As a possible alternative to organic–inorganic hybrid perovskite halide, inorganic Cs2SnI6 has drawn more and more research attention recently. In order to find more Cs2SnI6 derivatives as the potential solar cell absorber materials, I- ions in Cs2SnI6 are replaced by other halogen ions and forms the Cs2SnI6-nXn (X = F, Cl, Br; n = 1 ∼ 6) compounds, whose atomic structures, electronic structures and optical absorption are investigated by first principles calculations. When the alloying level n increases, the mean lattice constants, the weighted sn-X and Cs-X bond lengths all decreases linearly; the bond length of each sn-X diminishes slightly inside the octahedral structure; Eg of Cs2SnI6-nXn increases nonlinearly. Eleven Cs2SnI6-nXn compounds have an Eg between 1.0 eV and 2.0 eV and so can be potentially used as the light absorption layer of solar cells. Their partial DOS demonstrate that as the alloying level n increases, I 5p orbital in VBM and CBM is gradually substituted by Br 4p, or Cl 3p, or F 2p orbital. The eleven Cs2SnI6-nXn alloys all have a direct bandgap although the lattice distortion induced by the alloyed X- ion. At some doping levels, the Cs2SnI6-nXn alloys can have a much lower m*h and thus promise a better photovoltaic performance than that of Cs2SnI6.