Q88626190
high proper-motion star in the constellation Andromeda
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Q88626190
Summary
Q88626190 is a high proper-motion star[1].
Key Facts
- Q88626190's instance of is recorded as high proper-motion star[2].
- Q88626190's constellation is recorded as Andromeda[3].
- Q88626190's spectral class is recorded as F5[4].
- Q88626190's catalog code is recorded as 2MASS J00392221+2543501[5].
- Q88626190's catalog code is recorded as AG+25 70[6].
- Q88626190's catalog code is recorded as BD+24 91[7].
- Q88626190's catalog code is recorded as GPM 9.842375+25.730691[8].
- Q88626190's catalog code is recorded as GSC 01741-01540[9].
- Q88626190's catalog code is recorded as HD 3640[10].
- Q88626190's catalog code is recorded as PPM 90014[11].
- Q88626190's catalog code is recorded as SAO 74172[12].
- Q88626190's catalog code is recorded as TYC 1741-1540-1[13].
- Q88626190's catalog code is recorded as YZ 0 682[14].
- Q88626190's catalog code is recorded as YZ 25 191[15].
- Q88626190's catalog code is recorded as Gaia DR1 2806861424012747008[16].
- Q88626190's catalog code is recorded as Gaia DR2 2806861428308038144[17].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.11'}[18].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.59'}[19].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.261'}[20].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.068'}[21].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.009'}[22].
- Q88626190's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0472'}[23].
- Q88626190's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.1885'}[24].
- Q88626190's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+1.03'}[25].
- Q88626190's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+161.5900'}[26].
Body
Definition and Type
Q88626190's instance of is recorded as high proper-motion star[2].