The spiral structure of our galaxy was identified through the mapping of neutral hydrogen clouds, particularly using the 21 cm radio wavelength, which is unobstructed by dust. These hydrogen clouds exhibit Doppler shifts that reveal their movement and help outline the galaxy's rotating shape. Early suggestions of the Milky Way's spiral form date back to 1852, with ongoing debates about its place in the universe. Radio astronomers began mapping these structures before 1970, refining their techniques over time by combining data from gas clouds and bright stars. Current maps continue to evolve as new observations are made, enhancing our understanding of the galaxy's structure.