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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. List of most massive stars - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_stars

    1.3 Relevance of stellar evolution. 1.4 Mass limits. ... Download as PDF; Printable version; In other projects ... evolution [10] R136a3: Tarantula Nebula: 155 163,000

  4. Horizontal branch - Wikipedia

    en.wikipedia.org/wiki/Horizontal_branch

    The horizontal branch (HB) is a stage of stellar evolution that immediately follows the red-giant branch in stars whose masses are similar to the Sun's. Horizontal-branch stars are powered by helium fusion in the core (via the triple-alpha process) and by hydrogen fusion (via the CNO cycle) in a shell surrounding the core.

  5. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    A self-maintaining CNO chain starts at approximately 15 × 10 6 K, but its energy output rises much more rapidly with increasing temperatures [1] so that it becomes the dominant source of energy at approximately 17 × 10 6 K. [4] The Sun has a core temperature of around 15.7 × 10 6 K, and only 1.7% of 4 He nuclei produced in the Sun are born ...

  6. Blue loop - Wikipedia

    en.wikipedia.org/wiki/Blue_loop

    In the field of stellar evolution, a blue loop is a stage in the life of an evolved star where it changes from a cool star to a hotter one before cooling again. The name derives from the shape of the evolutionary track on a Hertzsprung–Russell diagram which forms a loop towards the blue (i.e. hotter) side of the diagram, to a place called the ...

  7. Stellar isochrone - Wikipedia

    en.wikipedia.org/wiki/Stellar_isochrone

    In stellar evolution, an isochrone is a curve on the Hertzsprung-Russell diagram, representing a population of stars of the same age but with different mass. [1] The Hertzsprung-Russell diagram plots a star's luminosity against its temperature, or equivalently, its color. Stars change their positions on the HR diagram throughout their life.

  8. 'World-changing' book claims to 'dismantle' the theory of ...

    www.aol.com/news/2016-06-27-world-changing-book...

    Click through 10 books that will change your life: Phillip E. Johnson, Professor Emeritus of Law at U. C. Berkeley and author of "Darwin on Trial" calls Axe's new research , "bold, insightful and ...

  9. Star chart - Wikipedia

    en.wikipedia.org/wiki/Star_chart

    SFA Star ChartsFree star charts; Geody Star ChartsFree (CC-by-sa) printer friendly star charts for several latitudes and times of the year; An online star chart; Monthly sky maps for every location on Earth Archived 2007-09-13 at the Wayback Machine; The Evening Sky Map – Free monthly star charts and calendar for northern hemisphere ...

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