Unusual Temperature Rules: Exploring the Bizarre Phenomena of the Quantum Realm

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One of the most paradoxical aspects of science is how we can delve into the universe’s deepest enigmas, like dark matter and quantum gravity, yet trip over basic concepts. Nobel laureate Richard Feynman once candidly admitted his struggle to grasp why mirrors flip images horizontally instead of vertically. While I don’t have Feynman’s challenges, I’ve been pondering the fundamental concept of temperature.

Since time immemorial, from the earliest humans poking fires to modern scientists, our understanding of temperature has dramatically evolved. The definition continues to change as physicists explore temperature at the quantum level.

My partner once posed a thought-provoking question: “Can a single particle possess a temperature?” While paraphrased, this inquiry challenges conventional wisdom.

His instinct was astute. A single particle cannot possess a temperature. Most science enthusiasts recognize that temperature applies to systems comprising numerous particles—think gas-filled pistons, coffee pots, or stars. Temperature is essentially an average energy distribution across a system reaching equilibrium.

Visualize temperature as a ladder, each rung representing energy levels. The more rungs, the greater the energy. For a substantial number of particles, we expect them to occupy various rungs, with most clustering at lower levels and some scaling higher ones. The distribution gradually tapers off as energy increases.

But why use this definition? While averages are helpful, one could argue the average height in a room with one tall person could misleadingly imply everyone else is six feet tall. Why not apply the same logic to temperature?

Temperature serves a predictive role, not merely a descriptive one. In the 17th and 18th centuries, as researchers strove to harness the potential of fire and steam, temperature became pivotal in understanding how different systems interacted.

This insight led to the establishment of the 0th law of thermodynamics—the last yet most fundamental principle. It states that if a thermometer registers 80°C for warm water and the same for warm milk, there should be no net heat exchange when these two are mixed. Though seemingly simple, this principle forms the basis for classical temperature measurements.

This holds true due to the predictable behavior of larger systems. Minute energy variances among individual particles become negligible, allowing statistical laws to offer broad insights.

Thermodynamics operates differently than Isaac Newton’s laws of motion, which apply universally regardless of how many objects are involved. Thermodynamic laws arise only in larger systems where averages and statistical regularities emerge.

Thus, a single particle lacks temperature—case closed.

Or so I believed until physics threw another curveball my way. In many quantum systems, composed of a few particles, stable properties often evade observation.

In small systems like individual atoms, states can become trapped and resist reaching equilibrium. If temperature describes behavior after equilibrium, does this not challenge its very definition?

What exactly is temperature?

fhm/Getty Images

Researchers are actively redefining temperature from the ground up, focusing on its implications in the quantum realm.

In a manner akin to early thermodynamics pioneers, contemporary scientists are probing not just what temperature is, but rather what it does. When a quantum system interacts with another, how does heat transfer? Can it warm or cool its neighbor?

In quantum systems, both scenarios are possible. Consider the temperature ladder for particles. In classical physics, heat always moves from a system with more particles to one with fewer, following predictable rules.

Quantum systems defy these conventions. It’s common for no particles to occupy the lowest rung, with all clustered around higher energy levels. Superposition allows particles to exist in between. This shift means quantum systems often do not exhibit traditional thermal order, complicating heat flow predictions.

To tackle this, physicists propose assigning two temperatures to quantum systems. Imagine a reference ladder representing a thermal system. One temperature indicates the highest rung from which the system can absorb heat, while the other represents the lowest rung to which it can release heat. This new framework enables predictable heat flow patterns outside this range, while outcomes within depend on the quantum system’s characteristics. This new “Zero Law of thermodynamics” helps clarify how heat moves in quantum domains.

These dual temperatures reflect a system’s capacity to exchange energy, regardless of its equilibrium state. Crucially, they’re influenced by both energy levels and their structural arrangement—how quantum particles distribute across energy levels and the transitions the overall system can facilitate.

Just as early thermodynamicists sought functionality, quantum physicists are likewise focused on applicability. Picture two entangled atoms. Changes in one atom will affect the other due to their quantum link. When exposed to external conditions, as they gain or lose energy, the invisible ties connecting them create a novel flow of heat—one that can be harnessed to perform work, like driving quantum “pistons” until the entanglement ceases. By effectively assigning hot and cold temperatures to any quantum state, researchers can determine ideal conditions for heat transfer, powering tasks such as refrigeration and computation.

If you’ve followed along up to this point, here’s my confession: I initially argued that a single particle could have temperature, though my partner’s intuition was spot on. In the end, we realized both perspectives hold some truth—while a single particle can’t be assigned a traditional temperature, the concept of dual temperatures in quantum systems offers intriguing insights.

Topics:

  • quantum physics/
  • lost in space and time

Source: www.newscientist.com

Astronomers Develop 3D Temperature Map of the Exoplanet WASP-18b

A newly released map of WASP-18b, a hot Jupiter exoplanet located approximately 325 light-years from Earth, showcases an atmosphere characterized by distinct temperature zones. Within this region, the scorching temperatures are capable of decomposing water vapor.

Hot Jupiter WASP-18b. Image credit: NASA’s Goddard Space Flight Center.

The WASP-18b map represents the first implementation of a method known as 3D eclipse mapping, or spectroscopic eclipse mapping.

This study features a 2D model. The paper, published in 2023 by members of the same research team, illustrated how eclipse mapping can leverage the sensitive observations from the NASA/ESA/CSA James Webb Space Telescope.

“This technique is unique in that it can simultaneously survey all three dimensions: latitude, longitude, and altitude,” stated Dr. Megan Weiner Mansfield, an astronomer at the University of Maryland and Arizona State University.

“This enables a greater level of detail than previously possible for studying these celestial objects.”

With this technology, astronomers can now begin to chart the atmospheric variations of many similar exoplanets observable through Webb, resembling how Earth-based telescopes once scrutinized Jupiter’s Great Red Spot and its striped cloud formations.

“Eclipse mapping allows us to capture images of exoplanets whose host stars are too bright for direct observation,” remarked Dr. Ryan Challenor, an astronomer at Cornell University and the University of Maryland.

“Thanks to this telescope and groundbreaking technology, we can start to understand exoplanets similarly to the neighboring worlds in our solar system.”

Detecting exoplanets is quite challenging as they typically emit less than 1% of the brightness of their host star.

Mapping a solar eclipse involves measuring a small fraction of the total brightness as the planet orbits behind the star, obscuring and revealing areas of the star in the process.

Scientists can link minute changes in light to specific regions, creating brightness maps. These maps can be rendered in various colors and translated into three-dimensional temperature readings based on latitude, longitude, and altitude.

“It’s quite difficult because you’re looking for changes where small sections of the Earth become obscured and then revealed,” Challenor explained.

WASP-18b has a mass approximately 10 times that of Jupiter, completes its orbit in just 23 hours, and achieves temperatures around 2,760 degrees Celsius (5,000 degrees Fahrenheit). Its strong signal makes it an excellent candidate for testing new mapping techniques.

While previous 2D maps relied on a single wavelength or color of light, the 3D map re-evaluated the same observations using Webb’s Near Infrared Imager and Slitless Spectrometer (NIRISS) across multiple wavelengths.

“Each color corresponds to different temperatures and altitudes within WASP-18b’s gaseous atmosphere, allowing them to be combined into a 3D map,” Dr. Challenor noted.

“Mapping at wavelengths that water absorbs can indicate the layers of water in the atmosphere, while wavelengths that water doesn’t absorb facilitate deeper probing.”

“When combined, these provide a three-dimensional temperature map of the atmosphere.”

The new perspective uncovered spectroscopically distinct zones (with varying temperatures and potentially different chemical compositions) on the visible dayside of WASP-18b (the side that perpetually faces its star due to its tidally locked orbit).

The planet exhibits a circular “hotspot” that receives the most direct stellar light, with winds insufficient to redistribute the heat.

Surrounding the hotspot is a cooler “ring” located closer to the planet’s visible outer edge.

Interestingly, the measurements indicated that water vapor levels within the hotspot were lower than the average for WASP-18b.

“We believe this suggests that the heat in this area is so intense that water is beginning to decompose,” explained Challenor.

“This was anticipated by theory, but it’s exhilarating to confirm it through actual observations.”

“Further observations from Webb could enhance the spatial resolution of this pioneering 3D eclipse map.”

“Already, this technique will aid in refining temperature maps of other hot Jupiters, which comprise hundreds of the more than 6,000 exoplanets discovered to date.”

Dr. Mansfield expressed: “It’s thrilling that we now possess the tools to visualize and map the temperature of another planet in such intricate detail.”

“We can apply this technique to other exoplanet types. For instance, even if a planet lacks an atmosphere, we might be able to use this method to map surface temperatures and discern its composition.”

“While WASP-18b was more predictable, we believe there’s potential to observe phenomena we never anticipated before.”

The map of WASP-18b is detailed in a paper published in the journal Nature Astronomy.

_____

RC Challenor et al.. Horizontal and vertical exoplanet thermal structures from JWST spectroscopic eclipse maps. Nat Astron published online October 28, 2025. doi: 10.1038/s41550-025-02666-9

Source: www.sci.news

Atmospheric Disturbance Caused Temperature Surge in Antarctica

The Antarctic is experiencing higher temperatures than expected

Eyal Bartov / Alamy

Since early September, air temperatures in Antarctica have soared beyond 35°C (63°F), accompanied by a significant reduction in wind speeds, with ozone depletion halting unexpectedly.

This scale of change is typically anticipated only every two decades, according to Martin Zicker from the University of New South Wales, Sydney, Australia. However, such phenomena appear to be occurring with increasing frequency, with similar transient disruptions noted last year, alongside more severe occurrences in both 2019 and 2002.

Jucker observes that four of these events have appeared within just 25 years, indicating ongoing unpredictable shifts in the global climate system.

Typically, air temperatures in Antarctica hover around -55°C (-67°F), but have been unrelentingly rising to -20°C (-4°F) since September 5th. Although still extremely cold, this shift has resulted in the polar vortex winds decreasing relatively gently to 100 km/h.

While this warming event has not yet met the formal criteria for sudden stratospheric warming, Jucker notes that for that classification to apply, the winds need to cease entirely—not just for weeks but in response to the warmth itself. He warns that the repercussions in the Southern Hemisphere could be dramatic over the ensuing months.

Initially, Australian meteorologists forecast a wetter spring than normal, but they are now signaling potential impacts from a powerful system over western Australia, likely pushing the region into warmer and drier conditions.

Unusual weather patterns may persist. Jucker indicates that one possible scenario could see a return of the polar vortex, bringing atmospheric temperatures back to their typical averages.

Conversely, the temperature anomaly might continue, with expectations of further increases up to 20°C (36°F). This could lead to erratic weather in the higher latitudes of the Southern Hemisphere.

The reason behind this anomaly remains unclear scientifically, but Jucker asserts that it’s almost guaranteed that rising sea surface temperatures in the Pacific Ocean, possibly increasing by 1°C (1.8°F) to 3.6°F, are connected.

“The presence of three significant typhoons in the Pacific can be traced to these warmer sea temperatures,” remarks Jucker. “We’ve witnessed markedly strange weather patterns over the last two years, coinciding with this substantial rise in ocean temperatures.”

Edward Dodridge from the University of Tasmania in Hobart, Australia, emphasizes the array of extreme changes occurring at the southernmost point of the globe. Recent years have seen a dramatic deceleration in sea ice loss, heatwaves, widespread breeding failures among Emperor Penguin colonies, and shifts in Antarctic circulation.

“Antarctica continues to astonish us,” he notes. “While each change is noteworthy on its own, my primary concern is witnessing shifts that not only reinforce themselves but also ripple through various components of the Antarctic ecosystem.”

“The loss of summer sea ice facilitates the fracturing of ice shelves, which in turn accelerates ocean warming. This warmer seawater melts the remaining ice shelves at an increased rate.”

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Source: www.newscientist.com

Impact of Microbiota Composition, pH, and Temperature on Key Flavor Characteristics of Premium Chocolate

Cocoa (Theobroma cacao) bean fermentation is a natural process characterized by various interactions that influence the flavor profile of high-quality chocolate. By grasping these intricate interactions, one can effectively reproduce the sought-after flavor characteristics in a controlled environment. Research utilizing bean samples fermented at Columbia Farm has demonstrated that pH, temperature, and the composition of microbiota—encompassing both bacteria and fungi—significantly impact the essential flavor qualities of premium chocolate. This discovery lays the groundwork for developing fermentation starters aimed at consistently recreating the attributes of fine chocolate.

Gopaulchan et al. We have confirmed the previously suggested role of pH and temperature variations as reliable indicators of chocolate flavor properties. Image credit: Sci.News.

The creation of fermented products like chocolate relies on the metabolic activities of microbial communities.

These communities transform raw cocoa beans into essential precursors for chocolate production.

Once harvested, cocoa beans undergo several processing stages before becoming chocolate, but fermentation remains a spontaneous process.

“The distinctive flavor of chocolate is shaped by the fermentation of cocoa beans,” stated a representative from University of Nottingham.

“In contrast to the fermentation of wine, cheese, or dough, where specific microorganisms are added to enhance flavor, cocoa bean fermentation occurs naturally, and the microorganisms involved are not well understood.”

“The flavor profile of the beans is closely tied to the geographical location of the farm, resulting in variations in chocolate quality and taste.”

In this research, Dr. Castrillo and co-authors performed DNA sequence-based analyses on fermented cocoa beans from three separate farms in Colombia.

They discovered that a unique microbial community underpins the distinctive fermentation processes at Antioch farms, yielding a superior flavor, as validated by professional tasters.

By analyzing sequencing data, the authors identified the microbial interactions and metabolic pathways involved in fermentation.

This allowed for the design of microbial communities that could mimic the exquisite flavor of chocolate in laboratory settings. This was confirmed through evaluations by the same expert tasters and chocolate metabolite analyses.

Further studies could inform the development of industrial fermentation starters, eliminating the geographical limitations on chocolate flavor.

“The findings from this study enhance our understanding of how the composition of microbial communities during fermentation is a crucial factor in determining chocolate flavor properties,” stated the researchers.

“We have created a reliable methodology to design fermentation starters that facilitate the controlled domestication of the unpredictable microbial fermentations that occur on cocoa farms.”

“This paves the way for the evolution of the modern chocolate industry, akin to the beer and cheese sectors, based on regulated cocoa fermentation utilizing synthetic microbial starters that can consistently replicate the unique flavor characteristics of cocoa beans and chocolate.”

The team’s study was published in the journal Nature Microbiology this week.

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D. Gopaulchan et al. The defined microbial community recreates the attributes of finely flavored chocolate fermentation. Nat Microbiol Published online on August 18th, 2025. doi:10.1038/s41564-025-02077-6

Source: www.sci.news

Gold can raise its temperature 14 times its melting point without actually melting.

Researchers deployed lasers to overheat gold samples, measuring temperatures with ultra-bright X-ray pulses

Greg Stewart/SLAC National Accelerator Research Institute

A thin layer of wafers that fire laser shots can heat to 14 times the melting point, pushing solids well beyond predicted limits, with some solids potentially lacking any defined melting point.

Overheating is a well-known phenomenon where a solid can exceed its melting point or even its boiling point without altering its state. For instance, water heated in a microwave can reach temperatures above 100°C (212°F) if the container is smooth and undisturbed, but will boil vigorously as soon as disturbed.

Many physicists have suggested an upper overheating limit of approximately three times the standard melting point in Kelvin, termed the entropy catastrophe. This occurs because the entropy, often viewed as the degree of disorder in a system, is greater when the material transitions to a liquid state. Remaining solid at temperatures above this point contradicts the second law of thermodynamics.

Recently, Thomas White from the University of Nevada, Reno, and his team found that gold can heat up to 14 times its melting point, exceeding even the entropy catastrophe.

White and his colleagues directed a powerful laser at a 50-nanometer-thick gold sheet for 45 seconds, then measured the temperature using reflective X-rays through a novel approach. By analyzing shifts in the frequency of the reflected X-rays, they determined the excess energy transferred to the gold, allowing them to calculate the heating effect on the sheet.

“The temperatures we measured were astonishingly high,” White remarked.

After ensuring no errors in their measurements, White and his team revisited existing theories, realizing that the rapid heating of gold likely reduced the solid’s entropy compared to its potential liquid state, surpassing predicted temperature limits. “It’s crucial to state that we haven’t violated the second law of thermodynamics,” White clarified.

The actual limitations of overheating are still open questions, he noted. “I may have thought the overheating limit was resolved in the 1980s, but now I believe it’s a question worthy of further exploration. Can we heat materials beyond their melting point?”

Utilizing this X-ray technology for measuring solid heating may also help simulate the effects of extreme heat and pressure from planetary interiors on materials within very short timescales, according to Sam Vinco at Oxford University. “Currently, there isn’t an effective thermometer for solids that operates on such brief timescales,” he noted.

It will also be fascinating to ascertain if this phenomenon applies to other solids beyond gold, Vinco stated, particularly regarding whether there’s a limit to heating before melting occurs. “What’s captivating is considering whether rapid heating could essentially circumvent traditional thermodynamic principles,” he added.

Source: www.newscientist.com

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Giant Atoms Kept “Confined” for Record Durations at Room Temperature

Manipulating Giant Atoms for Enhanced Quantum Computing

koto_feja/istockphoto/getty images

Recently, giant atoms have emerged as prime candidates for the development of advanced quantum simulators and computers, thanks to researchers demonstrating control over them for an extended period in room temperature environments.

Using electromagnetic pulses or laser light, scientists can modify the quantum properties of an atom—allowing for the adjustment of electron energy to encode information. Manipulating thousands of such atoms paves the way for constructing a quantum computer or simulating unusual quantum materials. However, spontaneous state changes in atoms can cause errors, with these atoms being controllable only within a limited “lifetime,” previously recorded at up to 1400 seconds. Despite advancements in trapping atoms longer, these methods typically required refrigeration systems, leading to logistical hurdles.

Zhenpu Zhang and Cindy Regal, along with their colleagues at the University of Colorado Boulder, have shattered previous room temperature records by employing Rydberg atoms. These atoms have outer electrons positioned far from the nucleus, resulting in a larger atomic diameter. The research team successfully loaded these atoms into a vacuum chamber, effectively blocking interfering air particles and employing laser-based “optical tweezers” for precise atom manipulation. This technique is standard for controlling Rydberg atoms, noted for their sensitivity to electromagnetic fields and light.

The team enhanced their setup by adding a copper layer inside the container, which they cooled to -269°C (-452°F). This cooling shields the atoms from thermal interference that could alter their states. Additionally, Zhang explains that air particles condense onto the copper walls, akin to how water droplets form on cold surfaces, further improving the vacuum within the chamber. Consequently, they managed to maintain control of approximately 3000 seconds (or 50 minutes), which is nearly double that achieved in previous experiments.

Zhang has been developing this innovative setup for five years from the ground up. Regal adds, “This represents a significant evolution in how we approach these experiments.”

Clement Sayrin of the Kastler Brossel Laboratory in France emphasized that this new methodology may facilitate manipulating even more atoms. “3000 seconds is quite impressive. Achieving such extended lifetimes for these atoms demands considerable effort,” he states. However, as the number of atoms in the chamber increases, so does the requirement for additional lasers to control them, potentially shortening the atomic lifespans and introducing further engineering challenges, according to Sayrin.

Topics:

  • Quantum Computing/
  • Quantum Physics

Source: www.newscientist.com

Research on the various cloud layers, temperature hot spots, and shifting chemistry found in the extraterrestrial realm

New observations from the NASA/ESA/CSA James Webb Space Telescope support the presence of three specific functions in the atmosphere (clouds, hot spots, and changes in carbon chemistry) of the rapidly rotating and free floating planetary mass object SIMP J013656.5+093347.

Impressions of the artist of SIMP 0136. Image credits: NASA/ESA/CSA/J. Olmsted, Stsci.

SIMP J013656.5+093347 (SIMP 0136 for short) is a rapidly rotating, free-floating object located just 20 light years from Earth.

It may have a mass of 13 Jupiter masses, does not orbit the star, and instead may be a brown dwarf.

Because it is separated, SIMP 0136 can be directly observed and is not afraid of mild contamination or variability caused by the host star.

The short rotation period, only 2.4 hours, allows for very efficient investigation.

“We've been working hard to get into the world,” said Allison McCarthy, a doctoral student at Boston University.

“We also thought that it might have an effect on temperature fluctuations, chemical reactions, and perhaps the activity of the aurora affecting brightness, but we weren't sure.”

Webb's NirSpec Instruments We captured thousands to 5.3 micron spectra of SIMP 0136. The object completed one full rotation, so I captured it one at a time, one at a time, one at a time, one at a time, over 3 hours.

This led to immediate observation Webb's Milli Musical Instrumentshundreds of measurements of light between 5 and 14 microns were collected. One is one every 19.2 seconds, one in another rotation.

The results were hundreds of detailed rays, each showing a very accurate wavelength (color) brightness change, with different sides of the object rotating into view.

“It was incredible to see the entire range of this object change over a few minutes,” said Dr. Joanna Foss, an astronomer at Trinity College Dublin.

“Until now, we only had a small near-infrared spectrum from Hubble, but we had some brightness measurements from Spitzer.”

Astronomers almost immediately noticed that there were several distinct ray shapes.

At any time, some wavelengths were growing brightly, while others were either dimmed or not changing at all.

Many different factors must affect brightness variation.

“Imagine looking at the Earth from afar,” said Dr. Philip Muirhead, a former member of Boston University.

“Looking each color individually gives you a variety of patterns that tell you something about the surface and the atmosphere, even if you don't understand the individual features.”

“As the ocean rotates towards vision, blue increases. The brown and green changes tell us something about the soil and vegetation.”

To understand what could cause variability in SIMP 0136, the team used an atmospheric model to show where each wavelength of light is occurring in the atmosphere.

“The different wavelengths provide information about the different depths in the atmosphere,” McCarthy said.

“We began to realize that the wavelengths that had the most similar ray shapes also investigated the same depth and reinforced this idea that they must be caused by the same mechanism.”

For example, one group of wavelengths occurs deeply in the atmosphere where there may be patchy clouds made of iron particles.

The second group comes from high clouds, which are thought to be made from small grains of silicate minerals.

Both of these light curve variations are related to the patchiness of the cloud layers.

The third group of wavelengths appears to be occurring at very high altitudes far above the clouds and tracking temperatures.

Bright hotspots may be associated with previously detected auroras at radio wavelengths, or hot gas upwelling from deeper in the atmosphere.

Some light curves cannot be explained by clouds or temperature, but instead show variations related to atmospheric carbon chemistry.

There may be chemical reactions in which carbon monoxide and carbon dioxide pockets rotate within and outside of view, or alter the atmosphere.

“We still don't understand the chemical part of the puzzle yet,” Dr. Vos said.

“But these results are really exciting because they show that the richness of molecules like methane and carbon dioxide can change over time from location.”

“If you're looking at a deplanet and only have one measurement, you should assume that it may not be representative of the entire planet.”

Survey results It will be displayed in Astrophysics Journal Letter.

____

Allison M. McCarthy et al. 2025. JWST weather report from isolated exoplanet analog SIMP 0136+0933: pressure-dependent variability driven by multiple mechanisms. apjl 981, L22; doi: 10.3847/2041-8213/AD9EAF

Source: www.sci.news

Webb verifies persistent temperature contrast on WASP-39b between morning and evening

Astronomers used the NASA/ESA/CSA James Webb Space Telescope to obtain and analyze morning and evening transmission spectra of the hot Saturn exoplanet WASP-39b, which orbits a star about 700 light-years away in the constellation Virgo. The spectrum is best explained by a model in which the evening boundary is 177 K hotter than the morning boundary.

This diagram shows what WASP-39b might look like, based on our current understanding of planets. Image credit: NASA/ESA/CSA/Webb/J. Olmsted, STScI.

WASP-39b is a hot gas giant that orbits the G7 type star WASP-39 every 4.1 days.

First discovered in 2011, this alien world has roughly the same mass as Saturn, but is 50% larger.

The planet's extreme expansion is due in part to its high temperature (about 900 degrees Celsius or 1,652 degrees Fahrenheit).

“WASP-39b has become a kind of benchmark planet for the Webb mission's exoplanet atmospheric studies,” said Dr. Nestor Espinoza, an astronomer at the Space Telescope Science Institute.

“The planet has a bulging, puffy atmosphere, so the signal coming from the starlight passing through the planet's atmosphere is quite strong.”

Webb spectra of WASP-39b's atmosphere released so far have revealed the presence of carbon dioxide, sulfur dioxide, water vapor, and sodium, and show the entire day/night boundary, without any detailed attempt to distinguish one from the other.

Now, the new analysis constructs two different spectra from the terminator region, essentially splitting the day/night boundary into two semicircles: one from the evening and one from the morning.

According to Webb's data, evenings will be much hotter, reaching a scorching 800 degrees Celsius (1,450 degrees Fahrenheit), before easing into a cooler 600 degrees Celsius (1,150 degrees Fahrenheit) in the morning.

“It's really amazing that we were able to resolve this small difference, and this is thanks to Webb's sensitivity to near-infrared wavelengths and its extremely stable photometric sensor,” said Dr. Espinoza.

“Any movement of the instrument or the observatory while collecting data would severely limit our ability to make this detection. This has to be exceptionally precise, and Webb is just that precise.”

“We don't have a planet like this in our solar system, but most of the planets we observe orbiting distant stars have shorter orbits and are closer to us, like WASP-39b,” said Dr James Kirk, astronomer at Imperial College London.

“Now we can test theories about these planets and, for the first time, directly measure the morning and evening sides of an exoplanet across a wide range of wavelengths.”

This transmission spectrum, taken with Webb's NIRSpec (Near-Infrared Spectrometer) PRISM in Bright Object Time Series mode, shows the amount of different wavelengths (colors) of near-infrared stellar light blocked by WASP-39b's atmosphere. The spectrum shows clear evidence of water and carbon dioxide on the exoplanet, as well as morning and evening temperature variations. Image credit: NASA / ESA / CSA / Webb / R. Crawford, STScI.

Extensive modeling of the resulting data will also allow researchers to investigate the structure of WASP-39b's atmosphere, its cloud cover, and why it's hotter in the evenings.

While the team plans to next investigate how cloud cover affects temperature, and vice versa, the astronomers confirmed that the main cause of WASP-39b's temperature difference is the circulation of gas around the planet.

For highly irradiated exoplanets that orbit relatively close to their stars, like WASP-39b, researchers typically expect gas to shift as the planet rotates around the star: a strong equatorial jet stream should move hotter gas on the dayside from the evening to the nightside.

Because the temperature difference is so large, the pressure difference is also large, resulting in faster wind speeds.

Using the General Circulation Model, a 3-D model similar to those used to predict weather patterns on Earth, the astronomers found that on WASP-39b, prevailing winds tend to move from the nightside across the morning boundary, around the dayside, across the evening boundary, and then back around the nightside.

As a result, the morning side of the boundary is cooler than the evening side.

In other words, the morning side is hit by winds of air cooled by the night side, and in the evening it is hit by winds of air heated by the day side.

The study suggests that wind speeds on WASP-39b could reach thousands of kilometers per hour.

“This analysis is particularly interesting because it provides previously unavailable 3D information about the planet,” Dr Espinoza said.

“The fact that it's hotter on the evening edge means that it's a bit bulging, which means that in theory there's a little swell at the boundary approaching the night side of the planet.”

of study Published in this week's journal Nature.

_____

N. Espinosa othersThe uneven boundary surface of exoplanet WASP-39b. NaturePublished online July 15, 2024; doi: 10.1038/s41586-024-07768-4

This article is based on press releases from NASA and Imperial College London.

Source: www.sci.news

At room temperature, metal-free organic molecules demonstrate strong phosphorescence

A metal-free organic 3-bromo-2-thienyl diketone exhibits fast and efficient room-temperature phosphorescence with high color purity under a variety of conditions, according to a new study led by chemists at Osaka University.

Artist's impression of fast phosphorescence. A beam of blue light enters the molecule, producing a thick yellow pillar, illustrating the acceleration of phosphorescence due to the mixing of singlet states. Image courtesy of YAP Co Ltd.

“Phosphorescence is a valuable optical feature used in applications such as OLEDs and cancer diagnostics,” said chemist Yosuke Tani of Osaka University and his colleagues.

“Until now, achieving highly efficient phosphorescence without using rare metals such as iridium or platinum has been a major challenge.”

“Phosphorescence, which occurs when a molecule goes from a high-energy state to a low-energy state, often competes with non-radiative processes where the molecule loses energy as heat,” the researchers added.

“This competition can slow down phosphorescence and make it less efficient.”

“Previous studies have shown that incorporating certain structural elements into organic molecules could make them phosphoresce faster, but these efforts have not matched the speed and efficiency of rare-metal-based materials.”

“Our breakthrough with thienyl diketones represents a major advance in this field.”

Dr. Tani and his co-authors were able to observe efficient narrowband room-temperature phosphorescence from 3-bromo-2-thienyl diketone in solution, amorphous polymer matrices, and crystalline solids.

“We discovered these molecules by chance and initially didn't understand why they performed so well,” Dr. Tani said.

“But as the research progressed, the pieces started to come together and we began to understand more.”

“Our work has led to a clearer understanding of the mechanisms behind the molecule's performance than any other organic phosphorescent material to date.”

“Still, we believe there is much more to explore and are excited about the potential applications.”

“This work provides new design guidelines for developing rare-metal-free organic phosphorescent materials, which have the potential to surpass and replace these materials in a variety of applications,” the authors conclude.

“The results of this research are expected to lead to major advances in areas such as OLEDs, lighting and medical diagnostics.”

This discovery paper In the journal Chemical Sciences.

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Yosuke Tani othersFast and efficient narrowband room-temperature phosphorescence from metal-free 1,2-diketones: rational design and mechanism. Chemical SciencesPublished online June 3, 2024; doi: 10.1039/D4SC02841D

Source: www.sci.news

January Breaks Record as Hottest Month; Global Temperature Surpasses 1.7°C Rise

Devastating wildfires break out in Chile following January's heat wave and drought

Javier Torres/AFP via Getty Images

Temperature records continue. According to the European Union's Copernicus Climate Change Agency, January this year was the hottest on record, with temperatures 1.7 degrees Celsius above the pre-industrial average.

This means there were 12 months in which the Earth's average surface temperature was more than 1.5 degrees Celsius above the average between 1850 and 1900, the pre-industrial reference point.

“2024 begins with another record month,” Samantha Burgess of the Copernicus Climate Change Service said in a statement. She said: “Rapid reductions in greenhouse gas emissions are the only way to stop global temperatures from rising.”

At the 2015 Paris Climate Conference, countries pledged to work to prevent global temperatures from rising more than 1.5 degrees Celsius above pre-industrial levels. Climate scientists will not consider this limit to have been breached until the Earth's long-term average temperature exceeds this level for many years.

The long-term average is now 1.25°C warmer than before the industrial revolution. Richard Betts At the Met Office, the UK's National Weather Service. However, carbon emissions are still increasing, and by this standard it seems certain that the 1.5°C limit will be breached soon, perhaps around 2030.

Long-term global averages are rising in line with climate model predictions. However, the extremely rapid warming over the past year or two has far exceeded expectations. Among other records, in 2023 he recorded for the first time a day warmer by 2 degrees Celsius than the average from 1850 to 1900.

It remains unclear why there has been such rapid warming over the past year or so, and how long it will continue. Factors that may have accelerated warming include the 2022 eruption of Tonga Volcano, which pumped large amounts of water into the stratosphere, and reduced aerosol pollution from ships.

For practical reasons, climate scientists have defined pre-industrial temperatures as the average from 1850 to 1900, since there are few records of temperatures before then. However, using this as a baseline could mean that the level of warming due to fossil fuel emissions is being underestimated.

One 2017 survey This indicates an error of approximately 0.2°C. Another announcement this week put the difference at 0.5°C, based on analysis of sponges, meaning we have already breached the 1.5°C limit, but other climate scientists They are not satisfied with this.

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Source: www.newscientist.com

New Low Temperature Record Set by Large Molecules

Vacuum chamber that cools four-atom molecules to near absolute zero

Max Planck Institute for Quantum Optics

The four-atom molecule is the largest uncooled molecule to just 100 billionths of a degree below absolute zero.

Techniques researchers use to cool individual atoms, such as applying lasers or magnetic forces to them, have little effect on molecules. This is especially true for molecules made up of many atoms. Because to be very cold, the molecules must be very still. The more moving parts a molecule has, the more opportunities it has to move and heat up.

“There's a joke that we study molecules not because they're easy, but because they're difficult,” he says. Luo Xinyu at the Max Planck Institute for Quantum Optics in Germany. He and his colleagues were able to make a four-atom molecule even cooler than before.

They started with thousands of molecules made up of one sodium atom and one potassium atom, trapped them in an airless chamber, and cooled them, or made them very still, with magnetic forces and bursts of light.of lowest possible temperature 0 Kelvin, or absolute zero; these molecules were only 97 billionths of a billionth of a degree Kelvin.

To turn these diatomic molecules into tetraatomic molecules, the researchers needed to combine them in pairs without warming them up. They used microwave fields to “glue” the molecules together, based on the following theoretical calculations. Tao Xi and Suey Chinese Academy of Sciences. “I didn't really know if I could put these molecules together, but Tao's team did the calculations and he said to me, 'This is possible, give it a try.'” says Luo.

Their attempt was successful. The researchers created about 1,100 molecules, each containing two potassium atoms and two sodium atoms, at a temperature of 134 billionths of a billionth of a kelvin. This is the largest molecule ever to reach this cryogenic temperature.

“One of the reasons we make molecules ultracold in the first place is so we can have more control over them, and this is a big step forward in that sense,” he says. john bourne At the University of Colorado Boulder. This new experiment is important not only because the molecules are at unprecedented temperatures, but also because at the coldest temperatures molecules can enter known quantum states and be forced into other states or processes. accuratelyhe says.

Luo says the atoms in these molecules are not “glued” to each other as strongly as the atoms in molecules at room temperature. But making them is a necessary step in studying complex chemical reactions, which are easier to observe when they are very cold and slow.

Next question is Is there something else, perhaps an even larger molecule? Using similar microwave technology, it could be made from similarly frigid materials at extremely low temperatures, he said. sebastian will At Columbia University in New York. “I think we are looking at exciting new opportunities in quantum chemistry!” he says.

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  • chemistry /
  • quantum physics

Source: www.newscientist.com

Physicists have successfully captured direct images of noble gas nanoclusters at room temperature

For the first time, physicists have directly imaged small clusters of noble gas atoms at room temperature. This result opens up exciting possibilities for fundamental research in condensed matter physics and applications in quantum information technology.

Xenon nanoclusters between two graphene layers. Sizes range from 2 to 10 atoms. Image credit: Manuel L'Engle.

“When I was researching the use of ion irradiation to modify the properties of graphene and other two-dimensional materials, I noticed something unusual. They can become trapped between the sheets,” the University of Vienna said. Dr. Jani Kotaski and his colleagues.

“This happens when noble gas ions pass through the first graphene layer fast enough to pass through, but not the second graphene layer.”

“Once trapped between the layers, the noble gases are free to move because they do not form chemical bonds.”

“But to accommodate the noble gas atoms, the graphene bends to form tiny pockets.”

“Here, two or more noble gas atoms can meet and form two-dimensional noble gas nanoclusters that are ordered and densely packed.”

The researchers' method overcomes the difficulty that noble gases do not form stable structures under experimental conditions at ambient temperatures.

“We observed these clusters using a scanning transmission electron microscope, and they are really fascinating and very fun to look at,” said Dr. Manuel L'Engle, a physicist at the University of Vienna.

“They rotate, jump, grow, and shrink as we imagine them.”

“Getting the atoms between the layers was the most difficult part of the job.”

“Achieving this gives us a simple system to study fundamental processes related to the growth and behavior of materials.”

“The next step is to study the properties of clusters containing different noble gases and how they behave at low and high temperatures,” Dr Kotasky added.

“With the use of noble gases in light sources and lasers, these new structures may enable future applications such as quantum information technology.”

a paper The findings were published in this week's magazine Natural materials.

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M. Langre other. Two-dimensional few atomic noble gas clusters within a graphene sandwich. nut.meter, published online on January 11, 2024. doi: 10.1038/s41563-023-01780-1

Source: www.sci.news

Extreme Temperature Record from 2023 to be Surpassed in 2024

The August drought in Villanueva, Spain was one of the most common extreme weather events in 2023.

Ander Girenea/AFP via Getty Images

Last year was the hottest year on record, but 2023 is unlikely to retain that dubious honor for long. In addition to warming caused by greenhouse gases, 2024 is expected to be even hotter due to the El Niño phenomenon in the Pacific Ocean. “We've never had an El Niño of this magnitude against a backdrop of global warming,” he says. adam scaife At the UK National Met Office…

Source: www.newscientist.com

New Study Finds Human Insulin is Less Sensitive to Temperature Than Previously Believed

A Cochrane review has shown that certain types of insulin can remain effective when stored at room temperature for several months, offering a practical solution for diabetes treatment in areas without stable refrigeration. This finding is particularly crucial for people with diabetes in low- and middle-income countries, as well as those affected by conflict, natural disasters, and environmental challenges.

Insulin storage options have been highlighted in the review, which summarizes the results of various studies investigating the effects of storing insulin outside the refrigerator. It was found that unopened vials and cartridges of certain types of human insulin can be stored for extended periods at temperatures up to 25°C and 37°C without any clinical consequences or loss of insulin activity. This has significant implications for people living in areas where access to refrigeration is limited.

Dr. Bernd Richter led a research team that conducted a comprehensive study on insulin stability under different storage conditions. The review analyzed 17 studies and found consistent insulin efficacy at temperatures ranging from 4°C to 37°C, providing reassurance that alternatives to powered cooling of insulin are possible without compromising its stability.

The study also identified areas for future research, such as better understanding the efficacy of insulin after storage under different conditions, studies of mixed insulin, effects of movement on insulin pumps, contamination of opened vials and cartridges, and cold environmental conditions.

The study was funded by the World Health Organization.

Source: scitechdaily.com

Uncovering the Hidden Physics of Temperature and Radiation

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A groundbreaking study investigated the complex relationship between Earth’s surface temperature and emitted longwave radiation, revealing deviations from the expected quaternary pattern. This research improves our understanding of climate sensitivity and the factors that influence it, such as greenhouse gases and atmospheric dynamics. Credit: SciTechDaily.com

Climate science research has revealed new insights into the relationship between surface temperature and emitted longwave radiation, challenging traditional models and improving our understanding of Earth’s climate sensitivity.

Want to know what causes Earth’s climate sensitivity? Recent research shows Advances in atmospheric science. We investigate a complex relationship that transforms the relationship between surface temperature and outgoing longwave radiation (OLR) from fourth-order to sublinear. Led by Dr. Jie Sun florida state university this study elucidates the hidden mechanisms that shape Earth’s climate and provides new insights into why the relationship between temperature and OLR deviates from the fourth-order pattern described by the Stefan-Boltzmann law. Masu.

Stefan-Boltzmann law and climate dynamics

What is the Stefan-Boltzmann law? Atmospheric greenhouse gases create a contrast between surface heat release and OLR, which is related to the fourth power of surface temperature.

Professor Hu Xiaoming of Sun Yat-sen University, corresponding author of the study, explained: This allows the relationship between surface temperature and OLR to follow a quartic pattern, since the radiation-emitting layer is lowered. ”

Diagram showing two main processes: sublinear surface temperature and outgoing longwave radiation (OLR). Left: Increased meridional surface temperature gradient due to the greenhouse effect of water vapor. Right: Poleward energy transport reroutes part of the OLR from warmer to colder regions. Credit: Ming Cai and Xiaoming Hu

Factors affecting surface temperature and OLR

This study reveals how various factors influence surface temperature and OLR. The water vapor greenhouse effect acts as a magnifying glass, amplifying temperature differences across the Earth’s surface without changing the latitudinal variation of the OLR. This suppresses the nonlinearity between OLR and surface temperature.

Polar energy transport, on the other hand, acts as an equalizer to harmonize temperature differences across different regions of the Earth. One of the by-products of this global heat redistribution is the rerouting of OLR from warmer to colder regions, which acts to reduce the differences in OLR between different regions. This further suppresses nonlinearities.

“Understanding these complex climate interactions is like deciphering a puzzle. Each piece brings us closer to deciphering the complexity of Earth’s climate,” said Ming Kai, a professor at Florida State University. Masu.”

By uncovering these relationships, scientists are learning more about Earth’s climate and how its complex components regulate overall climate sensitivity, i.e., not just the rate of energy output, but also where the output occurs to make significant progress in understanding.

Reference: “Sublinear relationship between planetary outward longwave radiation and surface temperature in a gray atmosphere radiative-convective transport climate model” Jie Sun, Michael Secor, Ming Cai, Xiaoming Hu, November 25, 2023. Advances in atmospheric science.
DOI: 10.1007/s00376-023-2386-1

Source: scitechdaily.com