I am currently working on analyzing submillimeter spectroscopic observations of the giant molecular cloud in R Coronae Australis (R Cr A), taken with an instrument known as SuperCam, a 64-pixel heterodyne receiver, previously installed on the Submillimeter Telescope on Mt. Graham, AZ. This is just one section of a larger 500-degree survey of the galactic plane, focused on the 12CO(3-2) and 13CO(3-2) transitions of the carbon dioxide molecule. Using the velocity and linewidth of CO, I am studying how turbulence and feedback from star formation affect the evolution of a large molecular cloud. These observations are unique in that they map a large area at the highest spatial resolution yet achieved. My hope is that these observations will help us to better understand the lifecycle of the ISM. I am working towards publishing a paper on these results in the next several months. I enjoy studying the Interstellar Medium because I feel that it brings me closer to understanding the origins of humanity, and hope to continue researching it after my undergraduate