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  2. 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 ...

  3. Hess diagram - Wikipedia

    en.wikipedia.org/wiki/Hess_diagram

    A Hess diagram plots the relative density of occurrence of stars at differing color–magnitude positions of the Hertzsprung–Russell diagram for a given galaxy or resolved stellar population. The diagram is named after R. Hess who originated it in 1924. [1] Its use dates back to at least 1948. [2]

  4. Main sequence - Wikipedia

    en.wikipedia.org/wiki/Main_sequence

    This evolution is reflected in a broadening of the main sequence band which contains stars at various evolutionary stages. [ 41 ] Other factors that broaden the main sequence band on the HR diagram include uncertainty in the distance to stars and the presence of unresolved binary stars that can alter the observed stellar parameters.

  5. Hertzsprung–Russell diagram - Wikipedia

    en.wikipedia.org/wiki/Hertzsprung–Russell_diagram

    Theoretical calculations of stellar structure and the evolution of stars produce plots that match those from observations. This type of diagram could be called temperature-luminosity diagram , but this term is hardly ever used; when the distinction is made, this form is called the theoretical Hertzsprung–Russell diagram instead.

  6. Hayashi track - Wikipedia

    en.wikipedia.org/wiki/Hayashi_track

    Stellar evolution tracks (blue lines) for the pre-main-sequence. The nearly vertical curves are Hayashi tracks. Low-mass stars have nearly vertical evolution tracks until they arrive on the main sequence. For more-massive stars, the Hayashi track bends to the left into the Henyey track. Even more-massive stars are born directly onto the Henyey ...

  7. The Birth and Death of the Sun - Wikipedia

    en.wikipedia.org/wiki/The_Birth_and_Death_of_the_Sun

    The Birth and Death of the Sun is a popular science book by theoretical physicist and cosmologist George Gamow, first published in 1940, exploring atomic chemistry, stellar evolution, and cosmology. [1] The book is illustrated by Gamow. It was revised in 1952.

  8. File:Star Life Cycle Chart.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Star_Life_Cycle_Chart.jpg

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  9. Ejnar Hertzsprung - Wikipedia

    en.wikipedia.org/wiki/Ejnar_Hertzsprung

    The so-called "Hertzsprung–Russell Diagram" has been used ever since as a classification system to explain stellar types and stellar evolution. He also discovered two asteroids, one of which is 1627 Ivar, an Amor asteroid. [5] His wife Henrietta (1881–1956) was a daughter of the Dutch astronomer Jacobus Kapteyn.