This course will examine the opportunities for chemistry that will be created by the next generation of radio astronomy interferometers. The National Radio Astronomy Observatory is in the process of commissioning a new interferometer for millimeter wave spectroscopy called the Atacama Large Millimeter/Submillimeter Array (ALMA). They are also upgrading their microwave array to become the Expanded Very Large Array (EVLA). Both telescopes will feature broadband spectral coverage with high spatial resolution that will make it possible to obtain multispecies chemical images in a single measurement. This course will examine the new capabilities of these next generation radio telescopes and the impact they will have on our understanding of interstellar chemistry. The course will cover spectroscopy topics related to the observations including molecular rotational spectroscopy and the principles of imaging with radio telescope interferometers. The existing literature on chemical mapping in radio astronomy will be explored to see how these images can be used to understand chemical and astronomical processes. Finally, the early science proposals for ALMA will be discussed and new proposals designed specifically to elucidate interstellar chemical processes will be developed. The course will include presentations from scientists at NRAO who have designed and are constructing these new facilities. The class will also meet with the students in a graduate seminar in the Astronomy Department to discuss how chemistry and astronomy can be combined to learn about our cosmic origins.