Bald Cypress tree rings reveal 2,000-year history of climate disruption
The bald cypress tree (Taxodium distichum) has been quietly standing sentinel to centuries of ecological change in the murky wetlands of the American Southeast. These towering trees are some of the oldest living organisms in Eastern North America, their gnarled "knees" that tower above the water as a defining feature.
However, even long-lived specimens such as these are beginning to show the worrying signs of enormous global change. New research has found that while these trees do not die of old age, external stressors such as a changing climate, rising sea levels, pests, and erratic weather drastically shorten their lifespans.
In collaboration with partner institutions, a team of scientists from Florida Atlantic University investigated 95 specimens of ancient bald cypress preserved in subfossil form near the Altamaha River, Georgia. The researchers used radiocarbon dating and tree ring analysis to reconstruct over two millennia's worth of growth patterns of these trees and found how environmental changes impacted the cypress specimens.
"The rings of the bald cypress are like nature's journal entries, written year by year and season by season, showing how even slow changes can shape the course of life," said Katharine G. Napora, the study's senior author.
The team's findings highlight a dramatic shift that began around 500 A.D. Before that point, bald cypress trees in the region regularly lived for more than 470 years. But after this period, their average lifespan fell sharply to 186 years.
This drop corresponds with the beginning of a sixth-century climatic disruption known as the Vandal Minimum, which marked the start of a worldwide cooling period believed to be the result of extreme volcanic activity combined with the possible impact of a comet.
"This shift wasn't a brief disruption. Even centuries later, the trees never regained their former longevity. Their lifespans continued to decline over time," said Napora.
"The last of the long-lived trees in the deposit died during another major climatic event, the Little Ice Age. Our findings underscore how long-lasting the localized effects of major climate shifts can be, especially for coastal forests that are already vulnerable to wind damage, saltwater intrusion, and rising seas."
Researchers found no evidence that human activities such as fire or logging contributed to the trees' demise. Dry spells may have encouraged the spread of mites and other pests, further stressing these trees.
"These ancient giants not only inspire awe but also serve as natural archives, helping scientists understand how trees have weathered past climate events – and how they might fare in the face of modern climate change," said Napora.
Despite the grim trend, hope endures. Isolated pockets of old-growth swamps still shelter bald cypress trees up to 2,600 years old.
"In their quiet persistence, these trees offer both a warning and a lesson: that the world is more interconnected than we often realize, and that the story of the Earth isn't only told through written history – it's etched into wood, embedded in landscapes and carried forward by living organisms," said Napora.
"The past lives on in the trunks of these ancient trees, reminding us that environmental shifts – whether natural or human-caused – reverberate through time in ways we are only beginning to understand," she concluded.
The study has been published in the Proceedings of the National Academy of Sciences.
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WIRED
37 minutes ago
- WIRED
The Mysterious Inner Workings of Io, Jupiter's Volcanic Moon
Jun 15, 2025 7:00 AM Recent flybys of the fiery world refute a leading theory of its inner structure—and reveal how little is understood about geologically active moons. Photograph: NASA/JPL-Caltech/SwRI/ASI/INAF/JIRAM The original version of this story appeared in Quanta Magazine. Scott Bolton's first encounter with Io took place in the summer of 1980, right after he graduated from college and started a job at NASA. The Voyager 1 spacecraft had flown past this moon of Jupiter, catching the first glimpse of active volcanism on a world other than Earth. Umbrella-shaped outbursts of magmatic matter rocketed into space from all over Io's surface. 'They looked amazingly beautiful,' said Bolton, who is now based at the Southwest Research Institute in Texas. 'It was like an artist drew it. I was amazed at how exotic it looked compared to our moon.' Scientists like Bolton have been trying to understand Io's exuberant volcanism ever since. A leading theory has been that just below the moon's crust hides a global magma ocean, a vast contiguous cache of liquid rock. This theory dovetails neatly with several observations, including ones showing a roughly uniform distribution of Io's volcanoes, which seem to be tapping the same omnipresent, hellish source of melt. But now, it appears that Io's hell has vanished—or rather, it was never there to begin with. During recent flybys of the volcanic moon by NASA's Juno spacecraft, scientists measured Io's gravitational effect on Juno, using the spacecraft's tiniest wobbles to determine the moon's mass distribution and therefore its internal structure. The scientists reported in Nature that nothing significant is sloshing about just beneath Io's crust. 'There is no shallow ocean,' said Bolton, who leads the Juno mission. Independent scientists can find no fault with the study. 'The results and the work are totally solid and pretty convincing,' said Katherine de Kleer, a planetary scientist at the California Institute of Technology. The data has reopened a mystery that spills over into other rocky worlds. Io's volcanism is powered by a gravity-driven mechanism called tidal heating, which melts the rock into magma that erupts from the surface. Whereas Io is the poster child for this mechanism, tidal heating also heats many other worlds, including Io's neighbor, the icy moon Europa, where the heat is thought to sustain a subterranean saltwater ocean. NASA launched the $5 billion Clipper spacecraft to search Europa's sky for signs of life in the proposed underground ocean. A map of Io's surface, created with images from the Voyager 1 and Galileo missions, shows the wide distribution of the moon's volcanoes. The large red ring is sulfurous fallout from the plume of the Pele volcano. Photograph: US Geological Survey But if Io doesn't have a magma ocean, what might that mean for Europa? And, scientists now wonder, how does tidal heating even work? Melting Magma Heat drives geology, the rocky foundation upon which everything else, from volcanic activity and atmospheric chemistry to biology, is built. Heat often comes from a planet's formation and the decay of its radioactive elements. But smaller celestial objects like moons have only tiny reserves of such elements and of residual heat, and when those reserves run dry, their geological activity flatlines. Or, at least, it should—but something appears to grant geologic life to small orbs throughout the solar system long after they should have geologically perished. Io is the most flamboyant member of this puzzling club—a burnt-orange, crimson, and tawny Jackson Pollock painting. The discovery of its over-spilling cauldrons of lava is one of the most famous tales in planetary science, as they were predicted to exist before they were discovered. NASA's Voyager 1 probe photographed Io in 1979, revealing the first glimpse of volcanism beyond Earth. In this photo mosaic, a lava plume is seen emanating from Loki Patera, now known to be the moon's largest volcano. Photograph: NASA/JPL/USGS On March 2, 1979, a paper in Science ruminated on Io's strange orbit. Because of the positions and orbits of neighboring moons, Io's orbit is elliptical rather than circular. And when Io is closer to Jupiter, it experiences a stronger gravitational pull from the gas giant than when it is farther away. The study authors figured that Jupiter's gravity must therefore be constantly kneading Io, pulling its surface up and down by up to 100 meters, and, per their calculations, generating a lot of frictional heat within it—a mechanism they described as 'tidal heating.' They conjectured that Io may be the most intensely heated rocky body in the solar system. 'One might speculate that widespread and recurrent surface volcanism would occur,' they wrote. Just three days later, Voyager 1 flew by. An image taken on March 8 documented two gigantic plumes arching above its surface. After ruling out all other causes, NASA scientists concluded that Voyager had seen an alien world's volcanic eruptions. They reported their discovery in Science that June, just three months after the prediction. The planetary science community quickly coalesced around the idea that tidal heating within Io is responsible for the never-ending volcanism on the surface. 'The unknown part that's been an open question of decades is what that means for the interior structure,' said Mike Sori, a planetary geophysicist at Purdue University. Where is that tidal heating focused within Io, and just how much heat and melting is it generating? Courtest of Mark Belan/Quanta Magazine NASA's Galileo spacecraft studied Jupiter and several of its moons around the turn of the millennium. One of its instruments was a magnetometer, and it picked up a peculiar magnetic field emanating from Io. The signal appeared to be coming from an electrically conductive fluid—a lot of fluid, in fact. After years of study, scientists concluded in 2011 that Galileo had detected a global magma ocean just below Io's crust. Whereas Earth's mantle is mostly solid and plasticky, Io's subsurface was thought to be filled with an ocean of liquid rock 50 kilometers thick, or almost five times thicker than the Pacific Ocean at its deepest point. A similar magnetic field was coming from Europa, too—in this case, apparently generated by a vast ocean of salty water. The implications were profound: With a lot of rocky material, tidal heating can make oceans of magma. With plenty of ice, it can create oceans of potentially habitable liquid water. Volcanic Vanishing Act By the time the Juno spacecraft started swinging around Jupiter in 2016, the belief that Io had a magma ocean was widespread. But Bolton and his colleagues wanted to double-check. A sequence of images taken over the course of eight minutes by NASA's New Horizons probe in 2007 shows an eruption by the Tvashtar Paterae volcanic region. The plume in this false-color image rises 330 kilometers from the moon's surface. Video: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute During flybys in December 2023 and February 2024, Juno came within 1,500 kilometers of Io's scorched surface. Although the remarkable images of active volcanoes drew everyone's attention, the goal of these flybys was to find out if a magma ocean truly lay beneath the moon's rocky skin. To investigate, the team used an unlikely tool: Juno's radio transponder, which communicates with Earth, sending and receiving signals. Because of Io's unevenly distributed mass, its gravitational field isn't perfectly symmetrical. That uneven gravitational field subtly alters the motion of Juno as it flies by, causing it to accelerate or decelerate a little. That means Juno's radio transmissions will experience the Doppler effect, where the wavelength shifts slightly in response to Io's uneven gravitational field. By looking at the incredibly small shifts in the transmissions, Bolton's team was able to create a high-fidelity picture of Io's gravitational field and use that to determine its internal structure. 'If there were indeed a global magma ocean, you'd see a lot more distortion as Io orbited around Jupiter and as the tidal forces flexed it and changed its shape,' said Ashley Davies, a volcanologist at NASA's Jet Propulsion Laboratory who wasn't involved with the new study. But Bolton's team did not find this level of distortion. Their conclusion was clear. 'There cannot be a shallow magma ocean fueling the volcanoes,' said study coauthor Ryan Park, a Juno co-investigator at the Jet Propulsion Laboratory. The Cassini-Huygens mission photographed Io against the backdrop of Jupiter in 2001. Photograph: NASA/JPL/University of Arizona So what else might be powering Io's volcanoes? On Earth, discrete reservoirs of magma of different types—from the tarlike viscous matter that powers explosive eruptions to the runnier, honey-esque stuff that gushes out of some volcanoes—are located within the crust at various depths, all created by the interactions of tectonic plates, the moving jigsaw pieces that make up Earth's surface. Io lacks plate tectonics and (perhaps) a diversity of magma types, but its crust may nevertheless be peppered with magma reservoirs. This was one of the original lines of thought until Galileo's data convinced many of the magma ocean theory. The new study doesn't rule out a far deeper magma ocean. But that abyssal cache would have to be filled with magma so iron-rich and dense (because of its great depth) that it would struggle to migrate to the surface and power Io's volcanism. 'And at some depth, it becomes tricky to distinguish between what we would call a deep magma ocean versus a liquid core,' Park said. For some, this raises an irreconcilable problem. Galileo's magnetometer detected signs of a shallow magma ocean, but Juno gravity data has emphatically ruled that out. 'People are not really disputing the magnetometer results, so you have to make that fit with everything else,' said Jani Radebaugh, a planetary geologist at Brigham Young University. Researchers disagree on the best interpretation of the Galileo data. The magnetic signals 'were taken as probably the best evidence for a magma ocean, but really they weren't that strong,' said Francis Nimmo, a planetary scientist at the University of California, Santa Cruz, and a coauthor of the new study. The induction data couldn't distinguish between a partly molten (but still solid) interior and a fully molten magma ocean, he said. Heavy Water Perhaps the main reason scientists study Io is because it teaches us about the fundamentals of tidal heating. Io's tidal heating engine remains impressive—there's clearly a lot of volcano-feeding magma being generated. But if it's not producing a subsurface magma ocean, does that mean tidal heating doesn't generate water oceans, either? Scientists remain confident that it does. Nobody doubts that Saturn's moon Enceladus, which is also tidally heated, contains an underground saltwater ocean; the Cassini spacecraft not only detected signs of its existence but directly sampled some of it erupting out of the moon's South Pole. And although there is some light skepticism about whether Europa has an ocean, most scientists think it does. The smooth, lightly scratched surface of Jupiter's icy moon Europa, photographed by the Juno spacecraft in 2022, shows no sign of what lies beneath: in all likelihood, a vast saltwater ocean. Photograph: NASA/JPL-Caltech/SwRI/MSSS Crucially, unlike Io's odd magnetic field, which seemed to indicate that it concealed an ocean's worth of fluid, Europa's own Galileo-era magnetic signal remains robust. 'It's a pretty clean result at Europa,' said Robert Pappalardo, the Europa mission's project scientist at the Jet Propulsion Laboratory. The icy moon is far enough from Jupiter and the intense plasma-flooded space environment of Io that Europa's own magnetic induction signal 'really sticks out.' But if both moons are tidally heated, why does only Europa have an inner ocean? According to Nimmo, 'there's a fundamental difference between a liquid-water ocean and a magma ocean. The magma wants to escape; the water really doesn't.' Liquid rock is less dense than solid rock, so it wants to rise and erupt quickly; the new study suggests that it doesn't linger at depth long enough inside Io to form a massive, interconnected ocean. But liquid water is, unusually, denser than its solid icy form. 'Liquid water is heavy, so it collects into an ocean,' Sori said. 'I think that's the big-picture message from this paper,' Sori added. Tidal heating might struggle to create magma oceans. But on icy moons, it can easily make watery oceans due to the bizarrely low density of ice. And that suggests life has a multitude of potentially habitable environments throughout the solar system to call home. Hell's Poster Child The revelation that Io is missing its shallow magma ocean underscores just how little is known about tidal heating. 'We've never really understood where in Io's interior the mantle is melting, how that mantle melt is getting to the surface,' de Kleer said. Our own moon shows evidence of primeval tidal heating too. Its oldest crystals formed 4.51 billion years ago from the stream of molten matter that got blasted off Earth by a giant impact event. But a lot of lunar crystals seem to have formed from a second reservoir of molten rock 4.35 billion years ago. Where did that later magma come from? Nimmo and coauthors offered one idea in a paper published in Nature in December: Maybe Earth's moon was like Io. The moon was significantly closer to Earth back then, and the gravitational fields from the Earth and the sun were battling for control. At a certain threshold, when the gravitational influence of both were roughly equal, the moon might have temporarily adopted an elliptical orbit and gotten tidally heated by Earth's gravitational kneading. Its interior might have remelted, causing a surprise secondary flourish of volcanism. But exactly where within the moon's interior its tidal heating was concentrated—and thus, where all that melting was happening—isn't clear. Perhaps if Io can be understood, so too can our moon—as well as several of the other satellites in our solar system with hidden tidal engines. For now, this volcanic orb remains maddeningly inscrutable. 'Io's a complicated beast,' Davies said. 'The more we observe it, the more sophisticated the data and the analyses, the more puzzling it becomes.' Original story reprinted with permission from Quanta Magazine, an editorially independent publication of the Simons Foundation whose mission is to enhance public understanding of science by covering research developments and trends in mathematics and the physical and life sciences.
Washington Post
an hour ago
- Washington Post
Genetic variant tied to doubled dementia risk for older men
A common genetic variant is linked to a doubled dementia risk for older men, a recent analysis in Neurology suggests. The study used data from Aspirin in Reducing Events in the Elderly (ASPREE), which followed elderly patients in the United States and Australia with no history of cardiovascular disease, dementia or cognitive decline between 2010 and 2017.
Yahoo
an hour ago
- Yahoo
The secret to a longer life could be this old-fashioned English breakfast
The best news in a long time is that a breakfast of scrambled eggs and fish — kippers, say, or smoked salmon — combined with a few cups of coffee isn't just a great way to start your day, but is also likely to make you live healthier and longer. So report two separate scientific studies. Israel-Iran clash delivers a fresh shock to investors. History suggests this is the move to make. I'm in my 80s and have 2 kids. How do I choose between them to be my executor? These defense stocks offer the best growth prospects, as the Israel-Iran conflict fuels new interest in the sector 'I'm 68 and my 401(k) has dwindled to $82,000': My husband committed financial infidelity and has $50,000 in credit-card debt. What now? 'He failed in his fiduciary duty': My brother liquidated our mother's 401(k) for her nursing home. He claimed the rest. Eggs — specifically egg yolks — and oily fish like herrings and salmon are rich sources of vitamin D, and new research published in the American Journal of Clinical Nutrition says that this vitamin, in particular, may help slow aging. Meanwhile, other research suggests that drinking up to 2½ regular cups of coffee a day can raise your chances of living longer and staying healthy — physically and mentally — in your senior years. What's not to like? The study on vitamin D, conducted among a population of older Americans by researchers at Mass General Brigham, the University of Massachusetts and the Medical College of Georgia, found that those who took a daily vitamin D supplement of 2,000 IU, or international units, a day — meaning 50 micrograms a day — experienced a significant benefit in a key area of cellular aging known as 'telomere shortening.' Telomeres are the crucial protective caps at the ends of our DNA strands (they are sometimes compared to the plastic caps at the ends of shoelaces), and they are critical to cellular health. They typically shorten as we age and as cells divide. 'We found that vitamin D3 supplementation significantly reduced telomere attrition over a four-[year] period … suggesting that vitamin D3 daily supplementation with or without n-3 FAs might have a role in counteracting telomere erosion or cell senescence,' researchers wrote. (This particular study found no health benefit from another prominent ingredient in oily fish, namely Omega-3 oils — but many others have done so.) Meanwhile, research unveiled at the annual jamboree of the American Society for Nutrition, held in the scientific hot spot of Orlando, Fla., finds that drinking up to 2½ cups of regular caffeinated coffee per day may help you live longer and healthier. Decaffeinated coffee and colas showed no benefits, they added. The researchers did not examine whether a healthy, life-extending coffee also includes, say, one of those extra-large 500-calorie desserts, complete with caramel syrup, sprinkles and whipped cream, which some people pick up every morning (at the drive-thru, so they don't have to walk to the counter). Hmm … what do you think? Some headlines have emphasized that the study found a health benefit only in women, but this is a bit misleading. The researchers didn't reveal a health benefit in men not because they couldn't find one, but because they didn't look. The study only involved following women — nearly 50,000 of them — over several decades. (One caveat is that some of the researchers involved in both studies teach at Harvard — so for about half of the U.S. population, this is probably just 'fake news.') The latest research adds to a growing accumulation of knowledge about what we should do if we want to raise our chances of living longer and healthier lives. Each individual study is open to challenges and queries, because they are always conducted in the real, outside world, where countless unmeasured factors will interfere with the results. You cannot genetically engineer 10,000 identical humans, keep them in a laboratory for 80 years and subject them to laboratory-condition tests over that time. But overall, the real-world results have tended to point in some clear directions. The big picture of how to lead a healthy lifestyle is best summarized by research into so-called blue zones, meaning areas of the world — from Okinawa, Japan to Sardinia, Italy — where scientists have found that people tend to live the longest and the healthiest lives. According to the Blue Zones Institute, based on what scientists and researchers have observed about people living in these areas, there are five key areas to focus on: eating a healthy diet; staying physically active; socializing with friends and family a lot; having some sense of purpose or higher belief; and doing things that lower stress. On the issue of food, the 'Mediterranean diet' tends to get the most scientific support: lots of fish, fruits, vegetables, nuts, legumes and whole grains; only small amounts of meat; and very little processed food or refined carbohydrates. I don't know if fish for breakfast is Mediterranean, or just old school. In Victorian England, breakfast staples in wealthier households included kippers and kedgeree. Kippers, also known back then as 'red herrings,' are smoked herrings. (You can buy them in cans in U.S. supermarkets, often from Canada. The contents can be heated in a microwave in seconds.) Kedgeree, almost unknown on our side of the Atlantic, is a cold dish involving fish, egg, curry powder and rice. Both may be acquired tastes. Personally, as I grew up with them, I find them both exquisite — and vastly superior to any sugared cereal. If these things make a comeback, as 'health foods' no less, it can only be good news. 'It might be another Apple or Microsoft': My wife invested $100K in one stock and it exploded 1,500%. Do we sell? My friend wants me to join in a political protest. I'm worried about my job. Am I a coward if I say no? My husband is in hospice care. Friends say his children are lining up for his money. What can I do? 'I'm not wildly wealthy, but I've done well': I'm 79 and have $3 million in assets. Should I set up 529 plans for my grandkids? My mother-in-law thought the world's richest man needed Apple gift cards. How on Earth could she fall for this scam?
