Spitzer Space Telescope - General Observer Proposal #3316 The Small Magellanic Cloud: A Template for the Primitive Interstellar Medium Principal Investigator: Alberto Bolatto Institution: University of California at Berkeley Co-Investigators: Snezana Stanimirovic, University of California at Berkeley Frank Israel, Leiden Observatory James Jackson, Boston University Adam Leroy, University of California at Berkeley Aigen Li, University of Arizona Ronak Shah, Boston University Joshua Simon, University of California at Berkeley Lister Staveley-Smith, Australia Telescope/CSIRO Science Category: local group galaxies Observing Modes: IracMap MipsScan Hours Approved: 48.8 Abstract: The Small Magellanic Cloud constitutes an excellent laboratory to study the properties of the dust in a low metallicity environment. We propose to obtain images of the entire SMC in all IRAC and MIPS wavebands, a feat only possible because of Spitzer's unparalleled sensitivity. With these observations we will quantify the distribution and properties of very small grains and PAHs throughout the SMC in relation to their environment. These data will allow us to constrain theoretical dust models, and provide information on the abundance, distribution, ionization state, composition, and evolution of PAHs and VSGs. MIPS observations will probe the distribution of small and large dust grains, and in combination with ground-based observations, will be used to provide an independent estimate of the amount of molecular gas in the SMC. Ultimately, this research will help constrain the properties of the ISM in primordial galaxies at high redshifts. The SMC images will be publicly released within 6 months of the last observations, for the benefit of the entire astronomical community and to allow other groups to perform follow-up observations.