Su-Shu Huang (黃授書, April 16, 1915 – September 15, 1977) was a Chinese-born United States astrophysicist. A graduate of the University of Chicago, Huang began his career with the study of the continuous absorption coefficients of two-electron systems, but eventually his research focus turned to the study of stellar atmospheres, radiative zone, and binary star and multiple star systems. In subsequent years, Huang began to cover the topic of life on extrasolar planets and the prerequisites thereof, coining the term "habitable zone" to refer to the region around a star where planets could support liquid water at their surfaces at a 1959 conference of the Astronomical Society of the Pacific.
In his early years he studied two-electron systems, Huang later studied stellar atmospheres, , and the dynamics of stars in binary or multiple star systems. Huang's research into the physics of stars later led him to delineate the types of stars that could support extraterrestrial life, leading to his coining of the term "habitable zone" and eventually his study of planetary habitability in a 1960 paper on the sizes of habitable planets. Huang's explorations into extraterrestrial life were also published in popular works, such as American Scientist and Scientific American.
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