Not nuclear, it takes an extremely hight temperature for Fusion to occur with in the sun or any other star. ADDED: Yes "nuclear". Fusion is one of the two type of nuclear reaction, the other being Fission.
Nuclear fusion in the sun requires extremely high temperatures, typically around 15 million degrees Celsius (27 million degrees Fahrenheit). At these temperatures, hydrogen nuclei have enough kinetic energy to overcome their electrostatic repulsion and collide to form helium, releasing vast amounts of energy in the process. This energy is what powers the sun and provides light and heat to our solar system.
Energy is released inside the sun through a process called nuclear fusion, where hydrogen atoms are fused together to form helium. This fusion process releases a tremendous amount of energy in the form of light and heat. The sun's immense gravitational pressure and temperature create the conditions necessary for nuclear fusion to occur.
The temperature of a protostar increases due to gravitational contraction. As the protostar contracts, potential energy is converted into kinetic energy, causing the particles to move faster and collide more frequently, resulting in an increase in temperature. This process eventually leads to the ignition of nuclear fusion and the star's main sequence phase.
Inside the sun, nuclear fusion reactions occur where hydrogen atoms combine to form helium, releasing vast amounts of energy in the process. This energy, in the form of heat and light, creates the intense pressure and temperature required to sustain these fusion reactions and keep the sun shining.
The core of the protostar reached an extremely high temperature
Temperature sensors are installed in nuclear reactors as part of the design. An array of thermocouple-based sensors is not uncommon.
Not nuclear, it takes an extremely hight temperature for Fusion to occur with in the sun or any other star. ADDED: Yes "nuclear". Fusion is one of the two type of nuclear reaction, the other being Fission.
of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH of course it has an inside were else would they keep the nuclear bombs BIATCH
Fusion takes place in the core, where the temperature and pressure are much higher, which is necessary for fusion.
Nuclear energy is the term for energy that comes from inside the nucleus of an atom. This energy can be released through processes such as nuclear fission or nuclear fusion.
i use nuclear family in a sentence like this i have a nuclear family inside me.
Nuclear reactors use controlled nuclear fission reactions to generate heat, which is then used to produce steam that drives turbines to generate electricity. The heat is produced in the reactor core where nuclear fuel rods containing uranium or plutonium undergo fission reactions. The reactor's cooling system helps regulate the temperature and prevent overheating.
Nuclear bombs, nuclear power plants, the sun.
Enclosing the nuclear reactor at low temperature helps to prevent overheating by removing excess heat produced during the nuclear fission process. This cooling system is crucial to ensure the reactor operates at a safe and stable temperature to prevent a meltdown or other catastrophic failures. It also helps regulate the reactor's power output and maintain operational efficiency.
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Inside a star, the force of gravity is balanced by the pressure generated from nuclear fusion reactions occurring in the star's core. These nuclear reactions create an outward pressure that counteracts the force of gravity trying to collapse the star. This delicate balance between gravity and pressure determines the size, temperature, and lifespan of a star.