WebWhen a star gets bigger, its heat spreads out, making its overall temperature cooler. But the core temperature of our red giant Sun increases until it's finally hot enough to fuse the helium created from hydrogen fusion. Eventually, it will transform the helium into carbon and other heavier elements. WebApr 13, 2024 · When a red supergiant has burnt out most of its fuel it resulst in a gravitational collaps, lowering its volume making the star smaller. When it shrinks the temperature get higher resulting in the start of thermonuclear fusion emiting great force and a giant explosion in the form of a supernova. Answer link
How does a red giant become a white dwarf? Socratic
WebA red giant forms after a star has run out of hydrogen fuel for nuclear fusion, and has begun the process of dying. A star maintains its stability through a fine balance between its own … WebRed supergiants quickly collapse, producing a giant explosion called a supernova. High mass red supergiants form neutron stars where the core of the supergiant (about 1.5 … howarth at home derby
Red giant stars: Facts, definition & the future of the sun
WebMay 7, 2015 · Stars larger than eight times the mass of our Sun begin their lives the same way smaller stars do: by fusing hydrogen into helium. However, a large star burns hotter and faster, fusing all the hydrogen in its core to helium in less than 1 billion years. The star then becomes a red supergiant, similar to a red giant, only larger. Unlike red ... WebOct 31, 2024 · How a red giant evolves will be largely dependent upon its mass. For low to medium mass stars, such as our sun, the process of nuclear fusion will generally stop … WebApr 11, 2012 · An artist's impression of the dust surrounding a red giant star. (Image credit: Anna Mayall ) When middleweight stars near the end of their cosmic lives, they shrug off their outer layers ... how many ml goes into a liter