Relatively small bodies in the solar system have no atmosphere (or very thin, called the exosphere) and no magnetic field: they are virtually unprotected from the influence of the space environment in which they are inserted. Such bodies (like most asteroids, moons, and comets far from the sun), are subject to the effects of so-called space weathering. To simulate and study this phenomenon in the laboratory, three samples of ordinary chondrite meteorites were irradiated by H(positive) beams with 1.0 MeV energy. One of the samples was also irradiated by a 2.0 MeV N(positive) beam. The effects of irradiation were monitored by Raman and UV-VIS-NIR spectroscopies. The Raman results show systematic variations in the wavenumber, intensity, and width of the studied vibrational bands, evidence of structural modifications. The shock sections of the destruction of Si-O bonds present in the crystalline structures were determined. Integrated sphere reflectance UV-VIS-NIR spectroscopy was used to monitor changes in spectral characteristics. The obtained spectra show progressive darkening and reddening of the irradiated samples; The extent of these modifications depends on the initial iron content in the structure. It is proposed that the redness observed with the increase of irradiation creep (or dose) is due to the increase in the absorption coefficient in the blue band, which, in turn, results from the decrease of the optical gap of the material. These results are relevant for modeling the physicochemical evolution of asteroids exposed to the solar Wind.