Q88846702
high proper-motion star in the constellation Delphinus
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Q88846702
Summary
Q88846702 is a high proper-motion star[1].
Key Facts
- Q88846702's instance of is recorded as high proper-motion star[2].
- Q88846702's constellation is recorded as Delphinus[3].
- Q88846702's spectral class is recorded as K7.0Ve[4].
- Q88846702's catalog code is recorded as BPM 96336[5].
- Q88846702's catalog code is recorded as TYC 1112-763-1[6].
- Q88846702's catalog code is recorded as GSC 01112-00763[7].
- Q88846702's catalog code is recorded as UCAC2 36385350[8].
- Q88846702's catalog code is recorded as UCAC3 206-292906[9].
- Q88846702's catalog code is recorded as 2MASS J21085175+1247381[10].
- Q88846702's catalog code is recorded as StKM 2-1499[11].
- Q88846702's catalog code is recorded as BD+12 4554[12].
- Q88846702's catalog code is recorded as UCAC4 514-132811[13].
- Q88846702's catalog code is recorded as PM J21088+1247[14].
- Q88846702's catalog code is recorded as Gaia DR1 1758940256201241984[15].
- Q88846702's catalog code is recorded as Gaia DR2 1758940260497926272[16].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.44'}[17].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.505'}[18].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.876'}[19].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.736'}[20].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.930'}[21].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.523'}[22].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.594'}[23].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.359'}[24].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.906'}[25].
- Q88846702's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.4390'}[26].
Body
Definition and Type
Q88846702's instance of is recorded as high proper-motion star[2].