Harlow Shapley: The Astronomer Who Resized Our Galaxy
From Rural Missouri to Astronomical Fame
Born November 2, 1885 in Nashville, Missouri, Harlow Shapley (1885-1972) grew up in poverty on a farm without electricity or running water. His formal education was limited until he discovered a library at age 16 and became fascinated with astronomy.
Educational journey:
1907: Entered the University of Missouri as a journalism student
1910: Transferred to Princeton University to study astronomy under Henry Norris Russell
1911: Obtained his bachelor's degree in astronomy
1913: Completed his PhD at Princeton with a thesis on eclipsing binary stars
Revolutionizing Our Understanding of the Milky Way
1. The Great Debate (1920)
Shapley became famous for his participation in the "Great Debate" with Heber Curtis on April 26, 1920 at the Smithsonian Institution:
Shapley argued that the Milky Way was much larger than previously thought (300,000 light-years in diameter)
He believed spiral nebulae were part of our galaxy (later proven incorrect)
Curtis argued for smaller galaxy size but correctly identified spiral nebulae as separate galaxies
Although both were partially wrong, this debate marked a turning point in astronomy.
2. Mapping the Milky Way (1918-1921)
Using RR Lyrae variable stars in globular clusters as standard candles, Shapley:
Determined the Sun is located about 30,000 light-years from the galactic center
Established the Milky Way's true size at about 100,000 light-years in diameter
Discovered the galactic center lies in the constellation Sagittarius
Published his findings in "Star Clusters" (1930), a foundational work in galactic astronomy
Major Contributions to Astronomy
1. Stellar Classification and Evolution
Shapley made significant contributions to our understanding of stars:
Developed the Hertzsprung-Russell diagram with Henry Norris Russell
Discovered the relationship between a star's color and its absolute magnitude
Established that giant stars are larger but cooler than main-sequence stars
2. Harvard Observatory Directorship (1921-1952)
As director of Harvard College Observatory, Shapley:
Expanded the observatory's research program significantly
Hired Cecilia Payne-Gaposchkin, who made groundbreaking discoveries about stellar composition
Established the Harvard Computers group of female astronomers
Oversaw the creation of the Henry Draper Catalogue of stellar spectra
3. Public Engagement and Education
Shapley was a passionate science communicator:
Wrote popular science books including "Star Clusters" (1930) and "Galaxies" (1943)
Hosted a weekly radio program on science from 1930-1956
Served as president of the American Astronomical Society (1943-1946)
Founded the Science Service organization to promote science journalism
Controversies and Later Career
Shapley was known for his strong personality and sometimes controversial views:
Initially resisted Edwin Hubble's evidence that spiral nebulae were separate galaxies
Engaged in public debates with Fred Hoyle about the nature of the universe
Opposed the idea of a steady-state universe, favoring an evolving universe model
Later in his career, he became an advocate for international scientific cooperation
After retiring from Harvard in 1952, Shapley continued his scientific work and public engagement until his death.
Legacy and Honors
Harlow Shapley's contributions to astronomy were immense:
Fundamentally changed our understanding of the Milky Way's size and structure
Mentored many prominent astronomers including Cecilia Payne-Gaposchkin and Bart Bok
Received numerous awards including:
Bruce Medal (1939)
Gold Medal of the Royal Astronomical Society (1940)
Henry Norris Russell Lectureship (1950)
Honored with:
The Shapley Supercluster of galaxies
Lunar crater Shapley
Asteroid 1123 Shapleya
Shapley died on October 20, 1972 in Boulder, Colorado, leaving behind a transformed understanding of our place in the universe.
Harlow Shapley's Major Contributions
Field
Year
Contribution
Impact
Galactic Astronomy
1918-1921
Determined Sun's position in Milky Way
Showed Sun is not at galactic center, revolutionized our understanding of galaxy structure
Stellar Astronomy
1914
Developed H-R diagram with Russell
Fundamental tool for understanding stellar evolution
Observational Astronomy
1921-1952
Director of Harvard College Observatory
Expanded research programs and mentored many prominent astronomers
Science Communication
1930-1956
Weekly science radio program
Pioneered science communication to the public
Galactic Structure
1930
Published "Star Clusters"
Foundational work in galactic astronomy still referenced today