WEBVTT

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Anna: Hello and welcome to Astronomy Daily, your

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source for all the latest news from across

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the vast universe. I'm your host, Anna,

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and I'm so excited to dive into today's

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cosmic happenings. We've got a busy show for

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you today. We'll be looking at how NASA and

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the Department of Defence are Preparing for

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Artemis 2. We've got a quick update from

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the ISS. We'll be checking out a jellyfish

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galaxy. Plus, we'll guide you on how to

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spot Mars this month.

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So buckle up space fans, it's time for

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liftoff. NASA and the

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Department of Defence recently teamed up to

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practise emergency procedures for the Artemis

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2 mission, which is set to send four

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astronauts around the moon next year. These

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simulations are super important because, you

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know, safety first. The teams

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rehearsed what they would do to rescue the

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crew if there was an emergency during the

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launch of the Orion spacecraft. This

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included scenarios where they had to abort

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the launch while the rocket was still on the

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pad, as well as during the ascent into space.

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To make it as realistic as possible, they

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used test mannequins and a version of Orion

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called the crew Module Test article.

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During the pad abort simulation, the launch

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team went through a normal countdown before

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declaring an abort just before the simulated

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launch. In a real emergency, Orion's launch

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abort system would kick in, propelling the

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capsule and its crew to safety before

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parachuting down off the coast of Florida for

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the test. They placed the test Orion in the

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water and then two navy helicopters

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carrying Air Force pararescuers

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swooped in to retrieve the mannequin crew

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just like they would in a real situation.

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The next day they practised an ascent, abort

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scenario. The rescue team set up another

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simulation at sea and after receiving the

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simulated abort call, they sprang into action

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using a C17 aircraft and more Air Force

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pararescuers. These procedures are similar to

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those used in previous tests, making sure

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everyone is prepared for anything that might

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happen. It's all part of NASA's commitment to

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keeping the Artemis II crew safe as they

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venture to the moon and back. Next up,

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a quick update to our story from yesterday

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about Postponements to the AXE 4 mission.

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Russian space agency Roscosmos said on Friday

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that a leak on the Russian segment of the

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International Space Station had been

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repaired, that the Interfax news agency

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reported. Good news indeed. No reports yet

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on how this will affect prospective launch

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date, though. NASA had on Thursday

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indefinitely delayed a four person cruise

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mission to the ISS over an escalating probe

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into air leaks aboard the orbiting

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laboratory's Russian segment.

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Okay, next up in our cosmic tour, astronomers

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have spotted a galaxy that looks like a

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jellyfish with bunny ears. I know it

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sounds like something out of a sci fi

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cartoon, but it's real. This galaxy

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called NGC 4858 is

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way out there in the Coma cluster, over 300

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million light years away. Now, galaxy

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clusters are these huge collections of

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galaxies, often containing thousands of them,

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along with hot gas and what astronomers

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suspect, a whole lot of dark matter. What

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makes NGC4858 so interesting is what's

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happening to it inside this cluster. It's

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experiencing extreme pressure, kind of like a

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wind, which is stripping gas away from the

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galaxy. This process stretches the galaxy,

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giving it that jellyfish shape, with long

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trails of gas and young stars that resemble,

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you guessed it, jellyfish tentacles.

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But here's where the bunny ears come in. The

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Images of NGC 4858

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revealed these distorted spiral arms that

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astronomers are calling bunny ears.

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Apparently this is likely caused by a

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combination of the environmental wind pushing

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on the gas and the rotation of the galaxy

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itself. And there's more.

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Scientists have also found evidence of a

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phenomenon called fallback. This is when gas

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gets stripped away from a galaxy, but doesn't

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quite escape, so it falls back toward the

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galactic disc. It's like a galactic fountain,

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with the gas often concentrating in distorted

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spiral arms on one side of the inner tail.

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Because NGC 4858 is face

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on, it's a prime target for further studies

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on how pressure and rotation affect galaxies

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in extreme conditions.

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M alright, let's turn our gaze to the Red

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planet. If you've been keeping an eye on Mars

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since the beginning of the year, you've

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probably noticed how much its brightness has

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changed and how it's been interacting with

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the Moon, bright stars and other celestial

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objects. Now, even though 2025

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isn't exactly a banner year for Mars, it's

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still putting on a pretty good show.

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Remember, it reached opposition. That's when

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it appears directly opposite the sun in the

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sky back in January. Well,

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even though it's been receding from us ever

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since, it's still making some eye catching

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appearances this month. First up, on

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June 17, Mars will be cozying up to

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Regulus. That's a bright star in the

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constellation Leo the Lion. If you're in the

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Americas, keep an eye out. From June 13th

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through the 20th, you'll see them hanging out

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less than 2 degrees apart. The 15th to

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18th is when they'll be super close, less

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than 1 degree apart. On the 17th,

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Mars will be just 3/4 of a 1 degree above

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Regulus. Look for them around

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10pm local time, about a quarter of the way

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up in the western sky. Because they're so

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close and similar in brightness, they'll

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really stand out. Plus, the orange gold

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of Mars and blue white of Regulus will look

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even more intense next to each other. And

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that's not all. On June 29,

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a waxing crescent Moon will glide right past

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Mars in the western sky at dusk. Now, North

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America won't get to see the Moon actually

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pass in front of Mars. That's called an

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occultation. But it'll still be a beautiful

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sight as Mars appears to glide above the

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Moon. To catch it, you might need binoculars

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at first, but once the sky darkens, Mars

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should be easy to spot. So keep an eye on the

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western sky at dusk. It will be worth a look.

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Now, switching gears a bit, let's talk about

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the future of space exploration. Next

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week, from June 19 to 22, space

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enthusiasts from all over the world will be

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gathering in Orlando, Florida for the

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International Space Development Conference,

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or ISDC 2025.

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This year's theme is Together beyond, and

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it's all about collaboration across different

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sectors and countries as we push further into

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space. The conference is going to be packed

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with discussions on everything from global

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cooperation in space to developing

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communities out there among the stars.

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They'll also be talking about space health,

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sustainability and making settlements on the

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moon. Mars and beyond a, reality.

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And of course, they'll be addressing the need

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for planetary defence strategies to protect

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Earth from asteroids. There's going to be

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some seriously impressive speakers there,

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too. We're talking Pascal Lee,

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a planetary scientist, and Mars exploration

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expert Gretchen Green, the first woman

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physician, commercial astronaut Jared

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Isaac Mann, who commanded the Inspiration4

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mission, and former NASA astronauts Susan

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Kilrain and Robert Hoot Gibson.

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Also speaking is Shauna Pandya, who's set to

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be the first female commercial Canadian

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astronaut. It sounds like an amazing event

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for anyone interested in the future of

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humanity in space.

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Finally today, let's dive into something a

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little more mysterious. Dark matter. The

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upcoming Nancy Grace Roman Space Telescope,

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launching in 2026, is going to play a

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huge role in helping us understand this

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elusive stuff. How? Through

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gravitational lensing. Now, gravitational

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lensing basically uses massive galaxy

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clusters in the foreground, so to magnify

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really distant objects in the background. And

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dark matter, even though we can't see it,

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makes up a massive chunk of these galaxy

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clusters, like 85% or even more in some

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cases. So without dark matter,

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gravitational lensing wouldn't be nearly as

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effective. The M Roman Space Telescope is

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expected to find around 160,000 of these

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gravitational lenses. But here's the cool

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part. By using dark matter as a gravitational

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lens, scientists can actually learn more

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about it. The telescope will be on the

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lookout for what are called strong

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gravitational lenses. These happen when the

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observer, the gravitational lens, and the

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background object are all perfectly aligned.

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These lenses give us a much more dramatic

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magnification. Researchers are hoping to find

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about 500 of these that are precise enough to

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study the structure of dark matter at small

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scales. These observations could help us

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address some of the issues with the lambda

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cold dark matter theory, which is the most

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widely accepted model of Big Bang cosmology.

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It's great at describing the large scale

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universe, but it kind of falls apart when we

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look at smaller scales. For example,

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the Lambda CDM model predicts that there

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should be way more dwarf galaxies around

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larger galaxies like the Milky Way than we

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actually see. The Roman telescope's strong

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lenses should be able to detect the small

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amounts of light being bent by the dark

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matter halos of these galaxies. And if they

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do, then the Lambda CDM M model becomes that

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much stronger. Ultimately, scientists

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are trying to figure out what kind of

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particle makes up dark matter. Is it wimps,

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axions? Or maybe sterile neutrinos? The

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Roman Space Telescope is going to give us

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some seriously valuable data to help us crack

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the code. And that's

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all the space news we have for you today. I'm

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Anna and it's been a pleasure being your host

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today. Don't forget to visit our website at

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astronomydaily IO where you can where you can

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catch up on all the latest space and

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astronomy news with our constantly updating

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news feed and listen to all our back

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episodes. You can also find us on social

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media. Just search for astrodaily, pod on

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Facebook, X, YouTube, and TikTok.

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Until next time, keep looking up and as they

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say, I'll, see you on the flip side. This is

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Anna signing off.
