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  2. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    Stars evolve because of changes in their composition (the abundance of their constituent elements) over their lifespans, first by burning hydrogen (main sequence star), then helium (horizontal branch star), and progressively burning higher elements. However, this does not by itself significantly alter the abundances of elements in the universe ...

  3. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Stellar evolution is not studied by observing the life of a single star, as most stellar changes occur too slowly to be detected, even over many centuries. Instead, astrophysicists come to understand how stars evolve by observing numerous stars at various points in their lifetime, and by simulating stellar structure using computer models.

  4. Stellar influences on an origin of life setting - Wikipedia

    en.wikipedia.org/wiki/Stellar_influences_on_an...

    As stars evolve, so do their emissions; younger stars tend to be the most active, meaning they have stronger winds, larger flaring events, and an increased frequency of CMEs. [13] This means that planets orbiting younger stars would endure more volatile stellar events that impact their habitable and abiogenesis zones, perhaps even making them ...

  5. Galaxy formation and evolution - Wikipedia

    en.wikipedia.org/wiki/Galaxy_formation_and_evolution

    However, the current rate of galaxy mergers does not explain how all galaxies move from the "blue cloud" to the "red sequence". It also does not explain how star formation ceases in galaxies. Theories of galaxy evolution must therefore be able to explain how star formation turns off in galaxies. This phenomenon is called galaxy "quenching". [16]

  6. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    Typical boundary conditions set the values of the observable parameters appropriately at the surface (=) and center (=) of the star: () =, meaning the pressure at the surface of the star is zero; () =, there is no mass inside the center of the star, as required if the mass density remains finite; () =, the total mass of the star is the star's ...

  7. Star formation - Wikipedia

    en.wikipedia.org/wiki/Star_formation

    Star formation theory, as well as accounting for the formation of a single star, must also account for the statistics of binary stars and the initial mass function. Most stars do not form in isolation but as part of a group of stars referred as star clusters or stellar associations .

  8. From VSCO's Hydro Flask to TikTok's Stanley, why and ... - AOL

    www.aol.com/news/vscos-hydro-flask-tiktoks...

    Nalgenes and CamelBaks were the big-brand water bottles up until 2015, but it wasn’t a big deal if you did or didn’t have one. Then came S’well, which offered more than 200 size-and-color ...

  9. Stellar chemistry - Wikipedia

    en.wikipedia.org/wiki/Stellar_chemistry

    The formation of stars is of particular interest. Research published in 2009 presents spectroscopic observations of so-called "young stellar objects" viewed in the Large Magellanic Cloud with the Spitzer Space Telescope. This research suggests that water, or, more specifically, ice, plays a large role in the formation of these eventual stars [3]