Astrophysical processes that result in the polarization of light include scattering, synchrotron emission, and Kerr rotation, among others. Polarization occurs whenever there is anisotropy in matter-radiation interactions, with ideal spherical symmetry being the only condition that can prevent it. Key mechanisms involve elastic and inelastic scattering on free electrons and atoms, which alter the polarization state of photons. Additionally, the presence of magnetic or electric fields can complicate polarization states, providing insights into distant objects through effects like Zeeman and Hanle. Overall, various processes contribute to the rich phenomenon of light polarization in the universe.