Nuclear Fusion: How California Scientists Are Revolutionizing Energy

(Image Credit: Forbes)

Technician inspects equipment at Lawrence Livermore National Laboratory, CA

(Image Credit: Washington Post)

Nuclear fusion reactor at JET Laboratory, UK

(Image Credit: BBC News)

November 29, 2023

Lily Sharkey

11th Grade

Dominican Academy


December 5, 2022, was the first time in history that nuclear fusion reached ignition- that is, nuclear fusion produced more energy than was put into it. On July 30, 2022, California scientists at the National Ignition Facility (NIF) reached ignition for the second time. If it can be successfully and continuously repeated, nuclear fusion can be the next clean and cheap energy source. However, nuclear fusion is still in its preliminary phase, and much more experimentation is required before it can become the next green power source. Thus, it is unclear if nuclear fusion will have an impact on current climate issues by the time it will be available commercially. 


Most nuclear power plants in the country utilize nuclear fission, which splits the nucleus of the atom. While fission creates great amounts of energy with little greenhouse effect, it does produce dangerous radiation waste byproducts that exist for a very long time. In contrast, fusion occurs when two nuclei combine, releasing energy; it produces less dangerous byproducts that decay faster. However, it requires great amounts of energy to combine nuclei, and the energy produced is usually less than the energy put in. The recent struggle with fusion was for it to reach ignition (scientific energy breakeven), or produce more energy than was put in.

When ignition was reached for the first time in December 2022, 2.05 megajoules were delivered to the nuclei via 192 lasers, which then produced 3.15 megajoules of energy. With 192 lasers aimed at a target smaller than a pea, it is comparable to throwing a perfect strike from a pitcher’s mound 350 miles away. When the experiment was recreated in July 2022, the amount of energy was even higher. Nuclear fusion is responsible for giving energy to the sun and other stars. As Omar Hurricane, chief scientist for the inertial confinement fusion program at Lawrence Livermore National Laboratory (LLNL) at NIF, says, “We’re basically making stars on Earth” (Osborne).

Laser setup at National Ignition Facility at Lawrence Livermore Laboratory, CA

(Image Credit: Smithsonian Magazine)

LLNL has for a long time been a pioneering center for nuclear fusion research. As early as the 1960s, scientists at LLNL proposed that nuclear fusion could be achieved in a laboratory- setting using lasers. Physicist and LLNL director from 1988-1994 John Nuckolls was a prominent figure in this early journey and kickstarted 60 years of research and development that would eventually lead to successful nuclear fusion at the lab today. Along this journey, scientists also created NIF, the world’s biggest and most powerful laser.

(Image Credit: Energy.gov)

Nuclear fusion is able to produce energy because the mass of the combined nuclei is smaller than that of the two individual nuclei; the leftover mass is converted into energy. This can be explained through Einstein’s equation E=mc2, which states that mass and energy can be converted into each other. Researchers are focused on a deuterium-tritium (DT) fusion reaction, which produces a neutron and a helium nucleus and releases substantial amounts of energy (compared to other reactions). These reactions also happen at lower temperatures than other reactions, which makes them easier to achieve.

Nuclear fusion reactions require so much energy because they take place between two atoms of the same element (usually hydrogen) that have the same positive charge; like charges repel each other, thus it is difficult to make them react. Fusion can occur easily on the sun because the surface of the sun has a temperature of around 100 million degrees Celsius and 100 billion times the pressure of Earth. As a result, it is difficult to maintain the high temperature and pressure for a significant amount of time to create enough energy. In contrast, the ignition achieved at LLNL in December 2022 produced enough energy to power 15-20 kettles.

(Image Credit: BBC News)

Although nuclear fusion idealistically can alter climate change and greenhouse emissions, many steps must be taken before that can be achieved. Nuclear fusion must be sustained for substantial periods of time to create enough energy. There is also the topic of how to deliver energy to homes- America’s power grid is too outdated for a single station to power the country, so smaller plants must be built. Only if significant breakthroughs are made, then it may it be possible to achieve net-zero emissions by 2050.

Reference Sources

“DOE Explains...Nuclear Fusion Reactions.” Energy.gov, 2022, 

https://www.energy.gov/science/doe-explainsnuclear-fusion-reactions#:~:text=Nuclear%20Fusion%20reactions%20power%20the,of%20the%20two%20original%20nuclei. Accessed 14 Oct. 2023.

“DOE National Laboratory Makes History by Achieving Fusion Ignition.” Energy.gov, 2022, 

https://www.energy.gov/articles/doe-national-laboratory-makes-history-achieving-fusion-ignition. Accessed 14 Oct. 2023.

“Five Things to Know about Nuclear Fusion and If It Can Power Your Home.” Washington Post, The Washington Post, 2022,

https://www.washingtonpost.com/technology/interactive/2022/nuclear-fusion-power-source-challenges/. Accessed 14 Oct. 2023.

Osborne, Margaret. “Scientists Repeat Nuclear Fusion Breakthrough in a Step toward More Clean Energy.” Smithsonian Magazine

Smithsonian Magazine, 9 Aug. 2023, 


https://www.smithsonianmag.com/smart-news/scientists-repeat-nuclear-fusion-breakthrough-in-a-step-toward-more-clean-energy-180982683/. Accessed 14 Oct. 2023.


Stallard, Esme. “Nuclear Fusion Breakthrough – What Is It and How Does It Work?” BBC News, BBC News, 13 Dec. 2022,


https://www.bbc.com/news/science-environment-63957085. Accessed 14 Oct. 2023.