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Stars shine due to nuclear fusion. The visible light produced by our star (the Sun) comprises all the colours of the spectrum as evidenced by a rainbow.
Fusion is the process by which the sun produces energy. In the sun's core, hydrogen atoms fuse together to form helium, releasing large amounts of energy in the form of heat and light in the process. This continuous fusion reaction is what powers the sun and allows it to shine.
True. Heat produced by nuclear fusion in the core of stars causes them to shine brightly and emit light and heat into space.
Stars produce energy by fusing hydrogen into helium through a process called nuclear fusion. This fusion reaction releases a tremendous amount of energy in the form of light and heat, which powers the star and allows it to shine.
Stars shine because they are gigantic burning hot gas spheres that release heat and light. They are so bright because there are atomic reactions inside them, that convert hydrogen into helium. Their temperature can reach 10.000 degrees centigrade.
The critical temperature for nuclear fusion in a star's core is around 10 million degrees Celsius. At this temperature, hydrogen nuclei can overcome their mutual repulsion and fuse to form helium, releasing energy in the process. This energy production is what causes a star to shine.
A protostar becomes a star when nuclear fusion is initiated in its core. This process starts when the temperature and pressure in the core reach a critical point, enabling hydrogen atoms to fuse into helium. Once this fusion reaction begins, the star will start to shine and enter the main sequence phase of its life cycle.
The high temperature of the Sun's core is necessary for nuclear fusion to occur. Fusion reactions at this temperature produce the tremendous amount of energy that allows the Sun to shine and sustain life on Earth.
Stars begin fusing when they reach a critical temperature and pressure in their cores, typically around 10 million degrees Celsius. This condition arises from gravitational collapse, which increases the core's density and temperature. Once these conditions are met, hydrogen nuclei (protons) can overcome their repulsion and collide, leading to nuclear fusion, where they combine to form helium and release vast amounts of energy. This process marks the transition from a protostar to a main-sequence star, enabling it to shine for millions to billions of years.
Fusion.
A protostar is heated up by gravitational forces causing it to contract and increase in temperature. Once the core reaches a high enough temperature and pressure, nuclear fusion reactions begin, releasing energy and making the protostar shine as a star.
fission is the splitting of atoms of uranium or plutionium by the means of neutrons. fusion is the opposite. fusion is the violent combining of atoms through magnatism and heat. our own sun uses fusion to shine.
In a newborn star, the fusion reactions occur primarily in its core, where the temperature and pressure are high enough to trigger nuclear fusion. This process generates the energy that powers the star and allows it to shine bright.
Innumerable stars are there in the space. Our sun is also a star. Almost all stars shine because of fusion of hydrogen nuclei.
Stars shine due to nuclear fusion. The visible light produced by our star (the Sun) comprises all the colours of the spectrum as evidenced by a rainbow.
stars are born from interstellar gas clouds, shine by nuclear fusion and then die
stars are born from interstellar gas clouds, shine by nuclear fusion and then die