Q85514816
high proper-motion star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q85514816
Summary
Q85514816 is a high proper-motion star[1].
Key Facts
- Q85514816's instance of is recorded as high proper-motion star[2].
- Q85514816's constellation is recorded as Scorpius[3].
- Q85514816's spectral class is recorded as M2[4].
- Q85514816's catalog code is recorded as TYC 7371-106-1[5].
- Q85514816's catalog code is recorded as PM J16519-3601[6].
- Q85514816's catalog code is recorded as UCAC4 270-096672[7].
- Q85514816's catalog code is recorded as CCDM J16520-3602A[8].
- Q85514816's catalog code is recorded as HIC 82521[9].
- Q85514816's catalog code is recorded as HIP 82521[10].
- Q85514816's catalog code is recorded as NLTT 43673[11].
- Q85514816's catalog code is recorded as 2MASS J16515793-3601378[12].
- Q85514816's catalog code is recorded as WDS J16520-3602A[13].
- Q85514816's catalog code is recorded as Gaia DR2 5971759327638421120[14].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.652'}[15].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.774'}[16].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.190'}[17].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.964'}[18].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.777'}[19].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.364'}[20].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.386'}[21].
- Q85514816's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.1815'}[22].
- Q85514816's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+18.3465'}[23].
- Q85514816's metallicity is recorded as {'unit': '1', 'amount': '-0.08'}[24].
- Q85514816's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+54.5063'}[25].
- Q85514816's SIMBAD ID is recorded as L 484-9[26].