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Category: 7. Science

  • Here’s how astronauts will soon solve murders in space

    Here’s how astronauts will soon solve murders in space

    A confined space, a limited number of suspects, a lack of contact with the outside world. These are the makings of a juicy murder mystery.

    They’re also eerily similar to conditions aboard the International Space Station (ISS), where astronauts – highly trained personnel selected for their resourcefulness, endurance and almost impossibly cool composure – spend months on end trapped together.

    Though we like to think of Earth’s best and brightest scientists as incorruptible, who hasn’t considered murdering a co-worker from time to time? And extended stays in high-stress environments are enough to make anyone snap.

    As cosmonaut Valery Ryumin chillingly wrote in his personal diary during a stint in space in 1980: “All the necessary conditions to perpetrate a murder are met by locking two men in a cabin of 5 x 6m [18 x 20ft] for two months.”

    In the worst-case scenario where something gruesome does happen in space, we’ll want to know who did it. But we’re starting off with a disadvantage: the forensic methods we’ve developed on Earth won’t necessarily cut it in the face of low-gravity, off-planet environments.

    With civilian space travel on the horizon, some experts are calling for investment in the emerging field of astroforensics – and the first research in this area has already landed.

    So, awkwardly pull on a trench coat over your spacesuit and perch a fedora on your helmet, because it’s time to go crime-solving… in space.

    Houston, we have a homicide

    One thing investigators are sure to notice missing in their first extraterrestrial case? Gravity.

    “Gravity is all pervasive around us – it’s the number-one environmental variable that we’re always dealing with,” says Zack Kowalske, a forensic detective in the Crime Scene Investigations (CSI) Unit at Roswell Police Department in Georgia, in the US.

    His PhD research, on how environmental factors influence forensic bloodstain analysis, led him to a rather unusual question: how would blood spatter patterns change in low or zero gravity?

    Bloodstain pattern analysis is a crucial forensic tool that uses fluid dynamics, physics and mathematics to calculate the trajectory of blood droplets to understand how they hit a surface. On Earth, gravity influences that pattern. In space, however…

    Experiments to determine how blood spatter patterns change in low-gravity environments have been performed during parabolic flights in Earth’s atmosphere – Photo credit: Zack Kowalske/George Pantalos

    We generally think of space as having no gravity. But astronauts on the ISS experience microgravity, which causes weightlessness even though at the station’s altitude, gravity is still about 90 per cent of the strength as here on Earth. That’s because the station’s orbit keeps it in a state of constant falling.

    To conduct the first-ever investigation of blood stains in microgravity, Kowalske collaborated with Dr George Pantalos, a researcher specialising in space medicine at the University of Louisville.

    They performed the experiment on a parabolic flight research plane (colloquially known as a ‘vomit comet’), which alternates between soaring up and diving down to generate short periods of microgravity. During the freefall period of the flight, Pantalos used a syringe to squirt synthetic blood onto a piece of paper.

    Bloodstain analysts try to calculate the angle at which blood droplets struck a surface – known as the angle of impact – so that they can reconstruct where the blood came from.

    Unfortunately for future space detectives, it turns out that gravity is a key component in deciphering these gruesome stains.

    On Earth, when a droplet of blood strikes a flat surface, the droplet collapses and spreads out in such a way that it can be used to determine the angle of impact. The experiment performed aboard the vomit comet revealed that, without gravity, the surface tension of the droplets stops the blood from spreading across the surface.

    “When you remove gravity as a variable, the next predominant physical force that takes over is surface tension,” says Kowalske.

    Without the spread, you’re essentially left with a smaller bloodstain of questionable origins. Did the astronaut get stabbed in the ISS’s core module or while coming out of the Cupola? The tiny blood puddles on the walls will leave space detectives scratching their heads.

    Three images of fake blood spatter in an experiment. The green and yellow markings show how it bounces off in unexpected trajectories in microgravity
    Footage from the experiment showed how surface tension can prevent a blood droplet from spattering and, in the case of the droplets circled in yellow and green, bounce off in unexpected trajectories – Photo credit: Zack Kowalske/George Pantalos

    Conducting this pioneering research wasn’t without its challenges, Kowalske says – especially when the parabolic flight returns to Earth. “As soon as that microgravity arc is over, you then go into double gravity, so your stains immediately get ruined,” he explains.

    And, because of the confined space in the research aircraft, they could only investigate blood stains created just 20cm (7.8in) from the paper.

    It’s also worth noting that blood droplets have a curved trajectory on Earth, where gravity is pulling them down. In zero-g, though, blood will travel in a straight line, indefinitely, until it hits a surface.

    “Inertia is going to keep these liquid drops on a straight flight path,” Kowalske says.

    Given the long, straight modules of the ISS, this could make tracking down their point of origin even trickier. The study is an important first step towards developing accurate forensic methods for microgravity environments, but many unanswered questions remain.

    Would the trajectory of blood droplets be influenced by the air currents that circulate oxygen around the closed environment of the ISS? How does blood dry in microgravity? And would the high-tech materials used inside the spacecraft have an impact on crime scene investigations?

    Many of these surfaces are water-repelling, or ‘hydrophobic’, which would further alter how blood droplets land on a surface in space.

    Dealing with blood in other areas of evidence will be different as well. For example, a victim’s blood wouldn’t pool on the ground and, if the murderer moved around, it wouldn’t leave a trail of telling drips behind them. No need for that magnifying glass, then.

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    Ballistics report

    So, suppose there’s a large amount of untraceable blood splattered over the walls of the ISS – now what? Space detectives will be on the hunt for a murder weapon.

    Thankfully, a gunshot on the ISS would create similar evidence as it does here on Earth. When a gun is fired, the explosive reaction inside the chamber creates a “plume of gases and residues”.

    These then condense into liquid droplets and solid particles that gradually settle and cover the crime scene, says Dr Chris Shepherd, a forensic ballistics expert at the University of Kent, in the UK.

    These gunshot residues would cover the gun, the person who fired it, the victim and the crime scene. And it would be much harder for the shooter to clean away that type of evidence on the ISS, where astronauts wash with a sponge and soap, rather than showering.

    A .22 caliber bullet fired from a rifle flies through the air. This image uses polarizing interferometry to show difference in air pressure, represented by different colors of light. The clear bow wave in front of the bullet shows that it is moving faster than the speed of sound. The exact velocity of this supersonic bullet can be calculated from measurements of the bow wake angle. This image freezes the motion by using a high speed flash with a duration of 1/2,000,000th of a second.
    Gravity affects a bullet’s trajectory on Earth. But the International Space Station’s low-gravity environment could make finding a recently fired bullet, and determining it’s point of origin, a lot harder – Image credit: Science Photo Library

    Airborne residues “would persist in the atmosphere of the space station for a significant time,” Shepherd explains. They would eventually be sucked up into the station’s ventilation system and would probably be caught in filters that keep the air safe and breathable for the ISS crew.

    Space crime scene investigators could then analyse these residues to determine the type of ammunition used.

    Even here on Earth, gunshot residue analysis is a tricky business.

    “Understanding how gunshot residues transfer between items [and] how long they persist in different environments – that’s something that we still don’t properly understand down here and I think it would be an even bigger challenge up there,” says Shepherd.

    Experts think it’s likely that firing a gun on the ISS would create the same ballistic fingerprint on the bullet and inside the barrel of the gun as it does on Earth, and these unique markings could be used to link a bullet to a weapon. But for obvious safety reasons, the ISS lacks a shooting range.

    This complicates the job of ballistics experts, who wouldn’t be able to reconstruct the shooting under the same conditions they were fired under.

    Microgravity would also interfere with bullets – once fired, they’d continue in infinite straight lines, instead of a trajectory curved by Earth’s gravity. In the relatively confined space of the ISS, however, a shooting is likely to be close-range, so the lack of gravity wouldn’t interfere too much.

    The bullet would probably end up stuck in the ultra-thick walls of the space station, or bounce off them and then float around inside the cabin.

    That said, a gun probably isn’t the best choice of weapon if you wanted to commit a murder in space. “I don’t think that would be the best way to go – there’d be a lot of very obvious evidence,” says Shepherd.

    Dusting for prints

    nap on your rubber gloves – it’s time to track down the murderers’ DNA. The closed environment of the ISS could work in favour of forensic investigators in this case. Trace evidence, such as hairs or fibres, would stay on board – either at the crime scene, or trapped inside air or water filters.

    “Having a closed system could be advantageous because everything is filtered and collected, so the evidence would remain and be difficult to dispose of,” says Dr Valerie Ryder, Toxicology Lead at NASA’s Johnson Space Center.

    Better rush it to the crime lab quickly, though. DNA evidence – the gold standard in forensic investigations – is likely to degrade faster in space due to the higher levels of solar radiation.

    Forensics officer collecting evidence. Having dusted a glass with powder, the officer is using an ultraviolet (UV) torch to reveal the fingerprints.
    Light – UV or laser – can be used to detect fingerprints, if the traditional method of dusting is problematic – Photo credit: Science Photo Library

    Though we don’t currently know how long such evidence lasts on the ISS, one study has found that DNA placed on the outside of a research rocket survived launch, spaceflight and re-entry into Earth’s atmosphere, despite being exposed to solar radiation and extremely high temperatures.

    Assuming the ISS killer wasn’t wearing a spacesuit or gloves, they’d also deposit fingerprints on surfaces in the spacecraft, just like they would on Earth. But collecting that evidence would present novel challenges.

    Traditional fingerprinting uses carbon or metal-based powders, which are dusted onto a surface and stick to the moisture left behind by a person’s fingers. Another method involves releasing fumes from a heated glue onto the surface, which bonds to the fingerprints.

    Perform these investigations in microgravity, though, and the fine dust and gases would become suspended in the air, remaining on the ISS indefinitely. This could potentially become a hazard to the crew.

    Space murderers beware though. Fingerprinting in space isn’t impossible. Astroforensics teams could potentially rely on laser scanners or ultraviolet light to collect your prints (although this hasn’t yet been tested on the ISS).

    Everyone’s a suspect

    With all these unknowns in the mix and astroforensics still developing as a field, what would investigators do if a murder on the ISS happened tomorrow?

    For starters, microgravity and the recycling of air and water on the space station would make it very difficult to avoid contaminating a crime scene.

    The onboard laboratory would come in handy, giving investigators access to plenty of equipment to process evidence from the crime. They’d be able to use the scanning electron microscopes to analyse gunshot residue, mass spectrometers to identify toxic substances and sequencing equipment to identify a suspect’s DNA.

    But investigators would still be limited in their analysis and would have to send samples back to Earth for concrete conclusions.

    It would also be extremely challenging to conduct an autopsy in microgravity because – you guessed it – bodily fluids would escape and float into the air.

    Photo of an astronaut performing tests in the lab aboard the ISS
    Some analysis of DNA evidence collected from a crime scene could be performed using the lab equipment already aboard the ISS – Photo credit: NASA

    Astronauts also suffer from reduced bone mineral density due to microgravity and this could alter impact patterns, making it more difficult to identify the murder weapon.

    Another major unknown is how different types of evidence might change and degrade over time on a spacecraft.

    “[On Earth] how we measure how much time has passed between an event and a consequence is determined by environmental factors. These either behave differently or don’t exist the same way in space,” says Dr Mehzeb Chowdhury, a criminologist and criminal law barrister at Northumbria University.

    Time of death would also be particularly difficult to determine.

    Forensic scientists use several lines of evidence to estimate when death occurred. On Earth, blood starts to pool in the body as soon as the heart stops beating and these pooling patterns are used to estimate the time of death.

    But in low- or zero-gravity conditions, blood might distribute more evenly throughout the body.

    On Earth, a dead body goes through a predictable sequence of decay because of active microbes and invertebrates. If the location of the body is known, the state of decay can be used to generate a remarkably accurate estimate of when death occurred.

    But on the ISS, there are far fewer microbes and essentially no decomposing invertebrates around. This means a space murder victim’s body would decay much more slowly, making it harder to determine the time of death.

    Considering all these factors, a conniving murderer could take advantage of the uncertainty around the timing of events to create an alibi or frame someone else.

    Another major challenge for space detectives would be impartiality. Initially, everyone would be a suspect, but they’d also be the only people available to collect evidence and investigate the crime.

    That’s why “we need to leverage things like robotics [and] artificial intelligence, and be able to record evidence in non-traditional ways,” says Chowdhury. “Otherwise, any kind of investigation or outcome that comes from it will be tainted.”

    The MABMAT forensics robot
    The MABMAT rover was developed to capture 360° images and videos of crime scenes that could later be used to recreate them in virtual reality so investigators could analyse them remotely – Image credit: Dr Mehzeb Chowdhury

    In 2016, as a PhD student at Durham University, Chowdhury developed a remote imaging robot called MABMAT, designed to collect 360° videos and photographs at difficult-to-access crime scenes.

    This type of system could also be equipped with high-resolution 3D fingerprinting technology or hyperspectral imaging to detect evidence that’s not visible to the naked eye.

    Chowdhury believes robots like MABMAT will become astroforensic investigators’ trusty sidekicks, allowing “Earth-based experts to study dynamic, four-dimensional crime scenes, taking into account space, motion and time, long after the physical environment had changed.”

    Ultimately, research into the field of astroforensics has only just begun and many unanswered questions remain. That’s why experts are urging space agencies to start investing in the tools to solve extraterrestrial crimes now. “We really need to have dedicated research in this area,” says Chowdhury.

    As more people spend extended periods of time in space, it’s a tragic reality that crimes will become unavoidable. “We are, by nature, a very violent species, so it’s not unreasonable to hypothesise that we’ll be a violent species out among the stars,” says Kowalske.

    In other words, it’s essential that when the first off-planet crimes happen, space Starsky and Hutch have the tools they need to conduct a rigorous and impartial investigation, bringing justice to the Solar System and beyond…

    About our experts

    Zack Kowalske is a forensic detective in the Crime Scene Investigations (CSI) Unit at Roswell Police Department in Georgia, in the US. He also has PhD research in forensic bloodstain analysis. He has been published in the likes of Forensic Science International: Reports, Journal of Forensic Sciences and Journal of Forensic Identification.

    Dr Chris Shepherd is a forensic ballistics expert at the University of Kent, in the UK. He has been published in various scientific journals including Science & Justice: Journal of the Forensic Science Society, International Journal of Legal Medicine and Journal of Forensic Sciences.

    Dr Valerie Ryder is the Toxicology Lead at NASA’s Johnson Space Center, in the US. She’s been published in the likes of Scientific Reports, Inhalation Toxicology and Aerospace Medical Association.

    Dr Mehzeb Chowdhury is a criminologist and criminal law barrister at Northumbria University, in the UK. He is published in International Journal of Police Science and Management, Salus and Science and Justice.

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    August 4, 2025
  • There’s Only One Black Moon In 2025 And It’s Happening This Month

    There’s Only One Black Moon In 2025 And It’s Happening This Month

    We like the August sky because there are usually lots of beautiful things to see. We have had amazing solar eclipses, like the Great American Eclipse in 2017, and we will have two brilliant ones next year and the year after. The best meteor shower of the year, too, is in August: the Perseids. But today we are telling you what you are not going to see this month: the Black Moon of August 23.

    The Moon goes through phases, with the whole progression lasting around a month. When it is completely illuminated, it’s a full Moon, while its opposite is the new Moon. In the former case, the Moon is on the side of the Earth away from the Sun. In the latter case, it is closer to the Sun, so it’s in the sky during the day and invisible to us.

    The Moon goes around the Earth 12.37 times every year, so some years will have 12 new Moons (or 12 full Moons) and some years will have 13. In a more accurate approximation, there are 235 new Moons within 19 years, so seven years in every 19 will have an extra new Moon.

    The extra full Moon has been historically called a Blue Moon. Given its relative rarity, we get the expression “once in a Blue Moon”. The concept of the Black Moon originated in astrological circles centuries ago to refer to an actual real Earth satellite that was hiding in orbit around the Earth. The term has been more recently co-opted to mark a similar concept to that of the Blue Moon, but for the new Moon.

    A Blue Moon can be defined as a monthly one (the second full Moon in a calendar month) or a seasonal one (the third full Moon in a season). Similarly, you can have a monthly Black Moon, happening roughly every 29 months, and a seasonal one, happening every 33 months. The last Black Moon we had was only 8 months ago, and it was a monthly one.

    The one this month will be a seasonal one. There won’t be another Black Moon, monthly or seasonal, until 2027 – another seasonal one, following the new Moon that will cause the incredible eclipse happening on August 2, 2027.

    If we can’t see it and there is not even an eclipse this time, what is the point of knowing there’s a Black Moon? Well, the Moon is beautiful, but its brightness is also pretty annoying when you want to see the night sky – especially when you want to see stuff like meteor showers.

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    August 4, 2025
  • 3I/ATLAS Has No Visible Tail or Spectral Fingerprints of Gas Around It | by Avi Loeb | Aug, 2025

    3I/ATLAS Has No Visible Tail or Spectral Fingerprints of Gas Around It | by Avi Loeb | Aug, 2025

    Zoom image will be displayed

    Intensity maps of 3I/ATLAS from stacking datasets collected on the 4th (top row) and 29th (bottom row) of July 2025, showing no visible cometary tail. The arrows point the directions to the Sun, north, east, and the negative velocity vector of the comet as seen on the plane of the sky. (Image credit: Santana-Ros et al. 2025)

    According to new data reported in a paper that was posted today on the arXiv, 3I/ATLAS exhibits “reddening colors … with no visible tail detected.” The authors explain these features as being “likely due to viewing geometry and low dust production.”

    When I argued in an essay on July 20, 2025 that the prematurely claimed elongation in the images of 3I/ATLAS might be an artifact resulting from the motion of the object, I was attacked by bloggers which insisted that it represents evidence for a cometary tail. Now that the dust has settled, literally speaking, we can ask again: could 3I/ATLAS be something other than a comet?

    This possibility is not discussed in the new paper. The concluding sentence of the paper’s abstract states: “Continued monitoring around perihelion is necessary to track changes in activity, color, which will provide insights into the evolution of interstellar materials under solar radiation.” I wholeheartedly agree with this imperative for a simple reason. The more data we collect, the more difficult it would be for scientists to shove anomalies of 3I/ATLAS under the carpet of traditional thinking. We are used to finding icy rocks which exhibit familiar cometary tails in the solar system, but an encounter with objects from interstellar space is a blind date on astronomical scales.

    The newly inferred rotation period of 16.16 hours for 3I/ATLAS is still not statistically robust, since it was derived from an observing time window spanning only 1.5 spin periods and so it may suffer from the well-known Shannon-Nyquist uncertainty in information theory.

    Recent days led to a rise in the number of commentators who, despite not being practicing scientists, are ready to unequivocally denounce non-cometary interpretations of the data on 3I/ATLAS. The truth will be revealed in the coming couple of months as 3I/ATLAS gets closer to the Sun and its anomalies will be easier to measure. If it continues to be deficient of carbon-based molecules or a visible cometary tail, will comet experts argue that it is a dark comet as they suggested recently for 1I/`Oumuamua?

    Let me reiterate a point which is avoided by these commentators. In my first published paper on 3I/ATLAS, I showed that a rock as wide as 20 kilometers — as inferred from the brightness of 3I/ATLAS, can only be delivered from interstellar space into the inner solar system once per 10,000 years. Yet, we discovered 3I/ATLAS over the past decade. Moreover, as shown in a second paper that I wrote with Adam Hibberd and Adam Crowl, the retrograde trajectory of 3I/ATLAS is fined tuned to be in the ecliptic plane (with a probability of 0.2%), and its arrival time is fine tuned to get unusually close to Jupiter, Mars and Venus (with a probability of 0.005%). I was asked in television and radio interviews this morning (including those here and here) to rank 3I/ATLAS on the `Loeb scale’ where `0’ is a definitely natural object and `10’ is a definitely technological object. As of now, I give 3I/ATLAS a rank of 6, but noted that this rank will be time-dependent as it reflects the limited data we have so far. Asking the question: `Is 3I/ATLAS alien technology?’ should not be censored for the simple reason that we must avoid being misguided by prejudice. In science, any question is legitimate, including whether COVID-19 came from a lab leak in the Wuhan Institute of Virology rather than the Huanan wet market. The scientific method allows for all possible questions, which are later answered by collecting data and ruling out possibilities. It is anti-scientific to suppress curiosity-driven questions about anomalies before conclusive data is gathered to explain them.

    The spectroscopic data reported in the new paper on 3I/ATLAS, as well as in three previous papers (here, here and here), does not show the features expected for atomic or molecular gas in a coma. The observed reddening in the spectrum of reflected sunlight from 3I/ATLAS is commonly interpreted as dust, but it could also be associated with a red surface for the object.

    A puzzling development on social media is that advocates for the Search for Extraterrestrial Intelligence (SETI) or Unidentified Anomalous Phenomena (UAP) are both pushing back against the possibility that 3I/ATLAS might be alien technology. This resistance is contradictory to their defining commitment to be curious and agnostic about all anomalies that might be associated with extraterrestrial technologies. Gladly, this resistance has no impact on my ongoing scientific research, as I already wrote four scientific papers on 3I/ATLAS (accessible here, here, here, and here).

    All in all, the verdict will be up to data and not opinions voiced on social media. Science is fun as long as we remain open minded and view it as a learning experience and not as a tool for virtue signaling.

    Over the past day, new figures were added to the latest paper I wrote a week ago with Adam Hibberd and Adam Crowl, which suggested to probe 3I/ATLAS with the Juno spacecraft when it passes within a distance of 54 million kilometers from Jupiter on March 16, 2026. The new figures show that two impulses of thrust can bring Juno to within 10 million kilometers from the path of 3I/ATLAS, using merely 60 kilograms of propellant, only 3% of the initial fuel that Juno had at its disposal. Here’s hoping that NASA will follow on our proposal for the benefit of interstellar space archaeology. The scientific exploration of our cosmic neighborhood is young and we still have a lot to learn.

    ABOUT THE AUTHOR

    Zoom image will be displayed

    (Image Credit: Chris Michel, National Academy of Sciences, 2023)

    Avi Loeb is the head of the Galileo Project, founding director of Harvard University’s — Black Hole Initiative, director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, and the former chair of the astronomy department at Harvard University (2011–2020). He is a former member of the President’s Council of Advisors on Science and Technology and a former chair of the Board on Physics and Astronomy of the National Academies. He is the bestselling author of “Extraterrestrial: The First Sign of Intelligent Life Beyond Earth” and a co-author of the textbook “Life in the Cosmos”, both published in 2021. The paperback edition of his new book, titled “Interstellar”, was published in August 2024.

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    August 4, 2025
  • First Mixed-Species Dinosaur Herd Found in Canada Badlands

    First Mixed-Species Dinosaur Herd Found in Canada Badlands | The Jerusalem Post

    Jerusalem Post/Archaeology

    In just 29 square meters researchers documented footprints from at least five ceratopsians, one ankylosaurid, one small theropod and two large tyrannosaurids moving in the same direction.

    Views of the Skyline Tracksite. shortly after discovery (A) and following excavation (B).
    Views of the Skyline Tracksite. shortly after discovery (A) and following excavation (B).
    (photo credit: Phil R. Bell, Brian J. Pickles, Sarah C. Ashby, Issy E. Walker, Sally Hurst, Michael Rampe et al.)
    ByJERUSALEM POST STAFF
    AUGUST 4, 2025 19:25

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    August 4, 2025
  • Why a NASA satellite that scientists and farmers rely on may be destroyed on purpose

    The Trump administration has asked NASA employees to draw up plans to end at least two major satellite missions, according to current and former NASA staffers. If the plans are carried out, one of the missions would be permanently terminated, because the satellite would burn up in the atmosphere.

    The data the two missions collect is widely used, including by scientists, oil and gas companies and farmers who need detailed information about carbon dioxide and crop health. They are the only two federal satellite missions that were designed and built specifically to monitor planet-warming greenhouse gases.

    It is unclear why the Trump administration seeks to end the missions. The equipment in space is state of the art and is expected to function for many more years, according to scientists who worked on the missions. An official review by NASA in 2023 found that “the data are of exceptionally high quality” and recommended continuing the mission for at least three years.

    Both missions, known as the Orbiting Carbon Observatories, measure carbon dioxide and plant growth around the globe. They use identical measurement devices, but one device is attached to a stand-alone satellite while the other is attached to the International Space Station. The standalone satellite would burn up in the atmosphere if NASA pursued plans to terminate the mission.

    NASA employees who work on the two missions are making what the agency calls Phase F plans for both carbon-monitoring missions, according to David Crisp, a longtime NASA engineer who designed the instruments and managed the missions until he retired in 2022. Phase F plans lay out options for terminating NASA missions.

    Crisp says NASA employees making those termination plans have reached out to him for his technical expertise. “What I have heard is direct communications from people who were making those plans, who weren’t allowed to tell me that that’s what they were told to do. But they were allowed to ask me questions,” Crisp says. “They were asking me very sharp questions. The only thing that would have motivated those questions was [that] somebody told them to come up with a termination plan.”

    Three other academic scientists who use data from the missions confirmed that they, too, have been contacted with questions related to mission termination. All three asked for anonymity because they are concerned that speaking about the mission termination plans publicly could endanger the jobs of the NASA employees who contacted them.

    Two current NASA employees also confirmed that NASA mission leaders were told to make termination plans for projects that would lose funding under President Trump’s proposed budget for the next fiscal year, or FY 2026, which begins Oct. 1. The employees asked to remain anonymous, because they were told they would be fired if they revealed the request.

    Congress funded the missions and may fund them again

    Presidential budget proposals are wish lists that often bear little resemblance to final congressional budgets. The Orbiting Carbon Observatory missions have already received funding from Congress through the end of the 2025 fiscal year, which ends Sept. 30. Draft budgets that Congress is currently considering for next year keep NASA funding basically flat. But it’s not clear whether these specific missions will receive funding again, or if Congress will pass a budget before current funding expires on Sept. 30.

    Last week, NASA announced it will consider proposals from private companies and universities that are willing to take on the cost of maintaining the device that is attached to the International Space Station, as well as another device that measures ozone in the atmosphere.

    NASA did not respond to questions from NPR about whether other missions will also be privatized, or about why the agency is making plans to potentially terminate projects that may receive funding in Congress’ next budget.

    In July, congressional Democrats sent a letter to acting NASA Administrator Sean Duffy warning his agency not to terminate missions that Congress has funded, and arguing that the White House Office of Management and Budget (OMB), and its director, Russ Vought, are overstepping by directing NASA and other agencies to stop spending money that Congress has already appropriated.

    “Congress has the power of the purse, not Trump or Vought,” said Rep. Zoe Lofgren, D-Calif., one of the authors of the letter and the ranking Democrat on the House Committee on Science, Space and Technology in an email to NPR. “Eliminating funds or scaling down the operations of Earth-observing satellites would be catastrophic and would severely impair our ability to forecast, manage, and respond to severe weather and climate disasters. The Trump administration is forcing the proposed cuts in its FY26 budget request on already appropriated FY25 funds. This is illegal.”

    A spokesperson for OMB told NPR via email that “OMB had nothing to do with NASA Earth Science leadership’s request for termination plans.” The White House Office of Science and Technology Policy did not respond to questions from NPR.

    In the past, Vought has been vocal about cutting what he sees as inappropriate spending on projects related to climate change. Before he joined the Trump administration, Vought authored sections of the Heritage Foundation’s Project 2025 roadmap for remaking the federal government. In that document, Vought wrote that “the Biden Administration’s climate fanaticism will need a whole-of-government unwinding” and argued that federal regulators should make it easier for commercial satellites to be launched.

    The data from these missions is even more valuable than intended

    The missions are called Orbiting Carbon Observatories because they were originally designed to measure carbon dioxide in the atmosphere. But soon after they launched, scientists realized that they were also accidentally measuring plant growth on Earth.

    Basically, when plants are growing, photosynthesis is happening in their cells. And that photosynthesis gives off a very specific wavelength of light. The OCO instruments in space measure that light all over the planet.

    “NASA and others have turned this happy accident into an incredibly valuable set of maps of plant photosynthesis around the world,” explains Scott Denning, a longtime climate scientist at Colorado State University who worked on the OCO missions and is now retired. “Lo and behold, we also get these lovely, high resolution maps of plant growth,” he says. “And that’s useful to farmers, useful to rangeland and grazing and drought monitoring and forest mapping and all kinds of things, in addition to the CO2 measurements.”

    For example, the U.S. Department of Agriculture and many private agricultural consulting companies use the data to forecast and track crop yield, drought conditions and more.

    The information can also help predict future political instability, since crop failures are a major driver of mass migration all over the world. For example, persistent drought in Honduras is one factor that has led many farmers there to migrate north, NPR reporting found. And damage to crops and livestock from extreme weather in Northern Africa has contributed to migration from that region. “This is a national security issue, for sure,” Crisp says.

    Carbon-monitoring satellites have revolutionized climate science

    The carbon dioxide data that the instruments were originally designed to collect has revolutionized scientists’ understanding of how quickly carbon dioxide is collecting in the atmosphere.

    That’s because measuring carbon dioxide with instruments in various locations on the Earth’s surface, as scientists have been doing since the 1950s, doesn’t provide information about the whole planet. Satellite data, on the other hand, covers the entire Earth.

    And that data showed some surprising things. “Fifty years ago we thought the tropical forests were like a huge vacuum cleaner, sucking up carbon dioxide,” Denning explains. “Now we know they’re not.”

    Instead, boreal forests in the northern latitudes suck up a significant amount of carbon dioxide, the satellite data shows. And the patterns of which areas absorb the planet-warming gas, and how much they absorb, are continuously changing as the climate changes.
    “The value of these observations is just increasing over time,” explains Anna Michalak, a climate researcher at Carnegie Science and Stanford University who has worked extensively on greenhouse gas monitoring from space. “These are missions that are still providing critical information.”

    It is expensive to end satellite missions

    The cost of maintaining the two OCO satellite missions up in space is a small fraction of the amount of money taxpayers already spent to design and launch the instruments. The two missions cost about $750 million to design, build and launch, according to David Crisp, the retired NASA engineer, and that number is even higher if you include the cost of an initial failed rocket launch that sent an identical carbon dioxide measuring instrument into the ocean in 2009.

    By comparison, maintaining both OCO missions in orbit costs about $15 million per year, Crisp says. That money covers the cost of downloading the data, maintaining a network of calibration sensors on the ground and making sure the stand-alone satellite isn’t hit by space debris, according to Crisp.
    “Just from an economic standpoint, it makes no economic sense to terminate NASA missions that are returning incredibly valuable data,” Crisp says.

    NASA’s recent call for universities and companies to potentially take over the cost of maintaining the OCO instrument attached to the International Space Station suggests the agency is also considering privatizing NASA science missions. Such partnerships raise a host of thorny questions, says Michalak, who has worked with private companies, nonprofit groups, universities and the federal government on greenhouse gas monitoring satellite projects.

    “On the one hand the private sector is really starting to have a role,” Michalak says. In recent years, multiple private groups in the U.S. have launched satellites that measure methane, a potent planet-warming gas that is poorly monitored compared to carbon dioxide.

    “Looking at it from the outside, it can look like the private sector is really picking up some of what the federal agencies were doing in terms of Earth observations,” she explains. “And it’s true that they’re contributing.” But, she says, “Those efforts would not be possible without this underlying investment from public funding.”


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    August 4, 2025
  • 3 powerful solar flares erupt in less than 24 hours, ending weeks of calm on the sun (video)

    3 powerful solar flares erupt in less than 24 hours, ending weeks of calm on the sun (video)

    After more than three weeks without a powerful solar flare, the sun has suddenly ramped up its activity, firing off three M-class solar flares in less than 24 hours.

    While the sun has been popping off plenty of smaller C-class flares lately, Sunday’s M2.9 eruption at 10:01 a.m. EDT (1401 GMT) on Aug. 3 was the first M-class flare since July 12, according to space weather website SolarHam.com’s post on X. The flare marked the end of a 22-day lull in moderate solar flare activity.

    Two more followed in rapid succession: an M2 flare at 1:05 a.m. EDT (0505) on Aug. 4 and an M1.4 peaked just 16 minutes later at 1:21 a.m. EDT (0521 GMT). All three eruptions came from sunspot region AR 4168, which rapidly developed a more complex magnetic structure over the weekend.


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    Space weather forecasters are watching for faint CMEs that could reach Earth later this week. (Image credit: Sun image captured by Daisy Dobrijevic using the Vaonis Vespera Pro. Inset image credit: NASA / SDO and the AIA, EVE, and HMI science teams, helioviewer.org)

    Solar flares are powerful bursts of radiation from the sun’s atmosphere, caused by sudden releases of magnetic energy near sunspots. They’re classified by strength into five categories: A, B, C, M, and X. Each level represents a tenfold increase in energy output. While C-class flares are generally minor, M-class flares are moderate and can sometimes disrupt radio communications. The most intense, X-class flares, have the potential to trigger widespread radio blackouts and even impact satellites and power grids on Earth.

    view of the sun showing multiple sunspot regions across the solar disk.

    A view of the sun captured on Aug. 3, from the U.K using Vaonis Vespera Pro. (Image credit: Daisy Dobrijevic)

    According to Spaceweather.com, both active regions 4168 and 4167 now harbor unstable “delta-class” magnetic fields, an arrangement known to power strong solar eruptions, including potential X-class flares and Earth-directed coronal mass ejections (CMEs).

    So far, no major space weather impacts have been confirmed, but the M2.9 flare may have launched a weak CME toward Earth. Vincent Ledvina, an aurora chaser and space physics student, noted on X that modeling suggests the CME could arrive around midnight UTC on Aug. 7, with only a 12% chance of impact.

    Looks like our M2.9 CME has been modeled by HUXt. Earth impact around August 7 midnight UTC with a 12% hit chance, so nothing worth getting hyped up about. Still, it’s good to know what’s coming, especially as we gear up for a high-speed stream later this week. pic.twitter.com/ux3U2aBnJjAugust 4, 2025

    Ledvina added that Monday morning’s M2 flare may have triggered a second weak CME, possibly a stealth CME, a slow and faint solar ejection that’s notoriously hard to spot. “This now marks the second Earth-directed CME from this region with potentially more to follow,” he wrote.

    Breaking space news, the latest updates on rocket launches, skywatching events and more!

    Developing: AR 4168 has just generated a potentially Earth-directed (weak) stealth CME as it fired off an M2.0 solar flare. More info to come later, but this now marks the second Earth-directed CME from this region with potentially more to follow. pic.twitter.com/atfutUH42UAugust 4, 2025

    Space weather forecaster Sara Housseal declared “Flare drought is over!” in a post after Sunday’s flare. While the eruptions are “likely nothing significant,” she added later in another post that they “could result in a bump in activity in a few days,” highlighting the challenges space weather forecasters face when working with “little to no data.” A limitation that stems from the lack of dedicated satellites and limited real-time imagery available to monitor faint, slow-moving CMEs.

    Space weather forecasters are keeping a close eye on sunspot region 4168. Its growing complexity and flaring activity suggest the region may still have more surprises in store.

    Keep up with northern lights forecasts and geomagnetic activity warnings with our aurora forecast live blog.


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    August 4, 2025
  • Nanophotonic devices rewrite the rules of light manipulation

    Nanophotonic devices rewrite the rules of light manipulation

    Nanophotonics focuses on controlling how light moves through tiny structures. Usually, these structures have fixed optical properties set during manufacturing. But quantum materials, because of their complex internal behaviors, could allow us to adjust how light behaves in these devices without changing their physical design.

    In a leap toward smarter, smaller light-controlling tech, MIT scientists have developed a new nanophotonics platform that bends the rules of modern optics. By manipulating light at the scale of billionths of a meter, they’ve created ultracompact optical devices that are not only tiny and energy-efficient but also flexible, able to switch between different light modes on demand.

    This kind of dynamic tunability has long been a missing piece in nanophotonics. Now, thanks to clever engineering and quantum materials, it’s becoming a reality.

    This breakthrough brings us closer to a future where light-based devices are not just tiny and mighty, but also smart. Imagine optical components that can reprogram themselves on the fly, adapting to changes in their environment without needing to be rebuilt.

    The nanophotonics orchestra presents: Twisting to the light of nanoparticles

    That’s the promise of combining quantum materials, which have rich and tunable properties, with the precision of nanophotonics, the science of sculpting light at the nanoscale.

    Nanophotonics primarily utilizes materials such as silicon to construct tiny structures that control light. These materials work well but have two significant limits: they don’t bend light very strongly, and once the device is made, its behavior can’t be changed without rebuilding it. Tunability is the secret sauce behind tomorrow’s photonics. It enables devices to adapt in real time, altering their imaging, sensing, light emission, and even learning capabilities, much like neural networks composed of photons.

    Chromium sulfide bromide (CrSBr) is a quantum material that solves key problems in nanophotonics. It interacts strongly with light thanks to excitons, tiny light-sensitive particles, and responds to magnetic fields, making it easy to control. Its high refractive index lets scientists build ultra-thin optical structures, far slimmer than those made with traditional materials.

    MIT researchers showed that by applying a small magnetic field, they could smoothly and reversibly change how light moves through CrSBr, without needing moving parts or temperature changes. This works because CrSBr’s refractive index shifts dramatically under magnetism, far more than in typical materials.

    Electronics at the speed of light

    CrSBr also creates polaritons, hybrid particles made of light and matter, that unlock new behaviors like stronger light interactions and quantum-level control. Unlike other systems, CrSBr does this naturally, without needing bulky optical cavities.

    Even better, CrSBr can be added to existing photonic circuits, making it a practical tool for building smarter, tunable optical devices.

    MIT’s results with CrSBr were achieved at very cold temperatures, around 132 kelvins. While that’s below room temperature, the material’s exceptional tunability makes it ideal for advanced applications like quantum simulation and reconfigurable light systems, where cryogenic setups are acceptable. According to researchers, CrSBr is so special that the cold is worth it. Still, the team is looking into similar materials that work at warmer, more practical temperatures.

    Journal Reference

    1. Demir, A.K., Nessi, L., Vaidya, S. et al. Tunable nanophotonic devices and cavities based on a two-dimensional magnet. Nat. Photon. (2025). DOI: 10.1038/s41566-025-01712-2

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    August 4, 2025
  • Programmable Chromosome Engineering systems enable precise DNA manipulations

    Programmable Chromosome Engineering systems enable precise DNA manipulations

    A team of Chinese researchers led by Prof. GAO Caixia from the Institute of Genetics and Developmental Biology of the Chinese Academy of Sciences has developed two new genome editing technologies, known collectively as Programmable Chromosome Engineering (PCE) systems.

    The study, published online in Cell on August 4, achieves multiple types of precise DNA manipulations ranging from kilobase to megabase scale in higher organisms, especially plants.

    Extensive research has demonstrated the immense potential of the site-specific recombinase Cre-Lox system for precise chromosomal manipulation. However, its broader application has been hindered by three critical limitations: (1) reversible recombination reactions-stemming from the inherent symmetry of Lox sites-can negate desired edits; (2) the tetrameric nature of Cre recombinase complicates engineering efforts, hindering activity optimization; and (3) residual Lox sites after recombination may compromise editing precision.

    The research team addressed each of these challenges and developed novel methods to advance the state of this technology. First, they built a high-throughput platform for rapid recombination site modification and proposed an asymmetric Lox site design. This led to the development of novel Lox variants that reduce reversible recombination activity by over 10-fold (approaching the background level of negative controls) while retaining high-efficiency forward recombination.

    They then leveraged their recently developed AiCE (AI-informed Constraints for protein Engineering), model-a protein-directed evolution system integrating general inverse folding models with structural and evolutionary constraints-to develop AiCErec, a recombinase engineering method. This approach enabled precise optimization of Cre’s multimerization interface, yielding an engineered variant with a recombination efficiency 3.5 times that of wild-type Cre.

    Lastly, they designed and refined a scarless editing strategy for recombinases. By harnessing the high editing efficiency of prime editors, they developed Re-pegRNA, a method that uses specifically designed pegRNAs to perform re-prime editing on residual Lox sites, precisely replacing them with the original genomic sequence, thereby ensuring seamless genome modifications.

    The integration of these three innovations led to the creation of two programmable platforms, PCE and RePCE. These platforms allow flexible programming of insertion positions and orientations for different Lox sites, enabling precise, scarless manipulation of DNA fragments ranging from kilobase to megabase scale in both plant and animal cells. Key achievements include: targeted integration of large DNA fragments up to 18.8 kb, complete replacement of 5-kb DNA sequences, chromosomal inversions spanning 12 Mb, chromosomal deletions of 4 Mb, and whole-chromosome translocations.

    As a proof of concept, the researchers used this technology to create herbicide-resistant rice germplasm with a 315-kb precise inversion, showcasing its transformative potential for genetic engineering and crop improvement.

    This pioneering work not only overcomes the historical limitations of the Cre-Lox system but also opens new avenues for precise genome engineering in a variety of organisms.

    Source:

    Chinese Academy of Sciences

    Journal reference:

    Sun, C., et al. (2025). Iterative recombinase technologies for efficient and precise genome engineering across kilobase to megabase scales. Cell. doi.org/10.1016/j.cell.2025.07.011.

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    August 4, 2025
  • Science Reveals the Surprising Origins of the Potato

    Science Reveals the Surprising Origins of the Potato

    There are more than a hundred ways to prepare a potato, and thousands of stories have begun with a shot of vodka distilled from this tuber. For centuries, the potato has been instrumental in feeding the world’s growing population. According to one study, the introduction of the potato from the Americas accounted for about a quarter of the population growth in the Old World between 1700 and 1900.

    Now, science reveals the vegetable’s surprising origins: It emerged 9 million years ago as a result of an unusual hybridization between an ancestor of the tomato and an ancient South American plant. This revelation rewrites the evolutionary history of one of the world’s most widely consumed foods and also explains how a simple tuber became a mainstay of the global diet.

    Researchers at the Chinese Academy of Agricultural Sciences conducted the most extensive genomic analysis to date on the domesticated potato. They studied cultivated varieties along with 44 wild species, conducting unprecedented genetic sequencing. The results revealed a stable mixture of genetic material between Solanum tuberosum (the traditional potato) and an ancestor of Solanum lycopersicum (the tomato).

    The finding suggests that potatoes as we know them today arose from a process of hybridization between an ancient tomato plant and other Solanum-related species from the Etuberosum family that, until then, did not produce tubers. The results have been published in the journal Cell.

    Both the potato and the tomato share a common ancestor that lived about 13 million years ago. Four million years later, their descendants successfully interbred. From this union emerged a new plant with the ability to form tubers: subway structures that store energy in the form of carbohydrates and allow reproduction without the need for seeds or pollination. This biological innovation facilitated the expansion of the first potatoes into regions with diverse climates, from warm to cold environments.

    The study also identified revealing genetic details. The SP6A gene, considered the “switch” that determines whether a plant will develop tubers, comes from the tomato. On the other hand, the IT1 gene, which regulates the growth of the subway stems that form the edible tuber, comes from plants of the Etuberosum family, native to South America.

    By considering the chronology of the hybridization and the geolocation of the species involved, the researchers proposed a hypothesis about the origin of the potato. During the Miocene, between 10 and 6 million years ago, the abrupt geological uplift of the Andes, driven by the collision of two tectonic plates, generated new cold climatic regions. Scientists believe this geological change forced plants to adapt to survive and expand, with two of them joining together to form Solanum tuberosum, which millions of years later would end up accompanying your hamburger in the form of French fries.

    This story originally appeared on WIRED en Español and has been translated from Spanish.

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    August 4, 2025
  • NASA’s Artemis Crew Trains in Moonbound Orion Ahead of Mission

    NASA’s Artemis Crew Trains in Moonbound Orion Ahead of Mission

    The first crew slated to fly in NASA’s Orion spacecraft during the Artemis II mission around the Moon early next year entered their spacecraft for a multi-day training at the agency’s Kennedy Space Center in Florida. Crew donned their spacesuits July 31 and boarded Orion to train and experience some of the conditions they can expect on their mission.

    NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen participated in a suited crew test and crew equipment interface test, performing launch day and simulated orbital activities inside Orion.

    sEAN dUFFY

    acting NASA Administrator

    “In about six months, Artemis II astronauts will journey around the Moon for the first time in 53 years,” Duffy said. “America rallied behind Apollo because it represented the best of us – now it’s Artemis’ turn. They’re not just carrying a flag – they’re carrying the pride, power, and promise of the United States of America.”

    With Orion powered on, the suited crew test was a close representation of what the crew can expect on launch day. The crew began the day by suiting up inside the spaceport’s Multi-Operation Support Building, donning their Orion crew survival system spacesuits, boarding the zero-emission crew transportation vehicles, and entering Orion, which is currently inside the Multi-Payload Processing Facility, where engineers have loaded its propellants over the course of several weeks.

    Once in Orion, the crew performed several launch day activities, including communications checkouts and suit leak checks. For the first time, the crew was connected to the spacecraft and its communications and life control systems, and all umbilicals were connected while the spacecraft operated on full power.

    Teams simulated several different ground and flight conditions to give the crew more experience managing them in real time. Some of the activities simulated scenarios where the crew was challenged to address potential issues while in space such as leaks and failure of the air revitalization system fan, which is needed to provide oxygen and remove carbon dioxide from the cabin. Getting this hands-on experience and learning how to act fast to overcome potential challenges during flight helps ensure the crew is ready for any scenario.

    The test provides astronauts the ability to train on the actual hardware they will use during flight, allowing them and support teams the opportunity to familiarize themselves with the equipment in configurations very close to what will be experienced during flight. It also allows teams to verify compatibility between the equipment and systems with flight controller procedures, so they can make any final adjustments ahead of launch.

    Shawn Quinn

    Shawn Quinn

    NASA’s Exploration Ground Systems Program manager

    “It signifies the immense amount of work that our operations and development teams put into making sure we are ready for launch.” Quinn said. “They have meticulously planned each operation, timing them to perfection – and now we put it to the test.”

    Exchanging their spacesuits for cleanroom garments for the crew equipment interface test, and with the spacecraft powered off, the crew also performed many of the activities they are likely to do in flight and conducted additional equipment checks. The crew practiced removing and stowing the foot pans on the pilot and commander seats, which will allow them to have more open space in the cabin after launch. They also accessed the stowage lockers and familiarized themselves with cameras, associated cables and mounts, and the environmental control and life support system hardware.

    In addition to getting practical experience with the actual hardware they’ll use in space, they also prepared for life in deep space, reviewing cabin labels, sleep arrangements and checklists, and the hygiene bay.

    Through the Artemis campaign, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars – for the benefit of all. 

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    August 4, 2025
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