Britannica AI Icon

Quick Summary

Spiral arms are a key structural feature of spiral galaxies, including our own Milky Way Galaxy. These arms are characterized by a higher luminosity and extend outward from a central nucleus or a bar-shaped structure. The appearance and extent of these arms can vary significantly between different types of spiral galaxies.123

In spiral galaxies, the arms are typically blue in color, indicating the presence of stars, star clouds, and interstellar gas and dust. The structure of these arms often follows a logarithmic spiral pattern. Astronomers study spiral arms using radio maps of hydrogen and molecular clouds, as these can be detected through interstellar dust that obscures optical views. The formation and dynamics of spiral arms are complex, with theories suggesting they are a result of density-wave patterns and differential rotation within the galactic disk.412

Summary created from Britannica articles using AI. AI can make mistakes, so verify using Britannica articles.

Ask Britannica AI about this topic

Britannica doesn't have a full article on this topic, so we've curated a list of our relevant coverage.