Hydrogen atoms are fusing into helium atoms in the Sun's core through the process of nuclear fusion. This fusion reaction releases a tremendous amount of energy that powers the Sun and produces light and heat.
In the Sun, hydrogen nuclei are fused together to form helium in a process called nuclear fusion. This fusion process releases a large amount of energy in the form of light and heat, which powers the Sun and sustains its brightness.
The sun constantly splits billions of hydrogen atoms giving off radiation and heat.answ2. the temperature and pressure in the interior of the Sun have sufficient energy to promote the reaction of two H atoms combining to make one He atom, and with the emission of a lot of heat energy.
The innermost and hottest part of the sun is called the core. It is where nuclear reactions occur, producing immense heat and energy through the fusion of hydrogen atoms into helium.
It is all natural gas that the sun produces itself.
The sun is just a huge ball of hydrogen and helium. The heat created on the sun is from billions of hydrogen atoms smelting together to helium atoms. All these atoms are held together by the gravity.
The Sun's energy comes from its great force of gravity smashing together the hydrogen atoms in the Sun's core. This is a process known as nuclear fusion.
they were discovered when the sun was made. when atoms fuse together in the sun that creates solar flares and more gas in the sun
When hydrogen atoms fuse together in the sun's core, they create helium. This process releases energy in the form of light and heat, which provides the sun's power.
No, the sun generates energy through nuclear fusion in its core, not through electrical energy. This process involves the fusion of hydrogen nuclei to form helium, releasing vast amounts of energy in the form of light and heat.
When hydrogen atoms fuse together inside the sun, they form helium atoms through a process called nuclear fusion. This fusion process releases a tremendous amount of energy in the form of light and heat, which is what powers the sun and sustains life on Earth.
Our Sun, as with all main-sequence stars, is heated by the energy of fusing hydrogen atom to make helium atoms. The gigantic gravity of a main-sequence star causes hydrogen atoms to be smashed together, or 'fused'. The huge heat that results keeps the Sun puffed up to its huge size. In another 4.5 billion years, more or less, the hydrogen will be largely used up, and the Sun will shrink to a point that helium atoms are smashed together, creating lithium atoms. When all the lithium atoms have been largely smashed together and used up, the Sun will shrink again, and beryllium atoms will result.
The sun gets its energy from the process of fusion, where hydrogen atoms are fused together in the high temperatures and pressures of the Sun's core to produce helium atoms and release energy in the form of gamma rays..
Hydrogen atoms are fusing into helium atoms in the Sun's core through the process of nuclear fusion. This fusion reaction releases a tremendous amount of energy that powers the Sun and produces light and heat.
In the core of the sun, hydrogen atoms are fused together to form helium atoms in a process called nuclear fusion. This fusion reaction releases a tremendous amount of energy in the form of light and heat, powering the sun and providing energy for life on Earth.
The sun, during Summer, becomes hotter due to an elevated frequency in the nuclear reactions produced in the sun and the opposite occurs during Winter. This is all due to the proximity of the planets in relation to the sun as the gravitational pull of the planets act to exacerbate the gravitational pull of the planets, causing the sun to effectively have two different gravitational pulls combining. this is what causes the increased or decreased frequency of hydrogen atoms effectively smashing together and therefore the sun becomes hotter or colder, causing the seasons on earth to change.
Most main sequence stars, including sun, produce heat and light by smashing atoms together to create explosions. Eventually, when the atoms continue to combine, they become too big to combine, and the star dies out. Then, it kind of implodes, and the friction of it becoming too dense makes it expand greatly past its original size, only temporarily. Shortly after, it finally explodes.