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Research team creates the world’s lightest isotope of magnesium to date

Image representing new isotope magnesium-18. Credit:S. M. Wang / Fudan University and Facility for Rare Isotope Beams

In collaboration with an international team of researchers, Michigan State University (MSU) has helped create the world’s lightest version—or isotope—of magnesium to date.

Forged at the National Superconducting Cyclotron Laboratory at MSU, or NSCL, this isotope is so unstable that it falls apart before scientists can measure it directly. Yet this isotope that isn’t keen on existing can help researchers better understand how the atoms that define our existence are made.

Led by researchers from Peking University in China, the team included scientists from Washington University in St. Louis, MSU, and other institutions.

“One of the big questions I’m interested in is where do the universe’s elements come from,” said Kyle Brown, an assistant professor of chemistry at the Facility for Rare Isotope Beams, or FRIB. Brown was one of the leaders of the new study, published online Dec. 22 by the journal Physical Review Letters.

“How are these elements made? How do these processes happen?” asked Brown.

The new isotope won’t answer those questions by itself, but it can help refine the theories and models scientists develop to account for such mysteries.

Earth is full of natural magnesium, forged long ago in the stars, that has since become a key component of our diets and minerals in the planet’s crust. But this magnesium is stable. Its atomic core, or nucleus, doesn’t fall apart.

The new magnesium isotope, however, is far too unstable to be found in nature. But by using particle accelerators to make increasingly exotic isotopes like this one, scientists can push the limits of models that help explain how all nuclei are built and stay together.

This, in turn, helps predict what happens in extreme cosmic environments that we may never be able to directly mimic on or measure from Earth.

“By testing these models and making them better and better, we can extrapolate out to how things work where we can’t measure them,” Brown said. “We’re measuring the things we can measure to predict the things we can’t.”

NSCL has been helping scientists worldwide further humanity’s understanding of the universe since 1982. FRIB will continue that tradition when experiments begin in 2022. FRIB is a U.S. Department of Energy Office of Science (DOE-SC) user facility, supporting the mission of the DOE-SC Office of Nuclear Physics.

“FRIB is going to measure a lot of things we haven’t been able to measure in the past,” Brown said. “We actually have an approved experiment set to run at FRIB. And we should be able to create another nucleus that hasn’t been made before.”

Heading into that future experiment, Brown has been involved with four different projects that have made new isotopes. That includes the newest, which is known as magnesium-18.

All magnesium atoms have 12 protons inside their nuclei. Previously, the lightest version of magnesium had 7 neutrons, giving it a total of 19 protons and neutrons—hence its designation as magnesium-19.

Image representing new isotope magnesium-18. Credit: S. M. Wang / Fudan University and Facility for Rare Isotope Beams

To make magnesium-18, which is lighter by one neutron, the team started with a stable version of magnesium, magnesium-24. The cyclotron at NSCL accelerated a beam of magnesium-24 nuclei to about half the speed of light and sent that beam barreling into a target, which is a metal foil made from the element beryllium. And that was just the first step.

“That collision gives you a bunch of different isotopes lighter than magnesium-24,” Brown said. “But from that soup, we can select out the isotope we want.”

In this case, that isotope is magnesium-20. This version is unstable, meaning it decays, usually within tenths of a second. So the team is on a clock to get that magnesium-20 to collide with another beryllium target about 30 meters, or 100 feet, away.

“But it’s traveling at half the speed of light,” Brown said. “It gets there pretty quickly.”

It’s that next collision that creates magnesium-18, which has a lifetime somewhere in the ballpark of a sextillionth of a second. That’s such a short time that magnesium-18 doesn’t cloak itself with electrons to become a full-fledged atom before falling apart. It exists only as a naked nucleus.

In fact, it’s such a short time that magnesium-18 never leaves the beryllium target. The new isotope decays inside the target.

This means scientists can’t examine the isotope directly, but they can characterize telltale signs of its decay. Magnesium-18 first ejects two protons from its nucleus to become neon-16, which then ejects two more protons to become oxygen-14. By analyzing the protons and oxygen that do escape the target, the team can deduce properties of magnesium-18.

“This was a team effort. Everyone worked really hard on this project,” Brown said. “It’s pretty exciting. It’s not every day people discover a new isotope.”

That said, scientists are adding new entries every year to the list of known isotopes, which number in the thousands.

“We’re adding drops to a bucket, but they’re important drops,” Brown said. “We can put our names on this one, the whole team can. And I can tell my parents that I helped discover this nucleus that nobody else has seen before.”



More information:
Y. Jin et al, First Observation of the Four-Proton Unbound Nucleus Mg18, Physical Review Letters (2021). DOI: 10.1103/PhysRevLett.127.262502
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Michigan State University

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Research team creates the world’s lightest isotope of magnesium to date (2021, December 23)
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Metal Planet Appears to Be Lightest World Around Another Star Ever Found

The sport of hunting for exoplanets, or planets around other star systems, has a new featherweight champion — a tiny world designated GJ 367 b with about half the mass of the Earth. The lightest exoplanet found to date, GJ 367 b zips around its parent star in a speedy 7.7 days and is unusually dense, appearing to be made of almost pure iron.

Called a “super-Mercury” for its location and composition, the lightweight entity’s existence challenges aspects of planetary formation theories. It could be hinting that miniature worlds come in a much wider diversity than previously believed.

“It’s absolutely great to have found a planet like this,” said Diana Valencia, an astrophysicist at the University of Toronto Scarborough who was not involved in the discovery. “It’s mind-blowing.”

GJ 367 b orbits a cool red star located roughly 31 light years from Earth. Researchers initially spotted it using NASA’s Transiting Exoplanet Survey Satellite (TESS), a space telescope that finds nearby worlds by measuring how much their stellar hosts dim as they move in front of the stars’ faces. Because this eclipse produces a little trough in the light received from a star, astronomers can use it to estimate a planet’s size.

The newly discovered world is around 5,700 miles across, about three-quarters that of our planet. Follow-up observations with the High Accuracy Radial Velocity Planet Searcher (HARPS), an instrument on a telescope at the La Silla Observatory in Chile, allowed researchers to figure out its mass.

The HARPS detector looks for the subtle wobble exoplanets induce on their parent stars, which gets stronger the heavier a planet is.

With its mass and diameter in hand, scientists could calculate GJ 367 b’s density, showing it is an outlier compared to most exoplanets. It is closer in size to Earth or Venus but with a composition more like Mercury, which is mainly iron.

“It’s a weird ball,” said Kristine W.F. Lam, an astronomer at the German Aerospace Center in Berlin and lead author of a paper out Thursday in Science.

Because it sits so close to its parent, one side of GJ 367 b likely always faces the blazing star. Its dayside temperatures should soar toward 2,700 degrees Fahrenheit, hot enough to melt rock and metal, making it a potential lava world, Dr. Lam added.

GJ 367 b offers scientists a way to study how worlds closer to stars form. The leading theory for how a place like Mercury was created is that, early in the solar system’s history, a rocky planet similar to Earth formed near the sun. Colossal space rocks subsequently pummeled this entity, stripping the world of its crust and mantle. This means Mercury is essentially a gigantic planetary core sitting next to the fiery sun.

But the problem with such a scenario is that it doesn’t entirely work, Dr. Valencia said. Collisions may have bashed proto-Mercury’s outer layers away, but the material wouldn’t get very far. Trapped by the sun’s gravity, the rocks and metals would stay in a close in orbit and eventually find their way back to the object’s surface.

It’s possible to invoke special circumstances for why this didn’t happen, but the existence of GJ 367 b and similar objects means such planets aren’t exactly rare, Dr. Valencia said.

“We have to think about how can you reliably, not sporadically, produce a super-Mercury,” she added.

One possibility is that there’s still something missing from models for planetary creation. Perhaps dense elements like iron somehow end up closer to a star during its younger days, Dr. Valencia said. For now, such an idea remains speculative, she added, though worlds like GJ 367 b might start nudging scientists in such a direction.

The team that discovered the petite planet is already planning more observations of the system. They would also like to use a giant telescope to pick up light from GJ 367 b, potentially uncovering whether it has an atmosphere or if its surface truly is molten.

Larger worlds have always been easier to detect than smaller bodies, and researchers have found an array of giant Jupiter-like entities with all manner of composition and orbital characteristics. As improved telescope techniques have opened up exploration at the other end of the size spectrum, odd little objects like GJ 367 b keep turning up.

“It jars you awake to remember that these planets have their own stories,” said Jonathan Fortney, a planetary scientist at the University of California, Santa Cruz, who also was not involved in the study. “It’s yet another way of showing that final planetary outcomes can be tremendously diverse.”

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The carbon-fiber Vaio Z is the world’s lightest laptop with an Intel H-series chip

Vaio is known for making laptops that pack a surprising amount of power into unbelievably thin form factors. The Vaio Z may be the company’s most ambitious product yet. It contains up to Intel’s four-core Core i7-11357H — and at a starting weight of 2.11 pounds, it’ll be the lightest laptop ever to house an Intel H-series processor. (Though models you can buy in the US are 2.32 pounds.)

Part of the reason the Vaio Z is so light is that it’s the first laptop ever to be made of “contoured carbon fiber.” You’ll find carbon fiber in some of the nicest lightweight laptops on the market, including the Dell XPS line — it’s a sturdy and lightweight material. But those laptops utilize sheets of carbon fiber that are held together with metal or plastic parts. Vaio has actually contoured the material around the edges of the Z’s chassis, so it’s carbon fiber all around.

Vaio says the device has passed 26 “surface drop” tests, and will deliver up to 13 and a half hours of battery life. In terms of other specs, you can get up to 2TB of storage, 32GB of memory, Iris Xe integrated graphics, and either an FHD or a 4K 14-inch display. There’s a backlit keyboard, a webcam with a physical shutter, a full-size HDMI port, and two USB-C ports as well. The chassis is a clamshell, though you can fold the screen down to 180 degrees.

Of course, this all doesn’t come cheap. The Vaio Z starts at — I’m not joking — $3,579. So it won’t be a practical purchase for most people, but it’s still an impressive achievement and an interesting proof-of-concept. Keep an eye out for our full review in a few days, where we’ll dive into the performance you can expect for that price. You can preorder units now on Vaio’s website.

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