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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.

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1y ago

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When does helium fusion begin in a star?

Hydrogen undergoes nuclear fusion to form helium at a temperature of 107 K


When will helium fusion begin?

5 min


Name the process that causes a star to begin producing vast amounts of energy?

Nuclear fusion is the process that causes a star to begin producing vast amounts of energy by converting hydrogen into helium through a series of fusion reactions in its core.


At what temperature do star begin the process of nuclear fusion?

Stars begin the process of nuclear fusion when their cores reach temperatures of around 10 million degrees Celsius. At this temperature, hydrogen atoms in the core of the star are able to overcome the electrostatic repulsion between positively charged protons and fuse together to form helium.


When a protostar rises to 10000000 degrees celsius will a protostar become a star before or after nuclear fusion?

A protostar must reach about 10 million degrees Celsius for nuclear fusion to start in its core, triggering the transition into a true star. This marks the point where hydrogen atoms begin fusing into helium, releasing energy in the process. So, a protostar will become a full-fledged star after nuclear fusion begins at this temperature.


How hot must the core of a protostar be to begin nuclear fusion?

The core of a protostar must reach temperatures of at least 10 million degrees Celsius for nuclear fusion to begin. At this temperature, hydrogen atoms can overcome their mutual repulsion and fuse to form helium, releasing energy in the process.


What element is fused in the core of a star?

In the core of a star, hydrogen is primarily fused into helium through the process of nuclear fusion. This fusion releases a tremendous amount of energy, which powers the star and generates heat and light. As the star evolves and exhausts its hydrogen fuel, it may begin fusing heavier elements, such as helium into carbon, in later stages of its lifecycle.


What triggers nuclear fusion stars?

Fusion in stars are usually the result of gravity.Once a mass of hydrogen accumulates enough mass, the gravity of all that mass compresses the core of the star to the point that the hydrogen atoms there begin fusing into helium. The process then cascades outward, and the end result is a star.


How does nuclear fusion occur in the Sun?

At this time hydrogen to helium burning. 1H + 1H --> 2H + e + ~1 MeV 2H + 2H --> 3H + 1H + ~4 MeV 2H + 3H --> 4He + n + ~17 MeV and several other side reactions. When it runs out of hydrogen, the core will begin helium burning. This is much harder to start so it requires much higher pressure and temperature. 3 4He --> 12C But this will not begin for another 6 billion years.


A protostar becomes a star when?

A protostar becomes a star when nuclear fusion begins in its core, converting hydrogen into helium and releasing energy. This process generates enough heat and pressure to balance the force of gravity, causing the protostar to shine brightly as a star.


Which type of fusion occurs in the red giant phase?

The primary type of fusion that occurs in the red giant phase is helium fusion. As the star's core runs out of hydrogen fuel, it contracts and heats up to the point where helium fusion can begin, converting helium into carbon and oxygen. This process generates energy and causes the star to expand and become a red giant.


Inside a prostar the nuclear fusion of hydrogen will begin when?

The core of the protostar reached an extremely high temperature