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  2. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Representative lifetimes of stars as a function of their masses The change in size with time of a Sun-like star Artist's depiction of the life cycle of a Sun-like star, starting as a main-sequence star at lower left then expanding through the subgiant and giant phases, until its outer envelope is expelled to form a planetary nebula at upper right Chart of stellar evolution

  3. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    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 in the CNO cycle. The CNO-I process was independently proposed by Carl von Weizsäcker [5] [6] and Hans Bethe [7] [8] in the late 1930s.

  4. Formation and evolution of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Formation_and_evolution_of...

    The Sun remains a main-sequence star today. [33] As the early Solar System continued to evolve, it eventually drifted away from its siblings in the stellar nursery, and continued orbiting the Milky Way's center on its own. The Sun likely drifted from its original orbital distance from the center of the galaxy.

  5. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The Sun produces on the order of 1% of its energy from the CNO cycle. [27] [a] [28]: 357 [29] [b] The type of hydrogen fusion process that dominates in a star is determined by the temperature dependency differences between the two reactions.

  6. Hayashi track - Wikipedia

    en.wikipedia.org/wiki/Hayashi_track

    In his 1961 papers, Hayashi showed that the convective envelope of a star is determined by = / / / / /, where E is unitless, and not the energy. Modelling stars as polytropes with index 3/2 (in other words, assuming they follow a pressure-density relationship of P = K ρ 5 / 3 {\displaystyle P=K\rho ^{5/3}} ), he found that E = 45 is the ...

  7. Hubble image of a star exploding may reveal the ... - AOL

    www.aol.com/article/2016/03/07/hubble-image-of-a...

    Astronomers think our sun will meet a similar fate one day. It will shed its outer gas layers and eventually fade into a white dwarf star.. The bad news is that Earth will likely get fried during ...

  8. The study authors said that their observations show the dynamic actions that can take place within other planetary systems, even after the host star dies. In about 5 billion years, our sun is ...

  9. What fate awaits the Earth when our sun dies? - AOL

    www.aol.com/news/2016-04-15-what-awaits-the...

    After the sun celebrates its 11 billionth birthday, scientists believe it will continue to expand to the point where it is 166 times bigger than it is now.