Q66611402

Summary

Q66611402 is a high proper-motion star^[1].

Key Facts

• Q66611402's instance of is recorded as high proper-motion star^[2].
• Q66611402's spectral class is recorded as F3V^[3].
• Q66611402's catalog code is recorded as HD 91248^[4].
• Q66611402's catalog code is recorded as GSC 05494-01663^[5].
• Q66611402's catalog code is recorded as HIC 51575^[6].
• Q66611402's catalog code is recorded as HIP 51575^[7].
• Q66611402's catalog code is recorded as 2MASS J10320142-1125277^[8].
• Q66611402's catalog code is recorded as PPM 223086^[9].
• Q66611402's catalog code is recorded as SAO 156040^[10].
• Q66611402's catalog code is recorded as TD1 14920^[11].
• Q66611402's catalog code is recorded as uvby98 100091248^[12].
• Q66611402's catalog code is recorded as BD-10 3076^[13].
• Q66611402's catalog code is recorded as FAUST 2663^[14].
• Q66611402's catalog code is recorded as TYC 5494-1663-1^[15].
• Q66611402's catalog code is recorded as YZC 11 3989^[16].
• Q66611402's catalog code is recorded as Gaia DR2 3755488209275682944^[17].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.82'}^[18].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.41'}^[19].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.3204'}^[20].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.642'}^[21].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.491'}^[22].
• Q66611402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.437'}^[23].
• Q66611402's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.8932'}^[24].
• Q66611402's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.05'}^[25].
• Q66611402's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+71.9777'}^[26].

Body

Definition and Type

Q66611402's instance of is recorded as high proper-motion star^[2].