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A white dwarf is what remains of a main-sequence star of low or medium mass (below approximately 9 to 10 solar masses (M☉)) after it has either expelled or fused all the elements for which it has sufficient temperature to fuse. What is left is then a dense sphere of electron-degenerate matter that cools … Meer weergeven A black dwarf is a theoretical stellar remnant, specifically a white dwarf that has cooled sufficiently to no longer emit significant heat or light. Because the time required for a white dwarf to reach this state is … Meer weergeven Once the Sun stops fusing helium in its core and ejects its layers in a planetary nebula in about 8 billion years, it will become a white dwarf and, … Meer weergeven • Degenerate matter – Type of dense exotic matter in physics • Heat death of the universe – Possible fate of the universe Meer weergeven Web6,248 Likes, 70 Comments - Megha Rao (@_megharao) on Instagram: "I wish I had the courage to love you in a way that wasn't humiliating or exhausting. That the po..." WebThey range in luminosity, color, and size – from a tenth to 200 times the Sun’s mass – and live for millions to billions of years. For stargazers. Many main sequence stars can be … camping naturiste aude bord mer