The process in which lighter elements stick together to create heavier elements is known as fusion. This is the process that will be used in the synthesis of a heavier atomic nuclei.
The stellar process in which the fusion of hydrogen produces other elements is called nucleosynthesis. This is a key process in the evolution of stars, where lighter elements such as hydrogen and helium are fused together to form heavier elements like carbon, oxygen, and iron.
Nitrogen originated from the process of nucleosynthesis in stars, where lighter elements combine to form heavier elements through nuclear fusion.
Scientists believe that phosphorus on Earth was created through nucleosynthesis in the core of massive stars, where lighter elements were fused together under high temperatures and pressures. This process enriched the universe with heavier elements, which were then scattered into space through supernova explosions and eventually incorporated into planets like Earth.
Gold was formed on Earth through a process called nucleosynthesis, which happened during the formation of the universe. This process involved the fusion of lighter elements in the cores of stars, leading to the creation of heavier elements like gold. Over time, these elements were scattered throughout the universe and eventually became part of the Earth's composition through processes like asteroid impacts.
This process is known as nuclear fusion, and it is the reaction that powers the sun and other stars. Two lighter atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process.
That process is known as nuclear fusion. In nuclear fusion, lighter elements such as hydrogen combine to form heavier elements, releasing energy in the process. This is the process that powers stars like our sun.
The nuclear process that converts helium and hydrogen into heavier elements is nuclear fusion. In this process, the nuclei of lighter elements combine to form the nuclei of heavier elements, releasing large amounts of energy in the process. This is the process that powers stars like our Sun.
Nuclear fusion, of lighter elements onto heavier elements.
Hydrogen undergoes fusion, not fission. Fusion is the process of combining lighter elements, like hydrogen, to form heavier elements and release energy. Fission, on the other hand, is the process of splitting heavier elements into lighter ones.
Nuclear fusion, of lighter elements onto heavier elements.
Heavier elements are formed through nuclear fusion processes that take place in the core of a star. Hydrogen atoms undergo fusion to form helium, and then this process continues to create heavier elements by fusing helium atoms together. As the star fuses lighter elements, it produces heavier elements through a series of nuclear reactions.
A star forms by the contraction of a large sphere of gases. This contraction causes the nuclear fusion of lighter elements into heavier elements, releasing energy in the process.
That is called "nuclear fusion".
The stellar process in which the fusion of hydrogen produces other elements is called nucleosynthesis. This is a key process in the evolution of stars, where lighter elements such as hydrogen and helium are fused together to form heavier elements like carbon, oxygen, and iron.
Nitrogen originated from the process of nucleosynthesis in stars, where lighter elements combine to form heavier elements through nuclear fusion.
A star is the object that forms from the contraction of a large sphere of gases, leading to nuclear fusion of lighter elements into heavier elements. This process releases energy in the form of light and heat.
Elements heavier than hydrogen are formed through nuclear fusion processes in stars. When lighter elements fuse together in the intense heat and pressure within a star's core, they can form heavier elements. This process continues throughout a star's life until elements up to iron are created. Elements heavier than iron are formed through supernova explosions or in the collisions of neutron stars.