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  2. Martin Schwarzschild - Wikipedia

    en.wikipedia.org/wiki/Martin_Schwarzschild

    Schwarzschild's 1958 book Structure and Evolution of the Stars [8] taught a generation of astrophysicists how to apply electronic computers to the computation of stellar models. In the 1950s and ’60s he headed the Stratoscope projects, which took instrumented balloons to unprecedented heights.

  3. Donald D. Clayton - Wikipedia

    en.wikipedia.org/wiki/Donald_D._Clayton

    Donald Delbert Clayton (March 18, 1935 – January 3, 2024) was an American astrophysicist whose most visible achievement was the prediction from nucleosynthesis theory that supernovae are intensely radioactive.

  4. Nuclear astrophysics - Wikipedia

    en.wikipedia.org/wiki/Nuclear_astrophysics

    This results in compositional evolution of cosmic gas in and between stars and galaxies, enriching such gas with heavier elements. Nuclear astrophysics is the science to describe and understand the nuclear and astrophysical processes within such cosmic and galactic chemical evolution, linking it to knowledge from nuclear physics and astrophysics.

  5. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Stellar evolution is the process by which a star changes over the course of its lifetime and how it can lead to the creation of a new star. Depending on the mass of the star, its lifetime can range from a few million years for the most massive to trillions of years for the least massive, which is considerably longer than the current age of the ...

  6. Subrahmanyan Chandrasekhar - Wikipedia

    en.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar

    Subrahmanyan Chandrasekhar (/ ˌ tʃ ə n d r ə ˈ ʃ eɪ k ər /; [3] 19 October 1910 – 21 August 1995) [4] was an Indian-American theoretical physicist who made significant contributions to the scientific knowledge about the structure of stars, stellar evolution and black holes.

  7. Theoretical astronomy - Wikipedia

    en.wikipedia.org/wiki/Theoretical_astronomy

    As the stellar 'generations' advance, the mass of the newly formed elements increases. A first-generation star uses elemental hydrogen (H) as a fuel source and produces helium (He). Hydrogen is the most abundant element, and it is the basic building block for all other elements as its nucleus has only one proton .

  8. Arthur Eddington - Wikipedia

    en.wikipedia.org/wiki/Arthur_Eddington

    Ian Barbour, in his book Issues in Science and Religion (1966), p. 133, cites Eddington's The Nature of the Physical World (1928) for a text that argues the Heisenberg uncertainty principle provides a scientific basis for "the defense of the idea of human freedom" and his Science and the Unseen World (1929) for support of philosophical idealism ...

  9. Roberta M. Humphreys - Wikipedia

    en.wikipedia.org/wiki/Roberta_M._Humphreys

    Roberta M. Humphreys is an American observational stellar astrophysicist. She is Professor Emerita at the University of Minnesota.Her work has included Galactic structure, observational stellar evolution, stellar populations, and large databases.