Q84913012
high proper-motion star in the constellation Boötes
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Q84913012
Summary
Q84913012 is a high proper-motion star[1].
Key Facts
- Q84913012's instance of is recorded as high proper-motion star[2].
- Q84913012's constellation is recorded as Boötes[3].
- Q84913012's spectral class is recorded as F8[4].
- Q84913012's catalog code is recorded as AG+11 1531[5].
- Q84913012's catalog code is recorded as AGKR 12375[6].
- Q84913012's catalog code is recorded as BD+12 2631[7].
- Q84913012's catalog code is recorded as GSC 00903-01007[8].
- Q84913012's catalog code is recorded as HD 120703[9].
- Q84913012's catalog code is recorded as HIC 67587[10].
- Q84913012's catalog code is recorded as HIP 67587[11].
- Q84913012's catalog code is recorded as PPM 130120[12].
- Q84913012's catalog code is recorded as SAO 100737[13].
- Q84913012's catalog code is recorded as TYC 903-1007-1[14].
- Q84913012's catalog code is recorded as YZ 11 4949[15].
- Q84913012's catalog code is recorded as 2MASS J13505584+1134481[16].
- Q84913012's catalog code is recorded as Gaia DR2 3727253025552144000[17].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.413'}[18].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.238'}[19].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.144'}[20].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.30'}[21].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.78'}[22].
- Q84913012's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.1920'}[23].
- Q84913012's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.8264'}[24].
- Q84913012's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.32'}[25].
- Q84913012's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.51'}[26].
Body
Definition and Type
Q84913012's instance of is recorded as high proper-motion star[2].