Q66612542

Summary

Q66612542 is an infrared source^[1].

Key Facts

• Q66612542's instance of is recorded as infrared source^[2].
• Q66612542's instance of is recorded as high proper-motion star^[3].
• Q66612542's spectral class is recorded as G8IV^[4].
• Q66612542's catalog code is recorded as HD 11234^[5].
• Q66612542's catalog code is recorded as CPC 21.2 243^[6].
• Q66612542's catalog code is recorded as GSC 09149-00791^[7].
• Q66612542's catalog code is recorded as HIC 8273^[8].
• Q66612542's catalog code is recorded as HIP 8273^[9].
• Q66612542's catalog code is recorded as IRAS 01459-7459^[10].
• Q66612542's catalog code is recorded as 2MASS J01463764-7444196^[11].
• Q66612542's catalog code is recorded as PPM 367401^[12].
• Q66612542's catalog code is recorded as SAO 255815^[13].
• Q66612542's catalog code is recorded as uvby98 100011234^[14].
• Q66612542's catalog code is recorded as TYC 9149-791-1^[15].
• Q66612542's catalog code is recorded as Gaia DR1 4638221838210702720^[16].
• Q66612542's catalog code is recorded as Gaia DR2 4638221842507845632^[17].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.1261'}^[18].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.877'}^[19].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.428'}^[20].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.344'}^[21].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.14'}^[22].
• Q66612542's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.37'}^[23].
• Q66612542's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.8123'}^[24].
• Q66612542's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+25.52'}^[25].
• Q66612542's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+92.4873'}^[26].

Body

Definition and Type

Recorded instance of include infrared source^[2] and high proper-motion star^[3].