In comparing my spectra to the spectra (right) sourced from Tinetti, G. et al. (2013) there are clear similarities. There is some alignment of atmospheric absorption lines from Venus (top) and Mars (bottom).This was a promising comparison, indicating that my procedure was headed in the right direction. The next steps of this project would have been to collect the full spectrum for Venus and implement telluric corrections. Due mostly to instrument limitations, there was little more I could explore in this project at my undergraduate institution.