WebSun 101 2 of 3 The Sun's Energy. Which two complementary forces keep the Sun from blowing itself up? fusion and magnetism; helium and hydrogen; photons and magnetism WebOct 6, 2024 · How much hydrogen is converted to helium each second in the Sun give your answer in KG? The Sun fuses 600 billion kg (that is 600 x 109 kg) of hydrogen every second. Can we convert hydrogen to helium? In the core of the Sun hydrogen is being converted into helium. This is called nuclear fusion. It takes four hydrogen atoms to fuse into each ...

How does the Sun fuse hydrogen into helium? – Wise-Answer

WebNov 13, 2024 · Hydrogen is at the surface, still fusing to helium; a little further down, helium fusing to carbon and oxygen; further down we have silicon until the core, where silicon fuses to iron. This is why the star still exists and doesn’t spontaneously explode the moment the first iron atom pops into existence. The Sun is a main-sequence star, and, as such, generates its energy by nuclear fusion of hydrogen nuclei into helium. In its core, the Sun fuses 620 million metric tons of hydrogen and makes 616 million metric tons of helium each second. The fusion of lighter elements in stars releases energy and the mass that … See more Nuclear fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles (neutrons or protons). The difference in mass between the reactants and … See more The release of energy with the fusion of light elements is due to the interplay of two opposing forces: the nuclear force, a manifestation of the strong interaction, which holds protons … See more A substantial energy barrier of electrostatic forces must be overcome before fusion can occur. At large distances, two naked nuclei repel one another because of the repulsive electrostatic force between their positively charged protons. … See more The key problem in achieving thermonuclear fusion is how to confine the hot plasma. Due to the high temperature, the plasma cannot be in direct contact with any solid material, so it has to be located in a vacuum. Also, high temperatures imply … See more In 1920, Arthur Eddington suggested hydrogen–helium fusion could be the primary source of stellar energy. Quantum tunneling was … See more An important fusion process is the stellar nucleosynthesis that powers stars, including the Sun. In the 20th century, it was recognized that … See more Thermonuclear fusion Thermonuclear fusion is the process of atomic nuclei combining or “fusing” using high temperatures to drive them close enough together for this to become possible. Such temperatures cause the matter to become a See more jiofi forgot username and password

Stellar nucleosynthesis - Wikipedia

WebAnswer (1 of 5): Good question. The power from the Sun is 1362 Watts/m2 at 1 AU distance. 1 AU=149.6 billion meters. That means a sphere or ball with that radius has an area of 4*pi*r^2 = 2.812*10^23 square meters. At 1362 Watts/m2 that’s 3.83*10^26 Watts = the power output of the Sun. Four p... WebJan 23, 2024 · The Sun fuses hydrogen atoms into helium atoms. This is nuclear fusion and it produces incredible energy. ... In about 5.5 billion years the Sun will run out of hydrogen and begin expanding as it ... jiofi image locked