It's the energy source for all stars (until their fuel is used up - white dwarf stage).
The phase of a star's life cycle where it is using hydrogen as fuel is called the main sequence phase. During this phase, a star converts hydrogen into helium through nuclear fusion in its core to produce energy and maintain its stability.
We are constantly bombarded by cosmic radiation from space, and background radiation from the soil. However, both are background, and we have no biological processes that depend on nuclear reactions to survive.
The two opposing forces are gravity, pulling the star in and the outward force from the ongoing nuclear fusion reactions. As the star approaches the end of it's life, changes in the reactions occur, which cause the forces to balance out in different ways, changing the size of the star.
The main sequence phase represents the longest period of time in a star's life cycle. This is when a star generates energy through nuclear fusion, balancing the forces of gravity pushing in and radiation pushing out. The duration of the main sequence phase varies depending on the star's mass.
We get most of our energy from the Sun; there, the energy is converted by nuclear fusion.On the other hand, technology is not yet ready to carry out nuclear fusion on our own, right here on Earth - except for some experiments.
Because thats the part of its life cycle it is now in.
Nuclear fusion
explain the destination life cycle explain the destination life cycle
Life on Earth gets its energy from the Sun, which produces the energy through nuclear fusion.
from nuclear fusion on the surface of the sun when it went nova, but it was also formed by plant life through the calvin cycle
Stars primarily use hydrogen, helium, and carbon as fuels for nuclear fusion. In the early stages of a star's life, hydrogen is fused into helium through the process of nuclear fusion in the core. As stars evolve, they can fuse helium into carbon and other heavier elements in later stages, depending on their mass and life cycle.
Nuclear fusion. Mainly, converting hydrogen-1 to helium-4.
explain the last stage of the life cycle of a beetle
Scientific evidence suggests that magnesium is formed by stars during nuclear fusion processes in their cores. As stars undergo fusion reactions, elements like helium and carbon fuse together to create magnesium through successive nuclear reactions. These elements are then released into space when the star reaches the end of its life cycle.
The nuclear energy that is most important for life on Earth is the nuclear fusion that powers the sun. This energy is essential for providing heat and light, which support life on our planet. Nuclear fission, used in nuclear power plants, also plays a role in providing electricity for human activities.
1.The sun is a huge ball of nuclear fusion. 2.We here on earth use nuclear fission to produce electricity. so the answer is 2.
Explain the origin of the defect distribution in a typical software development life cycle.?