Researchers Examine Neanderthal DNA to Gain Insights into Human Facial Development and Evolution

Research led by scientist Hannah Long at the University of Edinburgh has found that specific regions of Neanderthal DNA are more effective at activating genes responsible for jaw development than those in humans, potentially explaining why Neanderthals had larger lower jaws.

Neanderthal. Image credit: Natural History Museum Trustees.

“With the Neanderthal genome being 99.7% identical to that of modern humans, the variations between species are likely to account for differences in appearance,” Dr. Hanna stated.

“Both human and Neanderthal genomes consist of roughly 3 billion characters that code for proteins and regulate gene expression in cells. Identifying the regions that influence appearance is akin to searching for a needle in a haystack.”

Dr. Long and her team had a targeted approach, focusing on a genomic area linked to the Pierre Robin sequence, a condition marked by an unusually small mandible.

“Individuals with the Pierre Robin sequence often have significant deletions or rearrangements in this portion of the genome that affect facial development and restrict jaw formation,” Dr. Hanna explained.

“We hypothesized that minor differences in DNA could produce more nuanced effects on facial structure.”

Upon comparing human and Neanderthal genomes, researchers discovered that in this segment, approximately 3,000 letters long, there are only three one-letter variations between the species.

This DNA region doesn’t code for genes but regulates when and how certain genes, particularly SOX9, which plays a crucial role in facial development, are activated.

To confirm that these Neanderthal-specific differences were significant for facial development, scientists needed to demonstrate that the Neanderthal version could activate genes in the appropriate cells at the right developmental stage.

They introduced both Neanderthal and human versions of this region into zebrafish DNA and programmed the cells to emit different colors of fluorescent protein based on the activation of either region.

By monitoring zebrafish embryo development, researchers observed that cells responsible for forming the lower jaw were active in both human and Neanderthal regions, with the Neanderthal regions showing greater activity.

“It was thrilling when we first noticed the activity of specific cell populations in the developing zebrafish face, particularly near the forming jaw, and even more exhilarating to see how Neanderthal-specific variations could influence activity during development,” said Dr. Long.

“This led us to contemplate the implications of these differences and explore them through experimental means.”

Recognizing that Neanderthal sequences were more effective at activating genes, the authors questioned whether this would lead to enhanced target activity affecting the shape and function of the adult jaw, mediated by SOX9.

To validate this idea, they augmented zebrafish embryos with additional samples of SOX9 and discovered that cells involved in jaw formation occupied a larger area.

“Our lab aims to further investigate the effects of genetic differences using methods that simulate various aspects of facial development,” Dr. Long remarked.

“We aspire to deepen our understanding of genetic variations in individuals with facial disorders and improve diagnostic processes.”

“This study demonstrates how examining extinct species can enhance our knowledge of how our own DNA contributes to facial diversity, development, and evolution.”

The findings are published in the journal Development.

_____

Kirsty Utley et al. 2025: Neanderthal-derived variants enhance SOX9 enhancer activity in craniofacial progenitor cells, influencing jaw development. Development 152 (21): dev204779; doi: 10.1242/dev.204779

Source: www.sci.news

Introducing the Smart Pill: Enabling Doctors to Examine and Treat Your Intestines Internally.

Emerging technologies enable doctors to leverage microorganisms for diagnosing and treating diseases through gut microbiota. Recent studies highlight these advancements.

Researchers successfully used smartphone apps to genetically alter bacteria, causing them to emit light signals in response.

If proven safe and effective in humans, this treatment could address several illnesses that are currently challenging to manage.

This method encompassed three key elements: bacteria, technology, and pigs. Under the guidance of senior author Hanzi Wang from Tianjin University in China, scientists modified E. coli bacteria to react to specific chemical and optical stimuli.

They created swallowable capsules controlled via Bluetooth that communicate with these photoresponsive bacteria, targeting pigs afflicted with colitis, a type of inflammatory bowel disease that results in intestinal swelling.

The experiment has commenced, allowing scientists to introduce engineered E. coli into the inflamed intestines of pigs through these capsules.

Nitrates, which the body produces during intestinal inflammation, serve as indicators of active colitis. When the modified E. coli come into contact with nitrates, they illuminate.

These smart capsules can detect the optical signal, alerting researchers to the presence of E. coli via Bluetooth.

Through a smartphone app, researchers can command the capsule to start emitting light signals, prompting the E. coli to release anti-inflammatory antibodies to combat colitis.

This innovative approach enables scientists to effectively communicate with the bacteria, ensuring targeted treatment delivery.

Three pigs were infected with colitis, a type of inflammatory bowel disease with few treatment options currently available – Credit: Connect images via Getty

“This represents a remarkable technological advancement,” stated Dr. Lindsey Edwards, a senior lecturer in Microbiology at King’s College London, as reported by BBC Science Focus. Dr. Edwards was not involved in the research.

“Methods like this enable precise, real-time interactions with gut bacteria and have the potential to revolutionize treatment,” she added.

“There is an urgent need for new tools that allow us to harness the full potential of our microbiota to enhance health and better understand and manage microbial infections.”

At present, colitis has no existing treatments, and options are scarce. Dr. Edwards believes that such future methods could “open new pathways” for treating not only inflammatory bowel disease but also other gut-related conditions, including type 2 diabetes, heart disease, and chronic fatigue.

However, Dr. Alexandre Almeida, from the Department of Veterinary Medicine at Cambridge University and not part of this research, warns that this possibility is still distant.

“This is still a preliminary proof-of-concept study,” he noted. “The technology has only been tested in animals and specifically for detecting certain conditions.”

“Before human applications, we must evaluate the safety of this technology and address significant questions, such as how these engineered microorganisms influence the natural balance of other gut bacteria.”

Dr. Nicholas Ilott, a senior researcher at the Oxford Microbiome Research Center who did not participate in the study, stated that the technology is “incredibly exciting” and could prove to be “very valuable” in future medical treatments.

Read more:

About our experts

Dr. Lindsey Edwards is a senior lecturer in microbiology at King’s College London, UK. Her research focuses on mucosal barrier immunology, host-microbe interactions, and the priming of adaptive immune responses, along with intestinal and liver diseases.

Dr. Alexandre Almeida is a Principal Investigator and MRC Career Development Fellow at the University of Cambridge, UK, specializing in bioinformatics and genomic approaches for biological discoveries related to human health.

Dr. Nicholas Ilott is a senior researcher specializing in bioinformatics at the Microbiome Research Centre, Nuffield Department of Orthopaedic Surgery, Oxford University, UK, concentrating on host-microbe interactions in chronic liver and inflammatory bowel diseases.

Source: www.sciencefocus.com

Researchers examine how tides impact the interiors of planets and moons

A team of scientists from the University of Arizona, Delft University of Technology, and the California Institute of Technology's Lunar and Planetary Institute has developed a new method to calculate how tides affect the interiors of the solar system's planets and moons. Importantly, they investigated the effects of internal tides on objects that do not have perfectly spherical internal structures.

Europa's surface stands out in this newly reprocessed color view. Image scale is 1.6 km per pixel. North of Europe is on the right. Image credit: NASA / JPL-Caltech / SETI Institute.

Celestial tides refer to the deformations that celestial bodies experience when they interact with other bodies due to gravity.

Consider how Jupiter's powerful gravity pulls on its icy moon Europa.

Because Europa's orbit is not circular, the overwhelming gravitational pressure on Jupiter's moons changes as it moves along Jupiter's orbit.

When Europa is closest to Jupiter, the planet's gravity is most felt.

The energy of this deformation heats Europa's interior, allowing an ocean of liquid water to exist beneath the moon's icy surface.

“The same is true for Saturn's moon Enceladus,” says Dr. Alexander Byrne, a researcher at the California Institute of Technology.

“Enceladus has an ice shell that is expected to have much more aspherical symmetry than Europa.”

The body tides experienced by celestial bodies influence how the world evolves over time and, in cases like Europa and Enceladus, its potential habitability for life as we know it. may give.

“The tidal response of spherically symmetric objects has the same wavelength as the tidal forces. Lateral inhomogeneities generate additional tidal responses with spectra that depend on the spatial pattern of such fluctuations.” the researchers said.

“For Mercury, the Moon, and Io, the amplitude of this signal is as much as 1-10% of the dominant tidal response to long-wavelength shear modulus fluctuations, which exceed about 10% of the mean shear modulus.”

“For Europa, Ganymede, and Enceladus, a shell thickness variation of 50% of the average shell thickness could result in an additional signal of about 1% and about 10% for Jupiter's moons and Enceladus, respectively.”

The authors also discussed how their results can help scientists interpret observations made by missions to a variety of different worlds, from Mercury to the moon to the outer planets of our solar system. .

“Future missions such as BepiColombo and JUICE have the potential to measure these signals,” they said.

“Lateral changes in viscosity affect the distribution of tidal heating.”

“This may promote the thermal evolution of tidal bodies and influence the distribution of active areas.”

of findings will appear in Planetary Science Journal.

_____

Mark Rovira-Navarro others. 2024. A spectral method for calculating the tides of laterally inhomogeneous objects. planet. Science. J 5, 129; doi: 10.3847/PSJ/ad381f

This article is a version of a press release provided by NASA.

Source: www.sci.news

Hubble and Webb telescopes examine the planetary debris disk surrounding Vega

There is no clear evidence that one or more large exoplanets are punching through the frontal debris disk surrounding Vega, one of the brightest stars in the night sky.



Webb used the Mid-Infrared Instrument (MIRI) to obtain images of the circumstellar disk around Vega. Image credits: NASA / ESA / CSA / STScI / S. Wolff, University of Arizona / K. Su, University of Arizona / A. Gáspár, University of Arizona.

Vega is a young, massive star located about 25 light-years away in the constellation Lyra.

This star is classified as type A. This is the name of stars that tend to be larger, younger, and rotate much faster than the Sun.

Vega, also known as Alpharilla, Gliese 721, and HD 172167, is 455 million years old and has a mass equal to two solar masses.

It rotates around its axis every 16 hours. This is much faster than the Sun, which has a rotation period measured in 27 Earth days.

Vega is legendary because it provided the first evidence of matter orbiting a star.

this was the first made a hypothesis However, it took more than 200 years before the first observational evidence was collected in 1984.

A mysterious excess of infrared radiation from warm dust has been detected by NASA's Infrared Astronomy Satellite (IRAS). It was interpreted to be a shell or disk of dust extending from the star to twice Pluto's orbital radius.

In the new study, astronomers analyzed images of Vega's debris disk taken by the NASA/ESA Hubble Space Telescope and the NASA/ESA/CSA James Webb Space Telescope.

“Vega was one of the first typical planetary debris disks to be discovered,” Dr. Kate Hsu of the University of Arizona and colleagues said in their paper. paper Introducing the results of a web survey.

“This opens up a wide field of research, which is now being used to identify relatively low-mass exoplanets that are unreachable with other discovery techniques, as well as to reveal detailed properties of small bodies in other planetary systems. It is used in

“Vega continues to be an anomaly,” added Dr. Schuyler Wolf, an astronomer at the University of Arizona and lead author of the paper. paper Introducing Hubble's discoveries.

“The structure of the Vega system is markedly different from our solar system, where giant planets like Jupiter and Saturn prevent dust from dispersing like Vega.”

“For comparison, there is a nearby star called Fomalhaut, which is about the same distance, age, and temperature as Vega.”

“However, Fomalhaut's circumstellar structure is very different from Vega's. Fomalhaut has three nested debris belts.”

“Exoplanets have been suggested to be bodies that guide the dust around Fomalhaut, which gravitationally compresses it into a ring, but no planets have yet been positively identified.”

“Given the physical similarities between Vega and Fomalhaut's stars, why does Fomalhat appear to be able to form planets, but Vega not?” George Rieke, also of the University of Arizona The doctor said:

“What's the difference? Did the circumstellar environment, or the star itself, make the difference? What's puzzling is that the same physics is at work in both,” Wolff added.



Hubble used the Space Telescope Imaging Spectrograph (STIS) to obtain this image of the circumstellar disk around Vega. Image credits: NASA / ESA / CSA / STScI / S. Wolff, University of Arizona / K. Su, University of Arizona / A. Gáspár, University of Arizona.

Webb observed the infrared glow from a disk of sand-sized particles swirling around a scorching blue-white star that is 40 times brighter than the Sun.

Hubble captures the disk's outer halo, which contains smoke-sized particles that reflect starlight.

The distribution of dust within Vega's debris disk is layered. This is because the pressure of the star's light pushes smaller particles out faster than larger ones.

“Between the Hubble and Webb telescopes, we get a very clear view of Vega,” said Dr. András Gaspard, an astronomer at the University of Arizona and co-author of both papers.

“This is a mysterious system because it is unlike any other circumstellar disk we have observed.”

“Vega discs are smooth. Incredibly smooth.”

The Vega disk has a subtle gap about 60 AU (astronomical units) from the star (twice the distance of Neptune from the Sun), but otherwise it is very smooth the entire time until it disappears into the star's glare. is.

This indicates that there are no planets, at least up to the mass of Neptune, orbiting large orbits like our solar system.

“We are looking in detail at how much diversity there is in the circumstellar disk and how that diversity is tied to the underlying planetary system,” Dr. Hsu said.

“Even if we can't see what the hidden planets are, we’re still discovering a lot about planetary systems.”

“There are still many unknowns about the process of planet formation, but we think these new observations from Vega will help constrain models of planet formation.”

The two papers are astrophysical journal.

_____

Kate Y.L. Sue others. 2024. Imaging the Vega debris system using JWST/MIRI. APJin press. arXiv: 2410.23636

Skylar G. Wolf others. 2024. Hubble Space Telescope probes deep into the scattered light dust ring around Vega. APJin press. arXiv: 2410.24042

Source: www.sci.news

It’s Time to Examine the Value Proposition of the Subscription Economy for Customers.

subscription economy It continues to expand unabated.by someone Estimate, companies with subscription licensing have grown three to four times faster than the S&P 500 over the past 12 years. As his CSO at Zoho, a B2B subscription-based technology company founded more than a quarter of a century ago, I see a growing disparity between provider interests and customer outcomes, especially in his SaaS. I realized that.

The prevalence and significant growth of subscription licensing has created an irreproachable model. But if you look closely, software is no longer cheaper, broader, or deeper for customers. Meta, Netflix, Microsoft, Oracle, SAP, Salesforce, and others have recently announced price increases. 24% higher For certain products or services. New layoffs are also underway in the tech industry. Somewhere along the way, economies of scope and scale broke down, and enterprise customers were saddled with monthly, per-user checks.

Rather than contributing to this chasm, software providers can drive growth by passing on the unique benefits of cloud and subscription licensing to their customers. After all, this was the original promise of the model nearly 20 years ago. In my experience, longevity in the market depends on increasing productivity, agility, and revenue for enterprise customers. In other words, adding value rather than limiting it improves both the health and sustainability of the subscription economy and its merchants. Providers can approach this strategy in the following ways:

promote flexibility

Migrating from one tool or system to another is arduous, costly, and disruptive. Even if trial accounts are offered, they have limitations on data processing, storage, usage, and duration, and lack functionality. Increasing the length and scale of customer trials has two benefits for vendors. First, providers can understand the impact of users on enterprise performance, resources, and costs, allowing enterprises to make changes to delivery and pricing without impacting existing paying customers.

Companies can stand out by offering solutions through subscription licensing.

A second benefit of building customer flexibility and choice into your product is new business growth.As a point of Harvard Business Review outside, the Financial Times conducted an experiment in which it removed the ability for customers to view three free articles on the site and instead immediately imposed a paywall. Website traffic fell by 30% and new subscribers declined over time. “If you force every user to convert on the first visit, you’ll lose 79% of conversions, which equates to tens of millions of dollars in customer lifetime value.”

This is because customers prefer to experience the product and build a trusting relationship with the manufacturer before making a purchase decision. In the case of software, deals can run into the millions of dollars, and businesses are willing to shop around until they find the right solution from a trusted vendor at an affordable price. But with the current state of the industry, they may continue to shop forever.

Source: techcrunch.com