Indirect search for Dark Matter trapped inside celestial bodies is one of the main physics goals of neutrino telescopes. The analysis performed with the data recorded by ANTARES in 2007 and 2008 to detect the ux of neutrinos originating from Dark Matter inside the Sun is reviewed. The obtained limits on the neutrino ux and on the WIMP-nucleon cross-sections are presented and compared to other existing limits from direct and indirect detection experiments as well as predictions from SUSY models such as the CMSSM and the more phenomenological MSSM-7 model