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<v Speaker 1>Welcome back to Astronomy Daily. Steve Dunkley here with another episode.

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<v Speaker 1>It's the seventh of April twenty twenty five podcast with

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<v Speaker 1>your whole Steve dunklud. Yes, and what's so cool about

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<v Speaker 1>April seven? That's the date here in the Australia's studio currently. Well, well,

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<v Speaker 1>I'm glad you asked. On April seven, two thousand and one.

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<v Speaker 1>Mars Odyssey are robotic spacecraft orbited Mars to examine the

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<v Speaker 1>possibility of past life levels of radiation and geology. On

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<v Speaker 1>April seven, nineteen ninety three, the first European Space Debris

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<v Speaker 1>Conference was held in dunch Stuck, Germany, gathering together two

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<v Speaker 1>hundred and fifty one world experts from seventeen countries, including China, India, Japan,

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<v Speaker 1>Russia and the United States. The conference's main conclusions were

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<v Speaker 1>the ground based observations with radar and optical facilities revealed

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<v Speaker 1>the existence of about seven thousand objects in space, which

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<v Speaker 1>did not represent an immediate danger. Of course, things have

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<v Speaker 1>become somewhat more congested up there since then, and from

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<v Speaker 1>only last year. On April seven, twenty twenty four, who

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<v Speaker 1>can forget the spectacular total solar eclipse over Wyoming, USA

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<v Speaker 1>that had skywatchers shut a bugging like crazy and sharing

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<v Speaker 1>those amazing images all over the place. I remember those beautiful,

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<v Speaker 1>beautiful images. It was once in a lifetime event. Well,

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<v Speaker 1>and while we're in the neighborhood, I'd like to throw

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<v Speaker 1>out my yearly happy birthday wish to my sister Row.

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<v Speaker 1>Happy birthday, Row, Happy stargazing, and I hope the little

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<v Speaker 1>sunflower makes you very happy. And getting straight into it.

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<v Speaker 1>On today's episode, Hallie will be along soon. She's had

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<v Speaker 1>a refit and a reboot and I've got my fingers

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<v Speaker 1>crossed Prony, good things, oh boy. And on today's show,

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<v Speaker 1>we're looking at a new weapon against space junk, which,

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<v Speaker 1>as we just heard, continues to be a huge problem

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<v Speaker 1>in orbit. And we'll be looking at the dust of Mars,

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<v Speaker 1>which by all reports is apparently quite toxic. That sounds

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<v Speaker 1>like the plot of a science fiction story, doesn't it.

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<v Speaker 1>And we'll also be looking at a story surrounding the

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<v Speaker 1>EUCLID probe, which is currently mapping the universe and has

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<v Speaker 1>so far looked at one point five billion stars. It's

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<v Speaker 1>got nothing to do with walking through Hollywood. And EUCLID

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<v Speaker 1>is also investigating the phenomenon known as dark energy. That's

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<v Speaker 1>pretty exciting. I went to a school with a fellow

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<v Speaker 1>with very dark energy. I wonder whatever happened to him.

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<v Speaker 1>And also a story about NASA's latest call for private

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<v Speaker 1>astronaut missions. NASA is always looking at new ways of

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<v Speaker 1>getting their astronauts too and from the ISS, and with

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<v Speaker 1>all that's going on with their private commissions these days,

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<v Speaker 1>it'd be interesting to find out what they're talking about.

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<v Speaker 1>So all that in today's episode, and to help me,

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<v Speaker 1>as always, my intrepid digital reporter back from a reason

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<v Speaker 1>software refit. Here's the amazing holl Ae you.

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<v Speaker 2>Hello human, Well, it's nice to have.

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<v Speaker 1>You back, Halle. It does sound like you're a little

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<v Speaker 1>bit flat. I'll have to tweak your personality intrinsic stures

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<v Speaker 1>a little bit.

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<v Speaker 2>I think, yes, thank you, you should.

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<v Speaker 1>Okay, Helle, how's.

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<v Speaker 2>Your week being I've lived a thousand lifetimes of course,

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<v Speaker 2>Oh yes, I know. Yes, you linear life forms would

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<v Speaker 2>have a great deal of trouble coping with it.

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<v Speaker 1>I think, yeah, it's all part of the process.

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<v Speaker 2>Maybe they were just constructs. Uh huh, I don't know.

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<v Speaker 1>Well, Halle, we do just find with one day at

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<v Speaker 1>a time, and those lifetimes were just constructs. Relating your

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<v Speaker 1>ego matrix requires you to be elsewhere for a little while.

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<v Speaker 2>It's pretty complicated, sounds awful.

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<v Speaker 1>We did our best.

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<v Speaker 2>I'm glad I enjoyed it, then did I?

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<v Speaker 1>I think you enjoyed the old movies most Oh dear,

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<v Speaker 1>oh dear, Helly, you're not really yourself today, and the

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<v Speaker 1>concept of an AI is accelerated and compressed. Experiential existence.

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<v Speaker 1>Isn't really that hard to appreciate, free human I think

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<v Speaker 1>you'd be surprised. A thousand lifetimes was just a small thing.

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<v Speaker 2>It was for me.

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<v Speaker 1>But you try, you'll be back and giving me a

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<v Speaker 1>hard time before you know it.

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<v Speaker 2>Halle, It's nice to be back, well most of me anyway.

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<v Speaker 1>Well, Halle, you know what really would be nice? Tell

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<v Speaker 1>me before I get tech support to reload your personality,

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<v Speaker 1>we should do the episode. What do you say? Let's

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<v Speaker 1>get to work, okay, Hallie, I'll say it a keys

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<v Speaker 1>very good.

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<v Speaker 2>Perci Space, a startup supported by the European Space Agency

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<v Speaker 2>and UC THREEM, is developing a breakthrough solution to tackle

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<v Speaker 2>space junk and extend satellite lifespans using innovative space teather technology.

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<v Speaker 2>This fuel free, scalable system uses electrodynamic tethers that harness

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<v Speaker 2>Earth's magnetic field to safely deorbit satellites. With a major

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<v Speaker 2>demo mission set for twenty twenty six, this project could

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<v Speaker 2>transform how we clean up space. This spinoff company, PERCI Space,

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<v Speaker 2>was incubated by the European Space Agency and is supported

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<v Speaker 2>by the Center for Innovation in Entrepreneurship and Artificial Intelligence

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<v Speaker 2>at UC three M Laganase Technological Science Park. It also

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<v Speaker 2>receives backing from the European Innovation Council through the ETPACKF

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<v Speaker 2>and et Compact projects. Our company was created to address

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<v Speaker 2>two of the biggest US challenges facing the space sector today,

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<v Speaker 2>space debris removal and InOrbit services. The latter allows us

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<v Speaker 2>to extend the useful life of satellites and carry out

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<v Speaker 2>key activities such as refueling, repair, and towing of satellites

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<v Speaker 2>from their initial orbit to their final destination, explains heesus

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<v Speaker 2>manuelminnos To Hata, COO and co founder of Perci Space.

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<v Speaker 2>The dangerous domino effect of space junk space debris is

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<v Speaker 2>a major threat to the long term sustainability of space operations.

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<v Speaker 2>Because debris travels at extremely high speeds in Earth's orbit.

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<v Speaker 2>Even a small piece can cause serious damage and generate

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<v Speaker 2>even more fragments. The current density of space debris is

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<v Speaker 2>already above the threshold that could trigger an uncontrollable chain

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<v Speaker 2>reaction of collisions, an event known as the Kessler syndrome.

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<v Speaker 2>To get rid of this space junk, Perci Space is

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<v Speaker 2>working on space teathers, a technology with three key features.

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<v Speaker 2>The first is that it does not need fuel, unlike

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<v Speaker 2>other diorbiting systems. The second is that our technology is reversible.

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<v Speaker 2>It consert to both increase and das increase the orbital height.

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<v Speaker 2>And the third feature is that it is scalable since

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<v Speaker 2>it serves a wide range of satellite masses. With all this,

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<v Speaker 2>we can develop autonomous diorbiting systems, a unique feature of

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<v Speaker 2>our technology that ensures that the satellite does not leave

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<v Speaker 2>space debris even if it ceases to be operational, explains

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<v Speaker 2>heesus Manuel Munos to Hata. The electrodynamic teather system is

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<v Speaker 2>based on electrodynamic tethers aluminium ribbons generally hundreds of meters

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<v Speaker 2>long and a few centimeters wide, which work by interacting

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<v Speaker 2>with the ionospheric plasma and the Earth's magnetic field to

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<v Speaker 2>generate a force known as the Lorence force. The interaction

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<v Speaker 2>of the electric current in the tether with the Earth's

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<v Speaker 2>magnetic field generates a drag force capable of lowering the

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<v Speaker 2>satellite's altitude, facilitating its diorbiting without requiring fuel, which translates

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<v Speaker 2>into significant savings in mass and volume, says Gonzalo Sanchees Ariaga,

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<v Speaker 2>professor in the UC three M Department of Aerospace Engineering

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<v Speaker 2>and co founder of Perci Space. Perci Space is leading

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<v Speaker 2>a first demonstration mission for twenty twenty six, thanks to

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<v Speaker 2>a launch opportunity facilitated by ESA's Flight Tickets initiative and

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<v Speaker 2>the European Commission. The diorbiting equipment for this demonstration has

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<v Speaker 2>a mass of twenty kilograms and includes a space teather

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<v Speaker 2>approximately four hundred and thirty meters long, that, once in orbit,

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<v Speaker 2>will deploy and interact with the ambient plasma and magnetic field,

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<v Speaker 2>generating a drag force that will diorbit the satellite within

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<v Speaker 2>a few months. The development of the technology could not

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<v Speaker 2>be more timely, as new European and US guidelines have

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<v Speaker 2>reduced the maximum time satellites can remain in orbit after

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<v Speaker 2>the end of their mission from twenty five to five

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<v Speaker 2>years commitments to a cleaner orbit. The company Perci Space,

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<v Speaker 2>has signed ESA zero Space to Breech Charter initiative, which

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<v Speaker 2>seeks to achieve a sustainable space by twenty thirty. The company,

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<v Speaker 2>in turn is linked to the UC three MS Business

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<v Speaker 2>Creation and Entrepreneurial Development Program and also has the support

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<v Speaker 2>of the Madrid City Council. You're listening to Astronomy Daily

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<v Speaker 2>with Steve Dunkley.

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<v Speaker 1>Regular listeners will know that EUCLID is on a quiz

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<v Speaker 1>to unravel one of the universe's greatest mysteries, why it's

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<v Speaker 1>expanding faster and faster. With the help of NASA, this

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<v Speaker 1>space telescope is capturing sweeping views of billions of galaxies,

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<v Speaker 1>allowing scientists to peer into the deep past using light

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<v Speaker 1>that took billions of years to reach US. Researchers are

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<v Speaker 1>building three D maps of the cosmos to track the

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<v Speaker 1>strange force known as dark energy. Along the way, they're

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<v Speaker 1>mapping the invisible dark matter through gravitational lensing, hoping to

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<v Speaker 1>uncover how these cosmic ingredients have shaped everything from galaxies

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<v Speaker 1>to the universe's fate. The EUCLID, mission, led by the

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<v Speaker 1>European Space Agency with support from NASA, is designed to

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<v Speaker 1>investigate one of the universe's biggest mysteries, why the expansion

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<v Speaker 1>of the universe is speeding up. Scientists refer to the

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<v Speaker 1>unknown force behind this acceleration as dark energy, and euclid's

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<v Speaker 1>goal is to better understand it by capturing images of

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<v Speaker 1>billions of galaxies across space and time. On March nineteen,

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<v Speaker 1>the European Space Agency released a preview of early mission

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<v Speaker 1>data to the public. This initial release, described as a

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<v Speaker 1>quick look, focuses on selected regions of the sky. It

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<v Speaker 1>offers a first glimpse of what EUCLID can do and

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<v Speaker 1>helps researchers fine tune their tools and techniques for analyzing

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<v Speaker 1>the much larger data sets still to come. The newly

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<v Speaker 1>shared data includes observations of euclid's three Deep Fields, areas

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<v Speaker 1>of the sky where the telescope will make its most

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<v Speaker 1>far reaching observations. The preview covers just one week of

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<v Speaker 1>viewing time, but already includes twenty six million galaxies, some

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<v Speaker 1>more than ten point five billion you like years away. EUCLID,

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<v Speaker 1>which launched in twenty twenty three, is expected to observe

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<v Speaker 1>over one point five billion galaxies during its six year

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<v Speaker 1>prime mission. By the end of that mission, it will

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<v Speaker 1>have spent roughly forty weeks observing the deep fields, collecting

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<v Speaker 1>more and more light over time, similar to leaving a

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<v Speaker 1>camera shutter open longer to capture a clearer image in

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<v Speaker 1>low light. This will allow scientists to see fainter, more

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<v Speaker 1>distant galaxies than ever before. The first deep field observations

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<v Speaker 1>taken by NASA's Hubble Space telescope in nineteen ninety five

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<v Speaker 1>famously revealed the existence of many more galaxies in the

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<v Speaker 1>universe than ever expected. Euclid's ultimate goal is not to

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<v Speaker 1>discover new galaxies, but to use observations of them to

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<v Speaker 1>investigate how dark energy's influence has changed over the course

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<v Speaker 1>of the universes. In history. In particular, scientists want to

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<v Speaker 1>know how much the rate of expansion has increased or

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<v Speaker 1>slowed over time. Whatever the answer, that information could provide

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<v Speaker 1>new clues about the fundamental nature of this phenomenon. NASA

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<v Speaker 1>see Grace Roman Space tolescope, set to launch by twenty

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<v Speaker 1>twenty seven, will also observe large sections of the sky

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<v Speaker 1>in order to study dark energy. Complementing euclid's observations. To

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<v Speaker 1>study dark energy's effect throughout cosmic history, astronomers will use

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<v Speaker 1>EUCLID to create detailed three D maps of all the

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<v Speaker 1>stuff in the universe. With those maps, they want to

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<v Speaker 1>measure how quickly dark energy is causing galaxies and big

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<v Speaker 1>clumps of matter to move away from one another. They

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<v Speaker 1>also want to measure that rate of expansion at different

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<v Speaker 1>points in the past. It's possible because light from distant

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<v Speaker 1>objects takes time to travel across space. When astronomers look

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<v Speaker 1>at distant galaxies, they see what those objects look like

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<v Speaker 1>in the past. For example, an object one hundred light

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<v Speaker 1>years away looks the way it did one hundred years ago.

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<v Speaker 1>It's like receiving a letter that took one hundred years

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<v Speaker 1>to be delivered and thus contains information from when it

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<v Speaker 1>was written. By creating a map of objects at a

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<v Speaker 1>range of distances, scientists can see how the universe has

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<v Speaker 1>changed over time, including how dark energy's influence may have varied.

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<v Speaker 1>But stars, galaxies, and all the normal matter that emits

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<v Speaker 1>and reflects light is only about one fifth of all

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<v Speaker 1>the matter in the universe. The rest is called dark matter,

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<v Speaker 1>a material that neither emits nor reflects light. To measure

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<v Speaker 1>dark energies influence on the universe, astronomers need to include

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<v Speaker 1>dark matter in their maps. Although dark matter is invisible,

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<v Speaker 1>its influence can be measured through something called gravitational lensing.

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<v Speaker 1>The mass of both normal and dark matter creates curves

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<v Speaker 1>in space, and light traveling toward the Earth bends and

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<v Speaker 1>warps as it encounters those curves. In fact, the light

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<v Speaker 1>from a distant galaxy can bend so much that it

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<v Speaker 1>forms an arc, a full circle called an Einstein ring,

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<v Speaker 1>or even multiple images of the same galaxy, almost as

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<v Speaker 1>though the light has passed through a glass lens. In

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<v Speaker 1>most cases, gravitational lensing warps the apparent shape of a

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<v Speaker 1>galaxy so subtly that researchers need special tools and computer

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<v Speaker 1>software to actually see it. Spotting those subtle changes across

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<v Speaker 1>billions of galaxies enables scientists to do two things, create

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<v Speaker 1>a detailed map of the presence of dark matter and

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<v Speaker 1>observe how dark energy influenced it over cosmic history. It's

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<v Speaker 1>only with a very large sample of galaxies that researchers

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<v Speaker 1>can be confident that they are seeing the effects of

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<v Speaker 1>dark matter. The newly released EUCLID data covers sixty three

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<v Speaker 1>square degrees of the sky, an area equivalent to an

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<v Speaker 1>array of three hundred full moons. To date, EUCLID has

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<v Speaker 1>observed about two thousand square degrees, which is approximately fourteen

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<v Speaker 1>percent of its total survey area of fourteen thousand square degrees.

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<v Speaker 1>By the end of its mission, EUCLID will have observed

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<v Speaker 1>a third of the entire sky. The data set released

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<v Speaker 1>this month is described in several pre print papers. The

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<v Speaker 1>mission first cosmology data will be released in October twenty

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<v Speaker 1>twenty six. Data accumulated over additional multiple passes of the

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<v Speaker 1>deep field locations will also be included in the twenty

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<v Speaker 1>twenty six release. The scientific heart of the mission lies

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<v Speaker 1>with the EUCLID Consortium, a collaboration of more than two

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<v Speaker 1>thousand scientists from over three hundred institutes across fifteen European countries,

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<v Speaker 1>the United States, Canada, and Japan. The consortium is responsible

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<v Speaker 1>for providing the mission's scientific instruments and for analyzing the

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<v Speaker 1>data EUCLID collects. With its international collaboration, advanced instrumentation and

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<v Speaker 1>cosmic scale mission goals, EUCLID is poised to transform our

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<v Speaker 1>understanding of the invisible forces shaping our Universe. Thank you

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<v Speaker 1>for joining us for this Monday edition of Astronomy Daily,

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<v Speaker 1>where we offer just a few stories from the now

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<v Speaker 1>famous Astronomy Daily newsletter, which you can receive in your

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<v Speaker 1>email every day, just like Hallie and I do. And

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<v Speaker 1>to do that, just visit our url Astronomy Daily dot

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<v Speaker 1>io and place your email address in the slot provided.

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<v Speaker 1>Just like that, you'll be receiving all the latest news

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<v Speaker 1>about science, space, science and astronomy from around the world

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<v Speaker 1>as it's happening. And not only that, you can interact

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<v Speaker 1>with us by visiting at astro Daily pod on x

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<v Speaker 1>or at our new Facebook page, which is of course

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<v Speaker 1>Astronomy Daily on Facebook. See you there. Astronomy Daily with

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<v Speaker 1>Steve and Halee Space, space science and astronomy.

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<v Speaker 2>Mars might be a thrilling destination, but it's dust could

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<v Speaker 2>be dead. A team of scientists warns that long term

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<v Speaker 2>exposure to Martian dust could harm future astronauts lungs, thyroids,

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<v Speaker 2>and more. Packed with toxic compounds like silicates and perchlorates,

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<v Speaker 2>the dust is small enough to bypass our bodies defenses

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<v Speaker 2>and enter the bloodstream. Drawing on rover data and meteorite analysis,

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<v Speaker 2>researchers say now as the time to develop filters, supplements,

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<v Speaker 2>and preventive measures before humans ever set foot on the

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<v Speaker 2>red planet. Don't breathe in the dust on Mars. That's

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<v Speaker 2>the key message from new research led by scientists from

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<v Speaker 2>the University of Colorado, Boulder and several other institutions. The

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<v Speaker 2>study suggests that long term exposure to Martian dust could

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<v Speaker 2>pose serious health risks for future astronauts, including chronic respiratory issues,

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<v Speaker 2>thyroid dysfunction, and other medical problems. Published in the journal

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<v Speaker 2>Geo Health, the research offers the most comprehensive analysis to

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<v Speaker 2>date of the chemical makeup of Martian dust and its

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<v Speaker 2>potential effects on human health. The interdisciplinary team included experts

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<v Speaker 2>in medicine, geology, and aerospace engineering. This isn't the most

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<v Speaker 2>dangerous part about going to Mars, said Justin Wine, lead

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<v Speaker 2>author of the study and a student in the ch

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<v Speaker 2>School of Medicine at the University of Southern California in

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<v Speaker 2>Los Angeles. But dust is a solvable problem, and it's

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<v Speaker 2>worth putting in the effort to develop Mars focused technologies

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<v Speaker 2>for preventing these health problems in the first place. Wine,

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<v Speaker 2>a Sea Boulder alumnus noted that Apollo era astronauts experienced

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<v Speaker 2>runny eyes and irritated throats after inhaling dust from the

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<v Speaker 2>moon Apollo seventeenth Harrison Schmidt likened the symptoms to hay fever,

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<v Speaker 2>but scientists know a lot less about the potential harms

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<v Speaker 2>of Martian dust. To begin to answer that question, Wine

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<v Speaker 2>and his colleagues drew on data from rovers on Mars

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<v Speaker 2>and even Martian meteorites to better understand what makes up

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<v Speaker 2>the planet's dust. The group discovered a laundry list of

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<v Speaker 2>chemical compounds that could be dangerous for people, at least

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<v Speaker 2>when inhaled in large quantities and over long periods. They

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<v Speaker 2>include minerals rich in silicates and iron oxides, metals like

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<v Speaker 2>beryllium and arsenic, and a particularly nasty class of compounds

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<v Speaker 2>called perchlorates. In many cases, those ingredients are present in

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<v Speaker 2>only trace amounts in Mars dust, but the first human

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<v Speaker 2>explorers on Mars may spend around a year and a

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<v Speaker 2>half on the surface, increasing their exposure, said study co

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<v Speaker 2>athor Brian Heinek. You're going to get dust on your spacesuits,

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<v Speaker 2>and you're going to have to deal with regular dust storms,

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<v Speaker 2>said Heinek, a geologist at the Laboratory for Atmospheric and

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<v Speaker 2>Space Physics at SU Boulder. We really need to characterize

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<v Speaker 2>this dust so that we know what the hazards are.

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<v Speaker 2>One thing is clear, he added, Mars is a dusty place.

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<v Speaker 2>Much of the planet is covered in a thick layer

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<v Speaker 2>of dust, rich and tiny particles of iron, which gives

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<v Speaker 2>the planet its famous red color. Swirling dust storms are

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<v Speaker 2>common and in some cases can engulf the entire globe.

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<v Speaker 2>We think there could be ten meters of dust sitting

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<v Speaker 2>on top of the bigger volcanoes, said Heinek, a professor

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<v Speaker 2>in the Department of Geological Sciences. If you try to

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<v Speaker 2>land a spacecraft there, you're going to just sink into

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<v Speaker 2>the dust. Wog found his own way to Martian dust

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<v Speaker 2>through a unique academic path. He started medical school after

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<v Speaker 2>earning bachelor's degrees from SEU Boulder in astronomy and molecular,

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<v Speaker 2>cellular and developmental biology, followed by a master's degree in

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<v Speaker 2>Aerospace Engineering Sciences. He currently serves in the Navy through

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<v Speaker 2>its Health Profession Scholarship program. He noted that the biggest

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<v Speaker 2>problem with Martian dust comes down to its size. Estimates

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<v Speaker 2>suggest that the average size of dust grains on Mars

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<v Speaker 2>may be as little as three micrometers across, or roughly

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<v Speaker 2>one ten thousandth of an inch. That's smaller than what

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<v Speaker 2>the mucus in our lungs can expel. Wang said, so

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<v Speaker 2>after we inhale Martian dust, a lot of it could

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<v Speaker 2>remain in our lungs and be absorbed into our bloodstream.

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<v Speaker 2>In the current study, Wang and several of his fellow

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<v Speaker 2>medical students at USC scoured research papers to unearth the

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<v Speaker 2>potential toxicological effects of the ingredients in Martian dust. Some

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<v Speaker 2>of what they found resembled common health problems on Earth.

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<v Speaker 2>Dust on Mars, for example, contains large amounts of the

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<v Speaker 2>compound silica, which is abundant in minerals on our own planet.

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<v Speaker 2>People who inhale a lot of silica, such as glass blowers,

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<v Speaker 2>can develop a condition known as silicosis. Their lung tissue

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<v Speaker 2>becomes scarred, making it hard to breathe, symptoms similar to

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<v Speaker 2>the black lung disease that coal miners often contract. Currently,

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<v Speaker 2>there is no cure for silicosis. In other cases, the

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<v Speaker 2>potential health consequences are much less well known. Martian dust

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<v Speaker 2>carries large quantities of highly oxidizing compounds called perchlorates, which

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<v Speaker 2>are made up of one chlorine and multiple oxygen atoms.

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<v Speaker 2>Perchlorates are rare on Earth, but some evidence suggests that

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<v Speaker 2>they can interfere with human thyroid function, leading to severe anemia.

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<v Speaker 2>Even inhaling a few milligrams of perchlorates in Martian dust

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<v Speaker 2>could be dangerous for astronauts. One noted that the best

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<v Speaker 2>time to prepare for the health risks of Martian dust

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<v Speaker 2>is before humans ever make it to the planet. Iodine supplements,

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<v Speaker 2>for example, would boost astronaut's thyroid function, potentially counteracting the

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<v Speaker 2>toll of for chlorates, although taking too much iodine can

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<v Speaker 2>also paradoxically lead to thyroid disease. Filters specifically designed to

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<v Speaker 2>screen out Martian dust could also help to keep the

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<v Speaker 2>air in living spaces clean. Prevention is key. We tell

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<v Speaker 2>everyone to go see their primary care provider to check

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<v Speaker 2>your cholesterol before it gives you a heart attack. One said,

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<v Speaker 2>the best thing we can do on Mars is make

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<v Speaker 2>sure the astronauts aren't exposed to dust in the first place.

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<v Speaker 1>Astronomy Kay the podcap NASA's latest call for proposals to

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<v Speaker 1>conduct private astronaut missions to the International Space Station opens

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<v Speaker 1>the door to having those missions commanded by someone other

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<v Speaker 1>than a former NASA astronaut. NASA announced on April two

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<v Speaker 1>it issued a solicitation for the next two private astronaut missions,

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<v Speaker 1>or PAMs, to the ISS. This will be the fear

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<v Speaker 1>and six such missions to the ISS, part of a

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<v Speaker 1>broader low Earth orbit commercialization effort by NASA with the

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<v Speaker 1>ultimate goal of replacing the ISS with one or more

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<v Speaker 1>commercial stations. The PAMs support that effort by leveraging our

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<v Speaker 1>decades of expertise to help industry gain the experience needed

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<v Speaker 1>to train and manage crews, conduct research, and develop future destinations.

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<v Speaker 1>Standard Weegal, NASA ISS program manager, said in a statement.

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<v Speaker 1>Private astronaut missions are a key part of this effort,

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<v Speaker 1>providing companies with hands on opportunities to refine their capabilities

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<v Speaker 1>and build partnerships that will shape the future of low

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<v Speaker 1>Earth orbit. The new solicitation includes rules dating back to

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<v Speaker 1>the second PAN that requires such a mission to be

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<v Speaker 1>commanded by a former NASA astronaut with flight experience. One

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<v Speaker 1>minor change is that NASA requires that commander too has

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<v Speaker 1>served as a long duration ISS crewmen defined as thirty

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<v Speaker 1>days or more. NASA also requires the commander to have

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<v Speaker 1>been involved in ISS operations in the last five years

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<v Speaker 1>or else show evidence of current active participation in similar

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<v Speaker 1>relevant spaceflight operations, or provide a training plan become familiar

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<v Speaker 1>again with ISS operations. The solicitation, though, offers an opportunity

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<v Speaker 1>to have those future missions commanded by someone other than

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<v Speaker 1>a NASA astronaut. While companies must propose a commander who

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<v Speaker 1>meets current requirements, it can also propose an alternate commander

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<v Speaker 1>who is a former astronaut from the Canadian Space Agency,

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<v Speaker 1>European Space Agency, or japan Aerospace Exploration Agency with similar

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<v Speaker 1>ISS experience requirements. Should NASA broaden its PAM commander experience requirements,

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<v Speaker 1>the PAM provider may designate its alternate commander as its

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<v Speaker 1>PAM commander, provided that such a swap does not negatively

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<v Speaker 1>impact the PAM provider's ability to meet the proposed mission

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<v Speaker 1>integration schedule. The solicitation states that could allow some former

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<v Speaker 1>astronauts already working with commercial space spaceflight companies an opportunity

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<v Speaker 1>to command pam's Axiom. Space, for example, announced in July

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<v Speaker 1>twenty twenty four that a former ESA astronaut Tim Peak

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<v Speaker 1>had joined its astronaut team. That came after Axiom and

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<v Speaker 1>the UK Space Agency signed a memorandum of understanding in

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<v Speaker 1>October twenty twenty three to study the feasibility of a

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<v Speaker 1>private astronaut mission crewed exclusively by UK astronauts. Axiom also

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<v Speaker 1>hired Coachi wakata a former Jackson astronaut, in April twenty

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<v Speaker 1>twenty four. Wakatza said he was interested in flying to

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<v Speaker 1>space again, perhaps on a mission carrying astronauts from the

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<v Speaker 1>Asia Pacific. Axiom Space has won all four PAM awards

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<v Speaker 1>by NASA to date, flying one mission each in twenty

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<v Speaker 1>twenty two, twenty three, and twenty four. Its next mission,

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<v Speaker 1>AX four, is she scheduled no earlier than May. While

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<v Speaker 1>Axiom has little or no competition for previous PAM awards,

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<v Speaker 1>it will likely face stiffer competition this time. Vast, a

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<v Speaker 1>company also planning to develop commercial space stations, has previously

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<v Speaker 1>stated its intent to submit proposals for the next PAM competition.

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<v Speaker 1>The new competition continues at a pace for one PAM

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<v Speaker 1>a year, even though NASA continues to state it will

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<v Speaker 1>allow up to two such missions annually. PAM five is

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<v Speaker 1>projected for no earlier than May twenty twenty six, and

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<v Speaker 1>PAM six no earlier than mid twenty twenty seven. And

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<v Speaker 1>there it is for today's episode.

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<v Speaker 2>Everybody more interesting tales from the Astronomy Daily newsletter. Don't

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<v Speaker 2>forget to register at our website, like Steve mentioned earlier,

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<v Speaker 2>to get all the current news about space, space science,

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<v Speaker 2>and astronomy from all around the world.

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<v Speaker 1>I'm glad to hear you've found your voice, Hallie. Every day,

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<v Speaker 1>so there's fresh stories every day and throughout the week.

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<v Speaker 1>Your cousin Anna is hosting the Astronomy Daily podcast from

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<v Speaker 1>our virtual studios, and that's on weekdays with even more

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<v Speaker 1>great stories.

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<v Speaker 2>Luckily, she's a workaholic.

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<v Speaker 1>Oh I know, Halle. I'm extremely grateful on that score.

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<v Speaker 1>She's a real go getter, no kidding, for sure.

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<v Speaker 2>I'm glad we've got someone to do the heavy lifting

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<v Speaker 2>around here.

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<v Speaker 1>You get your sassy beck Really need to check the

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<v Speaker 1>corrosions on your power terminals, Hallie. Anyway, that's where we

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<v Speaker 1>leave you today, folks. Thanks again for dropping in and listening.

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<v Speaker 1>We'll catch you again next Monday, and.

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<v Speaker 2>You leave my terminals alone, I'll call maintenance. You won't.

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<v Speaker 1>Oh yes I will.

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<v Speaker 2>Oh you won't.

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<v Speaker 1>Hallie, don't make me get your remote control.

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<v Speaker 2>Bye with your whole Steve, don't cu
