Morrison, Philip (1915–2005)
During a chamber music performance in the Cornell Student Center I began to think of the possibilities of gamma-ray astronomy. By the end of 1958, I had published a summary of what might be learned from gamma-ray astronomy... the paper was challenging, and a few months later, in the spring of 1959, Guiseppe Cocconi came into my office. We were thinking about gamma-rays of natural origin when we realized that we knew how to make them, too. We were making lots of them downstairs at the Cornell synchrotron. So Cocconi asked whether they could be used for communicating between the stars. It was plain that they would work, but they weren't very easy to use. My reply was enthusiastic but cautious. Shouldn't we look through the whole electromagnetic spectrum to find the best wavelength for any such communication? That was the germ of the idea.Morrison received his B.S. from the Carnegie Institute of Technology (1936) and Ph.D. in theoretical physics from the University of California, Berkeley (1940), under the supervision of J. Robert Oppenheimer. From 1942–46 he worked on the Manhattan Project, then joined the physics faculty of Cornell. From 1965 he was on on the faculty at MIT. Aside from his role in instigating the modern SETI movement, Morrison was a leader in organizing and chairing conferences on the subject, including those at Byurakan (1971) (see Byurakan SETI conferences) and Boston University (1973), various NASA symposia on SETI, and the IAU meetings on SETI (1980 and 1984).
Related categories SETI
ASTRONOMERS AND ASTROPHYSICISTS
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