I think you meant hydrogen o and i don't know why it isn't next to hydrogen.
The next nuclear fusion cycle after helium fusion in a massive star is carbon fusion. This process involves fusing helium nuclei to form carbon. Carbon fusion typically occurs in the core of a massive star after helium fusion is completed.
Over the next few years, the amount of helium in the sun will gradually increase as hydrogen fuses into helium in its core through nuclear fusion. This process is part of the sun's natural life cycle and will continue until a significant portion of the hydrogen fuel is depleted.
it's an up arrow and down arrow next to each other, beneath that it says 1s2.
No, the first element on the Periodic Table is Hydrogen, but because of its unusual behaviour it is usually placed by itself, not next to any other elements. The second element is Helium.
Thousands of asteroids are being observed; some may come quite close to Earth within the next few hundred years. Right now, no specific date is known, for a specific asteroid to hit Earth.Thousands of asteroids are being observed; some may come quite close to Earth within the next few hundred years. Right now, no specific date is known, for a specific asteroid to hit Earth.Thousands of asteroids are being observed; some may come quite close to Earth within the next few hundred years. Right now, no specific date is known, for a specific asteroid to hit Earth.Thousands of asteroids are being observed; some may come quite close to Earth within the next few hundred years. Right now, no specific date is known, for a specific asteroid to hit Earth.
True because it is right next to neon
adjacent, neighbouring
The next nuclear fusion cycle after helium fusion in a massive star is carbon fusion. This process involves fusing helium nuclei to form carbon. Carbon fusion typically occurs in the core of a massive star after helium fusion is completed.
most stars are made of mainly hydrogen, a little helium and traces of other gases like oxygen
The amount of hydrogen will decrease and the amount of helium will increase.
The amount of hydrogen will decrease and the amount of helium will increase.
The amount of hydrogen will decrease and the amount of helium will increase.
Over the next few years, the amount of helium in the sun will gradually increase as hydrogen fuses into helium in its core through nuclear fusion. This process is part of the sun's natural life cycle and will continue until a significant portion of the hydrogen fuel is depleted.
Hit next frame (right arrow) instead of insert frame which places a frame before the current frame you are working on
Over the next few billion years, the hydrogen content in the sun will decrease as it fuses into helium through nuclear fusion. This process will cause the relative amount of helium to increase in the sun over time.
Right now, hydrogen is fusing into hydrogen. As the hydrogen gets used up, helium will begin fusing into the next heavier element. When the helium is about used up, the next heavier element will begin fusing into the next . . . . well, keep on going until you get iron as the result of fusing. The Sun has not enough pressure and heat to fuse iron into anything heavier, and the Sun will blossom out into a red giant. Of course, this is billions of years from now . . .
Huge releases of energy.