This document discusses neutron stars and explores them as natural laboratories for studying extremely dense matter. It provides background on stellar evolution and supernovae that form neutron stars. Neutron stars are incredibly small yet dense, with masses of around 1.35-2 times the sun's mass compressed into the size of Manhattan. They also spin incredibly fast due to conservation of angular momentum. The document examines using neutron stars to study how matter behaves under extreme density and discusses challenges in measuring their precise masses and radii from Earth. It outlines the author's research simulating neutron star atmospheres to help answer fundamental physics questions about their properties.