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Arago is a concept of space mission submitted to the European Space Agency's M7 science program. It will target a number of science cases in stellar physics including the characterisation of star-planet interactions. The concept is based on a 1-m class Ritchey-Chretien F/13 telescope mounted on an Ariel-type platform. The scientific payload includes a common polarimetric unit and 2 spectrographs connected via a dichroic splitter. The polarimetric unit consists of 6 MgF2 plates in pairs connected by optical contact and a Wollaston analyzer. Each of the spectral channels represents an echelle spectrograph. The first one will operate in the UV range 119-320 nm with the spectral resolving power of R>25 000. It consists of an off-axis parabolic collimator, an echelle grating in a quasi-Littrow mounting, a cross-disperser concave grating, and a CMOS camera. The cross-disperser grating works also as a camera mirror and represents a holographic grating recorded with aberrated wavefronts and on a spherical substrate. The spectral image is projected onto a d-doped CMOS detector. The second spectral channel operates in the visible range 350-888 nm with R>35 000 and uses an immersed grating. The image is focused with a 4-lens objective onto a CMOS detector. In addition, the optical design includes two stages of fine-guiding system. The first stage represents a projecting system tracking the image around the entrance pinhole and communicating with the platform actuators. The second one is fed by the 0-th diffraction order of the visible channel echelle. It is communicating with a tip-tilt mirror in front of the dichroic. The first stage should improve the platform pointing accuracy from 8" to 200 mas precision to guarantee that the star images passes through the instrument's entrance pinhole. The second stage should correct the pointing accuracy further as well as some thermo-elastic deformations.