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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. Stellar mass loss - Wikipedia

    en.wikipedia.org/wiki/Stellar_mass_loss

    A study in 2012 found that more than 70% of all massive stars exchange mass with a companion which leads to a binary merger in one-third of the cases. [6] Since the trajectory of evolution of these stars is greatly altered due to the mass loss to the companion, models of stellar evolution are focusing on replicating these observations. [7] [8]

  4. Future of an expanding universe - Wikipedia

    en.wikipedia.org/wiki/Future_of_an_expanding...

    The second, the Stelliferous Era, includes the present day and all of the stars and galaxies now seen. It is the time during which stars form from collapsing clouds of gas. In the subsequent Degenerate Era, the stars will have burnt out, leaving all stellar-mass objects as stellar remnants—white dwarfs, neutron stars, and black holes.

  5. Scientists find dead galaxy older than any ever found

    www.aol.com/scientists-dead-galaxy-older-ever...

    Star formation had already stopped in the galaxy some 13.1 billion years ago, just 700 million years after the universe began. While scientists have found similar “dead” galaxies before, it is ...

  6. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    At low metallicity, all stars will reach core collapse with a hydrogen envelope but sufficiently massive stars collapse directly to a black hole without producing a visible supernova. [ 104 ] Stars with an initial mass up to about 90 times the Sun, or a little less at high metallicity, result in a type II-P supernova, which is the most commonly ...

  7. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    Later in its life, a low-mass star will slowly eject its atmosphere via stellar wind, forming a planetary nebula, while a higher–mass star will eject mass via a sudden catastrophic event called a supernova. The term supernova nucleosynthesis is used to describe the creation of elements during the explosion of a massive star or white dwarf.

  8. Most Shocking Soap Star Deaths of All Time - AOL

    www.aol.com/entertainment/most-shocking-soap...

    The All My Children star died in January 2024 at age 50. Per a report from the San Diego County Medical Examiner’s Office, he “died by suicide after an apparent self-inflicted gunshot wound

  9. Heat death of the universe - Wikipedia

    en.wikipedia.org/wiki/Heat_death_of_the_universe

    The overarching plot of the Xeelee Sequence concerns the Photino Birds' efforts to accelerate the heat death of the universe by accelerating the rate at which stars become white dwarves. The 2019 hit indie video game Outer Wilds has several themes grappling with the idea of the heat death of the universe, and the theory that the universe is a ...