Q87277918
high proper-motion star in the constellation Auriga
Press Enter · cited answer in seconds
0 sources
Q87277918
Summary
Q87277918 is a high proper-motion star[1].
Key Facts
- Q87277918's instance of is recorded as high proper-motion star[2].
- Q87277918's constellation is recorded as Auriga[3].
- Q87277918's spectral class is recorded as M3.53[4].
- Q87277918's catalog code is recorded as Karmn J06140+516[5].
- Q87277918's catalog code is recorded as 2MASS J06140240+5140081[6].
- Q87277918's catalog code is recorded as LSPM J0614+5140[7].
- Q87277918's catalog code is recorded as USNO-B1.0 1416-00181966[8].
- Q87277918's catalog code is recorded as G 192-22[9].
- Q87277918's catalog code is recorded as GJ 3388[10].
- Q87277918's catalog code is recorded as NLTT 16225[11].
- Q87277918's catalog code is recorded as [RHG95] 1026[12].
- Q87277918's catalog code is recorded as WISEA J061401.93+514007.0[13].
- Q87277918's catalog code is recorded as UCAC4 709-041662[14].
- Q87277918's catalog code is recorded as PM J06140+5140[15].
- Q87277918's catalog code is recorded as Gaia DR2 971499272821709440[16].
- Q87277918's type of variable star is recorded as rotating variable star[17].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.860'}[18].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.360'}[19].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.122'}[20].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.5'}[21].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.525'}[22].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.607'}[23].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.252'}[24].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.918'}[25].
- Q87277918's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6883'}[26].
Body
Definition and Type
Q87277918's instance of is recorded as high proper-motion star[2].