When the temperature in the core reaches 10 million degrees Kelvin.
Life Cycle of a Star
"Stellar" means of or in relation to stars. As such, "stellar conditions" would be the conditions within a star or relative g to stars (depending on context)
Big Bang nucleosynthesis refers to the formation of light elements, such as hydrogen, helium, and trace amounts of lithium, during the first few minutes after the Big Bang when the universe was hot and dense. Stellar nucleosynthesis occurs within stars during their lifecycles, where nuclear fusion processes create heavier elements like carbon, oxygen, and iron. Supernova nucleosynthesis takes place during the explosive death of massive stars, leading to the creation of even heavier elements, such as gold and uranium, which are dispersed into space when the star explodes. Each process operates under different conditions and timescales, contributing uniquely to the chemical composition of the universe.
Star of three stellar masses, Red giant, Supernova, Neutron Star Hope this helps! :) 5/3/21
Nucleosynthesis occurs during various stages of a star's life, primarily during the main sequence and later during the red giant phase. In the main sequence, hydrogen is fused into helium in the star's core. As stars evolve into red giants, they can undergo further nucleosynthesis processes, such as the fusion of helium into heavier elements like carbon and oxygen. In the final stages of massive stars, nucleosynthesis can lead to the formation of even heavier elements during supernova explosions.
Several types of nucleosynthesis include primordial nucleosynthesis (which occurs within the first few minutes of the universe's existence), stellar nucleosynthesis (which occurs within stars through nuclear fusion processes), and explosive nucleosynthesis (which occurs during events like supernovae or neutron star mergers).
Chemical elements were formed by stellar nucleosynthesis.
Beryllium was not created during the stellar nucleosynthesis.
By stellar nucleosynthesis (excepting H, He and probably Li, Be).
The production of heavy atoms from light atoms inside of a star is called nucleosynthesis. This process involves fusion reactions that combine lighter elements into heavier elements through the intense heat and pressure found in stellar interiors.
10 million kelvin
This process is called stellar nucleosynthesis.
The process is called stellar nucleosynthesis.
As many other chemical elements uranium was formed by stellar nucleosynthesis.
Nucleosynthesis is the process by which atoms are formed in the cores of stars through nuclear reactions. It is responsible for creating elements heavier than helium, like carbon, oxygen, and iron. There are two main types of nucleosynthesis: primordial nucleosynthesis, which occurred in the early universe, and stellar nucleosynthesis, which occurs in the cores of stars.
Stellar nucleosynthesis refers to the process by which elements are formed within stars through nuclear fusion during their lifecycles, primarily converting hydrogen into helium and heavier elements in later stages. In contrast, big bang nucleosynthesis occurred in the first few minutes after the Big Bang, resulting in the formation of the lightest elements, primarily hydrogen, helium, and trace amounts of lithium and beryllium. While stellar nucleosynthesis builds upon the elements formed during the big bang, it occurs under different conditions and leads to the creation of heavier elements over billions of years.
Uranium was not formed on the earth but in the stars by stellar nucleosynthesis.