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The data of photometric measurements of the long-period eclipsing variableepsilon Aur in the two main minima 1982 and 2010 in the spectral range of 1--5microns are presented. Noted is the similarity of light curves in eclipse, itsasymmetry, and availability of the short interval increased brightness. We aredetecting the phase changing of the indicator color J-M and the effect ofshort-time changing of the color to be more blue at the moments during thebeginning and end of the eclipse.

Comparison of the infrared magnitudes of the eclipsing variable star  epsilon Aur during the two main luminance lows using observations from 1980  to 2015