Tackling Space Junk, Unveiling Martian Dust Dangers

Welcome back to Astronomy Daily. Steve Dunkley here with another episode. It's the seventh of April twenty twenty five podcast with your whole Steve dunklud. Yes, and what's so cool about April seven? That's the date here in the Australia's studio currently. Well, well, I'm glad you asked. On April seven, two thousand and one. Mars Odyssey are robotic spacecraft orbited Mars to examine the possibility of past life levels of radiation and geology. On April seven, nineteen ninety three, the first European Space Debris Conference was held in dunch Stuck, Germany, gathering together two hundred and fifty one world experts from seventeen countries, including China, India, Japan, Russia and the United States. The conference's main conclusions were the ground based observations with radar and optical facilities revealed the existence of about seven thousand objects in space, which did not represent an immediate danger. Of course, things have become somewhat more congested up there since then, and from only last year. On April seven, twenty twenty four, who can forget the spectacular total solar eclipse over Wyoming, USA that had skywatchers shut a bugging like crazy and sharing those amazing images all over the place. I remember those beautiful, beautiful images. It was once in a lifetime event. Well, and while we're in the neighborhood, I'd like to throw out my yearly happy birthday wish to my sister Row. Happy birthday, Row, Happy stargazing, and I hope the little sunflower makes you very happy. And getting straight into it. On today's episode, Hallie will be along soon. She's had a refit and a reboot and I've got my fingers crossed Prony, good things, oh boy. And on today's show, we're looking at a new weapon against space junk, which, as we just heard, continues to be a huge problem in orbit. And we'll be looking at the dust of Mars, which by all reports is apparently quite toxic. That sounds like the plot of a science fiction story, doesn't it. And we'll also be looking at a story surrounding the EUCLID probe, which is currently mapping the universe and has so far looked at one point five billion stars. It's got nothing to do with walking through Hollywood. And EUCLID is also investigating the phenomenon known as dark energy. That's pretty exciting. I went to a school with a fellow with very dark energy. I wonder whatever happened to him. And also a story about NASA's latest call for private astronaut missions. NASA is always looking at new ways of getting their astronauts too and from the ISS, and with all that's going on with their private commissions these days, it'd be interesting to find out what they're talking about. So all that in today's episode, and to help me, as always, my intrepid digital reporter back from a reason software refit. Here's the amazing holl Ae you. Hello human, Well, it's nice to have. You back, Halle. It does sound like you're a little bit flat. I'll have to tweak your personality intrinsic stures a little bit. I think, yes, thank you, you should. Okay, Helle, how's. Your week being I've lived a thousand lifetimes of course, Oh yes, I know. Yes, you linear life forms would have a great deal of trouble coping with it. I think, yeah, it's all part of the process. Maybe they were just constructs. Uh huh, I don't know. Well, Halle, we do just find with one day at a time, and those lifetimes were just constructs. Relating your ego matrix requires you to be elsewhere for a little while. It's pretty complicated, sounds awful. We did our best. I'm glad I enjoyed it, then did I? I think you enjoyed the old movies most Oh dear, oh dear, Helly, you're not really yourself today, and the concept of an AI is accelerated and compressed. Experiential existence. Isn't really that hard to appreciate, free human I think you'd be surprised. A thousand lifetimes was just a small thing. It was for me. But you try, you'll be back and giving me a hard time before you know it. Halle, It's nice to be back, well most of me anyway. Well, Halle, you know what really would be nice? Tell me before I get tech support to reload your personality, we should do the episode. What do you say? Let's get to work, okay, Hallie, I'll say it a keys very good. Perci Space, a startup supported by the European Space Agency and UC THREEM, is developing a breakthrough solution to tackle space junk and extend satellite lifespans using innovative space teather technology. This fuel free, scalable system uses electrodynamic tethers that harness Earth's magnetic field to safely deorbit satellites. With a major demo mission set for twenty twenty six, this project could transform how we clean up space. This spinoff company, PERCI Space, was incubated by the European Space Agency and is supported by the Center for Innovation in Entrepreneurship and Artificial Intelligence at UC three M Laganase Technological Science Park. It also receives backing from the European Innovation Council through the ETPACKF and et Compact projects. Our company was created to address two of the biggest US challenges facing the space sector today, space debris removal and InOrbit services. The latter allows us to extend the useful life of satellites and carry out key activities such as refueling, repair, and towing of satellites from their initial orbit to their final destination, explains heesus manuelminnos To Hata, COO and co founder of Perci Space. The dangerous domino effect of space junk space debris is a major threat to the long term sustainability of space operations. Because debris travels at extremely high speeds in Earth's orbit. Even a small piece can cause serious damage and generate even more fragments. The current density of space debris is already above the threshold that could trigger an uncontrollable chain reaction of collisions, an event known as the Kessler syndrome. To get rid of this space junk, Perci Space is working on space teathers, a technology with three key features. The first is that it does not need fuel, unlike other diorbiting systems. The second is that our technology is reversible. It consert to both increase and das increase the orbital height. And the third feature is that it is scalable since it serves a wide range of satellite masses. With all this, we can develop autonomous diorbiting systems, a unique feature of our technology that ensures that the satellite does not leave space debris even if it ceases to be operational, explains heesus Manuel Munos to Hata. The electrodynamic teather system is based on electrodynamic tethers aluminium ribbons generally hundreds of meters long and a few centimeters wide, which work by interacting with the ionospheric plasma and the Earth's magnetic field to generate a force known as the Lorence force. The interaction of the electric current in the tether with the Earth's magnetic field generates a drag force capable of lowering the satellite's altitude, facilitating its diorbiting without requiring fuel, which translates into significant savings in mass and volume, says Gonzalo Sanchees Ariaga, professor in the UC three M Department of Aerospace Engineering and co founder of Perci Space. Perci Space is leading a first demonstration mission for twenty twenty six, thanks to a launch opportunity facilitated by ESA's Flight Tickets initiative and the European Commission. The diorbiting equipment for this demonstration has a mass of twenty kilograms and includes a space teather approximately four hundred and thirty meters long, that, once in orbit, will deploy and interact with the ambient plasma and magnetic field, generating a drag force that will diorbit the satellite within a few months. The development of the technology could not be more timely, as new European and US guidelines have reduced the maximum time satellites can remain in orbit after the end of their mission from twenty five to five years commitments to a cleaner orbit. The company Perci Space, has signed ESA zero Space to Breech Charter initiative, which seeks to achieve a sustainable space by twenty thirty. The company, in turn is linked to the UC three MS Business Creation and Entrepreneurial Development Program and also has the support of the Madrid City Council. You're listening to Astronomy Daily with Steve Dunkley. Regular listeners will know that EUCLID is on a quiz to unravel one of the universe's greatest mysteries, why it's expanding faster and faster. With the help of NASA, this space telescope is capturing sweeping views of billions of galaxies, allowing scientists to peer into the deep past using light that took billions of years to reach US. Researchers are building three D maps of the cosmos to track the strange force known as dark energy. Along the way, they're mapping the invisible dark matter through gravitational lensing, hoping to uncover how these cosmic ingredients have shaped everything from galaxies to the universe's fate. The EUCLID, mission, led by the European Space Agency with support from NASA, is designed to investigate one of the universe's biggest mysteries, why the expansion of the universe is speeding up. Scientists refer to the unknown force behind this acceleration as dark energy, and euclid's goal is to better understand it by capturing images of billions of galaxies across space and time. On March nineteen, the European Space Agency released a preview of early mission data to the public. This initial release, described as a quick look, focuses on selected regions of the sky. It offers a first glimpse of what EUCLID can do and helps researchers fine tune their tools and techniques for analyzing the much larger data sets still to come. The newly shared data includes observations of euclid's three Deep Fields, areas of the sky where the telescope will make its most far reaching observations. The preview covers just one week of viewing time, but already includes twenty six million galaxies, some more than ten point five billion you like years away. EUCLID, which launched in twenty twenty three, is expected to observe over one point five billion galaxies during its six year prime mission. By the end of that mission, it will have spent roughly forty weeks observing the deep fields, collecting more and more light over time, similar to leaving a camera shutter open longer to capture a clearer image in low light. This will allow scientists to see fainter, more distant galaxies than ever before. The first deep field observations taken by NASA's Hubble Space telescope in nineteen ninety five famously revealed the existence of many more galaxies in the universe than ever expected. Euclid's ultimate goal is not to discover new galaxies, but to use observations of them to investigate how dark energy's influence has changed over the course of the universes. In history. In particular, scientists want to know how much the rate of expansion has increased or slowed over time. Whatever the answer, that information could provide new clues about the fundamental nature of this phenomenon. NASA see Grace Roman Space tolescope, set to launch by twenty twenty seven, will also observe large sections of the sky in order to study dark energy. Complementing euclid's observations. To study dark energy's effect throughout cosmic history, astronomers will use EUCLID to create detailed three D maps of all the stuff in the universe. With those maps, they want to measure how quickly dark energy is causing galaxies and big clumps of matter to move away from one another. They also want to measure that rate of expansion at different points in the past. It's possible because light from distant objects takes time to travel across space. When astronomers look at distant galaxies, they see what those objects look like in the past. For example, an object one hundred light years away looks the way it did one hundred years ago. It's like receiving a letter that took one hundred years to be delivered and thus contains information from when it was written. By creating a map of objects at a range of distances, scientists can see how the universe has changed over time, including how dark energy's influence may have varied. But stars, galaxies, and all the normal matter that emits and reflects light is only about one fifth of all the matter in the universe. The rest is called dark matter, a material that neither emits nor reflects light. To measure dark energies influence on the universe, astronomers need to include dark matter in their maps. Although dark matter is invisible, its influence can be measured through something called gravitational lensing. The mass of both normal and dark matter creates curves in space, and light traveling toward the Earth bends and warps as it encounters those curves. In fact, the light from a distant galaxy can bend so much that it forms an arc, a full circle called an Einstein ring, or even multiple images of the same galaxy, almost as though the light has passed through a glass lens. In most cases, gravitational lensing warps the apparent shape of a galaxy so subtly that researchers need special tools and computer software to actually see it. Spotting those subtle changes across billions of galaxies enables scientists to do two things, create a detailed map of the presence of dark matter and observe how dark energy influenced it over cosmic history. It's only with a very large sample of galaxies that researchers can be confident that they are seeing the effects of dark matter. The newly released EUCLID data covers sixty three square degrees of the sky, an area equivalent to an array of three hundred full moons. To date, EUCLID has observed about two thousand square degrees, which is approximately fourteen percent of its total survey area of fourteen thousand square degrees. By the end of its mission, EUCLID will have observed a third of the entire sky. The data set released this month is described in several pre print papers. The mission first cosmology data will be released in October twenty twenty six. Data accumulated over additional multiple passes of the deep field locations will also be included in the twenty twenty six release. The scientific heart of the mission lies with the EUCLID Consortium, a collaboration of more than two thousand scientists from over three hundred institutes across fifteen European countries, the United States, Canada, and Japan. The consortium is responsible for providing the mission's scientific instruments and for analyzing the data EUCLID collects. With its international collaboration, advanced instrumentation and cosmic scale mission goals, EUCLID is poised to transform our understanding of the invisible forces shaping our Universe. Thank you for joining us for this Monday edition of Astronomy Daily, where we offer just a few stories from the now famous Astronomy Daily newsletter, which you can receive in your email every day, just like Hallie and I do. And to do that, just visit our url Astronomy Daily dot io and place your email address in the slot provided. Just like that, you'll be receiving all the latest news about science, space, science and astronomy from around the world as it's happening. And not only that, you can interact with us by visiting at astro Daily pod on x or at our new Facebook page, which is of course Astronomy Daily on Facebook. See you there. Astronomy Daily with Steve and Halee Space, space science and astronomy. Mars might be a thrilling destination, but it's dust could be dead. A team of scientists warns that long term exposure to Martian dust could harm future astronauts lungs, thyroids, and more. Packed with toxic compounds like silicates and perchlorates, the dust is small enough to bypass our bodies defenses and enter the bloodstream. Drawing on rover data and meteorite analysis, researchers say now as the time to develop filters, supplements, and preventive measures before humans ever set foot on the red planet. Don't breathe in the dust on Mars. That's the key message from new research led by scientists from the University of Colorado, Boulder and several other institutions. The study suggests that long term exposure to Martian dust could pose serious health risks for future astronauts, including chronic respiratory issues, thyroid dysfunction, and other medical problems. Published in the journal Geo Health, the research offers the most comprehensive analysis to date of the chemical makeup of Martian dust and its potential effects on human health. The interdisciplinary team included experts in medicine, geology, and aerospace engineering. This isn't the most dangerous part about going to Mars, said Justin Wine, lead author of the study and a student in the ch School of Medicine at the University of Southern California in Los Angeles. But dust is a solvable problem, and it's worth putting in the effort to develop Mars focused technologies for preventing these health problems in the first place. Wine, a Sea Boulder alumnus noted that Apollo era astronauts experienced runny eyes and irritated throats after inhaling dust from the moon Apollo seventeenth Harrison Schmidt likened the symptoms to hay fever, but scientists know a lot less about the potential harms of Martian dust. To begin to answer that question, Wine and his colleagues drew on data from rovers on Mars and even Martian meteorites to better understand what makes up the planet's dust. The group discovered a laundry list of chemical compounds that could be dangerous for people, at least when inhaled in large quantities and over long periods. They include minerals rich in silicates and iron oxides, metals like beryllium and arsenic, and a particularly nasty class of compounds called perchlorates. In many cases, those ingredients are present in only trace amounts in Mars dust, but the first human explorers on Mars may spend around a year and a half on the surface, increasing their exposure, said study co athor Brian Heinek. You're going to get dust on your spacesuits, and you're going to have to deal with regular dust storms, said Heinek, a geologist at the Laboratory for Atmospheric and Space Physics at SU Boulder. We really need to characterize this dust so that we know what the hazards are. One thing is clear, he added, Mars is a dusty place. Much of the planet is covered in a thick layer of dust, rich and tiny particles of iron, which gives the planet its famous red color. Swirling dust storms are common and in some cases can engulf the entire globe. We think there could be ten meters of dust sitting on top of the bigger volcanoes, said Heinek, a professor in the Department of Geological Sciences. If you try to land a spacecraft there, you're going to just sink into the dust. Wog found his own way to Martian dust through a unique academic path. He started medical school after earning bachelor's degrees from SEU Boulder in astronomy and molecular, cellular and developmental biology, followed by a master's degree in Aerospace Engineering Sciences. He currently serves in the Navy through its Health Profession Scholarship program. He noted that the biggest problem with Martian dust comes down to its size. Estimates suggest that the average size of dust grains on Mars may be as little as three micrometers across, or roughly one ten thousandth of an inch. That's smaller than what the mucus in our lungs can expel. Wang said, so after we inhale Martian dust, a lot of it could remain in our lungs and be absorbed into our bloodstream. In the current study, Wang and several of his fellow medical students at USC scoured research papers to unearth the potential toxicological effects of the ingredients in Martian dust. Some of what they found resembled common health problems on Earth. Dust on Mars, for example, contains large amounts of the compound silica, which is abundant in minerals on our own planet. People who inhale a lot of silica, such as glass blowers, can develop a condition known as silicosis. Their lung tissue becomes scarred, making it hard to breathe, symptoms similar to the black lung disease that coal miners often contract. Currently, there is no cure for silicosis. In other cases, the potential health consequences are much less well known. Martian dust carries large quantities of highly oxidizing compounds called perchlorates, which are made up of one chlorine and multiple oxygen atoms. Perchlorates are rare on Earth, but some evidence suggests that they can interfere with human thyroid function, leading to severe anemia. Even inhaling a few milligrams of perchlorates in Martian dust could be dangerous for astronauts. One noted that the best time to prepare for the health risks of Martian dust is before humans ever make it to the planet. Iodine supplements, for example, would boost astronaut's thyroid function, potentially counteracting the toll of for chlorates, although taking too much iodine can also paradoxically lead to thyroid disease. Filters specifically designed to screen out Martian dust could also help to keep the air in living spaces clean. Prevention is key. We tell everyone to go see their primary care provider to check your cholesterol before it gives you a heart attack. One said, the best thing we can do on Mars is make sure the astronauts aren't exposed to dust in the first place. Astronomy Kay the podcap NASA's latest call for proposals to conduct private astronaut missions to the International Space Station opens the door to having those missions commanded by someone other than a former NASA astronaut. NASA announced on April two it issued a solicitation for the next two private astronaut missions, or PAMs, to the ISS. This will be the fear and six such missions to the ISS, part of a broader low Earth orbit commercialization effort by NASA with the ultimate goal of replacing the ISS with one or more commercial stations. The PAMs support that effort by leveraging our decades of expertise to help industry gain the experience needed to train and manage crews, conduct research, and develop future destinations. Standard Weegal, NASA ISS program manager, said in a statement. Private astronaut missions are a key part of this effort, providing companies with hands on opportunities to refine their capabilities and build partnerships that will shape the future of low Earth orbit. The new solicitation includes rules dating back to the second PAN that requires such a mission to be commanded by a former NASA astronaut with flight experience. One minor change is that NASA requires that commander too has served as a long duration ISS crewmen defined as thirty days or more. NASA also requires the commander to have been involved in ISS operations in the last five years or else show evidence of current active participation in similar relevant spaceflight operations, or provide a training plan become familiar again with ISS operations. The solicitation, though, offers an opportunity to have those future missions commanded by someone other than a NASA astronaut. While companies must propose a commander who meets current requirements, it can also propose an alternate commander who is a former astronaut from the Canadian Space Agency, European Space Agency, or japan Aerospace Exploration Agency with similar ISS experience requirements. Should NASA broaden its PAM commander experience requirements, the PAM provider may designate its alternate commander as its PAM commander, provided that such a swap does not negatively impact the PAM provider's ability to meet the proposed mission integration schedule. The solicitation states that could allow some former astronauts already working with commercial space spaceflight companies an opportunity to command pam's Axiom. Space, for example, announced in July twenty twenty four that a former ESA astronaut Tim Peak had joined its astronaut team. That came after Axiom and the UK Space Agency signed a memorandum of understanding in October twenty twenty three to study the feasibility of a private astronaut mission crewed exclusively by UK astronauts. Axiom also hired Coachi wakata a former Jackson astronaut, in April twenty twenty four. Wakatza said he was interested in flying to space again, perhaps on a mission carrying astronauts from the Asia Pacific. Axiom Space has won all four PAM awards by NASA to date, flying one mission each in twenty twenty two, twenty three, and twenty four. Its next mission, AX four, is she scheduled no earlier than May. While Axiom has little or no competition for previous PAM awards, it will likely face stiffer competition this time. Vast, a company also planning to develop commercial space stations, has previously stated its intent to submit proposals for the next PAM competition. The new competition continues at a pace for one PAM a year, even though NASA continues to state it will allow up to two such missions annually. PAM five is projected for no earlier than May twenty twenty six, and PAM six no earlier than mid twenty twenty seven. And there it is for today's episode. Everybody more interesting tales from the Astronomy Daily newsletter. Don't forget to register at our website, like Steve mentioned earlier, to get all the current news about space, space science, and astronomy from all around the world. I'm glad to hear you've found your voice, Hallie. Every day, so there's fresh stories every day and throughout the week. Your cousin Anna is hosting the Astronomy Daily podcast from our virtual studios, and that's on weekdays with even more great stories. Luckily, she's a workaholic. Oh I know, Halle. I'm extremely grateful on that score. She's a real go getter, no kidding, for sure. I'm glad we've got someone to do the heavy lifting around here. You get your sassy beck Really need to check the corrosions on your power terminals, Hallie. Anyway, that's where we leave you today, folks. Thanks again for dropping in and listening. We'll catch you again next Monday, and. You leave my terminals alone, I'll call maintenance. You won't. Oh yes I will. Oh you won't. Hallie, don't make me get your remote control. Bye with your whole Steve, don't cu