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  1. Há 1 dia · In this fascinating video, we explore the concept of the black dwarf, the theoretical final stage of stellar evolution. Join us as we delve into the science ...

    • 11 min
    • Zeey
  2. Há 5 dias · However, if some massive stars are collapsing completely into black holes without supernova explosions, then they cannot contribute to the creation and recycling of elements.

  3. en.wikipedia.org › wiki › SunSun - Wikipedia

    Há 21 horas · The Sun is a G-type main-sequence star (G2V), informally called a yellow dwarf, though its light is actually white. It formed approximately 4.6 billion years ago from the gravitational collapse of matter within a region of a large molecular cloud.

  4. en.wikipedia.org › wiki › SupernovaSupernova - Wikipedia

    Há 2 dias · A supernova occurs during the last evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion. The original object, called the progenitor, either collapses to a neutron star or black hole, or is completely destroyed to form a diffuse nebula.

  5. en.wikipedia.org › wiki › Black_holeBlack hole - Wikipedia

    Há 1 dia · A black hole is a region of spacetime where gravity is so strong that nothing, including light and other electromagnetic waves, is capable of possessing enough energy to escape it. Einstein's theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.

  6. Há 4 dias · Biography. Background. Bob Irvine holds an Honours MA in English and Philosophy from the University of Aberdeen, and a PhD from Edinburgh. He taught at Brunel University in London before returning to his current post in 1999. Teaching & PhD supervision. Research. Projects. Publications. This article was published on 13 May, 2024.