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Astronomers Produce the Largest Image Ever Taken of the Heart of the Milky Way
The central region of our Milky Way, sometimes referred to as the “Bulge,” remains something of an enigma to astronomers. Because it is densely packed with stars and clouds of dust and gas, capturing images of its interior has historically been very difficult. But with advances in radio astronomy over many decades, which can capture light that is otherwise blocked at visible wavelengths, astronomers have made some immensely fascinating finds there. In addition to the well-known supermassive black hole (SMBH), Sagittarius A*, there is chemistry at work that could shed light on the origins of life in our galaxy.
Using the Atacama Large Millimeter/submillimeter Array (ALMA), an international team of astronomers has captured the central region of the Milky Way in unprecedented detail. The image reveals a region measuring 650 light-years in diameter filled with a complex network of filaments composed of dense clouds of cosmic gas, known as the Central Molecular Zone (CMZ). As the largest ALMA image taken to date, the rich dataset will allow astronomers to examine the rich chemistry and how stars evolve in the most extreme region of our galaxy.
The research that led to this dataset was conducted by members of the ALMA CMZ Exploration Survey (ACES), a scientific collaboration of more than 160 scientists from more than 70 institutions across Europe, North and South America, Asia, and Australia. The ACES is dedicated to studying the cold gas and identifying chemical signatures in the CMZ, ranging from simple compounds (such as silicon monoxide) to complex organic molecules (such as hydrocarbons). Their work is described in a series of papers that were published in the *Monthly Notices of the Royal Astronomical Society*.
ACES is the largest survey of its kind conducted with the ALMA array toward the Galactic Center, which produced a mosaic of radio images spanning a section of night sky as big as three full Moons, positioned side-by-side. The project was instigated and led by Principal Investigator Steven Longmore, who was joined by co-PIs from each participating institution. One such person is Ashley Barnes, an astronomer at the European Southern Observatory (ESO), which oversees the ALMA array. As she described their observations of the CMZ in an ESO press release:
It’s a place of extremes, invisible to our eyes, but now revealed in extraordinary detail. The observations provide a unique view of the cold gas — the raw material from which stars form — within the so-called Central Molecular Zone (CMZ) of our galaxy. It is the first time the cold gas across this whole region has been explored in such detail. It is the only galactic nucleus close enough to Earth for us to study in such fine detail. The dataset reveals the CMZ like never before, from gas structures dozens of light-years across all the way down to small gas clouds around individual stars.
The image shows cold molecular gas flowing along filaments that feed into clumps, from which new stars are born. While astronomers understand how this process works in the outer disk of the Milky Way, the conditions in the center are far more extreme. How new stars form and evolve under such conditions is still a mystery to astronomers. With this new dataset, astronomers hope to test whether theories of star formation still apply in extreme environments. Said Longmore:
The CMZ hosts some of the most massive stars known in our galaxy, many of which live fast and die young, ending their lives in powerful supernova explosions, and even hypernovae. By studying how stars are born in the CMZ, we can also gain a clearer picture of how galaxies grew and evolved. We believe the region shares many features with galaxies in the early Universe, where stars were forming in chaotic, extreme environments.
The observations also provided a few surprises. Whereas the team anticipated that their observations would yield a high level of detail, they were still awestruck by the complexity and richness revealed in the final mosaic. This detailed survey is likely to be followed up with even more detailed observations once ALMA is upgraded, and when next-generation telescopes become operational.
“The upcoming ALMA Wideband Sensitivity Upgrade, along with ESO’s Extremely Large Telescope, will soon allow us to push even deeper into this region — resolving finer structures, tracing more complex chemistry, and exploring the interplay between stars, gas, and black holes with unprecedented clarity,” says Barnes. “In many ways, this is just the beginning.”
Further Reading: ESO
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Weaker Santa Ana winds and heat hits LA

After a very windy Saturday, weather in the region is expected to remain gusty through Sunday.
The ongoing Santa Ana winds are not forecast to “be as strong as Saturday’s,” according to the National Weather Service., but parts of L.A. County could reach both wind and heat advisory levels with 35- to 45-mph gusts and high temperatures up to 92 degrees on Sunday.
L.A. Marathon organizers implemented a new safety option for runners to finish at the 18-mile mark and still receive a finisher’s medal, if temperatures get too hot. Although elite runners have already crossed the finish line of the 26.2-mile race, competitors are expected to be on the streets of Los Angeles through the early afternoon.
The moderate Santa Ana wind event began to pick up on Friday, creating concerns in the mountains and canyon passes. Officials warned everyone to stay alert for downed trees and power lines, avoid windows during windstorms and exercise caution while traveling. On Saturday, many L.A. roads were marked by plant debris.
Several small fires broke out across the area Saturday but were knocked down within hours by responding firefighters. One of the blazes was at a three-story home in the 8500 block of W. Oak Ct. in the Hollywood Hills. The Los Angeles Fire Department said more than 100 firefighters extinguished the blaze in less than two hours and reported no injuries.
Cooler conditions are likely to settle in early this week, with another warm and dry spell expected Wednesday.
Times staff writers Grace Toohey and Alexandra Del Rosario contributed to this report.
News
Gen Z-Backed Rapper Is on Course to Lead Nepal With Landslide Win
A youth-led uprising brought Nepal’s government down last year. Now, a 35-year-old politician demanding change is set to become prime minister.
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Astronauts Use Bacteria and Fungi to Harvest Metals in Space
It’s a well-known fact that if humanity wishes to explore deep space and to live and work on other planets, we need to bring Earth’s environment with us. This includes life support systems that leverage biological processes – aka. Bioregenerative Life Support Systems (BLSS) – but also the many species of microbes that are essential to living systems. Humans already bring microbes with them when they travel to space, in particular, to the International Space Station (ISS). These microbes become part of the natural environment, sticking to surfaces, growing in nooks and crannies, and getting into everything.
Given their constant presence, it’s paramount that we understand how they survive in space. In addition, they have potential uses that could enable greater self-sufficiency in space. For example, certain types of bacteria and fungi extract minerals from rocks as a source of nutrients. In a recent study aboard the ISS, researchers from Cornell and the University of Edinburgh investigated how these species could be used to extract platinum from a meteorite under microgravity conditions. Their results suggest that this could be an effective method for obtaining mineral resources in space and lessening dependence on Earth.
The study was led by Rosa Santomartino, an assistant professor of biological and environmental engineering in Cornell’s College of Agriculture and Life Sciences (CALS), and Alessandro Stirpe, a research associate in microbiology at Cornell and the School of Biological Sciences at the University of Edinburgh. They were joined by researchers from the Medical University of Graz in Austria, Rice University, Cancer Research UK, the UK Centre for Astrobiology at the University of Edinburgh, Kayser Space Ltd, and Kayser Italia. Their study was published on Jan. 30th in npj Microgravity.
*A bioreactor, produced by the BioAsteroid project at the University of Edinburgh. Credit: University of Edinburgh*
The work was part of the BioAsteroid project, a collaborative effort between the University of Edinburgh and the European Space Agency (ESA). This project is led by Charles Cockell, a professor of astrobiology at the University of Edinburgh and a senior author on the study. Cockell and his colleagues developed “biomining reactors” that were deployed to the ISS in late 2020/early 2021 to investigate how gravity affects the interaction between microbes and rock in microgravity.
These reactors contained samples of an L-chondrite asteroid that were treated with the bacterium Sphingomonas desiccabilis and the fungus Penicillium simplicissimum. These microbes are promising for resource extraction because they produce carboxylic acids that bind to minerals and release them from rocks. However, there is still some ambiguity as to how this mechanism works. To this end, the experiment also included a metabolomic analysis, in which a portion of the liquid culture was extracted and analyzed for biomolecules and secondary metabolites. As Santomartino said in a Cornell Chronicle press release:
This is probably the first experiment of its kind on the International Space Station on [a] meteorite. We wanted to keep the approach tailored in a way, but also general to increase its impact. These are two completely different species, and they will extract different things. So we wanted to understand what and how, but keep the results relevant to a broader perspective, because not much is known about the mechanisms that influence microbial behavior in space.
The experiment was conducted aboard the ISS by NASA astronaut Michael Scott Hopkins while the researchers conducted their own control version in the lab. This allowed them to examine how the experiment would work in microgravity compared to Earth’s gravity. Santomartino and Stirpe then analyzed the experiment data, which revealed that of the 44 different elements, 18 were extracted through biological processes. Said Stirpe:
We split the analysis to the single element, and we started to ask, OK, does the extraction behave differently in space compared to Earth? Are these elements more extracted when we have a bacterium or a fungus, or when we have both of them? Is this just noise, or can we see something that maybe makes a bit of sense? We don’t see massive differences, but there are some very interesting ones.
NASA astronaut Michael Scott Hopkins performs the insertion of the experiment containers in KUBIK (left) and the six hardware units inserted into the KUBIK onboard the ISS (right). Credits: ESA/NASA/
Their analysis revealed that the microbes had consistent results in both Earth gravity and microgravity. However, it also showed distinct changes in microbial metabolism, especially with the fungus samples. In microgravity, the fungus increased its production of carboxylic acids and other molecules, leading to the extraction of more palladium, platinum, and other elements. Meanwhile, the non-biological leaching experiment proved to be less effective in microgravity than on Earth. Said Santomartino:
In these cases, the microbe doesn’t improve the extraction itself, but it’s kind of keeping the extraction at a steady level, regardless of the gravity condition. And this is not just true for the palladium, but for different types of metals, although not all of them. Indeed, another complex but very interesting result, I think, is that the extraction rate varies a lot depending on the metal you are considering and on the microbe and gravity conditions.
This experiment has successfully demonstrated the potential for “biomining,” which could be used by future astronauts exploring the Moon and Mars. In addition to life support systems that rely on cyanobacteria and other photosynthetic organisms to clean the air and generate edible algae, microbes and fungi could be used to leach minerals from the local regolith. These, in turn, could be used to generate building materials for structures and tools, reducing the amount of supplies that need to be sent from Earth.
In addition, biomining has potential applications here on Earth, providing a biological means for extracting metals in resource-limited environments or from mine waste. This technique could also lead to biotechnologies that facilitate the emergence of a zero-waste, circular economy. But the team cautions that more research is required, as there are many variables and uncertainties regarding the impact space has on microbes.
“Depending on the microbial species, depending on the space conditions, depending on the method that researchers are using, everything changes,” Santomartino said. “Bacteria and fungi are all so diverse, one to each other, and the space condition is so complex that, at present, you cannot give a single answer. So maybe we need to dig more. I don’t mean to be too poetic, but to me, this is a little bit [of] the beauty of that. It’s very complex. And I like it.”
Further Reading: Cornell Chronicle, npj Microgravity.
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