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Isotopes of hydrogen

physical science Maturity 11-13

Hydrogen is a tiny part of our world.

H-1 atom.png
H-1 atom.png
It can be very light. Some kinds are a bit heavier. These help us make power. They are all very small.
H-2 atom.png
H-2 atom.png
Can you find hydrogen in water?

39 words

Hydrogen is a tiny part of our world.

H-1 atom.png
H-1 atom.png
Most hydrogen is very light. It has no extra pieces in its middle.
H-2 atom.png
H-2 atom.png
Some hydrogen is a bit heavier. It has one extra piece inside. This makes heavy water.
H-3 atom.png
H-3 atom.png
Another kind is even heavier. It can turn into helium. This kind is not stable. It can be used in lights. Hydrogen is full of surprises.

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Hydrogen is a very special element. It has three kinds of isotopes. Isotopes are versions of an element with different weights.

H-1 atom.png
H-1 atom.png

The most common kind is called protium. It has one proton in its center. It has no neutrons. Most hydrogen on Earth is protium.

H-2 atom.png
H-2 atom.png

The next kind is called deuterium. It has one proton and one neutron. Scientists call this a deuteron. Water with much deuterium is called heavy water. It can help cool nuclear reactors.

H-3 atom.png
H-3 atom.png

The third kind is called tritium. It has one proton and two neutrons. This kind is radioactive. That means it can break apart over time. It can turn into helium-3. Tritium can be used in special lights.

There are even heavier kinds of hydrogen. Scientists make these in labs. They do not last long. Some of them last for less than a zeptosecond. A zeptosecond is a tiny bit of time. These heavy kinds fall apart very fast.

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Hydrogen is a very special element. It has different versions called isotopes. These isotopes have different weights.

H-1 atom.png
H-1 atom.png
Most hydrogen is a type called protium. It is very common. It makes up more than 99.98% of all hydrogen. Protium has only one proton in its center. It is the only stable version with no neutrons.
H-2 atom.png
H-2 atom.png
Some scientists think protons might decay. This would happen over a huge amount of time. As of 2018, experiments show the proton lasts a very long time. This makes protium stable for us to use.

Other isotopes have more parts in their centers. Deuterium is the second kind. It has one proton and one neutron. Scientists call this center a deuteron.

H-2 atom.png
H-2 atom.png
Tritium is the third kind. It has one proton and two neutrons. This center is called a triton. Tritium is radioactive. This means it breaks apart over time. It turns into helium-3. This happens in about 12.3 years.
H-3 atom.png
H-3 atom.png
Scientists can make tritium in a nuclear reactor. They do this by hitting lithium with neutrons.

People have studied these isotopes for a long time. We learned about deuterium in 1932. We learned about tritium in 1934.

H-3 atom.png
H-3 atom.png
Scientists also make much heavier versions in labs. These are called synthetic isotopes. They do not stay together for long. Some last for less than one zeptosecond. A zeptosecond is a tiny, tiny bit of time. In 2003, scientists made hydrogen-7. A group from Russia, Japan, and France did this. They used a special machine called a cyclotron.
H-1 atom.png
H-1 atom.png

There are many important facts about these atoms. Deuterium is found in seawater. Seawater can have about 150 parts per million of it. This is much more than in the early Solar System.

H-2 atom.png
H-2 atom.png
Heavy water is water with lots of deuterium. It can be used to cool nuclear reactors. It can also be used as fuel for fusion. Tritium is used in self-powered lights. It is also used in fusion bombs.
H-3 atom.png
H-3 atom.png
Scientists use these isotopes as labels in experiments. They help track how things move and change.

You can see how these isotopes connect to our world. Most of the hydrogen in your body is protium.

H-1 atom.png
H-1 atom.png
But the heavy ones help us understand space and energy. For example, deuterium and tritium can fuse together. This happens at very high temperatures. When they collide, they give off energy. This is the same idea as nuclear fusion.
H-3 atom.png
H-3 atom.png
Learning about these tiny parts helps us learn about the stars. It also helps us make new technology for Earth.

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Hydrogen is a unique element because it has several different versions called isotopes. Isotopes are atoms of the same element that have different numbers of neutrons in their nuclei. This means they have different masses even though they are all hydrogen. Hydrogen is the only element where the isotopes have special names that people still use today. These include protium, deuterium, and tritium. Understanding these variations helps scientists study everything from the birth of the universe to nuclear energy.

Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg
Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg

To understand how these work, we must look at the nucleus of the atom. The nucleus is the center of the atom and contains protons and neutrons. Protium, or hydrogen-1, is the most common form. It has only one proton and no neutrons.

H-1 atom.png
H-1 atom.png
Because it has no neutrons, it is the only stable nuclide in existence without them. Deuterium, or hydrogen-2, adds one neutron to the mix. Its nucleus is called a deuteron.
H-2 atom.png
H-2 atom.png
Tritium, or hydrogen-3, contains two neutrons. This nucleus is called a triton.
H-3 atom.png
H-3 atom.png
As you add more neutrons, the atoms become heavier and often more unstable.

There are three naturally occurring isotopes that stay around for a long time. Protium is extremely common, making up more than 99.98% of all hydrogen. It is considered stable because the proton has never been observed to decay. Deuterium is also stable and is found in the environment. Tritium is different because it is radioactive. It undergoes beta decay, which means it breaks down into helium-3. This process has a half-life of about 12.3 years. Scientists can find trace amounts of tritium from cosmic rays or nuclear power plants.

H-3 atom.png
H-3 atom.png

Beyond the natural isotopes, scientists create synthetic isotopes in laboratories. These heavy isotopes are highly unstable and disappear very quickly. For example, hydrogen-4 is made by hitting tritium with fast-moving deuterons. It decays by emitting a neutron. Hydrogen-5 is even more unstable. It has the shortest half-life of any known nuclide at only $10^{-22}$ seconds. Researchers also created hydrogen-6 in 2025 using an electron beam. Finally, hydrogen-7 was synthesized in 2003 by a team from Russia, Japan, and France. They used a machine called a cyclotron to donate neutrons to a hydrogen nucleus.

Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg
Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg

History shows how our knowledge of these atoms grew through discovery. Scientists identified deuterium in 1932 and tritium in 1934. These discoveries changed how we understand nuclear physics. We also learned about the concentration of these atoms in space. Deuterium was produced during Big Bang nucleosynthesis. On Earth, deuterium levels vary. It makes up about 26 to 184 parts per million of hydrogen on our planet. In seawater, the concentration is often around 150 parts per million. This is much higher than the 27 parts per million found in the early Solar System.

H-2 atom.png
H-2 atom.png

These isotopes have many important uses in technology and science. Water that is rich in deuterium is called heavy water. Heavy water is used as a coolant and a neutron moderator in nuclear reactors. Deuterium is also a possible fuel for commercial nuclear fusion. Tritium has its own special roles. It is used in self-powered lighting devices and fusion bombs. Scientists also use both deuterium and tritium as tracers. These tracers act like tiny labels to help track chemical and biological processes.

H-3 atom.png
H-3 atom.png

Hydrogen isotopes connect to the largest and smallest systems in the universe. The way deuterium is distributed helps us understand how the Solar System evolved. For instance, heat from the Sun over billions of years changed how much deuterium stayed in different places. In the stars, isotopes play a role in energy production. When deuterium and tritium nuclei collide at high temperatures, they undergo fusion. This process releases massive amounts of energy through the loss of mass. This connection between tiny atoms and giant stars is one of the most important ideas in science.

Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg
Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg

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🖼️ Images & Media (4)
File:Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg
Hydrogen Deuterium Tritium Nuclei Schmatic-en.svg
File:H-1 atom.png
H-1 atom.png
File:H-2 atom.png
H-2 atom.png
File:H-3 atom.png
H-3 atom.png
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