

• Q66640437's instance of is recorded as high proper-motion star^[2].
• Q66640437's spectral class is recorded as F7V^[3].
• Q66640437's catalog code is recorded as HD 221269^[4].
• Q66640437's catalog code is recorded as CPC 21 5299^[5].
• Q66640437's catalog code is recorded as GSC 09129-01123^[6].
• Q66640437's catalog code is recorded as HIC 116079^[7].
• Q66640437's catalog code is recorded as HIP 116079^[8].
• Q66640437's catalog code is recorded as 2MASS J23311856-6422172^[9].
• Q66640437's catalog code is recorded as PPM 366475^[10].
• Q66640437's catalog code is recorded as SAO 255506^[11].
• Q66640437's catalog code is recorded as uvby98 100221269^[12].
• Q66640437's catalog code is recorded as Gaia DR1 6390320589466239488^[13].
• Q66640437's catalog code is recorded as TYC 9129-1123-1^[14].
• Q66640437's catalog code is recorded as Gaia DR2 6390320593762537984^[15].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.36'}^[16].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.84'}^[17].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.7224'}^[18].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.865'}^[19].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.616'}^[20].
• Q66640437's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.571'}^[21].
• Q66640437's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.0949'}^[22].
• Q66640437's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.02'}^[23].
• Q66640437's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+123.5346'}^[24].
• Q66640437's SIMBAD ID is recorded as HD 221269^[25].
• Q66640437's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+352.82727094709590'}^[26].