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Webb Finds Early Galaxies Weren’t Too Big for Their Britches After All

Hundreds of small galaxies against the black background of space. Several white spiral galaxies are near image center. Most of the galaxies are various shades of orange and red, and many are too tiny to discern a shape. A handful of foreground stars show Webb's six diffraction spikes.

It got called the crisis in cosmology. But now astronomers can explain some surprising recent discoveries.

When astronomers got their first glimpses of galaxies in the early universe from NASA’s James Webb Space Telescope, they were expecting to find galactic pipsqueaks, but instead they found what appeared to be a bevy of Olympic bodybuilders. Some galaxies appeared to have grown so massive, so quickly, that simulations couldn’t account for them. Some researchers suggested this meant that something might be wrong with the theory that explains what the universe is made of and how it has evolved since the big bang, known as the standard model of cosmology.

According to a new study in the Astronomical Journal led by University of Texas at Austin graduate student Katherine Chworowsky, some of those early galaxies are in fact much less massive than they first appeared. Black holes in some of these galaxies make them appear much brighter and bigger than they really are.

“We are still seeing more galaxies than predicted, although none of them are so massive that they ‘break’ the universe,” Chworowsky said.

The evidence was provided by Webb’s Cosmic Evolution Early Release Science (CEERS) Survey , led by Steven Finkelstein, a professor of astronomy at UT Austin and study co-author.

Image A : CEERS Deep Field (NIRCam)

Black holes add to brightness.

According to this latest study, the galaxies that appeared overly massive likely host black holes rapidly consuming gas. Friction in the fast-moving gas emits heat and light, making these galaxies much brighter than they would be if that light emanated just from stars. This extra light can make it appear that the galaxies contain many more stars, and hence are more massive, than we would otherwise estimate. When scientists remove these galaxies, dubbed “little red dots” (based on their red color and small size), from the analysis, the remaining early galaxies are not too massive to fit within predictions of the standard model.

“So, the bottom line is there is no crisis in terms of the standard model of cosmology,” Finkelstein said. “Any time you have a theory that has stood the test of time for so long, you have to have overwhelming evidence to really throw it out. And that’s simply not the case.”

Efficient Star Factories

Although they’ve settled the main dilemma, a less thorny problem remains: There are still roughly twice as many massive galaxies in Webb’s data of the early universe than expected from the standard model. One possible reason might be that stars formed more quickly in the early universe than they do today.

“Maybe in the early universe, galaxies were better at turning gas into stars,” Chworowsky said.

Star formation happens when hot gas cools enough to succumb to gravity and condense into one or more stars. But as the gas contracts, it heats up, generating outward pressure. In our region of the universe, the balance of these opposing forces tends to make the star formation process very slow. But perhaps, according to some theories, because the early universe was denser than today, it was harder to blow gas out during star formation, allowing the process to go faster.

More Evidence of Black Holes

Concurrently, astronomers have been analyzing the spectra of "little red dots" discovered with Webb, with researchers in both the CEERS team and others finding evidence of fast-moving hydrogen gas, a signature of black hole accretion disks. This supports the idea that at least some of the light coming from these compact, red objects comes from gas swirling around black holes, rather than stars – reinforcing Chworowsky and their team’s conclusion that they are probably not as massive as astronomers initially thought.  However, further observations of these intriguing objects are incoming, and should help solve the puzzle about how much light comes from stars versus gas around black holes.

Often in science, when you answer one question, that leads to new questions. While Chworowsky and their colleagues have shown that the standard model of cosmology likely isn’t broken, their work points to the need for new ideas in star formation.

“And so there is still that sense of intrigue,” Chworowsky said. “Not everything is fully understood. That’s what makes doing this kind of science fun, because it’d be a terribly boring field if one paper figured everything out, or there were no more questions to answer.” The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

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View/Download the research results from the Astronomical Journal .

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Laura Betz  -  [email protected] , Rob Gutro - [email protected] NASA’s Goddard Space Flight Center , Greenbelt, Md.

Marc Airhart - [email protected] University of Texas at Austin

Christine Pulliam - [email protected] Space Telescope Science Institute , Baltimore, Md.

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ARTICLE : Webb Science - Galaxies Through Time

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The image is divided horizontally by an undulating line between a cloudscape forming a nebula along the bottom portion and a comparatively clear upper portion. Speckled across both portions is a starfield, showing innumerable stars of many sizes. The smallest of these are small, distant, and faint points of light. The largest of these appear larger, closer, brighter, and more fully resolved with 8-point diffraction spikes. The upper portion of the image is blueish, and has wispy translucent cloud-like streaks rising from the nebula below. The orangish cloudy formation in the bottom half varies in density and ranges from translucent to opaque. The stars vary in color, the majority of which have a blue or orange hue. The cloud-like structure of the nebula contains ridges, peaks, and valleys – an appearance very similar to a mountain range. Three long diffraction spikes from the top right edge of the image suggest the presence of a large star just out of view.

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Boeing’s No Good, Never-Ending Tailspin Might Take NASA With It

The Boeing CST-100 Starliner taking flight into space on a rocket.

By Clive Irving

Mr. Irving is an investigative journalist who has covered aviation and aerospace for more than 30 years.

Fifty-five years ago, when humans first walked on the moon, the Apollo 11 astronauts left Earth through the massive power of the Saturn V rocket. The greatest punch came from the rocket’s first stage, which provided 7.5 million pounds of thrust. The awesome spectacle of that first stage was thanks to the work by engineers at Boeing.

Fast forward to the present day, and here is a new spectacle in space provided by Boeing. It’s not awesome.

Two astronauts, Suni Williams and Butch Wilmore, arrived at the International Space Station on June 6 , expecting to stay for just over a week. Now they won’t be heading back to Earth until February. Their ride was on the Boeing Starliner spacecraft, now deemed by NASA to be too risky for the return trip because of a host of troublesome technical glitches.

NASA spin doctors object to headlines declaring that the astronauts are “stranded” or “stuck” in space, pointing out correctly that they are not in jeopardy.

But make no mistake: This is a fiasco. And not just because of the strain it puts on Ms. Williams and Mr. Wilmore and their families. Boeing’s engineering woes extend beyond Starliner; they threaten NASA’s bigger goals of going back to the moon through its Artemis program, for which Boeing has become an essential partner. I was told that a number of retired astronauts are increasingly troubled by Boeing’s performance. This loss in confidence helps put the entire Artemis program into a new state of uncertainty.

Consider the fact that on Aug. 7, Steve Stich, the manager for NASA’s commercial crew program, used the term “multiple failure” to describe the possible concerns he and his team were contemplating about the spacecraft’s propulsion system.

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Energy & Environmental Science

Active site switching on high entropy phosphides as bifunctional oxygen electrocatalysts for rechargeable/robust zn–air battery †.

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* Corresponding authors

a Catalonia Energy Research Institute – IREC, Sant Adria de Besòs, 08930 Barcelona, Spain E-mail: [email protected]

b Enginyeria Electrònica i Biomèdica Facultat de Física, Universitat de Barcelona, 08028 Barcelona, Spain

c Jiangsu Key Laboratory of Advanced Metallic Materials, Southeast University, Nanjing 211189, China

d Institute of Science and Technology Austria, Am Campus 1, 3400 Klosterneuburg, Austria

e Hebei Key Lab of Optic-electronic Information and Materials, College of Physics Science and Technology, Hebei University, Baoding 071002, China

f Songshan lake materials laboratory, Dongguan 523820, China

g Institut de Ciència de Materials de Barcelona (ICMAB-CSIC), Campus de la UAB, 08193 Bellaterra, Spain

h National Engineering Research Center for Marine Aquaculture, Marine Science and Technology College, Zhejiang Ocean University, Zhoushan, Zhejiang Province 316004, China

i Department of Physics, Freie Universität Berlin, Arnimallee 14, 14195 Berlin, Germany

j Materials Chemistry Group for Thin Film Catalysis – CatLab, Helmholtz-Zentrum Berlin für Materialien und Energie, Albert-Einstein-Str. 15, 12489 Berlin, Germany E-mail: [email protected] , [email protected]

k College of Mechanical and Electrical Engineering, Nanjing Forestry University, Nanjing 210037, China E-mail: [email protected]

l NOMATEN Centre of Excellence, National Centre for Nuclear Research, Otwock 05-400, Poland

m Department of Chemistry, Technische Universität Berlin, Straße des 17 Juni 135, Sekr. C2, 10623 Berlin, Germany

n ICREA, Pg. Lluis Companys 23, 08010 Barcelona, Catalonia, Spain

High-entropy materials (HEMs) offer a quasi-continuous spectrum of active sites and have generated great expectations in fields such as electrocatalysis and energy storage. Despite their potential, the complex composition and associated surface phenomena of HEMs pose challenges to their rational design and development. In this context, we have synthesized FeCoNiPdWP high entropy phosphide (HEP) nanoparticles using a low-temperature colloidal method, and explored their application as bifunctional electrocatalysts for the oxygen evolution and reduction reactions (OER/ORR). Our analysis provides a detailed understanding of the individual roles and transformations of each element during OER/ORR operation. Notably, the HEPs exhibit an exceptionally low OER overpotential of 227 mV at 10 mA cm −2 , attributed to the reconstructed HEP surface into a FeCoNiPdW high entropy oxyhydroxide with high oxidation states of Fe, Co, and Ni serving as the active sites. Additionally, Pd and W play crucial roles in modulating the electronic structure to optimize the adsorption energy of oxygen intermediates. For the ORR, Pd emerges as the most active component. In the reconstructed catalyst, the strong d–d orbital coupling of especially Pd, Co, and W fine-tunes ORR electron transfer pathways, delivering an ORR half-wave potential of 0.81 V with a pure four-electron reduction mechanism. The practicality of these HEPs catalysts is showcased through the assembly of aqueous zinc–air batteries. These batteries demonstrate a superior specific capacity of 886 mA h g Zn −1 and maintain excellent stability over more than 700 hours of continuous operation. Overall, this study not only elucidates the role of each element in HEMs but also establishes a foundational framework for the design and development of next-generation bifunctional oxygen catalysts, broadening the potential applications of these complex materials in advanced energy systems.

Graphical abstract: Active site switching on high entropy phosphides as bifunctional oxygen electrocatalysts for rechargeable/robust Zn–air battery

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Active site switching on high entropy phosphides as bifunctional oxygen electrocatalysts for rechargeable/robust Zn–air battery

R. He, S. Wang, L. Yang, S. Horta, Y. Ding, C. Di, X. Zhang, Y. Xu, M. Ibáñez, Y. Zhou, S. Mebs, H. Dau, J. N. Hausmann, W. Huo, P. W. Menezes and A. Cabot, Energy Environ. Sci. , 2024, Advance Article , DOI: 10.1039/D4EE01912A

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  • 23 August 2024

Stone Age builders had engineering savvy, finds study of 6,000-year-old monument

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Archaeologists used laser scans and diagrams from earlier excavations to investigate the construction of the Dolmen of Menga. Credit: Cavan Images/Getty

The Neolithic farmers and herders who built a massive stone chamber in southern Spain nearly 6,000 years ago possessed a good rudimentary grasp of physics, geometry, geology and architectural principles, finds a detailed study of the site.

Using data from a high-resolution laser scan, as well as unpublished photos and diagrams from earlier excavations, archaeologists pieced together a probable construction process for the monument known as the Dolmen of Menga. Their findings, published on 23 August in Science Advances 1 , reveal new insights into the structure and its Neolithic builders’ technical abilities.

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Stonehenge’s enigmatic centre stone was hauled 800 kilometres from Scotland

The dolmen pre-dates the main stone circle at Stonehenge in the United Kingdom by about 1,000 years, but the construction process described in the study would have involved similar techniques and demanded a similar level of engineering.

“These people had no blueprints to work with, nor, as far as we know, any previous experience at building something like this,” says study co-author Leonardo García Sanjuán, an archaeologist at the University of Seville in Spain. “And yet, they understood how to fit together huge blocks of stone” with “a precision that would keep the monument intact for nearly 6,000 years”.

“There’s no way you could do that without at least a basic working knowledge of science,” he adds.

Super-solid structure

To construct the dolmen, its builders transported 32 giant stone blocks from a quarry around one kilometre away and used them to form the walls, pillars and roof of a massive chamber measuring around 28 metres long, 6 metres wide and 3.5 metres high. The largest of these blocks, one of the capstones that forms part of the roof, is 8 metres long and weighs an estimated 150 tonnes. By comparison, the biggest stone used to build Stonehenge weighs about 30 tonnes.

Transporting these huge slabs from the quarry to the site without breaking them would have required particular care, the researchers say, particularly with the soft sandstone used for the roof. They suggest that this could have been done using specially built wooden tracks to reduce friction as the stones were dragged along, much as the builders of Stonehenge are thought to have done.

The interior of the Dolmen of Menga, its walls and ceilling built of stone slabs, with a central pillar.

The dolmen’s stones are fitted together with high precision, suggesting that the people who built the tomb understood principles of science and engineering. Credit: Album/Alamy

Another task that demanded precision and skill was finessing the upright slabs into sockets carved 1.5 metres deep into the bedrock. The laser scans revealed that the builders used counterweights and ramps to move the uprights carefully into the sockets, tilting them at precise, millimetre-scale angles. The stones were carved into facets that meant they locked against their neighbours when the weights and ramps were removed.

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These ancient whittled logs could be the earliest known wooden structure

“I’ve always been amazed by the engineering skills needed to build this dolmen,” says Michael Parker Pearson, an archaeologist at University College London. “This paper reveals just how precisely that has to have been done, with an extraordinary eye on dimensions and angles. With such big stones, they could not have afforded to make mistakes when manoeuvring them into position. If even just one was a few centimetres out, that would have been hard to correct once an upright stone was set in its trench.”

Parker Pearson adds that the prehistoric engineers’ understanding of physics and geometry resulted in a ‘super-solid monument’. “It’s the sort of thing we see at Stonehenge a thousand years later, with the mortise and tenon joining of uprights and lintels.”

But unlike Stonehenge, the Dolmen of Menga is in a seismically active, earthquake-prone area. Despite this, after nearly 6,000 years, the stonework is still snug and secure, says García Sanjuán. “These people really knew what they were doing.”

doi: https://doi.org/10.1038/d41586-024-02776-w

Lozano Rodríguez, J. A. et al. Sci. Adv. 10 , eadp1295 (2024).

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