- This “City-Killer” Asteroid Has a 4% Chance of Hitting the Moon SciTechDaily
- In 2032, Earth May Witness A Once-In-5,000-Year Event On The Moon IFLScience
- Toshi Hirabayashi / The Conversation Archives Popular Science
- How astronomers rank dangerous asteroids (and what that means for you) The Planetary Society
- How do scientists calculate the probability that an asteroid could hit Earth? The Fayette Advertiser
Category: 7. Science
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This “City-Killer” Asteroid Has a 4% Chance of Hitting the Moon – SciTechDaily
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Mars was once a desert with intermittent oases • The Register
New models from recent Martian probe data suggest the fourth planet from the Sun once hosted a fluctuating desert environment with intermittent oases of water.
Researchers led by the University of Chicago’s Edwin Kite found evidence for carbon dioxide cycling on the Red Planet in data from Curiosity rover. The discovery of hidden carbonates in Gale Crater potentially unlock the reason why the once warm, water-rich planet saw a thinning out of its atmosphere and a loss of liquid water on its surface.
To summarize, the researchers modelled a situation where:
- Increased solar luminosity melts water on Mars, leading to more liquid water
- The liquid water interacts with carbon dioxide in the atmosphere, which then reacts to minerals in the rocks, trapping the carbon in the rocks themselves and thus reducing the greenhouse effect, making Mars colder and dryer
- Lower volcanic activity on Mars (compared to Earth) means that this trapped carbon dioxide is not returned to the atmosphere, leading to a fluctuation desert/oases steady state, which is also driven by changes in orbit
- Over billions of years, leaking atmosphere lowers the planet’s atmospheric pressure, causing more evaporation of water (the pressure on the surface then drops below the triple point of water, when all three phases – solid, liquid, and gas can exist)
- Liquid water is no longer stable on the surface, and we get the cold, dry Mars we see today
Scientists had already digested evidence of wet and dry periods on Mars, but puzzled over what was driving the cycles and how all the liquid water ended up disappearing.
Secret was locked away in the rocks
As on Earth, atmospheric carbon dioxide on Mars can be stored in rocks as carbonates. So Kite’s team built a climate model based on the assumption that the carbonates from the Gale Crater reflect cycles on the Red Planet and let it run over 3.5 billion years.
“Past climates with surface and shallow-subsurface liquid water are recorded by Mars’s sedimentary rocks, including strata in the approximately 4-kilometer-thick [circa 2.5 miles thick] record at Gale Crater,” the paper published in Nature this week said.
“Those waters were intermittent, spatially patchy and discontinuous, and continued remarkably late in Mars’s history,” they hypothesize.
The researchers propose that carbonate formation on Mars actually helped drive changes in the planet’s climate. In their model, increasing solar luminosity makes water more available, leading to carbonate formation, which in turn, sucks carbon dioxide from the atmosphere, curtailing the greenhouse effect and leading to a colder and drier planet.
“Chaotic orbital forcing modulated wet–dry cycles. The negative feedback restricted liquid water to oases and Mars self-regulated as a desert planet. We model snowmelt as the water source, but the feedback can also work with groundwater as the water source. Model output suggests that Gale faithfully records the expected primary episodes of liquid water stability in the surface and near-surface environment,” the researchers said.
In the end, the loss of Mars’ atmosphere means it approaches water’s triple point, resulting in a reduction of liquid water and making the surface environment less habitable.
The researchers said their model can explain why oases on Mars were patchy and intermittent, but more surface missions would be required to test its assumptions.
“We assume that the carbonate content found at Gale is representative, and as a result, we present a testable idea rather than definitive evidence,” the paper said. ®
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Latest Baikonur Launch Pays Tribute to 1975 Apollo-Soyuz Mission
In July 1975, millions of people watched on television as a U.S. Apollo spacecraft docked with a Soviet Soyuz capsule in a crewed mission in orbit that symbolized collaboration between the two superpowers at the height of Cold War enmity.
That remarkable moment 50 years ago is being commemorated on a Soyuz rocket carrying a Russian cargo spacecraft that launched from the Baikonur Cosmodrome in Kazakhstan – early on Friday, Baikonur time – and is scheduled to reach the International Space Station after a two-day trip. The spacecraft is loaded with more than 2.5 tons of fuel, drinking water, food, medicine, science equipment, and other supplies for the crew on the station.
The Soyuz rocket currently heading to the ISS is painted white and blue and has an emblem marking the anniversary of the Soyuz-Apollo docking, which was the first international space mission. It had begun on July 15, 1975, when two Soviet cosmonauts launched from Baikonur and, hours later, three American astronauts blasted off from Cape Canaveral, Florida. The Russians and the Americans connected in space two days later, shaking hands, exchanging gifts, and sharing a meal.
The show of comity in space contrasted with the intense competition between the two global rivals that was known as the “space race,” which included the Soviet launch of the Sputnik satellite into orbit in 1957 and the Apollo 11 landing of American astronauts on the moon in 1969.
“I really believe that we were sort of an example … to the countries. We were a little of a spark or a foot in the door that started better communications,” Apollo astronaut Vance Brand had said, according to a NASA account of the Apollo-Soyuz mission.
Tensions between Russia and the United States escalated after Moscow launched a large-scale invasion of Ukraine in 2022, though relations improved after U.S. President Donald Trump took office for a second term in January. The U.S. and Russian space agencies have continued to collaborate over the course of the protracted war.
Roscosmos, the Russian space agency, refers to the cargo spacecraft currently in orbit as Progress MS-31, while the U.S. agency NASA uses the term Progress 92 because it’s the 92nd Russian resupply craft to launch in support of the International Space Station since its construction began in 1998. The Apollo-Soyuz mission has been described as a precursor of the ISS project.
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Drone footage reveals Australia’s “unprecedented” coral mortality
Professor Jane Williamson from the School of Natural Sciences at Macquarie University, senior author on the study, said the findings underscored the urgent need for action on climate change.
The research team used high-resolution drone imagery to map coral bleaching in March 2024, returning in June to assess survival and mortality rates across the same reef areas.
“Using drone-derived imagery, we followed the amount of bleached and living coral during and after the bleaching event,” said Professor Williamson. “Use of this technology lets us upscale the effects of the bleaching event over larger areas but still in high precision.”
The team recorded the highest coral bleaching mortality on the Great Barrier Reef, with over 92% of corals experiencing mortality.
“Our results are concerning for coral resilience, considering the increasing frequency and intensity of extreme heat events predicted for the near future, with potentially irreversible consequences for reef ecosystems such as those studied in our Great Barrier Reef,” Williamson added.
More alarming still is that coral mortality actually exceeded 99% in some areas measured.
Coral reefs at Lizard Island have experienced repeated disturbances over the past decade, including severe bleaching in 2016 and 2017, cyclones, and Crown-of-Thorns outbreaks. These events have only compounded the ecosystem’s vulnerability, despite some signs of recovery in recent years.
The team behind the assessment are now running additional surveys at Lizard Island to track the recovery, if any, of corals into 2026 as part of an Australian Museum Lizard Island Critical Grant.
Click here for more from the Oceanographic Newsroom.
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Tiandu scientists successfully prototype lunar regolith 3D printer – VoxelMatters
- Tiandu scientists successfully prototype lunar regolith 3D printer VoxelMatters
- 3D Printing On The Moon: Project Olympus parametric-architecture.com
- Who Can Build on the Moon? Understanding the Wild West of Lunar Architecture Architectural Digest
- Ceramics will be critical to the lunar economy—but we don’t know how to make them on site Phys.org
- How to make building blocks for a lunar habitat Phys.org
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Curiosity Cracked Open a Rock on Mars And Discovered a Huge Surprise : ScienceAlert
A rock on Mars spilled a surprising yellow treasure after Curiosity accidentally cracked through its unremarkable exterior.
When the rover rolled its 899-kilogram (1,982-pound) body over the fragile lump of mineral in May last year the deposit broke open, revealing yellow crystals of elemental sulfur: brimstone.
Although sulfates are fairly common on Mars, this represents the first time sulfur has been found on the red planet in its pure elemental form.
Related: Largest Mars Rock on Earth Could Sell For US$4 Million
What’s even more exciting is that the Gediz Vallis Channel, where Curiosity found the rock, is littered with objects that look suspiciously similar to the sulfur rock before it got fortuitously crushed – suggesting that, somehow, elemental sulfur may be abundant there in some places.
frameborder=”0″ allow=”accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share” referrerpolicy=”strict-origin-when-cross-origin” allowfullscreen>“Finding a field of stones made of pure sulfur is like finding an oasis in the desert,” said Curiosity project scientist Ashwin Vasavada of NASA’s Jet Propulsion Laboratory in July 2024.
“It shouldn’t be there, so now we have to explain it. Discovering strange and unexpected things is what makes planetary exploration so exciting.”
Sulfates are salts that form when sulfur, usually in compound form, mixes with other minerals in water.
When the water evaporates, the minerals mix and dry out, leaving the sulfates behind.
These sulfate minerals can tell us a lot about Mars, such as its water history, and how it has weathered over time.
The sulfur Curiosity found on Mars. (NASA/JPL-Caltech/MSSS) Pure sulfur, on the other hand, only forms under a very narrow set of conditions, which are not known to have occurred in the region of Mars where Curiosity made its discovery.
There are, to be fair, a lot of things we don’t know about the geological history of Mars, but the discovery of scads of pure sulfur just hanging about on the Martian surface suggests that there’s something pretty big that we’re not aware of.
Curiosity’s view of the Gediz Valley channel. (NASA/JPL-Caltech/MSSS) Sulfur, it’s important to understand, is an essential element for all life. It’s usually taken up in the form of sulfates, and used to make two of the essential amino acids living organisms need to make proteins.
Since we’ve known about sulfates on Mars for some time, the discovery doesn’t tell us anything new in that area. We’re yet to find any signs of life on Mars, anyway.
A rock very similar to the one broken by Curiosity, photographed nine days after the sulfur discovery. (NASA/JPL-Caltech/MSSS) But we do keep stumbling across the remains of bits and pieces that living organisms would find useful, including chemistry, water, and past habitable conditions.
Stuck here on Earth, we’re fairly limited in how we can access Mars. Curiosity’s instruments were able to analyze and identify the sulfurous rocks in the Gediz Vallis Channel, but if it hadn’t taken a route that rolled over and cracked one open, it could have been sometime until we found the sulfur.
Curiosity’s path (in yellow) towards Gediz Vallis channel (top-center). (NASA/JPL-Caltech/UC Berkeley) The next step will be to figure out exactly how, based on what we know about Mars, that sulfur may have come to be there.
That’s going to take a bit more work, possibly involving some detailed modeling of Mars’s geological evolution.
Meanwhile, Curiosity will continue to collect data on the same.
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The Gediz Vallis channel is an area rich in Martian history, an ancient waterway whose rocks now bear the imprint of the ancient river that once flowed over them, billions of years ago.
Curiosity drilled a hole in one of the rocks, taking a powdered sample of its interior for chemical analysis, and is still trundling its way deeper along the channel, to see what other surprises might be waiting just around the next rock.
An earlier version of this article was published in July 2024.
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Satellite spies both ISS and China’s Tiangong space station photo of the day for July 4, 2025
Since 1998, when the International Space Station (ISS) launched, there has been a place for astronauts around the world to run experiments in space, from growing food to learning how low-Earth orbit affects the human body.
More recently, the Chinese Tiangong Space Station was fully completed, with its third and final module, the Mengtian, added on Oct. 31, 2022. Tiangong sits at the same height as the ISS.
What is it?
The ISS is a joint venture between NASA, Roscosmos, the European Space Agency (ESA), the Japanese Aerospace Exploration Agency (JAXA) and other organizations. It’s been continuously inhabited since 2000 and serves as a microgravity laboratory for research in biology, physics, medicine and earth sciences. The ISS is significantly larger than the Tiangong Space Station, as the ISS has 16 modules while Tiangong only has three.
As China was excluded from the ISS program, it created its own space station, Tiangong, which shows the nation’s prowess in space exploration. Tiangong, which means “Heavenly Palace” in Chinese, was built by the Chinese Manned Space Agency (CMSA) and provides a platform for scientific research for countries not involved in the ISS program.
Where is it?
These two photographs were taken from space, about 250 miles (402 km) from Earth.
A comparison of the ISS (left) and the Chinese Tiangong Space Station (right) (Image credit: Maxar Technologies) Why is it amazing?
These two photos were taken by a Maxar WorldView Legion satellite from low-Earth orbit. In a tweet, Maxar Technologies discussed how their satellites could capture these images with crisp clarity as both space stations continue to move in their respective orbits.
It’s difficult to photograph something moving as quickly as the ISS or the Tiangong Space Station. The ISS orbits Earth every 90 minutes at a speed of about 17,500 mph (28,000 km/h) and the Tiangong moves at a similar rate. Being able to capture the detail on both space stations shows the timing and engineering capabilities of the Maxar satellite.
Want to learn more?
You can read more about the ISS, the Tiangong Space Station, and observation satellites as companies like Maxar continue to study Earth from space.
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Biting the ‘Bullet’: Amazing new JWST photo shows titanic collision of galaxy clusters
NASA’s James Webb Space Telescope (JWST) has produced a new image of the Bullet Cluster, which is a titanic collision between two individual galaxy clusters.
The image, produced in conjunction with NASA’s Chandra X-ray Observatory, reveals not only the location and mass of dark matter present, but also points the way toward one day figuring out what dark matter is actually made of.
In the new image, we see the hot gas within the Bullet Cluster in false-color pink, detected by Chandra. The inferred location of dark matter is represented in blue (also false color), as measured by the JWST. Note that the blue and the pink are separate — what has caused the dark matter and the gas to separate, and how were astronomers able to produce this map of the material within the Bullet Cluster?
Located 3.9 billion light-years away, the Bullet Cluster has been an occasionally controversial poster child for dark-matter studies. Back in 2006, the Hubble Space Telescope and the Chandra X-ray Observatory worked together to image the Bullet, showing the presence of its dark matter based on how light from more distant galaxies was being gravitationally lensed by the dark matter’s mass.
Collisions between galaxy clusters are the perfect laboratories for testing our ideas about dark matter, because they are nature’s way of throwing together huge amounts of the stuff. This gives us a chance to test how dark matter particles interact with each other, if at all, and the degree of any interaction would be a huge clue as to the properties of the mysterious dark matter particle.
Yet despite the dramatic Hubble and Chandra images, the Bullet Cluster — and, indeed, other galaxy cluster collisions — haven’t always played ball. For instance, the velocities at which the sub-clusters are colliding seem too high for the standard model of cosmology to explain.
Now the JWST has entered into the fray. A team led by Ph.D. student Sangjun Cha of Yonsei University in Seoul, South Korea, and professor of astronomy James Jee at both Yonsei and the University of California, Davis, have used the most powerful space telescope ever built to get a best-ever look at the Bullet Cluster.
Hubble and Chandra had previously shown that, as the two individual galaxy clusters in the Bullet Cluster collided, the galaxies and their surrounding dark matter haloes had passed right through each other. This makes sense for the galaxies — the distances between them are so great that the chance of a head-on collision between any two is slim. It also suggests that the degree with which dark matter particles interact with each other — what we refer to as their collisional cross section — is small; otherwise, the interaction would have slowed the clouds of dark matter down, and we would detect it closer to where Chandra sees the hot, X-ray emitting intracluster gas. In contrast to the dark matter, these huge gas clouds can’t get out of each other’s way, so they slam into each other and don’t progress any further.
The end result is that the hot gas is found stuck in the middle of the collision, and the galaxies and dark matter belonging to each sub-cluster are found on opposite sides, having glided right through one another.
“Our JWST measurements support this,” Jee told Space.com. “The galaxy distribution closely traces the dark matter.”
JWST was able to produce a better map of the distribution of matter, both ordinary and dark, in the Bullet Cluster by detecting, for the first time, the combined glow from billions of stars that have been thrown out of their galaxies and are now free-floating in the space between the galaxies in each sub-cluster. Cha and Jee’s team were then able to use the light from these “intracluster stars” to trace the presence of dark matter and gain a more accurate map of its distribution in the Bullet Cluster.
However, this has just raised more mysteries. The more refined map of the dark matter shows that, in the larger sub-cluster, on the left, the dark matter is arranged in an elongated, “hammerhead” shape that, according to Jee, “cannot be easily explained by a single head-on collision.”
This elongated mass of dark matter is resolved into smaller clumps centered on what we call the brightest cluster galaxies — giant elliptical galaxies that are the brightest galaxies in the sub-cluster located at its gravitational core. In contrast, the dark matter halo around the sub-cluster on the opposite side is smaller and more compact.
Cha and Jee’s team suspect that the elongated, clumpy mass of dark matter could only have formed when that particular sub-cluster, which was a galaxy cluster in its own right before the Bullet collision, underwent a similar collision and merger with another galaxy cluster billions of years before the formation of the Bullet.
The JWST and Chandra’s image of the Bullet Cluster. Pink represents hot gas, while blue is the location of dark matter. (Image credit: NASA/ESA/CSA/STScI/CXC) “Such an event would have stretched and distorted the dark-matter halo over time, resulting in the elongated morphology that we observe,” said Jee.
Despite the new discoveries such as this from JWST’s more refined observations of the Bullet cluster, it is still not enough to resolve the issue of the collision velocities of the two sub-clusters.
“Even with these updates, the required collision velocity remains high relative to expectations from cosmological simulations,” said Jee. “The tension persists and remains an active area of research.”
Dark matter makes up over a quarter of all the mass and energy in the universe, and roughly 85% of all matter, so figuring out its secrets, in particular its collisional cross-section and the cause of those high velocities, is going to be essential if we want to better understand this universe in which we live.
Alas, the JWST observations of the Bullet Cluster alone are not enough to confirm what the collisional cross-section of dark matter must be. However, they do tighten the estimate of the upper limit for the value of the cross-section, constraining the list of possibilities.
Astronomers are already in the process of rigorously measuring as many galaxy cluster collisions as possible, seen from all angles and distances, to try and constrain this value further. Gradually, we’ll be able to rule out different models for what dark matter could be, until we’re left with just a few. Coupled with experimental data from direct dark matter searches from detectors deep underground, such as the LUX-ZEPLIN experiment at the Sanford Underground Research Facility in South Dakota, we could soon be on the cusp of answering one of science’s greatest mysteries: what is dark matter?
The JWST observations were reported on June 30 in The Astrophysical Journal Letters.
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Giant radio telescope in the Utah desert could reveal hidden corners of the cosmos — and brand-new physics
A gigantic array of radio dishes proposed for the Utah desert could advance our understanding of physics and help us decode cosmic radio signals. Now, scientists have outlined how it would work.
Beginning in the 1950s, radio astronomy has opened up a powerful view into the inner workings of the universe, revealing everything from how stars form to incredible images of our galaxy’s gigantic black hole. Now, astronomers are building a gigantic array of radio dishes, called the Deep Synoptic Array 2000 (DSA-2000). The array consists of 2,000 radio dishes, each 16 feet (5 meters) across, laid out in a radio-quiet part of the Utah desert.
Now, an international team of astronomers has demonstrated how DSA-2000 will be a premier instrument for revealing some of the most hidden corners, particles and processes in the cosmos.
Because DSA-2000 will have both a wide field of view and a high resolution, it will be like the world’s ultimate digital camera but at radio frequencies, the team explained in a paper uploaded to the preprint database arXiv in May. These capabilities will allow the DSA-2000 to detect a wide variety of phenomena that are not possible with our current radio telescopes.
And there are a whole lot of unexplored radio transmissions in the universe. For example, astronomers think the vast majority of the mass of every galaxy comes in the form of dark matter, an invisible entity that has so far escaped direct detection.
One potential candidate for dark matter is called the axion, a hypothetical particle trillions of times lighter than the lightest known particles. Axions can collect around dense objects like neutron stars, and under the influence of extremely strong magnetic fields (which neutron stars have in spades), they can convert to photons with just the right frequency range that DSA-2000 could pick up those signals.
Related: ‘Staggering’ first images from Vera C. Rubin Observatory show 10 million galaxies — and billions more are on the way
Another candidate for dark matter is called the dark photon, which is like our normal, familiar photons (light particles) but … dark. Dark photons can also collect around neutron stars, where they can get whipped up into a frenzy due to the star’s extreme rotation. In a process called superradiance, the dark photons get boosted to extremely high energies, where they start to resonate with regular photons, giving off blasts of signals that could be directly detected by DSA-2000.
This means that DSA-2000 could potentially offer our first direct glimpse of a new form of matter in the universe. But that’s not all.
In 2023, astronomers with the NANOGrav experiment announced the detection of gravitational waves through pulsar timing arrays. DSA-2000 could take that one step further by precisely measuring the rotation rates of approximately 3,000 pulsars — rapidly spinning neutron stars that pulsate in regular intervals. This would allow the new instrument to find any subtle variations in the spins of pulsars, such as those due to unseen orbiting companions, like black holes or small clumps of dark matter.
Lastly, DSA-2000 could detect tens of thousands of fast radio bursts (FRBs) — tremendous explosions that manifest as blips and bloops in the radio spectrum. This unprecedented number of detections would allow scientists to build a comprehensive survey of the nearby universe, which would aid our understanding of everything from dark energy to the nature of ghostly particles called neutrinos.
The universe is trying to whisper its secrets to us. All the answers are there, if we listen carefully enough.
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The Earth Is Spinning Faster This Summer
While the shortest day of the year typically falls in winter, summer will have its fair share of abnormally short days this year. According to TimeandDate, Earth will spin unusually fast in July and August, resulting in shorter days.
From the point of view of the sun, it takes Earth roughly 86,400 seconds (24 hours) to complete one full rotation. This changes slightly from day to day, and these small variations are measured with atomic clocks. The number of milliseconds above or below 86,400 seconds is referred to as length of day.
Until 2020, the shortest length of day ever recorded was -1.05 milliseconds, meaning it took the Earth 1.05 milliseconds less than 86,400 seconds to complete one rotation. Since then, Earth has beaten this record every year, with the shortest day of all being -1.66 milliseconds.
This month,TimeandDate reports that Earth will get close to its previous record. On July 9, the length of date is expected to be -1.30 milliseconds, followed by -1.38 milliseconds on July 22 and -1.51 milliseconds on August 5.
“Nobody expected this,” Leonid Zotov, a leading authority on Earth rotation at Moscow State University, told the outlet. “The cause of this acceleration is not explained.” Zotov added that most scientists believe it is something inside the Earth. “Ocean and atmospheric models don’t explain this huge acceleration,” he said.
Despite this acceleration, Zotov predicts that Earth will slow down soon. “I think we have reached the minimum,” he told TimeandDate. “Sooner or later, Earth will decelerate.” In the meantime, scientists will continue to study the reason behind Earth’s length of day variations.
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