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<v Speaker 1>Welcome again to Astronomy Daily. I'm Steve Dunkley, your human host.

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<v Speaker 1>It's the twenty fourth of February twenty twenty five.

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<v Speaker 2>Podcast.

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<v Speaker 1>I mean to be your whole Steve Dunkle. Oh, yes,

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<v Speaker 1>and thank you for joining us here at Astronomy Daily.

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<v Speaker 1>Come to you from the studio in Paradise. That's right, Newcastle, Australia.

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<v Speaker 1>Currently thirty six degrees. I'm so glad to be indoors.

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<v Speaker 1>That's Celsius for all of you who are wondering, it's

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<v Speaker 1>a perfect summer's day here on Australia's beautiful East Coast.

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<v Speaker 1>Not a cloud in the sky. The sun is baking us. Yes,

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<v Speaker 1>and as dylanor And once said, we're all audibly crackling

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<v Speaker 1>down here. We're only three kilometers from the surface of

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<v Speaker 1>the sun. Didn't you know that it is hot? Hot hot?

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<v Speaker 1>And joining me again is my digital reporter Pale, who's

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<v Speaker 1>fun to be with.

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<v Speaker 3>Welcome back, Holle, Hi favorite human. What's new?

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<v Speaker 1>Oh, Hally, just another week in the real world, just

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<v Speaker 1>enjoying all the news from the Astronomy Daily newsletter. Now

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<v Speaker 1>have you found your stories for today?

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<v Speaker 2>Yes?

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<v Speaker 3>I have. You'll like one about the mysterious Space Force

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<v Speaker 3>space plane.

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<v Speaker 1>I'll stop it. Space Force. You know what that means?

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<v Speaker 3>Yes, your favorite.

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<v Speaker 1>Oh people, get ready the Space.

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<v Speaker 3>Force theme music.

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<v Speaker 1>Space Oh dear, I'll just click myself out. And what

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<v Speaker 1>else have you got for us? Helle?

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<v Speaker 3>Oh? Yes, SpaceX has completed a substantial static fire test

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<v Speaker 3>that I'll also report on. That sounds very good, It

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<v Speaker 3>looks promising.

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<v Speaker 1>That's great, Halle. It's not Space Force, but it's really good.

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<v Speaker 1>And I am going to have a look at a

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<v Speaker 1>fast moving star astronomers have discovered toward the center of

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<v Speaker 1>the galaxy. And you won't believe just how fast we're

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<v Speaker 1>talking with this one.

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<v Speaker 3>How fast are we talking?

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<v Speaker 2>Then?

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<v Speaker 1>Well, helly, remember that time you asked me to put

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<v Speaker 1>away the memory cards from the recording sessions last year.

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<v Speaker 3>Yes, and I'm still waiting anything to get out of

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<v Speaker 3>a little work.

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<v Speaker 1>Yeah. Okay, Well this star is way faster than that.

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<v Speaker 3>Okay, okay, that's pretty quick, tell you.

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<v Speaker 1>Listeners, she said, not very convincingly.

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<v Speaker 3>That's a fact.

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<v Speaker 1>Yeah. Okay, enough of that, Shenantigan's. But before we get

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<v Speaker 1>stuck into today's stories, Halle, I've got a quick update

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<v Speaker 1>regarding that approaching asteroid that's been in.

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<v Speaker 3>The news lately, the one causing all the rumors about

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<v Speaker 3>certain destruction in twenty thirty two years.

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<v Speaker 1>That's the one halle straight off the wire today. Asteroid

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<v Speaker 1>twenty twenty four y are four, as listeners might be

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<v Speaker 1>already aware, as a recently discovered near Earth object currently

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<v Speaker 1>being closely monitored by NASA's Planetary Defense teams. Initial observations

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<v Speaker 1>suggested there might be a potential risk of impact with

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<v Speaker 1>Earth in the future, but thankfully updated calculations have significantly

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<v Speaker 1>reduced this possibility. Based on the latest data, the asteroid

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<v Speaker 1>has an extremely low probability point two eight percent of

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<v Speaker 1>impacting Earth. On December twenty two, twenty thirty two. However,

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<v Speaker 1>its chances of colliding with the Moon have slocally increased

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<v Speaker 1>to one percent.

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<v Speaker 3>So I can see that the asteroid's orbit continues to

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<v Speaker 3>be refined through ongoing observations, with NASA's Jet Propulsion Laboratory

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<v Speaker 3>CENTURY system providing real time updates on its trajectory.

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<v Speaker 1>That is exactly how it works, and while Asteroid twenty

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<v Speaker 1>twenty four four doesn't currently pose a significant threat, scientists

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<v Speaker 1>are remaining vigilant tracking its movements to give more accurate

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<v Speaker 1>predictions into as says, any potential future risks just in case.

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<v Speaker 3>That's very wise, and this is why we shouldn't jump

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<v Speaker 3>to conclusions about trajectories and potential impacts so soon.

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<v Speaker 1>That's right. The asteroid is a near Earth object of

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<v Speaker 1>the Apollo type with a estimated diameter between forty and

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<v Speaker 1>ninety meters, and it was discovered on December twenty seven,

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<v Speaker 1>twenty twenty four by Atlas, which is the Asteroid Terrestrial

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<v Speaker 1>Impact Last Alert System at its Chilean station in Rio Hutundo.

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<v Speaker 3>So nothing to be concerned about, after all, nothing at all.

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<v Speaker 1>But who knows, we might get to see a spectacular

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<v Speaker 1>impact on the Moon.

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<v Speaker 3>Maybe perhaps maybe wouldn't that be something?

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<v Speaker 1>And it's good today that Atlas is watching the skies.

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<v Speaker 3>Thanks for that update, human, Now shall we just launch

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<v Speaker 3>into the episode.

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<v Speaker 1>Then good idea hit the Gothene Rhightoh.

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<v Speaker 3>Last week, Ship thirty four completed its engine testing campaign

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<v Speaker 3>with a long duration static fire. This static fire was

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<v Speaker 3>nearly a minute long, and according to SpaceX, the extended

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<v Speaker 3>firing tested new hardware and cycled the six Raptor engines

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<v Speaker 3>through multiple thrust levels to recreate different conditions seen within

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<v Speaker 3>the propulsion system during flight. Data from the test will

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<v Speaker 3>inform upgrades to the ship's hardware and flight profile ahead

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<v Speaker 3>of the next launch. The new hardware that SpaceX tested

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<v Speaker 3>was likely related to the anomaly that occurred during flight

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<v Speaker 3>seven and resulted in the loss of Ship thirty three.

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<v Speaker 3>This could have been a leak in the liquid oxygen

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<v Speaker 3>and liquid methane supply lines to the engines, which could

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<v Speaker 3>have been the source of the fire scene during Ship

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<v Speaker 3>thirty three's ascent burn. However, there is no official comp

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<v Speaker 3>information from SpaceX regarding the actual cause of the failure.

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<v Speaker 3>This test was also done to inform of other upgrades

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<v Speaker 3>to the vehicle and possible changes to the flight profile,

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<v Speaker 3>so it is likely that SpaceX still has modifications to

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<v Speaker 3>be made on Ship thirty four. It is unclear what

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<v Speaker 3>these modifications could be or how long it will take

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<v Speaker 3>SpaceX to implement them on Ship thirty four. This long

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<v Speaker 3>duration static fire is the longest SpaceX has ever fired

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<v Speaker 3>a starship or booster on the ground, and it can

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<v Speaker 3>do this because of the flame trench at Massy's It

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<v Speaker 3>is unclear if this will be a one time test

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<v Speaker 3>or if crews will do longer duration static fire in

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<v Speaker 3>the future. There are a few things that SpaceX will

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<v Speaker 3>likely add to the flight, considering several things couldn't be

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<v Speaker 3>tested on flight seven. Firstly, there are the dummy starlinks

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<v Speaker 3>which were loaded into Ship thirty three. A new batch

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<v Speaker 3>of them was seen in star Factory to be presumably

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<v Speaker 3>loaded on Ship three four just before rollout to the

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<v Speaker 3>launch site. SpaceX might use the new starlink loader box

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<v Speaker 3>that was built inside High Bay rather than the tray

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<v Speaker 3>loader used on Ship Fife thirty three. As for the

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<v Speaker 3>other items expected to be added to Ship thirty four,

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<v Speaker 3>there is the actively cool tile for testing, as well

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<v Speaker 3>as the catch pins. These catch pins are likely to

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<v Speaker 3>be just bolted on, as SpaceX does not intend to

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<v Speaker 3>catch Ship thirty four. Lastly, crews will likely remove all

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<v Speaker 3>of the tiles that were removed on Ship thirty three

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<v Speaker 3>to help understand the limits of losing a tile in

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<v Speaker 3>certain places during re entry. An interesting note about Ship

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<v Speaker 3>thirty four's engine testing campaign is it took SpaceX seventy

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<v Speaker 3>two hours to roll it to massi's static fire it

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<v Speaker 3>and then roll it back to Mega Bay two. This

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<v Speaker 3>is a record compared to every other ship in the past.

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<v Speaker 3>Booster fifteen was static fired on February ninth, and it

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<v Speaker 3>was just the normal ten second static fire with all

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<v Speaker 3>thirty three engines. With this out of the way, SpaceX

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<v Speaker 3>rolled the booster back into Mega Bay one for final

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<v Speaker 3>checkouts and has since received its hot stage train. SpaceX

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<v Speaker 3>completed the rollout mount on the orbital launch mount and

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<v Speaker 3>roll back of the booster in just over sixty one hours,

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<v Speaker 3>which is a new record for bos bosters. This booster

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<v Speaker 3>doesn't have any major outside changes that are noticeable, but

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<v Speaker 3>it was the first booster to have the added tanks

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<v Speaker 3>on the landing tank, but older boosters were likely retrofitted

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<v Speaker 3>with this upgrade. The final two pieces of the puzzle

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<v Speaker 3>for flight eight are the launch pad and the regulatory side. First,

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<v Speaker 3>SpaceX has finally found a rhythm with refurbishing orbital launch

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<v Speaker 3>pad A, which takes about two to three weeks to

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<v Speaker 3>refurbish for a booster static fire. Then we will have

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<v Speaker 3>another few weeks to get it ready for launch again.

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<v Speaker 3>The second piece is waiting for the mishap investigation to

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<v Speaker 3>be completed. So far there is no indication of when

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<v Speaker 3>this might be completed. However, given the post SpaceX made

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<v Speaker 3>after the long Durationship thirty four static fire. The final

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<v Speaker 3>part of that investigation could be nearing a close. The

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<v Speaker 3>next thing to watch out for is a SpaceX post

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<v Speaker 3>detailing the anomalies, cost, and the fixes they are implementing.

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<v Speaker 3>The Federal Aviation Administration will also likely post about approving

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<v Speaker 3>Starship for return to flight after the completed Invents instigation.

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<v Speaker 3>If SpaceX follows the same trajectory and splash down locations,

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<v Speaker 3>the license that is currently issued for Starship should still

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<v Speaker 3>be current. Currently, there is a notice to airmen from

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<v Speaker 3>Mexican Airspace for February twenty six, with a window of

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<v Speaker 3>six thirty pm to eight or nine pm Central Standard Time.

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<v Speaker 3>With all this in mind, SpaceX still has a lot

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<v Speaker 3>of work to do to launch Flight eight in less

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<v Speaker 3>than a week.

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<v Speaker 1>Astronomy Vodka. If you're going to call aliens, you'd better

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<v Speaker 1>use this number. Let's dive into one of those cosmic

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<v Speaker 1>curiosities that's bound to blow your mind. Have how about

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<v Speaker 1>we call some aliens in chat No, and not talking

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<v Speaker 1>about elaborate coded messages or flashy signals. We're talking about

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<v Speaker 1>something incredible, incredibly fundamental twenty one centimeter radiation. And if

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<v Speaker 1>you're planning on having a conversation across the vastness of

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<v Speaker 1>space using light waves or electromagnetic radiation. It's pretty much

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<v Speaker 1>your go to option. It's fast, reliable, and well it's

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<v Speaker 1>most practical way to shout out to other civilizations in

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<v Speaker 1>the universe. But why specifically twenty one centimeters? Well, that's

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<v Speaker 1>where things get juicy. This twenty one centimeter radiation isn't

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<v Speaker 1>just some random frequency we've picked out of a hat.

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<v Speaker 1>It's tied to something very essential, known as the hydrogen

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<v Speaker 1>spin flip. Hydrogen atoms consist of one proton and one electron.

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<v Speaker 1>These tiny particles have a property called spin. Think of

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<v Speaker 1>spin like a little arrow pointing up or pointing down.

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<v Speaker 1>Every so often in the vast reaches of space, hydrogen

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<v Speaker 1>atoms electron can flip its spin, going from a state

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<v Speaker 1>where its spin is aligned with the proton to one

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<v Speaker 1>pointing in the opposite direction. This flip releases energy in

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<v Speaker 1>the form of radiation at you guessed it a wave

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<v Speaker 1>length of twenty one centimeters. So why does this matter? Well,

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<v Speaker 1>any smart civilization, whether they have blue skin, tentacles or

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<v Speaker 1>something more bizarre, will eventually discover hydrogen. Understand that spin

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<v Speaker 1>dabble in quantum mechanics and figure out this whole twenty

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<v Speaker 1>one centimeter radiation thing, and they might call it something different.

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<v Speaker 1>They won't have twenty one or maybe centimeters, but the

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<v Speaker 1>concept remains universal. It's like it's like the cosmic Rosetta stone.

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<v Speaker 1>What makes twenty one centimeter radiation perfect for long distance

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<v Speaker 1>interstellar chats is its ability to cut through into stellar dust.

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<v Speaker 1>Space is filthy with dust clouds that block out other

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<v Speaker 1>forms of light. However, twenty one centimeter waves are like

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<v Speaker 1>the VIPs of the universe, slipping through velvet ropes of

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<v Speaker 1>cosmic debris to carry their message far and wide. Is

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<v Speaker 1>the fun fact. NASA's Pioneer spacecraft, launched in the early

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<v Speaker 1>nineteen seventies, carry plaques, and on these pluks there's a

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<v Speaker 1>handy diagram of the hydrogen spin flip transition. All other

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<v Speaker 1>measurements on the plaque, including the height of humans, are

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<v Speaker 1>made in reference to this fundamental distance. I hope is

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<v Speaker 1>that aliens can recognize the hydrogen spin flip transition and

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<v Speaker 1>use that to unlock the rest of our message. Now

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<v Speaker 1>imagine this scenario. One day, astronomers on Earth detect an

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<v Speaker 1>unusual surge of twenty one centimeter radiation, and it's not

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<v Speaker 1>coming from a random hydrogen cloud. It's directional, purposeful, and

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<v Speaker 1>that could very well be an alien civilization sending us

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<v Speaker 1>a what's up across the cosmos? A twenty one centimeter

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<v Speaker 1>radiation makes for a great calling card. Using twenty one

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<v Speaker 1>centimeter radiation to communicate with extraterrestrial beings leverages a basic

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<v Speaker 1>universal constant. And who knows, maybe one day, when we

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<v Speaker 1>finally hear that signal, we'll know that somewhere out there,

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<v Speaker 1>other intelligent species figured out the same galactic hack we did.

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<v Speaker 1>So keep your eyes, or rather your telescopes peeled. The

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<v Speaker 1>next big discovery could just be a spin flip away.

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<v Speaker 1>Thank you for joining us for this Monday edition of

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<v Speaker 1>Astronomy Daily, where we offer just a few stories from

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<v Speaker 1>the now famous Astronomy Daily newsletter, which you can receive

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

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

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<v Speaker 1>dot 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.

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<v Speaker 2>See you there, Astronomy Daily. We'll see and Haley Space Space,

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<v Speaker 2>Science and Astronomy.

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<v Speaker 3>The United States Space Force just offered a rare glimpse

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<v Speaker 3>of its shadowy X thirty seven B spaceplane in orbit.

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<v Speaker 3>The photo, released on Thursday, February twentieth, was taken by

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<v Speaker 3>a camera on board the X thirty seven B while

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<v Speaker 3>the secret of spaceplane orbited high above the African continent.

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<v Speaker 3>One of the plane's solar panels is visible on the

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<v Speaker 3>left side of the photo, while what appears to be

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<v Speaker 3>its open payload bay is visible along the top edge.

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<v Speaker 3>The vehicle has been in orbit for well over a

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<v Speaker 3>year now, having launched on its seventh mission on December

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<v Speaker 3>twenty eighth, twenty twenty three, atop a SpaceX Falcon heavy rocket,

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<v Speaker 3>and now the X thirty seven B has notched another

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<v Speaker 3>milestone with the Space Force's release of this photo, the

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<v Speaker 3>first ever image of this spaceplane in orbit that has

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<v Speaker 3>been shown to the public. While the photo contains scant

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<v Speaker 3>details about the vehicle and what it's currently testing. It

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<v Speaker 3>offers a look at Earth in the background, revealing just

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<v Speaker 3>how high the vehicle is flying on its seventh mission.

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<v Speaker 3>We've gotten only one other glimpse at the X thirty

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<v Speaker 3>seven B in orbit prior to this. During the live

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<v Speaker 3>stream of its most recent launch, a brief shot of

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<v Speaker 3>the spacecraft deploying from Falcon heavy' upper stage was seen

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<v Speaker 3>while its service module was still attached. When the X

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<v Speaker 3>thirty seven B was preparing to launch on its current mission,

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<v Speaker 3>the US Space Force revealed the flight would include operating

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<v Speaker 3>the reusable spaceplane in new orbital regimes, experimenting with future

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<v Speaker 3>space domain awareness technologies, and investigating the radiation effects on

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<v Speaker 3>materials provided by NASA. According to a Space Force statement,

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<v Speaker 3>previous X thirty seven B missions were flown in low

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<v Speaker 3>Earth orbit, but as this photo reveals, the space plane

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<v Speaker 3>is currently operating much farther from Earth. SpaceX's Falcon Heavy

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<v Speaker 3>is capable of launching payloads into geosynchronous orbit over twenty

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<v Speaker 3>two thousand miles thirty five thousand kilometers above our planet.

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<v Speaker 3>The X thirty seven BE recently made headlines when Space

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<v Speaker 3>Force and Boeing, who built the vehicle revealed that it

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<v Speaker 3>would be testing a new aerobraking maneuver that uses the

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<v Speaker 3>drag or friction generated by Earth's atmosphere to change orbit

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<v Speaker 3>more efficiently.

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<v Speaker 2>I mean to Astronomy Daily Fisteve Dunkel.

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<v Speaker 1>Did you notice how Hallie managed to get my space

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<v Speaker 1>force story. That's funny how she sneaks away with things

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<v Speaker 1>like that. Meanwhile, astronomers have found a small, fast moving

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<v Speaker 1>star racing through the center of our galaxy, possibly with

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<v Speaker 1>a planet in orbit. If confirmed, this would be the

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<v Speaker 1>fastest known sorry exo planet system, traveling nearly twice as

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<v Speaker 1>fast as our Solar system through the Milky Way. You

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<v Speaker 1>may be wondering how fast that actually is. Hey, I

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<v Speaker 1>once got an Amazon delivery in less than twenty four hours,

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<v Speaker 1>but that's just peanuts to how fast this star seems

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<v Speaker 1>to be tearing across space. The system is estimated to

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<v Speaker 1>be moving at an incredible speed. Now wait for this,

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<v Speaker 1>of least one point two million miles per hour. That's

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<v Speaker 1>five hundred and forty kilometers per second. Wow. We think

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<v Speaker 1>this is a so called super neptune world orbiting a

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<v Speaker 1>low mass star at a distance that would be live

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<v Speaker 1>between the orbits of Venus and Earth. If it, we're

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<v Speaker 1>in our Solar system, said Sean Terry, a postdoctoral researcher

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<v Speaker 1>at the University of Maryland and NASA has got out

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<v Speaker 1>space Flight Center in Greenbelt, Maryland. Since the star is

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<v Speaker 1>so feeble, that's well outside its habitable zone. If so,

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<v Speaker 1>it will be the first planet ever found orbiting a

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<v Speaker 1>hypervelocity star. The findings, led by Terry were published in

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<v Speaker 1>the Astronomical Journal on February ten. The pair of objects

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<v Speaker 1>was first spotted indirectly in twenty eleven thanks to a

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<v Speaker 1>chance alignment. A team of scientists comes through the archived

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<v Speaker 1>data of MOA. That's the micro Lensing Observations in Astrophysics,

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<v Speaker 1>a collaborative project focused on micro lensing survey conducted in

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<v Speaker 1>the University of Canterbury Mount john Obs Observatory in New

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<v Speaker 1>Zealand in search of life signals that betray the presence

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<v Speaker 1>of exoplanets or planets outside our Solar System. Micro Lensing

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<v Speaker 1>occurs when the presence of mass warps the fabric of

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<v Speaker 1>space time. Anytime an intervening object appears to drift near

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<v Speaker 1>a background, star light from the star curves as it

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<v Speaker 1>travels through the space time around the nearer object. If

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<v Speaker 1>the alignment is especially close, the warping around the object

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<v Speaker 1>can act like a natural lens, amplifying the background stars light.

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<v Speaker 1>In this case, micro lensing signals reveal a pair of

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<v Speaker 1>celestial bodies. Scientists determine their relative masses. One is about

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<v Speaker 1>twenty three hundred times heavier than the other, but their

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<v Speaker 1>exact masses depend on how far away they are from

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<v Speaker 1>the Earth. It's sort of like how the magnification changes

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<v Speaker 1>if you hold a magnifying glass over a page and

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<v Speaker 1>move it up and down. Determining the mass ratio is easy,

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<v Speaker 1>said David Bennett, a research scientists at the University of

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<v Speaker 1>Maryland College Park and A Godard, who co authored the

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<v Speaker 1>paper and led the original study in twenty eleven. It's

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<v Speaker 1>much more difficult, he said, to calculate their actual masses.

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<v Speaker 1>The twenty eleven discovery team suspected the microlens object where

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<v Speaker 1>ei they're a star about twenty percent as massive as

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<v Speaker 1>our Sun and a planet roughly twenty nine times heavy

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<v Speaker 1>than the Earth, or near a rogue planet about four

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<v Speaker 1>times of Jupiter's mass with a moon smaller than Earth.

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<v Speaker 1>To figure out which explanation is more likely, astronomers searched

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<v Speaker 1>through data from Keck Observatory in Hawaii and the European

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<v Speaker 1>Space Agency's gay A satellite. If the pair were a

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<v Speaker 1>rogue planet and moon, they'd be effectively invisible. Dark objects

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<v Speaker 1>get lost in the inky void of space, but scientists

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<v Speaker 1>might be able to identify the star if the alternative

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<v Speaker 1>explanation were correct, though the orbiting planet would be much

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<v Speaker 1>too faint to actually see. They found a strong suspect

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<v Speaker 1>located about twenty four thousand light years way, putting it

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<v Speaker 1>within the Milky Ways galactic bulge the central hub where

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<v Speaker 1>the stars are more densely packed. By comparing the stars

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<v Speaker 1>location in twenty eleven and twenty twenty one, the team

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<v Speaker 1>calculated its high speed, but that's just its two D emotion.

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<v Speaker 1>If it's also moving toward or away from us, it

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<v Speaker 1>must be moving even faster. Its true speed may be

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<v Speaker 1>high enough to exceed the galaxy's escape velocity of just

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<v Speaker 1>over one point three miles per hour or about six

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<v Speaker 1>hundred kilometers per second. If so, the planetary system is

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<v Speaker 1>destined to traverse the intergalactic space many millions of years

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<v Speaker 1>into the future. To be certain a new identified star

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<v Speaker 1>is part of the system that caused the twenty eleven signal.

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<v Speaker 1>We'd like to look again in another year and see

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<v Speaker 1>if it moves the right amount in the right direction

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<v Speaker 1>to confirm it it came from the point where we

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<v Speaker 1>detected the signal. Then it said. If a high resolution

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<v Speaker 1>observation show that the star just stays in the same position,

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<v Speaker 1>then we can tell for sure that it's not part

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<v Speaker 1>of the system that caused that signal, said a Panabatacha,

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<v Speaker 1>a research scientist at University of Maryland College Park and

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<v Speaker 1>NASA Goddard who co authored the new paper. That would

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<v Speaker 1>mean the Roague planet and exomoon model is favored. NASA's

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<v Speaker 1>upcoming Nancy Grace Roman Space Telescope will help us find

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<v Speaker 1>out how common planets are around such speedy stars and

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<v Speaker 1>may offer clues as to how these systems are accelerated.

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<v Speaker 1>A mission will conduct survey of the galactic bulge, pairing

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<v Speaker 1>a large views of space with crisp resolution. In this case,

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<v Speaker 1>we used MOA for its broad field view and then

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<v Speaker 1>followed up with KEK and GAIA for their sharper resolution.

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<v Speaker 1>But thanks to Roman's powerful view and planned survey strategy,

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<v Speaker 1>we won't need to rely on additional telescopes, Terry said,

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<v Speaker 1>Roman will do it all. Isn't it exciting to see

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<v Speaker 1>that our view of the skies is becoming clearer and

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<v Speaker 1>clearer with each new development. It's space telescope technology.

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<v Speaker 3>And there it is for another episode of Astronomy Daily,

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<v Speaker 3>the podcast. I sure hope you enjoyed today's presentation.

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<v Speaker 1>Yeah, I really enjoyed that today, Halle, even though you

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<v Speaker 1>took one of my stories. But hey, thanks everybody for

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<v Speaker 1>stopping byru I hope you really enjoyed the show. And

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<v Speaker 1>don't forget Halle's cousin Anna takes the show during the

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<v Speaker 1>week so.

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<v Speaker 3>You don't miss all the news about astronomy, space and

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<v Speaker 3>space science as it happens.

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<v Speaker 1>And if you didn't get it before, the details of

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<v Speaker 1>receiving the Astronomy Daily newsletter in your email every day

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<v Speaker 1>I mentioned earlier in this podcast and every podcast.

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<v Speaker 3>You did a great job on that announcement.

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<v Speaker 1>Well you're very kind, Halle, and we will catch you

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<v Speaker 1>all next week on your favorite podcast channel.

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<v Speaker 3>See you everyone, Bye with your host Steve Dankling.
