Since its inception in 1901, numerous Fellows and Honorary Fellows of the Society have been awarded the Nobel Prize. The first two recipients were Honorary Fellows Hendrik A Lorentz and Pieter Zeeman in 1902 for the Nobel Prize in Physics. The Society's first women winner was Honorary Fellow Marie Curie in 1903 for the Nobel Prize in Physics. Marie Curie was the first person to win or share two Nobel Prizes, being awarded the Nobel Prize in Chemistry in 1911.
In 1964, Dorothy Hodgkin became not only the first female Fellow of the Society to win a Nobel Prize (Chemistry) but also the first female member of the University of Cambridge to do so. The Nobel Prize is one of many prestigious awards in the field of science that our members have been awarded and these include; The Copley Medal, The Royal Medal, The Dalton Medal, The Lomonosov Gold Medal, Max Planck Medal, The Goethe Prize, The Dirac Medal, The Eddington Medal, and the Albert Einstein Award to name but a few.
We currently have 47 Nobel Prize winners.
2017 | Nobel Prize in Chemistry Honorary Fellow
2020 | Nobel Prize in Physics Fellow
2010 | Nobel Prize in Medicine Fellow
2009 | Nobel Prize in Chemistry Honorary Fellow
2002 | Nobel prize in Physiology or Medicine Honorary Fellow
2002 | Nobel Prize in Physiology or Medicine Honorary Fellow
2001 | Nobel Prize in Physiology or Medicine Honorary Fellow
1997 | Nobel Prize in Chemistry Honorary Fellow
1991 | Nobel Prize for Physics Honorary Fellow
1983 | Nobel Prize in Physics Fellow
1982 | Nobel Prize in Chemistry Fellow
1979 | Nobel Prize in Physics Fellow
1977 | Nobel Prize in Physics Fellow
1977 | Nobel Prize in Economics Fellow
1974 | Nobel Prize in Physics Fellow
1967 | Nobel Prize in Chemistry Fellow
1967 | Nobel Prize in Physiology or Medicine Honorary Fellow
1964 | Nobel Prize in Chemistry Fellow
1963 | Nobel Prize in Medicine Fellow
1962 | Nobel Prize in Medicine Fellow
1962 | Nobel Prize in Chemistry Fellow
1960 | Nobel Prize in Physiology or Medicine Honorary Fellow
1957 | Nobel Prize in Chemistry Fellow
1954 | Nobel Prize in Physics Fellow
1952 | Nobel Prize in Chemistry Fellow
1951 | Nobel Prize in Physics Fellow
1948 | Nobel Prize in Physics Fellow
1947 | Nobel Prize in Physics Fellow
1937 | Nobel Prize in Physics Fellow
1935 | Nobel Prize in Physics Fellow
1933 | Nobel Prize in Physics Fellow
1932 | Nobel Prize in Physiology or Medicine Fellow
1929 | Nobel Prize in Medicine Fellow
1928 | Nobel Prize in Physics Fellow
1927 | Nobel Prize in Physics Honorary Fellow
1927 | Nobel Prize in Physics Fellow
1922 | Nobel Prize in Chemistry Fellow
1922 | Nobel Prize in Physics Honorary Fellow
1919 | Nobel Prize in Physiology or Medicine Honorary Fellow
1918 | Nobel Prize in Physics Honorary Fellow
1915 | Nobel Prize in Physics Fellow
1908 | Nobel Prize in Chemistry Fellow
1906 | Nobel Prize in Physics Fellow
1904 | Nobel Prize in Physics Fellow
1903 | Nobel Prize in Physics Honorary Fellow
1902 | Nobel Prize in Physics Honorary Fellow
From Darwin’s paper on evolution to the development of stem cell research, publications from the Society continue to shape the scientific landscape.
Mathematical Proceedings is one of the few high-quality journals publishing original research papers that cover the whole range of pure and applied mathematics, theoretical physics and statistics.
Biological Reviews covers the entire range of the biological sciences, presenting several review articles per issue. Although scholarly and with extensive bibliographies, the articles are aimed at non-specialist biologists as well as researchers in the field.
The Spirit of Inquiry celebrates the 200th anniversary of the remarkable Cambridge Philosophical Society and brings to life the many remarkable episodes and illustrious figures associated with the Society, including Adam Sedgwick, Mary Somerville, Charles Darwin, and Lawrence Bragg.
Become a Fellow of the Society and enjoy the benefits that membership brings. Membership costs £20 per year.
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What we call the Milky Way, our Galaxy, has been the focus of myth, story and study in every society with a recorded history for millennia. Understanding its structure defeated Isaac Newton. One hundred years ago it was realized that the Milky Way is just one amongst a Universe of galaxies. With electronics, digital systems, and spacecraft we have learned how to measure the structure and assembly history of the Milky Way Galaxy over its 13 billion year history, even identifying ancient stars from the earliest proto-structures to form. We quantify the formation of the chemical elements over time and their distribution in space. We use dynamics to weigh the unseen. We can calculate the future of the Milky Way until it ends its existence as an isolated Galaxy, merging with Andromeda some 5 billion years from now, and the death of the Sun a few billion years after that. This lecture will tell that story.
Present-day efforts to preserve endangered crop varieties emphasize "safety duplication"—a strategy better known as backup—as an essential step in conservation. Important collections of seeds or other plant genetic materials are copied, in whole or part, and sent to physically distant sites to provide security in the case of local disaster. This talk traces the history of seed banking to understand how, why and with what consequences copying collections came to occupy this central place. The intertwined histories of the central long-term seed storage facility of the United States (opened in 1958) and the international seed conservation system developed in the 1970s reveal how changing conceptions of security, linked to changing economic, political and technological circumstances, transformed both the guiding metaphors and the practices of seed conservation. Seed banking gave way to seed backup: whereas early long-term cold storage facilities vested security in robust infrastructures and the capacities of professional staff, between the 1960s and 1990s, this configuration gave way to one in which security was situated in copies rather than capacities. This history ultimately raises questions about the security promised and achieved through present-day infrastructures for crop genetic resources conservation.
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