Big Ideas Lab
That periodic table is not just decor. It’s a map... and it's not finished.
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Lawrence Livermore National Laboratory is hiring. If you're passionate about tackling real-world challenges in science, engineering, business, or skilled trades, there's a place for you at the lab. Right now, positions are open for a Senior Guidance, Navigation, and Controls Engineer and a Senior Business Operations Specialist. These are just a few of the more than 100 exciting roles available. At Lawrence Livermore, you'll work on projects that matter, from national security to cutting-edge scientific advancements. Join a team that values innovation, collaboration, and professional growth.
Explore opportunities at llnl.gov/careers, where your next career move could make history. You're standing in your kitchen, and you reach for that little white shaker. The stuff we sprinkle into everything, from pasta water to roasted vegetables to soup... salt.
Are you a saltaholic?
Inside that pinch of salt is a chemistry paradox, hiding in plain sight. Salt is made from sodium, a soft metal so reactive it can catch fire when it touches water.
In its elemental form, sodium will be highly reactive and you will deeply regret licking it.
It's burning my tongue! Salt also contains chlorine, a toxic, greenish-yellow gas that was weaponized in World War I. These elements are hazardous on their own, but bond together to form something safe, stable, and essential.
There's a periodic table that's titled "Can I Lick It?"
Hey, can I lick this?
This transformation, dangerous elements becoming safe compounds, represents fundamental chemistry. But it's elementary compared to what's happening in laboratories today, where scientists are creating elements that don't occur in nature.
These entirely new elements must be built by forcing smaller atoms together. As a result, they are large, unstable, and exist for only fractions of a second before they break apart, leading to extremely rare discoveries.
If you go to Stinson Beach and you want to search for the one perfect grain of sand on the entire beach, there's a lot of grains of sand out there. That's kind of the whole heavy element discovery experience. And maybe that helps blow somebody's mind as to just exactly how difficult that is.
These super-heavy elements challenge our understanding of matter itself and teach us how atoms hold together at the very edge of stability. In those fleeting moments before they vanish, they reveal secrets about the building blocks of the universe. These new elements help scientists explore the forces inside atomic nuclei and expand the boundaries of the periodic table. But how do scientists create these short-lived particles? This is the story of element discovery.
Welcome to the Big Ideas Lab, your exploration inside Lawrence Livermore National Laboratory. Hear untold stories, meet boundary-pushing pioneers, and get unparalleled access inside the gates. From national security challenges to computing revolutions, discover the innovations that are shaping tomorrow today.
Lawrence Livermore National Laboratory is hiring. If you're passionate about tackling real-world challenges in science, engineering, business, or skilled trades, there's a place for you at the lab. Right now, positions are open for a Senior Guidance, Navigation, and Controls Engineer, and a Senior Business Operations Specialist. These are just a few of the more than 100 exciting roles available. At Lawrence Livermore, you'll work on projects that matter, from national security to cutting-edge scientific advancements. Join a team that values innovation, collaboration, and professional growth.
Explore opportunities at llnl.gov/careers, where your next career move could make history.
Remember the periodic table on the wall of your high school science classroom? It's actually not finished. Scientists are still discovering new elements.
They constitute everything that you see in life. Everything that's around you, everything that you breathe, consists of elements.
Roger Henderson is a Senior Radio Chemist at Lawrence Livermore National Lab.
There's a whole array of things that elements do for us in our everyday lives. Carbon, hydrogen, and oxygen, when combined into gasoline, power, internal combustion engine vehicles. Now, the electric vehicles that we use, you're just pumping electrons into the battery so that they can then turn that into kinetic motion. But now, lithium, which is related to sodium, is a major component in typical lithium metal battery elements, like I have in the bottom of my Tesla.
These familiar elements represent part of the periodic table. On that table, every element gets a number. Hydrogen is number one. It has one proton in its nucleus. Carbon is number six. Six protons. Oxygen, eight, with eight protons.
The number is literally a headcount of how many protons are crammed into the center of each atom. Most of the elements we know fall somewhere in the middle. The basic, naturally occurring elements, from hydrogen at number 1 to uranium at 92, form the foundation of chemistry, biology, and everyday materials. But then, there's a gap. Elements 93 through 103 exist, but they're all synthetic, human-made. And once you get past 104, you enter the realm of "superheavy" elements. Atoms with extremely large, unstable nuclei that don't occur naturally.
Superheavy elements live beyond the normal realm of the periodic table that anybody would encounter on a daily basis.
These elements are created in a lab through nuclear reactions. Or, witnessed from far away, in other galaxies. Don Shaughnessy leads the Nuclear and Chemical Sciences Division at Lawrence Livermore National Lab.
When there's stars that explode, and we can catch glimpses in these telescopes, they're seeing evidence of heavy element production in these supernovas.
Every atom is essentially a miniature solar system. But instead of planets orbiting a sun, you have a dense core. The nucleus, packed with particles. The nucleus contains protons, positively charged particles that should, by all rights, explode apart instantly. It's like trying to hold together a bunch of identical magnets. And heavier elements have more magnets. But the nucleus does hold together because of two stabilizing forces.
Neutrons, which dilute the electromagnetic repulsion, and a strong nuclear force, the most powerful force in nature, but only at extremely short distances.
But the cool thing there is that now we're dealing with nuclear theory, which is a description of why elements exist.
Nuclear theory is the scientific framework that explains how atomic nuclei hold together, and why some combinations of protons and neutrons can exist, even briefly, while others immediately disintegrate.
Why don't they just fall apart? Principal components of an atom are neutrons, which are neutrally charged particles, and protons, which are positively charged. Now, the protons, of course, since they have the same charge, they want to repel each other, and so they would rather not be right close to each other. The neutrons help to remediate that effect, then you also have the nuclear strong force that kind of holds everything together.
It's a precise balance of competing forces. As atomic numbers increase, more protons mean greater electromagnetic repulsion. The strong nuclear force remains constant, but the repulsive force grows exponentially. Eventually, no amount of neutrons can maintain stability. Scientists use theoretical models to explain how these atoms stay together, even though their nuclei are packed with many positively charged protons in an extremely small space, where electromagnetic forces are constantly pushing them apart.
The super-heavy elements exist because nuclear theory says, "Yeah, that'll hold together at least for, maybe, a couple of milliseconds before it starts falling apart."
Super-heavy elements are synthetic and born from controlled chaos, smashing atomic nuclei together, hoping they stick, even if only for a moment. The challenge is keeping them together long enough to detect, study, and confirm that the atom ever existed. These nuclei don't want to exist.
Every force in the universe is screaming at them to tear themselves apart. But occasionally, in a moment that defies the most probable outcome, nuclei crash together at exactly the right angle, at exactly the right speed, with exactly the right energy. And for one infinitesimal instant, something new appears in the universe. Something that has never existed before. The question is, can scientists catch it before it disappears forever? Lawrence Livermore National Laboratory is hiring.
If you're passionate about tackling real-world challenges in science, engineering, business, or skilled trades, there's a place for you at the lab. Right now, positions are open for a Senior Guidance, Navigation, and Controls Engineer and a Senior Business Operations Specialist. These are just a few of the more than 100 exciting roles available. At Lawrence Livermore, you'll work on projects that matter, from national security to cutting-edge scientific advancements. Join a team that values innovation, collaboration, and professional growth. Explore opportunities at llnl.gov/careers,
where your next career move could make history.
To make a new element, we actually have to take two existing elements and basically just smash them together so that they combine all of their particles.
And atoms aren't eager to collide.
That is not easy to do because they don't want to do that under normal circumstances. So we have to accelerate them to very high energies and speeds to basically get them to smash together. We don't have a particle accelerator here at Livermore, so we collaborated with the Dubna Laboratory, which is in Russia.
In the late 1980s, Lawrence Livermore partnered with the Joint Institute for Nuclear Research in Dubna, Russia, an international collaboration which lasted for over three decades. While Livermore provided rare and carefully-prepared target materials, Dubna had the particle accelerator to run the experiments. Lawrence Livermore supplied specially-prepared samples of heavy elements, rare, highly radioactive materials that required expert handling and precise manufacturing. But getting it there wasn't easy.
The other challenge, I would say, is getting material there because it has to go on a plane. We don't charter a plane specifically for these things, so it has to go kind of commercial freight. And then you find out that it's up to the pilot of that plane to come out and look at it and decide if they want to take the risk of having that.
Once the material was safely on its way to Russia, a decades-long scientific partnership built on trust, precision, and a shared pursuit of discovery blossomed.
This is the captain speaking. We are on our final approach.
Finally, it made it and the experiment went. It was successful, but there was a chance there that that material would never leave the San Francisco airport. And we used to joke, was it like on one of those luggage things, just spinning around, this drum with all these radioactive tags on it and no one wanted to touch it? But it finally went. Luckily, that material's long-lived enough that the delay didn't really dampen the experiment, but it did dampen the timeline that our Russian colleagues had to do that experiment.
Despite the shipping delays and logistical hurdles, experiments ultimately moved forward.
It was a great partnership for many years where we supplied target material and data analysis, detection equipment. They had the accelerator, and so we would run experiments there where you would then accelerate one atom into a target of a different atom and smash them together.
These experiments demand careful setup, constant tuning, and, most important, patience. Discovering a new element can take months, or often years.
There's a lot of trial and error with these because you have to get the right energy of the beam coming into your target. You can sometimes see weeks without a positive result and you start to doubt, right? Is this the right energy? Are we doing the right thing? And it can be very frustrating. And so really, the one thing that we absolutely have and need for these experiments is patience because you have to just sit and wait and see if you're going to get the result that you think you're going to get.
Once the experiment is up and running, the focus shifts to careful observation, looking for any signal that a superheavy element may have formed.
Once you have everything in place and the accelerator is running, then you're basically just watching the readout from the instrument that is trying to detect the creation of a superheavy element. It might be a bit boring, but on the other hand, when you do get an indication from the instrument that, hey, I just caught something of interest, then it can get pretty exciting.
Even when the scientific experiment works, the new atom is too small and too unstable to observe before it starts to fall apart. Instead, scientists track the particles and energy it releases as it decays, looking for an indication that proves it existed.
And what you're looking for then at the end are just electronic signals of something decaying through radioactive decay that's indicative of that new element.
That decay happens in a predictable pattern. Each new atom, if it forms, sheds particles and energy as it tries to stabilize, leaving a kind of fingerprint.
When we did discovery experiments for element 117, we were looking at an element that hit our detector system and then we watched it literally fall apart by spinning out helium atoms or alpha particles one at a time until finally the system says, I've had enough of this, and then it splits in half, roughly speaking, and then it's all done. But the fission at the end was a couple of hours and it's gone.
Element 117, later named tenocine, was one of the last elements added to the periodic table. Like some other superheavy elements, tenocine was created by fusing a rare isotope of berkelium with a calcium beam in a particle accelerator.
The resulting atom appeared in Livermore's detection system and began to decay, one particle at a time. Those decay steps and the time between each one matched predictions for element 117. And even though the atom of element 117 lasted less than a second, the pattern it left behind confirmed Tennessean's creation. The group did this four other times discovering elements 114 through 118, with element 116 being given the name Livermoreum in recognition of the role the laboratory had in these experiments. But why bother creating new elements if they're so short-lived?
What it is doing is allowing the next generation of people to understand how materials interact with each other and how elements behave and basically how our universe is put together. It's about understanding the universe around us, which sounds very big and kind of out there, but it's real. Trying to understand why are we here? Why do things on Earth look the way they do?
By recreating cosmic processes here on Earth, scientists can better understand the structure of matter, which brings us back to something central to this work: the periodic table.
That periodic table is not just a wall decor in the high school classes. It actually is a map and a guide for us of how elements behave and how they're predicted to behave based on that chart. So it's important we get that chart right and it's important we understand how things work if we're going to continue to push the envelope on materials.
Scientists are chasing something they'll never see or hold.
You've made something that you will never see, touch, or be able to manipulate at all. You're basically looking for an electronic signal that says, "Hey, this thing existed, and it was gone." These things undergo radioactive decay, and every time they do, they emit a signal that we can see in a detector.
Despite how rare, how fragile, how fleeting these discoveries are, scientists keep searching. Even now, at this very moment, there's a race happening. Labs in California, Russia, Germany, and Japan are all hunting for the same prize: elements 119 and 120. Because every new element adds a missing piece to the puzzle of how matter is built and how the universe came to be. One impossible atom at a time.
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Page updated November 1, 2026 · transcript and summary are machine-generated