Q90881658
high proper-motion star in the constellation Lynx
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Q90881658
Summary
Q90881658 is a high proper-motion star[1].
Key Facts
- Q90881658's instance of is recorded as high proper-motion star[2].
- Q90881658's constellation is recorded as Lynx[3].
- Q90881658's spectral class is recorded as M4[4].
- Q90881658's catalog code is recorded as LSPM J0625+5610[5].
- Q90881658's catalog code is recorded as NLTT 16475[6].
- Q90881658's catalog code is recorded as 2MASS J06255299+5610250[7].
- Q90881658's catalog code is recorded as USNO-B1.0 1461-00174928[8].
- Q90881658's catalog code is recorded as G 192-26[9].
- Q90881658's catalog code is recorded as GEN# +9.80192026[10].
- Q90881658's catalog code is recorded as GJ 3393[11].
- Q90881658's catalog code is recorded as LHS 1848[12].
- Q90881658's catalog code is recorded as USNO 510[13].
- Q90881658's catalog code is recorded as [RHG95] 1043[14].
- Q90881658's catalog code is recorded as PLX 1476.11[15].
- Q90881658's catalog code is recorded as WISEA J062553.13+561019.6[16].
- Q90881658's catalog code is recorded as Gaia DR2 997801721262070912[17].
- Q90881658's type of variable star is recorded as rotating variable star[18].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.34'}[19].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8'}[20].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.257'}[21].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.653'}[22].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.359'}[23].
- Q90881658's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2403'}[24].
- Q90881658's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+50.4742'}[25].
- Q90881658's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+19.8121'}[26].
Body
Definition and Type
Q90881658's instance of is recorded as high proper-motion star[2].