WebMay 7, 2015 · The star has become a red giant. What happens next in the life of a star depends on its initial mass. Whether it was a "massive" star (some 5 or more times the mass of our Sun) or whether it was a "low or medium mass" star (about 0.4 to 3.4 times the mass of our Sun), the next steps after the red giant phase are very, very different. III. The End WebThe star will continue to expand to between 200-800 times the radius of our sun to become a red giant. Stars larger than our sun will increase in size to form a Red Supergiant star. It will expand to about 1500 times the radius of our sun. Both red giants and red supergiants decrease in surface temperature down to around 3500 Kelvin.
Red Giant National Schools
WebNov 17, 2015 · Explanation: Basically a Red Giant is formed when a Star like our Sun burns all of it's hydrogen to helium and then rearranges itself. This process takes about 10 Billion years. After becoming a Red Giant the Sun will become bigger and more denser than it … WebRed supergiants develop from main-sequence stars with masses between about 8 M☉ and 30 or 40 M☉. [10] Higher-mass stars never cool sufficiently to become red supergiants. cheap self catering holidays to tenerife
Formation of a Red Giant Physics Van UIUC
WebOct 15, 2015 · As this outer layer contains a bigger volume than the original core of the Sun, it heats up significantly, releasing far more energy. This increase in light pressure from the core pushes much ... WebApr 1, 2024 · All these stars go through a giant phase, He core burning and asymptotic giant branch phases. Above this then carbon burning will be initiated in the core and it is likely that burning will continue through to iron, followed by core-collapse and a supernova. Share Improve this answer Follow answered Apr 1, 2024 at 16:03 ProfRob 132k 8 309 488 WebPlanetary nebulae seem to mark the transition of a medium mass star from red giant to white dwarf. Stars that are comparable in mass to our Sun will become white dwarfs within 75,000 years of blowing off their envelopes. Eventually they, like our Sun, will cool down, radiating heat into space and fading into black lumps of carbon. cheap self catering tenerife