How special is the Milky Way Galaxy?  

How special is the Milky Way Galaxy?


September 25, 2024

Above: A mosaic of the satellite galaxies across the Milky Way-like systems that the SAGA team has surveyed. The images are sorted by their luminosity from left to right. Credit: Yao-Yuan Mao (Utah), with images from the DESI Legacy Surveys Sky Viewer

A 'saga' about 101 galaxies like the Milky Way and their companions

Is our home galaxy, the Milky Way Galaxy, a special place? A team of scientists started a journey to answer this question more than a decade ago. Commenced in 2013, the Satellites Around Galactic Analogs (SAGA) Survey studies galaxy systems like the Milky Way. Now, the SAGA Survey just published three new research articles that provide us with new insights into the uniqueness of our own Milky Way Galaxy after completing the census of 101 satellite systems similar to the Milky Way’s.   

These “satellites” are smaller galaxies in both mass and size which orbit a larger galaxy, usually called the host galaxy. Just as with smaller satellites that orbit the Earth, these satellite galaxies are captured by the gravitational pull of the massive host galaxy and its surrounding dark matter. The Milky Way Galaxy is the host galaxy of several satellite galaxies, of which the two largest are the Large and Small Magellanic Clouds (LMC and SMC). While LMC and SMC are visible to the naked eye from the Southern Hemisphere, there are many other fainter satellite galaxies orbiting around the Milky Way Galaxy that can only be observed with a large telescope.  

The goal of the SAGA Survey is to characterize satellite systems around other host galaxies that have similar stellar masses as the Milky Way Galaxy. Yao-Yuan Mao, a University of Utah faculty member in the Department of Physics and Astronomy, is co-leading the SAGA Survey with Marla Geha at Yale University and Risa Wechsler at Stanford University. Mao is the lead author of the first article in the series of three that have all been accepted by the Astrophysical Journal. This series of articles reports on the SAGA Survey’s latest findings and makes the survey data available to other researchers worldwide.  

 An outlier galaxy? 

An image of a Milky Way-like galaxy and its system of satellite galaxies. The SAGA survey identified six small satellite galaxies in orbit around this Milky Way analog. Credit: Yasmeen Asali (Yale), with images from the DESI Legacy Surveys Sky Viewer https://www.legacysurvey.org/acknowledgment/

 In the first study led by Mao, the researchers highlighted 378 satellite galaxies identified across 101 Milky Way-mass systems. The number of confirmed satellites per system ranged from zero to 13 — compared to four satellites for the Milky Way. While the number of satellite galaxies in the Milky Way system is on par with the other Milky Way-mass systems, “the Milky Way appears to host fewer satellites if you consider the existence of the LMC,” Mao said. The SAGA Survey has found that systems with a massive satellite like the LMC tend to have a higher total number of satellites, and our Milky Way seems to be an outlier in this regard. 

An explanation for this apparent difference between the Milky Way and the SAGA systems is the fact that the Milky Way has only acquired the LMC and SMC quite recently, compared with the age of the universe). The SAGA article explains that if the Milky Way Galaxy is an older, slightly less massive host with the recently added LMC and SMC, one would then expect a lower number of satellites in the Milky Way system not counting other smaller satellites that LMC/SMC might have brought in.  

This result demonstrates the importance of understanding the interaction between the host galaxy and the satellite galaxies, especially when interpreting what we learn from observing the Milky Way. Ekta Patel, a NASA Hubble Postdoctoral Fellow at the U but not part of the SAGA team, studies the orbital histories of Milky Way satellites. After learning about the SAGA results, Patel said, “Though we cannot yet study the orbital histories of satellites around SAGA hosts, the latest SAGA data release includes a factor of ten more Milky Way-like systems that host an LMC-like companion than previously known. This huge advancement provides more than 30 galaxy ecosystems to compare with our own, and will be especially useful in understanding the impact of a massive satellite analogous to the LMC on the systems they reside in.”  

Why do galaxies stop forming stars? 

The second SAGA study of the series is led by Geha, and it explores whether these satellite galaxies are still forming stars. Understanding the mechanisms that would stop the star formation in these small galaxies is an important question in the field

Yao-Yuan Mao

of galaxy evolution. The researchers found, for example, that satellite galaxies located closer to their host galaxy were more likely to have their star formation “quenched,” or suppressed. This suggests that environmental factors help shape the life cycle of small satellite galaxies.  

The third new study is led by Yunchong (Richie) Wang, who obtained his PhD with Wechsler. This study uses the SAGA Survey results to improve existing theoretical models of galaxy formation. Based on the number of quenched satellites in these Milky Way-mass systems, this model predicts quenched galaxies should also exist in more isolated environments — a prediction that should be possible to test in the coming years with other astronomical surveys such as the Dark Energy Spectroscopic Instrument Survey.  

Gift to the astronomy community 

In addition to these exciting results that will enhance our understanding of galaxy evolution, the SAGA Survey team also brings a gift to the astronomy community. As part of this series of studies, the SAGA Survey team published new distance measurements, or redshifts, for about 46,000 galaxies. “Finding these satellite galaxies is like finding needles in a haystack. We had to measure the redshifts for hundreds of galaxies to just identify one satellite galaxy,” Mao said. “These new galaxy redshifts will enable the astronomy community to study a wide range of topics beyond the satellite galaxies.”  

The SAGA Survey was supported in part by the National Science Foundation and the Heising-Simons Foundation. Other authors of these three SAGA studies include Yasmeen Asali, Erin Kado-Fong, Nitya Kallivayalil, Ethan Nadler, Erik Tollerud, Benjamin Weiner, Mia de los Reyes, John F. Wu, Tom Abel, and Peter Behroozi. 

By David Pace

U Scientists Nominate Iconic Utah Sites as Global Geoheritage Locations

U Scientists Nominate Iconic Utah Sites
as Global Geoheritage Locations


Sep 24, 2024
Above: The view of Great Salt Lake’s North Arm from Gunnison Island. Credit: Brian Maffly

In 1875, Grove Karl Gilbert laid eyes on Utah’s remote and recently named Henry Mountains, and was fascinated by the “deep carving of the land which renders it so inhospitable to the travel and the settler, [but] is to the geologist a dissection which lays bare the very anatomy of the rocks.”

He observed a “great depth of uplifted and arching strata”, which form domes of sedimentary rock over chambers of hardened “molten rock,” or what came to be called laccoliths.

G.K. Gilbert’s scientific exploration of the Henry Mountains led to the development of a mechanical model for mountain building that has remained valid for 150 years. In recognition of the its role in the history of geoscience, the southern Utah range has been selected as a world geoheritage site by the International Union of Geological Sciences (IUGS), along with two other features in Utah: the Great Salt Lake and Coyote Buttes, the sandstone landscape on the Arizona state line that includes The Wave.

Nominated by University of Utah geoscientists, the three sites were among the Second 100 IUGS Geological Heritage sites announced on Aug. 27 at the 37th International Geological Congress in South Korea.  “These are the world’s best demonstrations of geologic features and processes,” the union said in a statement. “They are the sites of fabulous discoveries of the Earth and its history. They are sites that served to develop the science of geology.”

U research professor Marie Jackson, who mapped the three southern domes of the Henry Mountains for her doctoral dissertation in the 1980s, applauded the selection, which is a testament to G. K. Gilbert’s forward-thinking genius in the 19th century.

“This world was unexplored. These domes record raw geologic processes that were here for the viewing,” she said.

Jackson and Marjorie Chan, both professors in the Department of Geology and Geophysics, nominated the Utah sites and compiled descriptions for the IUGS geoheritage catalog. The MSc thesis of their former U graduate student Winston Seiler is devoted to The Wave.

Read the full article by Brian Maffly in @TheU.

How Harmful is Great Salt Lake Dust? U Scientists Investigate

How Harmful is Great Salt Lake Dust?
U Scientists Investigate


September 17, 2024

As Utah’s Great Salt Lake shrinks, exposing more of its playa, concerns grow about the dust the dry lakebed emits. But scientists lack the data to fully understand what pollutants are present in these airborne sediments.

Researchers from the University of Utah, including atmospheric scientist Kevin Perry and biologist Michael Werner, are attempting to get a handle on this question and the latest findings are concerning.

Sediments in the lake’s exposed playa are potentially more harmful than other major dust sources affecting the Wasatch Front’s air quality, according to a study published online recently in the journal Atmospheric Environment.

NBC News Dust researcher Kevin Perry poses with his fat bike and a PI-SWERL machine, which can measure wind erosion and dust emission.
Photo credit: Evan Bush

“You’re talking about a very large dust source located next to a very large population, and you’ve got elevated levels of manganese, iron, copper and lead. Lead is a concern for developmental reasons,” said senior author Kerry Kelly, a professor of chemical engineering. “Manganese, iron and copper, these are transition metals and are known to be very irritating to your lungs. Once you get irritation, that can lead to this whole inflammatory response. And that’s part of the problem with particulate matter and it’s adverse health effects like asthma.”

Another recent study led by sociology professor Sara Grineski found dust from the lakebed disproportionately affects disadvantaged neighborhoods in Salt Lake County.

In a separate forthcoming study led by U biologist Michael Werner’s lab, another team of researchers characterized levels of toxic metals deposited in submerged lakebed sediments sampled during the lake’s record low-water year of 2021, noting how these levels have changed since the years of Utah’s mining era.

To conduct the published study, Kerry Kelly’s lab, which specializes in air quality, teamed up with researchers in the U’s College of Science. They examined previously collected sediment samples from the Great Salt Lake, comparing them with sediments from other dust sources in the Great Basin, namely Sevier Lake, Fish Springs Lake and West Desert in western Utah and Tule Lake in northeastern California. These places are known to contribute to dust pollution reaching Salt Lake City.

In recent years, co-author Kevin Perry, a professor of atmospheric sciences, has systematically gathered exposed lakebed sediments, logging hundreds of miles on a bike. His prior research has identified “hotspots” on the playa that appear to be enriched with potentially toxic elements.

Read the full article by Brian Maffly @TheU.

Honoring fallen soldiers: How science is using teeth to bring families closure

Honoring fallen soldiers: How science is using teeth to bring families closure


September 16, 2024
Above: Ben Rivera, a technician in the Bowen Lab, prepares a wisdom tooth for analysis. Credit: Bowen Lab.

More than 80,000 American service members remain missing from previous wars, most from World War II. When remains are found, their age often makes identification difficult—but not impossible.

Even without a name, fingerprints, or facial features, our history leaves indelible marks on us, locked in the atoms of the toughest structures in our bodies: the enamel of our teeth. Subtle differences in tooth chemistry could help determine the identity of fallen soldiers and other human remains—if we can learn to read that history.

Gabe Bowen, the lead researcher for the FIND-EM project, takes a groundwater sample from a well. Credit: Bowen Lab.

Now, a collaboration between geography and dentistry researchers aims to find ways to map a person’s remains to the region where they grew up, based on slight differences in tooth enamel that are determined by the composition of local tap water.

While the researchers’ immediate goal is to help identify fallen soldiers, the project has the potential to strengthen the field of forensic investigation as a whole, according to Gabe Bowen, PhD, professor of geology and geophysics at the University of Utah and the lead on the project. “The ultimate goal is to produce a resource that will be very broadly useful,” Bowen says. “Cold cases, border crossers, humanitarian crises—any situation where we end up with individuals of unknown identity.”

The molar code:

To match someone’s teeth to where they grew up, the researchers are amassing a database of teeth donated by volunteers nationwide and comparing their enamel composition to groundwater data. They’re using wisdom teeth, which are commonly removed in modern dental care.

“I think it’s beautiful that in the natural progression of people’s treatment, we would be removing these teeth anyway,” says Michael Bingham, clinical research coordinator in the School of Dentistry at the University of Utah. “We can take something that would, in theory, be discarded, and use it to do this beautiful project of reuniting families with their service members’ remains.”

While the researchers need more tooth donors to get a comprehensive map, their results so far are promising.

Read the full article by Sophia Friesen @UofUhealth

New tools for peering into cell function.

New tools for peering into cell function


Sep 9, 2024
Above: Ming Hammond, professor of chemistry. PHOTO CREDIT: Dave Titensor, University of Utah

U chemists discover how key contrast agent works, paving the way to create markers needed for correlative microscopy.

Two labs at the University of Utah’s Department of Chemistry joined forces to improve imaging tools that may soon enable scientists to better observe signaling in functioning cells and other molecular-scale processes central to life.

Rodrigo Noriega, assistant professor of chemistry and co-author of the study.

The Noriega and Hammond labs, with complementary expertise in materials chemistry and chemical biology, made critical discoveries announced this month in the Journal of the American Chemical Society that could advance this goal. Their joint project was kickstarted through a team development grant from the U College of Science and the 3i Initiative to encourage faculty with different research interests to work together on big-picture problems.

“We’re trying to develop a new kind of imaging method, a way to look into cells and be able to see both their structural features, which are really intricate, while also capturing information about their activity,” said co-author Ming Hammond, a professor of chemistry. "Current methods provide high-resolution details on cellular structure but have a challenging ‘blind spot’ when it comes to function. In this paper, we study a tool that might be applied in electron microscopy to report on structure and function at the same time.”

Biological samples often need “markers,” or molecules that are the source of detectable signals, explained co-author Rodrigo Noriega, an assistant professor of chemistry. A widely used type of markers are flavoproteins which, when photoexcited, trigger a chemical reaction that yields metal-absorbing polymer particles whose high contrast in electron microscopy is easily seen.

Scientists had long assumed that a mechanism involving singlet oxygen generation, a special kind of reactive oxygen species, was at play. However, the U team found that electron transfer between the photoexcited marker and the polymer building blocks is the main contributor to the process.

You can read the full story by Brian Maffly in @TheU.

 

LEDs just got a whole lot smarter

LED's just got a whole lot smarter


Sep 05, 2024

Traditional electronics use semiconductors to transmit data through bursts of charged carriers (electrons or holes) to convey messages in “1s” and “0s.”

Spintronic devices can process an order of magnitude more information by assigning binary code to the orientation of electrons’ magnetic poles, a property known as spin— an “up” spin is a 1, a “down” is a 0.

A major barrier to commercial spintronics is setting and maintaining the electron spin orientation. Most devices tune spin-orientation using ferromagnets and magnetic fields, a burdensome and unreliable process. Decades of research has shown that carriers lose their spin orientation moving from materials with high-conductivity to low-conductivity—for example, from metallic ferromagnets to undoped silicon and conjugated polymer materials that make up most modern semiconductors.

Valy Vardeny ( Distinguished Professor)

For the first time, scientists transformed existing optoelectronic devices into ones that can control electron spin at room temperature, without a ferromagnet or magnetic field.

Most optoelectronic devices, such as LEDs, only control charge and light but not the spin of the electrons. In the new study led by the University of Utah physicists and researchers at the National Renewable Energy Laboratory (NREL), replaced the electrodes of store-bought LEDs with a patented spin filter, made from hybrid organic-inorganic halide perovskite material.

“It’s a miracle. For decades, we’ve been unable to efficiently inject spin-aligned electrons into semiconductors because of the mismatch of metallic ferromagnets and non-magnetic semiconductors,” said Valy Vardeny, Distinguished Professor in the Department of Physics & Astronomy at the U and co-author of the paper. “All kinds of devices that use spin and optoelectronics, like spin-LEDs or magnetic memory, will be thrilled by this discovery.

The study was published in the journal Nature on June 19, 2024.

Spin filters

In 2021, the same collaborators developed the technology that acts as an active spin filter made of two successive layers of material, called chiral hybrid organic-inorganic halide perovskites. Chirality describes molecule’s symmetry, where its mirror image cannot be superimposed on itself. Human hands are the classic example; hold yours out, palms facing away. The right and left hands are arranged as mirrors of one another—you can flip your right hand 180° to match the silhouette, but now the right palm is facing you while the left palm faces away. They’re not the same.

Some molecules, such as DNA, sugar and layers of chiral hybrid organic-halide perovskites, have their atoms arranged in chiral symmetry. The filter works by using a “left-handed” oriented chiral layer to allow electrons with “up” spins to pass, but block electrons with “down” spins, and vice versa. At the time, the scientists claimed the discovery could be used to transform conventional optoelectronics into spintronic devices simply by incorporating the chiral spin filter. The new study did just that.

Read the full article by Lisa Potter in @TheU.

Is the Past the Key to Our Future Climate?

Is the Past the Key to Our Future Climate?


September 3, 2024
Above: forams under microscopic level

New research from U geologists links rapid climate change 50 million years ago to rising CO2 levels.

At the end of the Paleocene and beginning of the Eocene epochs, between 59 to 51 million years ago, Earth experienced dramatic warming periods, both gradual periods stretching millions of years and sudden warming events known as hyperthermals. Driving this planetary heat-up were massive emissions of carbon dioxide (CO2) and other greenhouse gases, but other factors like tectonic activity may have also been at play.

Gabriel Bowen

New research led by University of Utah geoscientists pairs sea surface temperatures with levels of atmospheric COduring this period, showing the two were closely linked. The findings also provide case studies to test carbon cycle feedback mechanisms and sensitivities critical for predicting anthropogenic climate change as we continue pouring greenhouse gases into the atmosphere on an unprecedented scale in the planet’s history.

“The main reason we are interested in these global carbon release events is because they can provide analogs for future change,” said lead author Dustin Harper, a postdoctoral researcher in the Department of Geology & Geophysics. “We really don’t have a perfect analog event with the exact same background conditions and rate of carbon release.”

But the study published on 26th August'24 in the Proceedings of the National Academy of Sciences, or PNAS, suggests emissions during two ancient “thermal maxima” are similar enough to today’s anthropogenic climate change to help scientists forecast its consequences. The research team analyzed microscopic fossils—recovered in drilling cores taken from an undersea plateau in the Pacific—to characterize surface ocean chemistry at the time the shelled creatures were alive. The findings indicate that as atmospheric levels of COrose, so too did global temperatures.

“We have multiple ways that our planet, that our atmosphere is being influenced by CO2 additions, but in each case, regardless of the source of CO2, we’re seeing similar impacts on the climate system,” said co-author Gabriel Bowen, a U professor of geology & geophysics.

Read the full article by Brian Maffly @TheU.

Elevating Public Understanding of Geoscience

Elevating Public Understanding of Geoscience


August 26, 2024. Above: Marjorie Chan

Marjorie Chan, Distinguished Professor Emerita at the Department of Geology and Geophysics at the University of Utah, is the 2024 recipient of the Outstanding Contribution to the Public Understanding of the Geosciences award.

The award is presented by the American Geosciences Institute (AGI) to a person, organization, or institution in recognition of an outstanding contribution to the public understanding of geoscience. "Dr. Chan has demonstrated extraordinary commitment to public outreach and community service throughout her career," according to the press release issued by AGI. "Her earliest efforts focused on inspiring and supporting young women in the geosciences, and over the decades her concerns expanded to promoting public awareness of environmental issues and the urgent need to conserve geological resources."

Chan has given hundreds of public lectures, served as a volunteer consultant on scores of ecological and preservation projects as well as art collaborations, advised and created instructive material for secondary teachers and oversaw major Earth science community initiatives. The U has Chan to thank for coordinating the design and construction of the first LEED-certified building on the academic campus which includes educational visual displays that have since inspired geoscience building designs across the nation.

A PASSION FOR EARTH SCIENCE

Lobby of the Sutton Building, University of Utah

"I am very honored to be recognized by AGI for a career that has been so engaging and fulfilling,” says Chan who served as department chair during which time she was appointed the U’s first Geology and Geophysics faculty coordinator of outreach. “Being a part of the Earth science community has been an experience beyond my expectations. I’ve learned from so many wonderful people and made connections across cultures and countries that I will never forget. This has inspired me to share my passion for Earth science with the public. “

That passion for sharing has led to Chan's being featured in documentaries including National Geographic and Discovery Channel television shows. Additionally, she has been a guest on National Public Radio’s Science Friday, and has served as a science advisor for PBS-Nova Science Now. Her NASA science and outreach activities include Endeavor 2016 Dynamic Mars Webinars for K-12 teachers, Mars for Earthlings webinars and short courses and development of teaching modules for higher education instructors.

As the 2014 Geological Society of America (GSA) Distinguished International Lecturer Chan has given 53 lectures spanning India, New Zealand, Australia, China, Japan, and South Korea. In addition to receiving two national meeting presentation awards from SEPM (Society for Sedimentary Geology), she is the winner of the GSA Distinguished Service Award (2020) and the GSA Sloss Award for Lifetime Achievements in Sedimentary Geology (2019). She was also elected GSA Fellow in 1995. In her national committee work she has chaired the GSA Diversity Committee (2012-2013), the GSA Sedimentary Geology Division (2014-2015) and the U.S. National Committee for Geological Sciences (2022-2023).

Referring to the recent honor, Chan says “the award recognizes the impact of many important mentors and colleagues, and their investment in me. Being honored by AGI is an affirmation of the value in giving back to a profession that has brought me so much enrichment in my life.”

The Frederick Albert Sutton Building, the first LEED-certified building on U academic campus.

From Precambrian to Pleistocene

Chan earned a PhD in Geology from the University of Wisconsin-Madison in 1982 and a BS in Geology from the University of California-Davis in 1977. During an academic career of more than 40 years at the U, she has authored or co-authored more than 150 peer-reviewed articles on a range of sedimentary topics. Her work has spanned the Precambrian up to the Pleistocene with recent research that applied terrestrial examples to better understand Martian geology.

When it comes to outreach Chan knows that public engagement is often an afterthought or less valued than research and teaching. “I feel that spreading our knowledge more widely is a core principle of scholarship. Our societal future relies on public understanding of the complexities in the natural world.”

Chan, who retired this year, is being recognized for the award at the Friends of AGI Awards Reception during the GSA Connects conference in Anaheim, California, on September 24, 2024.

 

by David Pace

About The American Geosciences Institute, AGI is a federation of scientific and professional organizations representing over a quarter-million geoscientists, is a nonprofit 501(c)(3) organization dedicated to serving the geoscience community and addressing the needs of society. AGI headquarters are in Alexandria, Virginia.

Scientists Find Hope in Cone Snail Venom

Scientists Find Hope in Cone Snail Venom


Aug 23, 2024
Above : Ho Yan Yeung, PhD (left) and Thomas Koch, PhD (right, also an author on the study) examine a freshly-collected batch of cone snails. Image credit: Safavi Lab.

Based on work by Toto Olivera, the father of research on cone snail venom, scientists are now finding clues for how to treat diabetes and hormone disorders in a toxin from one of the most venomous animals on the planet.

An international research team led by University of Utah scientists has identified a component within the venom of a predatory marine cone snail, the geography cone, that mimics a human hormone called somatostatin, which regulates the levels of blood sugar and various hormones in the body. The hormone-like toxin’s specific, long-lasting effects, which help the snail hunt its prey, could also help scientists design better drugs for people with diabetes or hormone disorders, conditions that can be serious and sometimes fatal.

The results were published Aug. 20 in the journal Nature Communications.

A blueprint for better drugs

Somatostatin acts like a brake pedal for many processes in the human body, preventing the levels of blood sugar, various hormones, and many other important molecules from rising dangerously high. The cone snail toxin, called consomatin, works similarly, the researchers found—but consomatin is more stable and specific than the human hormone, which makes it a promising blueprint for drug design.

By measuring how consomatin interacts with somatostatin’s targets in human cells in a dish, the researchers found that consomatin interacts with one of the same proteins that somatostatin does. But while somatostatin directly interacts with several proteins, consomatin only interacts with one. This fine-tuned targeting means that the cone snail toxin affects hormone levels and blood sugar levels but not the levels of many other molecules.

In fact, the cone snail toxin is more precisely targeted than the most specific synthetic drugs designed to regulate hormone levels, such as drugs that regulate growth hormone. Such drugs are an important therapy for people whose bodies overproduce growth hormones. Consomatin’s effects on blood sugar could make it dangerous to use as a therapeutic, but by studying its structure, researchers could start to design drugs for endocrine disorders that have fewer side effects.

Consomatin is more specific than top-of-the-line synthetic drugs—and it also lasts far longer in the body than the human hormone, thanks to the inclusion of an unusual amino acid that makes it difficult to break down. This is a useful feature for pharmaceutical researchers looking for ways to make drugs that will have long-lasting benefits.

Learning from cone snails

Finding better drugs by studying deadly venoms may seem unintuitive, but Helena Safavi, associate professor of biochemistry in the U’s Spencer Fox Eccles School of Medicine and the senior author on the study, explained that the toxins’ lethality is often aided by pinpoint targeting of specific molecules in the victim’s body. That same precision can be extraordinarily useful when treating disease.

“Venomous animals have, through evolution, fine-tuned venom components to hit a particular target in the prey and disrupt it,” Safavi said. “If you take one individual component out of the venom mixture and look at how it disrupts normal physiology, that pathway is often really relevant in disease.” For medicinal chemists, “it’s a bit of a shortcut.”

Among Safavi’s coauthors are faculty from the U’s School of Biological Sciences, including Baldomero Olivera and Samuel Espino. The U has been a hotspot for research into the venom’s pharmacological properties since Olivera arrived in Utah in 1970 from his native Philippines, bringing his interest in cone snails with him.

Read the full, original story by Sophia Friesen in UofU Health.
Read about Toto Olivera’s 2022 Golden Goose Award for early research in cone snails here.

Deep Beneath Our Feet: A Seismic Surprise

Deep Beneath Our Feet: A Seismic Surprise


Aug 20, 2024
Above: Earth’s interior. Credit: Michael Thorne

For the decades since their discovery, seismic signals known as PKP precursors have challenged scientists. Regions of Earth’s lower mantle scatter incoming seismic waves, which return to the surface as PKP waves at differing speeds.

The origin of the precursor signals, which arrive ahead of the main seismic waves that travel through Earth’s core, has remained unclear, but research led by University of Utah geophysicists sheds new light on this mysterious seismic energy.

PKP precursors appear to propagate from places deep below North America and the western Pacific and possibly bear an association with “ultra-low velocity zones,” thin layers in the mantle where seismic waves significantly slow down, according to research published in AGU Advances, the American Geophysical Union’s lead journal. (The AGU highlighted the research in its magazine Eos.)

“These are some of the most extreme features discovered on the planet. We legitimately do not know what they are,” said lead author Michael Thorne, a U associate professor of geology and geophysics. “But one thing we know is they seem to end up accumulating underneath hotspot volcanoes. They seem like they may be the root of whole mantle plumes giving rise to hotspot volcanoes.”

These plumes are responsible for the volcanism observed at Yellowstone, the Hawaiian Islands, Samoa, Iceland and the Galapagos Islands.

Thorne’s team, which included research assistant professor Surya Pachhai, devised a way to model waveforms to detect crucial effects that previously went unnoticed. Using a cutting-edge seismic array method and new theoretical observations from earthquake simulations, the researchers developed, they analyzed data from 58 earthquakes that occurred around New Guinea and were recorded in North America after passing through the planet.

Their new method allowed them to pinpoint where the scattering occurred along the boundary between the liquid metal outer core and the mantle, known as the core-mantle boundary, located 2,900 kilometers below Earth’s surface.

Read the full article by Brian Maffly @TheU.