Q77888657
high proper-motion star in the constellation Sculptor
Press Enter · cited answer in seconds
0 sources
Q77888657
Summary
Q77888657 is a high proper-motion star[1].
Key Facts
- Q77888657's instance of is recorded as high proper-motion star[2].
- Q77888657's constellation is recorded as Sculptor[3].
- Q77888657's catalog code is recorded as LEHPM 222[4].
- Q77888657's catalog code is recorded as 2MASS J00081796-2832300[5].
- Q77888657's catalog code is recorded as BPM 46040[6].
- Q77888657's catalog code is recorded as CD-29 15[7].
- Q77888657's catalog code is recorded as EGM 5[8].
- Q77888657's catalog code is recorded as G 266-52[9].
- Q77888657's catalog code is recorded as G 267-36[10].
- Q77888657's catalog code is recorded as NLTT 343[11].
- Q77888657's catalog code is recorded as TYC 6418-825-1[12].
- Q77888657's catalog code is recorded as GEN# -0.02900015[13].
- Q77888657's catalog code is recorded as CTLGM 5909[14].
- Q77888657's catalog code is recorded as RAVE J000818.0-283230[15].
- Q77888657's catalog code is recorded as Gaia DR1 2321430991719108864[16].
- Q77888657's catalog code is recorded as Gaia DR2 2321430996015010048[17].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.604'}[18].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.278'}[19].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.214'}[20].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.284'}[21].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.702'}[22].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.923'}[23].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.565'}[24].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.421'}[25].
- Q77888657's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5562'}[26].
Body
Definition and Type
Q77888657's instance of is recorded as high proper-motion star[2].