Tag Archives: nuclear fusion

Nuclear Fusion

The sun Nuclear fusion is the process that creates the massive amount of energy needed to power the sun. In the sun’s core 4 Hydrogen atoms collide to create 1 Helium atom, 2 electrons, 2 neutrinos, and 2 gamma ray photons. The amount of Helium created is less than the overall mass of Hydrogen used […] Continue reading

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The Potential for Nuclear Fusion on Earth

Stars like the Sun have been powering themselves through the use of nuclear fusion for billions of years, and the Sun is expected to be powered for billions more before it runs out of its source of hydrogen fuel through the proton-proton chain. As outlined on my previous blog post, one second of energy created […] Continue reading

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Nuclear Fusion: The Heartbeat of Stars

In order for stars to generate the enormous amounts of energy that they do, a very specific, energy-intensive process is needed: nuclear fusion. It is this process that allows stars to shine brightly for billions of years. But how exactly does nuclear fusion work? In short, in the cores of stars, temperatures reach the millions […] Continue reading

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Combining Forces: Nuclear Fusion in the Solar System

Business Insider Ignition Image Shown above is from the National Ignition Facility, where scientists successfully produced (and reproduced) a nuclear fusion reaction that had more energy output than input. The underlying math behind this lies in E=mc2, which shows that Mass (m) can be converted into a large amount of energy at the sacrifice of […] Continue reading

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Blog 3- The Sun and its Core!

As I was growing up, I never truly understood what the sun exactly was. I had understood that it emitted light and eventually I learned that it was basically a big ball of really really REALLY hot gasses. However I never understood the intricacies behind the Sun’s structure. The most interesting part of the sun’s […] Continue reading

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Blog 3: Our Sun and Nuclear Fusion

The sun releases energy through a remarkable process known as nuclear fusion, which unfolds under the extreme temperatures and densities found deep within its core. Unlike the nuclear fission reactions used on Earth, which split atomic nuclei to release energy, the sun’s energy is generated by combining smaller nuclei into larger, heavier ones. This fusion […] Continue reading

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Keeping Stars Alive

How exactly do stars live? Above is an image of the sun given by SOHO, which is an extraordinarily massive object, which due to that possesses a very large gravitational pull, not just on others but also on itself. Everything that has mass possesses this trait, however these bodies are either two light, or are […] Continue reading

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Blog 3 – Nuclear Fusion

Nuclear fusion is the process of combining, or fusing, two or more small nuclei into a larger one, creating energy as a byproduct. Stars like the Sun constantly emit energy through nuclear fusion because their cores are filled with high-speed, hot plasma. More specifically, the Sun’s extremely hot core of 15 million K allows for […] Continue reading

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Nuclear Fusion: The energy of the universe… but not the energy of the Earth?

Nuclear fusion is the fundamental source of energy generation in our universe. Stars (like our Sun) undergo nuclear fusion in their cores and emit energy in the form of heat and light. This stellar energy stands in the way of a dark, cold, lifeless universe, and provides the necessary ingredients for life on Earth. Sadly, […] Continue reading

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blog post 03

Nuclear fusion reactions power stars. In nuclear fusion, 2 atoms’ nuclei merge and form a heavier single nucleus. The leftover mass becomes energy. In stars like the Sun, this is generally the transformation of Hydrogen to Helium (proton-proton chain). Other, more massive stars, use the CNO cycle (uses more elements) to accomplish energy transformation. The […] Continue reading

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