In 1942, Brown was invited to join the staff of the Met Lab by Glenn Seaborg because they wanted his help in using the chemistry of plutonium to separate it from uranium generated in fuel rods of the atomic reactors. Brown and his co-worker, Orville Hill, discovered that plutonium could be separated from uranium using gaseous evaporation of fluorides prepared from dry fluoridation.
Later, Brown was transferred to Oak Ridge's Clinton Engineering Works (X-10) site. At Oak Ridge, Brown worked to develop procedures for isolating gram quantities of plutonium from its trace occurrences in metallic uranium fuel rods. His group's work was the backup plan for the liquid chemical separation methods being developed at the same time. While at Oak Ridge, Brown also became the assistant director of chemistry.
After the atomic bombs were dropped on Hiroshima and Nagasaki, Brown became a strong advocate for regulating nuclear weapons. In 1946, Brown published Must Destruction Be Our Destiny?, a book that warned readers about the extreme dangers posed by atomic weapons. To maximize his political impact, he held 102 lectures about his book and work within three months of publication.
He also used his book sale royalties to support the work of an organization for atomic scientists that eventually became a part of the Federation of American Scientists. The Federation's goal was to promote proper regulation of nuclear power and weapons.
Harrison Scott Brown was born on September 26, 1917 in Sheridan, Wyoming. After his father died, he moved with his mother to San Francisco in 1927. Brown learned how to play the piano from his mother, who worked as a dental assistant, music teacher, and piano player for silent movies.
Brown attended Galileo High School, where he apparently built his own chemistry laboratory. After graduating from high school, he attended the University of California at Berkeley. In 1938, Brown graduated with a B.S. degree in chemistry.
Following in his mentor, Professor Robert D. Fowler, across the country, he decided to pursue graduate studies at Johns Hopkins University. Before moving to Baltimore, he married Adele Scrimger and had a son, Eric. As a graduate student, Brown developed mass spectrometric techniques to study cobalt's isotopic composition.
After the discovery of nuclear fission in 1939, Brown and Fowler began to focus on the diffusion properties of uranium hexafluoride. By 1940, the two had the largest gaseous uranium fluoride generating capacity in the United States. They became major suppliers of uranium tetrafluoride and hexafluoride to the atomic fission projects at the Manhattan Project's Columbia University and University of Chicago sites.
Brown received his Ph.D. in chemistry from Johns Hopkins University in 1941.
In 1946, Brown returned to the University of Chicago to work as an assistant professor in the Department of Chemistry and the Institute for Nuclear Studies. Working with former Manhattan Project colleagues, Brown helped develop the new scientific field of nuclear geochemistry. The research and studies in this field greatly impacted understandings in Earth and planetary sciences.
Nuclear mass abundance data from Brown's research helped Maria G. Mayer develop the concept of the nuclear shell model. At this point in time, Brown was focused on three fields:
- Estimating relative elemental abundances in the solar system by determining the composition of meteorites.
- Determining the temporal progress of magmatic evolution of the Earth's crust by measuring uranium/lead ages of common igneous rock.
- Determining the age of the Earth by measuring the isotopic composition of lead in iron meteorites.
Beginning in 1949, Brown began traveling to Jamaica, where he first observed the problems of rapid population growth and technology struggles in developing countries. Brown's travels led him to write, The Challenge of Man's Future, a book about the structure and fate of human society.
In 1951, Brown moved from the University of Chicago to teach at the California Institute of Technology as a geochemistry professor. In 1955, Brown was elected to the National Academy of Sciences at the rather early age of thirty-seven years old. By now, Brown had also remarried to Rudd Owen, his colleague and fellow humanitarian advocate.
Foreign Affairs and Global Impact
Working with Bertrand Russell and Albert Einstein in the 1950s, he helped organize and direct the Pugwash Conferences, which were aimed at discussing the dangers of nuclear weapons and the need for regulation.
In 1957, Brown was asked to organize a new committee on oceanography for the National Academy of Sciences by its president, Detlev Bronk. Known as NASCO, the committee published its first report, "Oceanography 1960," which described the future of oceanographic research and proposed a ten-year plan for large-scale expansion of the field.
From 1962-1974, he served as the foreign secretary of the National Academy of Sciences. During his tenure, he helped transform the office into a development agency for fostering science and technology in developing nations from Africa, Asia, and Latin America. He also worked to facilitate East-West exchanges and collaborations.
Brown was served as the president of the International Council of Scientific Unions from 1974-1976. At the same time, Brown chaired a large-scale study of world food and nutrition and was asked to recommend what the United States could do to help.
Finishing in 1977, the study concluded that adequate food and nutrition levels could be sustainably achieved for ten billion people if research was done and used in developing countries to increase yields per hectare. It also stressed the focus on nitrogen fixation by leguminous and cereal plants. In 1977, he also became director of the Resource System Institute at the East-West Center in Hawaii.
After retiring from the East-West Center in 1983, he moved to Albuquerque with his third wife, Theresa Tellez. Despite his age and progressive paralysis in his spine, Brown became the editor-in-chief of the Bulletin of the Atomic Scientists. He continued to work at the Bulletin until he died on December 8, 1986 at the age of sixty-nine.
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