Imre Friedmann
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Imre Friedmann
E. Imre Friedmann (1921 – June 11, 2007) was a biologist, Robert O. Lawton Distinguished Professor of Biology at Florida State University and the NASA Ames Research Center, and Director, Polar Desert Research Center. He studied endolithic microbial communities and astrobiology. After escaping the Holocaust, Friedmann received his Ph.D. in botany from the University of Vienna, Austria in 1951, and he died on June 11, 2007. Friedmann made important discoveries of life in extreme environments, particularly cryptoendolithic microbial communities that grow within rocks in deserts, including those of Antarctica and the Negev Desert in Israel. He was also interested in terraforming and wrote several articles about the possibility of terraforming Mars using microbes. In later years he was involved with investigations of martian meteorite ALH84001, which was claimed to contain evidence for early microbial life on Mars. He was a Foreign Member of the Hungarian Academy of ...
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Roseli Ocampo-Friedmann
Roseli Ocampo-Friedmann (November 23, 1937 – September 4, 2005) was a Filipino-American microbiologist and botanist who specialized in the study of cyanobacteria and extremophiles. Her work has been cited in work exploring the terraforming of Mars. Biography Ocampo-Friedmann was born Roseli Ocampo on November 23, 1937 in Manila, Philippines to Eliseo and Generosa Ocampo. She earned a degree in botany from the University of the Philippines in 1958. After completing her master's at Hebrew University in Jerusalem in 1966, she returned to the Philippines to work for Manila's National Institute of Science and Technology. In 1968, she joined Dr. Imre Friedmann at Florida State University where she received her PhD in 1973. Roseli married Friedmann in 1974. In 1987, she became a professor at Florida A&M University in Tallahassee, while working summers at Florida State University with Friedmann. Later in her career, she served as a scientific consultant for the SETI Insti ...
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Mars
Mars is the fourth planet from the Sun. It is also known as the "Red Planet", because of its orange-red appearance. Mars is a desert-like rocky planet with a tenuous carbon dioxide () atmosphere. At the average surface level the atmospheric pressure is a few thousandths of Earth's, atmospheric temperature ranges from and cosmic radiation is high. Mars retains some water, in the ground as well as thinly in the atmosphere, forming cirrus clouds, frost, larger polar regions of permafrost and ice caps (with seasonal snow), but no liquid surface water. Its surface gravity is roughly a third of Earth's or double that of the Moon. It is half as wide as Earth or twice the Moon, with a diameter of , and has a surface area the size of all the dry land of Earth. Fine dust is prevalent across the surface and the atmosphere, being picked up and spread at the low Martian gravity even by the weak wind of the tenuous atmosphere. The terrain of Mars roughly follows a north-south ...
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