Walter Baade: Deciphering Stars and Galaxies

A Life Dedicated to Stellar Astronomy

Born on March 24, 1893, in Schröttinghausen (Germany), Wilhelm Heinrich Walter Baade (1893-1960) left his mark on astronomy through meticulous observations and fundamental discoveries about the structure of galaxies. Trained at the University of Göttingen, he emigrated to the United States in 1931 to escape the rise of Nazism, joining the Mount Wilson Observatory in California.

During World War II, blackouts in Los Angeles provided him with an exceptionally dark sky, ideal for observations. In this context, he identified two distinct stellar populations in the Andromeda Galaxy (M31):

• Population I: Young, metal-rich stars located in spiral arms;
• Population II: Old, metal-poor stars concentrated in the galactic halo.

Major Contributions to Astrophysics

Baade revolutionized several fields:

• Recalibration of the Cosmic Distance Scale: In 1952, he demonstrated that the Cepheid variables observed by Edwin Hubble (1889-1953) belonged to Population II, which were less luminous than expected. This suddenly doubled the estimated size of the Universe.
• Collaboration with Fritz Zwicky: With Fritz Zwicky (1898-1974), he proposed in 1934 the existence of neutron stars and supernovas as distinct phenomena.
• Identification of Stars in the Galactic Core: His infrared observations (despite the technical limitations of the time) revealed the exceptional density of stars at the center of the Milky Way.

Legacy and Recognition

Although less publicized than some of his contemporaries, Baade received the RAS Gold Medal in 1954 and the Bruce Medal in 1955. His name is now associated with:

• The Baade's Window, a dark region in the Milky Way;
• The asteroid 1501 Baade;
• The Walter Baade Telescope (Magellan I) in Chile.

Summary Table of Key Discoveries