Although less well known outside the field than Edwin Hubble,
"Walter Baade" was arguably the most influential observational
astronomer of the twentieth century. Written by a fellow astronomer
deeply familiar with Baade and his work, this is the first
biography of this major figure in American astronomy. In it, Donald
Osterbrock suggests that Baade's greatest contribution to
astrophysics was not, as is often contended, his revision of
Hubble's distance and age scales for the universe. Rather, it was
his discovery of two distinct stellar populations: old and young
stars. This discovery opened wide the previously marginal fields of
stellar and galactic evolution--research areas that would be among
the most fertile and exciting in all of astrophysics for decades to
come.
Baade was born, educated, and gained his early research
experience in Germany. He came to the United States in 1931 as a
staff member of Mount Wilson Observatory, which housed the world's
largest telescope. There, he pioneered research on supernovae. With
the 100-inch telescope, he studied globular clusters and the
structure of the Milky Way, every step leading him closer to the
population concept he discovered during the wartime years, when the
skies of southern California were briefly darkened. Most Mount
Wilson astronomers were working on weapons-development crash
programs devoted to bringing Baade's native country to its knees,
while he, formally an enemy alien in their midst, was confined to
Los Angeles County but had almost unlimited use of the most
powerful telescope in the world.
After his great discovery, Baade continued his research with the
new 200-inch telescope at Palomar. Always respected and well liked,
he became even more famous among astronomers as they shifted their
research to the fields he had opened. Publicity-shy and seemingly
unconcerned with publication, however, Baade's celebrity remained
largely within the field. This accomplished biography at last
introduces Baade--and his important work--to a wider public,
including the newest generation of skywatchers.
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