WebMar 8, 2024 · A high-mass star converts its hydrogen to helium, helium to carbon, carbon to magnesium, carbon and helium to oxygen, oxygen to sulphur, oxygen and helium to neon, and silicon and helium to nickel. The … WebHowever, in high mass stars, the temperature and pressure in the core can reach high enough values that carbon fusion can begin, and then oxygen fusion can begin, and then even heavier elements—like neon, magnesium, …
Star Definition, Light, Names, & Facts Britannica
WebMay 7, 2015 · Like low-mass stars, high-mass stars are born in nebulae and evolve and live in the Main Sequence. However, their life cycles start to differ after the red giant phase. A massive star will undergo a supernova … WebHigh‐Mass Stars versus Low‐Mass Stars The amount of energy being generated each second at any point in the interior of the star is determined by how much hydrogen is being converted into helium each second per unit mass. This … iot topology
Top 10 Most Massive Stars in the Universe - ThoughtCo
WebHigh‐Mass Stars versus Low‐Mass Stars The amount of energy being generated each second at any point in the interior of the star is determined by how much hydrogen is … WebJan 10, 2024 · Interestingly, the theoretical limit to a star's mass is about 120 solar masses (that is, that's how massive they can become and still remain stable). Yet, there are stars at the top of the following list are … WebMar 17, 2024 · star, any massive self-luminous celestial body of gas that shines by radiation derived from its internal energy sources. Of the tens of billions of trillions of stars composing the observable universe, only a very … on which part of the document is the header