http://www.astronomy.com/magazine/2024/01/why-does-the-universe-make-so-many-tiny-stars WebLow-mass stars, like the Sun, lose material through modest winds, about 10 −14 M ⊙ yr −1 while in the hydrogen core burning (main sequence) phase. Turbulence and magnetic …
How Are Elements Formed in Stars? Sciencing
http://shakerscience.weebly.com/uploads/2/7/7/0/27700095/hrdiagrampractice_1.doc Web6 mrt. 2016 · In contrast with the Sun, massive stars, much more massive then our Sun about 8 times the mass of our Sun, after they burn all their helium into carbon can also burn that carbon into other heavier elements like Magnesium, Neon and Sodium etc. and just not that they can also burn Magnesium into Oxygen, Oxygen to Silicon and from Silicon to Iron. herts uni apprenticeships
21.2 The H–R Diagram and the Study of Stellar Evolution
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