A Type Ic Supernova is a powerful explosion that occurs when a massive star exhausts its nuclear fuel and collapses under its own gravity. These supernovae are characterized by the absence of hydrogen in their spectra, which distinguishes them from other types of supernovae. They typically arise from stars that have lost their outer layers of hydrogen and helium, often due to strong stellar winds or interactions with companion stars. Type Ic supernovae are important for understanding the life cycles of massive stars and the chemical enrichment of the universe. They are often associated with gamma-ray bursts and can produce heavy elements like iron and nickel during the explosion, contributing to the formation of new stars and planets.