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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. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    Stellar structure models describe the internal structure of a star in detail and make predictions about the luminosity, the color and the future evolution of the star. Different classes and ages of stars have different internal structures, reflecting their elemental makeup and energy transport mechanisms.

  4. Hertzsprung–Russell diagram - Wikipedia

    en.wikipedia.org/wiki/Hertzsprung–Russell_diagram

    The spectral type is not a numerical quantity, but the sequence of spectral types is a monotonic series that reflects the stellar surface temperature. Modern observational versions of the chart replace spectral type by a color index (in diagrams made in the middle of the 20th Century, most often the B-V color) of the stars.

  5. Stellar birthline - Wikipedia

    en.wikipedia.org/wiki/Stellar_birthline

    The stellar birthline is a predicted line on the Hertzsprung–Russell diagram that relates the effective temperature and luminosity of pre-main-sequence stars at the start of their contraction. [1] Prior to this point, the objects are accreting protostars , and are so deeply embedded in the cloud of dust and gas from which they are forming ...

  6. 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.

  7. Hertzsprung gap - Wikipedia

    en.wikipedia.org/wiki/Hertzsprung_gap

    Hertzsprung–Russell diagram with the Hertzsprung Gap visible as an area containing few stars between the main sequence and red-giant branch. The Hertzsprung gap is a feature of the Hertzsprung–Russell diagram for a star cluster.

  8. List of stellar properties - Wikipedia

    en.wikipedia.org/wiki/List_of_stellar_properties

    Pages Related to Stellar properties, Pages using the word stellar in a physics context. ... Stellar evolution; Stellar flare; Stellar flux; Stellar fog; Stellar halo;

  9. Category:Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Category:Stellar_evolution

    Pages in category "Stellar evolution" The following 51 pages are in this category, out of 51 total. This list may not reflect recent changes. ...