Q91182587
high proper-motion star in the constellation Grus
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Q91182587
Summary
Q91182587 is a high proper-motion star[1].
Key Facts
- Q91182587's instance of is recorded as high proper-motion star[2].
- Q91182587's constellation is recorded as Grus[3].
- Q91182587's spectral class is recorded as F3V[4].
- Q91182587's catalog code is recorded as CD-40 14725[5].
- Q91182587's catalog code is recorded as CPC 18 11438[6].
- Q91182587's catalog code is recorded as CPD-40 9674[7].
- Q91182587's catalog code is recorded as GSC 07996-00700[8].
- Q91182587's catalog code is recorded as HD 211562[9].
- Q91182587's catalog code is recorded as PPM 302434[10].
- Q91182587's catalog code is recorded as SAO 213720[11].
- Q91182587's catalog code is recorded as TYC 7996-700-1[12].
- Q91182587's catalog code is recorded as uvby98 100211562[13].
- Q91182587's catalog code is recorded as 2MASS J22184242-3933123[14].
- Q91182587's catalog code is recorded as Gaia DR1 6570645375504992896[15].
- Q91182587's catalog code is recorded as GEN# +1.00211562[16].
- Q91182587's catalog code is recorded as Gaia DR2 6570645379800900736[17].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.222'}[18].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.000'}[19].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.969'}[20].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.05'}[21].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.48'}[22].
- Q91182587's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.9283'}[23].
- Q91182587's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.4624'}[24].
- Q91182587's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.08'}[25].
- Q91182587's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+95.5804'}[26].
Body
Definition and Type
Q91182587's instance of is recorded as high proper-motion star[2].