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Computational astrophysics refers to the methods and computing tools developed and used in astrophysics research. Like computational chemistry or computational physics , it is both a specific branch of theoretical astrophysics and an interdisciplinary field relying on computer science , mathematics , and wider physics .
Anthony W. Case (born 1980) is an American astrophysicist who has designed instruments to study the solar wind and cosmic rays on unmanned spacecraft. A native of Oregon, he earned his undergraduate degree in physics from the University of Oregon and a doctorate in astronomy at Boston University. [1]
The team devised a way to measure the surface gravity of distant stars to help determine if the planets in their orbit have life-supporting conditions.
While many institutes of education do not boast an astroinformatics program, such programs most likely will be developed in the near future. Informatics has been recently defined as "the use of digital data, information, and related services for research and knowledge generation". However the usual, or commonly used definition is "informatics ...
Annette S. Lee is an American astrophysicist and professional artist. [1] Lee is the director of Native Skywatchers, a program created to record, map, and share Indigenous star knowledge. [ 2 ] She is mixed-race Lakota and works with Ojibwe , Dakota and Lakota communities to preserve those cultures' astronomical and ecological knowledge.
The Enzmann starship proposed in 1964 is a large fusion-powered spacecraft that could function as an interstellar ark, supporting a crew of 200 with extra space for expansion, on multi-year journeys at subluminal speeds to nearby star systems. [3] In 1955 Project Orion considered nuclear propulsion for spacecraft, suitable for deep space voyages.
In 1996, he joined the faculty of the University of Rochester, where he is a professor of astrophysics. Frank's research focus is astrophysical fluid dynamics . His research group developed the AstroBEAR adaptive mesh refinement code used for simulating magneto fluid dynamics flows in astrophysical contexts. [ 3 ]