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The Wide-field High-resolution Infrared TElescope (WHITE) will be dedicatedin the first years of its life to carrying out a few (well focused in terms ofscience objectives and time) legacy surveys.  WHITE would have an angular resolution of ~0.3'' homogeneous over ~0.7 sq.deg. in the wavelength range 1 - 5 um, which means that we will veryefficiently use all the available observational time during night time and daytime. Moreover, the deepest observations will be performed by summing upshorter individual frames. We will have a temporal information that can be usedto study variable objects.  The three key science objectives of WHITE are : 1) A complete survey of theMagellanic Clouds to make a complete census of young stellar objects in theclouds and in the bridge and to study their star formation history and the linkwith the Milky Way. The interaction of the two clouds with our Galaxy might theclosest example of a minor merging event that could be the main driver ofgalaxy evolution in the last 5 Gyrs. 2) The building of the first sample ofdusty supernovae at z<1.2 in the near infrared range (1-5 um) to constrain theequation of state from these obscured objects, study the formation of dust ingalaxies and build the first high resolution sample of high redshift galaxiesobserved in their optical frame 3) A very wide weak lensing survey over thatwould allow to estimate the equation of state in a way that would favourablycompete with space projects.