Q88539478
high proper-motion star in the constellation Sculptor
Press Enter · cited answer in seconds
0 sources
Q88539478
Summary
Q88539478 is a high proper-motion star[1].
Key Facts
- Q88539478's instance of is recorded as high proper-motion star[2].
- Q88539478's constellation is recorded as Sculptor[3].
- Q88539478's spectral class is recorded as F5V[4].
- Q88539478's catalog code is recorded as CD-35 15919[5].
- Q88539478's catalog code is recorded as CPC 18 12022[6].
- Q88539478's catalog code is recorded as CPD-35 9441[7].
- Q88539478's catalog code is recorded as GSC 07518-00383[8].
- Q88539478's catalog code is recorded as HD 222954[9].
- Q88539478's catalog code is recorded as HIC 117180[10].
- Q88539478's catalog code is recorded as HIP 117180[11].
- Q88539478's catalog code is recorded as PPM 304146[12].
- Q88539478's catalog code is recorded as SAO 214755[13].
- Q88539478's catalog code is recorded as SRS 18263[14].
- Q88539478's catalog code is recorded as TYC 7518-383-1[15].
- Q88539478's catalog code is recorded as 2MASS J23452609-3458524[16].
- Q88539478's catalog code is recorded as Gaia DR1 2311942034573380352[17].
- Q88539478's catalog code is recorded as Gaia DR2 2311942038868428672[18].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.444'}[19].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.206'}[20].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.153'}[21].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.26'}[22].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.72'}[23].
- Q88539478's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1890'}[24].
- Q88539478's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.0277'}[25].
- Q88539478's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.36'}[26].
Body
Definition and Type
Q88539478's instance of is recorded as high proper-motion star[2].