The heaviest element that can be produced prior to supernova is Iron (Fe).
The first element that is converted in a star's core is hydrogen. Through nuclear fusion, hydrogen atoms fuse together to form helium, releasing energy in the process. This fusion process is what powers a star and allows it to shine.
In the definition, sun is a star because it produces its own light and heat. How does it produce such great energy? It uses hydrogen. Hydrogen is the element which is abundand in the sun in order to produce solar energy.
When elements are combined to produce another element, this process is called nuclear fusion. Nuclear fusion is the process in which two lighter atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. This is the process that powers the sun and other stars.
No. Magnesium is an element. No chemical or biological process can synthesize elements. We get magnesium from food.
The combination of the center of atoms to produce a heavier element is called nuclear fusion.
The most common element in a young star is hydrogen. During the star formation process, vast amounts of hydrogen gas collapse under gravity to form a new star. This hydrogen fuel is what powers nuclear fusion reactions in the star's core, creating energy and sustaining the star's brightness.
A massive star with iron in its core will stop nuclear fusion, leading to its collapse and eventual explosion as a supernova. Iron is the element at which fusion becomes endothermic, meaning energy is no longer released in the process.
By the star's spectrum.
Oxygen is the element that gives us life. It is essential for respiration, which is the process our cells use to produce energy. Without oxygen, our bodies wouldn't be able to function properly.
Nuclear fusion, or the heating-up and smashing together of hydrogen nuclei, is the process via which stars produce energy.
When hydrogen is fused in the suns core Helium is produced.