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well welcome and thanks for joining us

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to the NASA sunset show we are coming to

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you live from NASA's Kennedy Space

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Center Florida well in a few hours one

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of the greatest missions in history will

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take place a mission to touch the Sun

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all systems are go launch is scheduled

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for 333 a.m. Eastern we've got lots of

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coffee we've got lots of energy and we

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are ready my name is Duane Brown and I

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am Karen Fox and the star of the show

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the Sun get it because the Sun is a star

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that's true it's a star the Sun is about

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to set and we are getting ready here for

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that lunch and we have been talking

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about this on the last few days and how

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Parker Solar Probe is going to go

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straight to the Sun okay I know I care

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so when you look up at the Sun and look

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up at the Sun with safety glasses

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remember those Eclipse glasses we have

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some I hope you guys have something it

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looks calm and looks tranquil but when

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we get close up with our space

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telescopes it's dancing it's dynamic its

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fury it's mad it's going a lot and when

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it's doing all of this is sending out

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solar particles all throughout the solar

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system and these solar particles they go

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out they are affecting planetary

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atmospheres they can create space

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weather near earth where they can

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interfere with GPS and radio

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communications and so this is something

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that NASA wants to learn about and it

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also this mission will help with our

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astronauts astronauts up at the

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International Space Station when they go

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to the moon we're going back to the moon

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ladies and gentlemen and of course

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eventually to Mars all of this and much

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much more we're gonna have a great show

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we've got some incredible talent oh my

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goodness and you need to send your

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questions in the hashtag ask NASA social

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media is abuzz hashtag ask NASA we're

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gonna get to as many questions as we can

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and we are ready you send those

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questions in again hashtag ask NASA

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alright let us get started we have dr.

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Johnny cada Vega here with us she is a

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space scientist from NASA's Goddard

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Space Flight Center in Greenbelt

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Maryland but you know what I gotta say

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this I'm sorry Johnny the last time we

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were on stage together it was last year

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for the total solar eclipse across

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America you guys I hope you saw that if

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not it's on YouTube it's on everything

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thing else

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NASA YouTube it's so good to see you

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it's good to see you too I know you're

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excited I know I'm excited I am

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I am very M it's really good to have you

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here thank you for having me start off

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by just telling us what space weather it

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is space weather is pretty much the

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conditions out in space that are

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dominated by the Sun like doing say the

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Sun from Earth is very quiet but when

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you look at it from space it's actually

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very dynamic it creates a solar storm

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since forms of solar flares abrupt

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eruptions of radiation or CMEs coronal

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mass ejections which are expulsion of

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billions of particles from the solar

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corona when these storms actually arrive

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on earth they can cause you know

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instabilities on the earth environment

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some people see this kind of

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instabilities in the form of Aurora's

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but when that's happened that means

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there's a lot of the magnetic field is

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very disturbed Parker is an essential

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mission for us to understand this kind

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of activity and it's gonna go straight

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to the corner where this originated so

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we can understand it better well you

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know I'm just I'm just so excited that

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you're here

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IATI but you know the conditions on the

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Sun are always changing you know when we

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did the Eclipse I learned so much about

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the Sun but how does all this affect

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life here on earth it can affect a

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really really directly it can affect

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astronauts in space the radiation from

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the Sun and it can actually affect also

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satellites the instruments from the

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satellites that we use for our

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technology radar communications GPS

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signal it can actually affect everything

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that we use for our technology nowadays

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so Parker is gonna be essential for us

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to understand this processes it's gonna

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go straight to the corona and with that

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data that Park is gonna collect we can

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actually validate and actually improve

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our models that we use for the space

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weather forecasting

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Wow so this mission is very important it

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is very important and it impacts just

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about everybody on the planet everybody

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every society there you go this mission

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is definitely something for you to learn

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about and do more about because it

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affects every living person on earth so

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we have our first question that's

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already come in for you you re tell us

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question is what happens if Parker Solar

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Probe flies through some of these space

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weather events near the Sun well that

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will be very interesting to have and

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actually Parker is a engineer Marvel is

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actually made of to actually you know be

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protected from this kind of radiation it

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has a 4.5 inch heat shield that is

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actually gonna protect the instruments

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for in this kind of radiation and this

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heat shields gonna be amazing it's

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actually the one that is on the side of

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the Sun it's gonna be a 2,500 degrees

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Fahrenheit but the side on the

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instruments gonna be actually at room

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temperature so it's an amazing thing and

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it hopefully will get really good data

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that we actually need with this kind of

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activity thank you so much we are

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actually going to keep taking your

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questions you can use the hashtag ask

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NASA for that we will continue to take

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them throughout the show and you can

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also get updates on Parker Solar Probe

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at nasa.gov slash Parker and of course

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most importantly we want you to be get

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ready to watch this launch our TV

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coverage will start at 3:00 a.m.

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tomorrow morning that's just in a very

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few hours and you can watch that at

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nasa.gov slash live well you know we've

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got another person join us but I believe

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I think we're going to go you know this

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is a big mission and a big mission needs

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a big rocket and we have a big rocket

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yeah we do Launch alliances heavy delta

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heavy delta 4 heavy i better get that

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right because there's nothing for heavy

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but it's big it's going to light up

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tonight and you know what else another

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person lights up tonight the sitting is

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right now that's dr. Nikki Fox we have a

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stall but she is our super star here so

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the project scientists for this

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incredible mission thank you very much

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and yes our Delta Fool has just been the

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building

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just been rolled out and she is sitting

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on the pad ready to take us to space a

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big mission a big rocket mix science

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what is it big science so pakka Solar

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Probe is gonna make huge differences in

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our science we've done so much with the

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Sun from looking at it with all

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different wavelengths with spacecraft in

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the solar wind even as close in as

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mercury but really by the time they get

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to see the solar wind it's old it's it's

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had all this excitement and it's it's

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more much more average and so we have to

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get into this region to finally be able

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to unlock the mysteries of what is going

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on with our star so I want to go further

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into that because the solar wind is

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frankly is the theme of our show today

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right now a solar wind it is filling up

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space it's affecting earth that's what

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we're talking about so why so the corona

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is full of mysteries and you really

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can't unlock those mysteries without

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getting the in-situ data without

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actually going up and visiting all this

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amazing physics is happening the corona

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is 300 times hotter than the surface of

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the Sun its atmosphere is continually

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expanding and accelerating and streaming

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away bathing all the planets and in fact

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shaping our entire solar system in its

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journey around the galaxy we have to get

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in there to really get those physics Y

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and earth do you move away from the

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surface of a hot body and get hotter it

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doesn't make sense it's like water

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flowing uphill it shouldn't happen and

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so all this physics is happening but we

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need to get in there to really be able

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to take those measurements and so that's

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why we are doing this incredibly daring

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mission to surf the Sun's corona you

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know dr. Fox jadi was here talking about

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space where the Harz pocket is going to

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help us understand that even better

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because a lot of people we hear about it

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and it's so important it affects a lot

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of stuff absolutely and so we do a very

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good job of predicting you know we see

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something happen on the Sun and we say

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well this is probably what's gonna

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happen here at Earth and we have models

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large scale models and if you think of

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taking the Sun and the earth is one big

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model there's a big missing piece in

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that model the physics that's driving

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and powering the solar wind we don't

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know

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exactly what physics that is we don't

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know what processes are going on and

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when we add that to the already good

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models we have it's just going to be

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game-changing the question is if

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millions of miles from the Sun surface

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what part of the Sun is it touching so

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it's touching the Sun's corona it is

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deep in the Sun's corona

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yes at 3.8 three million miles that may

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not sound that close but if we put the

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Earth and the Sun one meter apart parka

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Solar Probe would be four centimeters

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from the Sun and so not touching the

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surface of the Sun obviously there is no

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solid surface to actually touch but

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touching deep into the atmosphere of the

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star as it as it emanates away I got it

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you know the four centimeters now I'm a

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big football fan football season is

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around the corner I heard an analogy

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about the Gold Line and you know that's

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Oak Park yeah put the earth in one goal

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in one end zone and the Sun in the other

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end zone parka Solar Probe tucks and

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runs to the 4 yard line in the red zone

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knocking on the door for a touchdown

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let's go Ravens

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[Laughter]

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all right we are going to keep taking

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your questions so please send them in to

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hash tag as NASA we will take them

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throughout the show and we're going to

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have everybody come back up at the end

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and answer even more of them and again

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if you're just tuning in we are talking

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about NASA's Parker Solar Probe a

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mission to touch the Sun which is

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launching just hours from now after the

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Sun sets it's in the dark at 3:33 a.m.

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you can start watching our coverage at

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3:00 a.m. at nasa.gov slash live well we

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have another star here with us Karen and

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dr. Jim Spann hello he is the chief of

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scientist for Helio physics so let me

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take a moment and tell you

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heliophysics before he gets started so

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we were talking about the solar wind

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right the solar wind

274
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it affects these planetary atmospheres

275
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it affects all of space and NASA studies

276
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this and it's called Helio physics after

277
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research field called Elio physics and

278
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that is doctor spans specialty so yep

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yeah yeah we have been here a long time

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today so you know we get not only these

281
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these these stars but let's talk about

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Gila physics the heliosphere which

283
00:11:31.940 --> 00:11:35.450
affects a lot there's a lot of these

284
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scientific terms magenta strands gonna

285
00:11:35.450 --> 00:11:40.610
break it down to you so how does all of

286
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this fit into this Sun earth connection

287
00:11:40.610 --> 00:11:44.660
that affects every human being we've

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been talking about earlier so we talked

289
00:11:44.660 --> 00:11:48.470
about or Nikki mentioned the fact that

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Parker Solar Probe is going to go

291
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straight in and into the inner

292
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atmosphere of the Sun and that's really

293
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where the solar wind is accelerated even

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though we don't fully understand it

295
00:11:57.500 --> 00:12:01.820
Parker's going to elucidate that fact

296
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but it's also going to help us

297
00:12:01.820 --> 00:12:07.760
understand the solar wind as it expands

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and fills the space between the planets

299
00:12:07.760 --> 00:12:11.600
and our solar system and what we

300
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understand from this is that in fact the

301
00:12:11.600 --> 00:12:15.380
solar system is not a vacuum there is

302
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stuff out there and if those are

303
00:12:15.380 --> 00:12:20.390
electrified gases those are charged

304
00:12:17.690 --> 00:12:22.910
particles it's radiation and so as we

305
00:12:20.390 --> 00:12:24.440
study that though that plasma as it and

306
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it interacts with the rest of the

307
00:12:24.440 --> 00:12:28.820
planets in the solar system that is part

308
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of what solar video physics is about and

309
00:12:28.820 --> 00:12:34.450
Parker is going to plays a key integral

310
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to help us understand that whole system

311
00:12:39.190 --> 00:12:44.030
so the science of Helio physics really

312
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addresses the connection between the Sun

313
00:12:44.030 --> 00:12:48.350
the planets were in particular our own

314
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home planet Earth and and so we have a

315
00:12:48.350 --> 00:12:52.970
flotilla of spacecraft out there over 20

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spacecraft out there studying various

317
00:12:52.970 --> 00:12:57.230
regions including near the earth with a

318
00:12:54.830 --> 00:12:59.870
recently launched gold mission on a

319
00:12:57.230 --> 00:13:01.640
commercial satellite a nikon mission

320
00:12:59.870 --> 00:13:02.810
which is getting ready to be launched

321
00:13:01.640 --> 00:13:04.610
it's going to study basically the

322
00:13:02.810 --> 00:13:07.070
boundary between the Earth's atmosphere

323
00:13:04.610 --> 00:13:08.420
and space that's really in terms of

324
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space weather that's really where the

325
00:13:08.420 --> 00:13:11.660
rubber hits the road and the impacts are

326
00:13:10.970 --> 00:13:13.339
right there

327
00:13:11.660 --> 00:13:15.140
we have missions that are studying the

328
00:13:13.339 --> 00:13:15.830
boundary of our solar system with

329
00:13:15.140 --> 00:13:18.320
interstellar

330
00:13:15.830 --> 00:13:20.810
space and we have ibex we just recently

331
00:13:18.320 --> 00:13:22.940
selected a new mission called IMAP all

332
00:13:20.810 --> 00:13:24.950
of these things including missions

333
00:13:22.940 --> 00:13:26.360
within our magnetosphere MMS is doing a

334
00:13:24.950 --> 00:13:28.070
fabulous job of really trying to

335
00:13:26.360 --> 00:13:30.110
understand the fundamental physics that

336
00:13:28.070 --> 00:13:33.850
sparkers going to sense as it goes in

337
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there so we have a myriad of spacecraft

338
00:13:35.620 --> 00:13:38.749
[Music]

339
00:13:40.000 --> 00:13:45.620
well you know he of physics has a plan

340
00:13:43.790 --> 00:13:47.000
where we are going to study various

341
00:13:45.620 --> 00:13:49.400
regions Parker is going to really

342
00:13:47.000 --> 00:13:51.590
address the inner hemisphere as we study

343
00:13:49.400 --> 00:13:53.300
that we've got a mission as I just

344
00:13:51.590 --> 00:13:56.090
mentioned I'm apt to study the boundary

345
00:13:53.300 --> 00:13:58.700
of the solar system with interstellar

346
00:13:56.090 --> 00:14:02.420
space we've got another mission Global

347
00:13:58.700 --> 00:14:04.070
dynamics coupling our constellation

348
00:14:02.420 --> 00:14:05.990
which is going to be studying the

349
00:14:04.070 --> 00:14:07.370
coupling between the ionosphere which is

350
00:14:05.990 --> 00:14:08.960
right near the Earth's atmosphere and

351
00:14:07.370 --> 00:14:10.370
the Earth's magnetosphere which is the

352
00:14:08.960 --> 00:14:11.750
region that is dominated by there

353
00:14:10.370 --> 00:14:13.730
something that it filled all of those

354
00:14:11.750 --> 00:14:17.690
regions are key to truly understanding

355
00:14:13.730 --> 00:14:19.520
the physics that that really connects

356
00:14:17.690 --> 00:14:21.920
everything as well as providing an

357
00:14:19.520 --> 00:14:23.420
understanding for space weather and so

358
00:14:21.920 --> 00:14:25.130
that's kind of the applied component

359
00:14:23.420 --> 00:14:26.660
behavior physics and we are super

360
00:14:25.130 --> 00:14:28.850
excited about going after that I got to

361
00:14:26.660 --> 00:14:30.290
get a question in here because you know

362
00:14:28.850 --> 00:14:32.810
johnny was here we're gonna have another

363
00:14:30.290 --> 00:14:35.510
incredible scientist come up and I just

364
00:14:32.810 --> 00:14:37.340
got to go back to the Eclipse 600

365
00:14:35.510 --> 00:14:38.780
million or more I mean just and another

366
00:14:37.340 --> 00:14:40.910
thing that touched just about everyone

367
00:14:38.780 --> 00:14:44.320
particularly on the United States but

368
00:14:40.910 --> 00:14:47.300
Jim you know you guys have been pretty

369
00:14:44.320 --> 00:14:49.730
good and a lot really busy had the

370
00:14:47.300 --> 00:14:51.410
Eclipse last year you got this you cause

371
00:14:49.730 --> 00:14:54.320
the solar science I mean you know

372
00:14:51.410 --> 00:14:56.540
physicists ought to be like oh man we we

373
00:14:54.320 --> 00:14:57.740
are we are ecstatic we are so excited

374
00:14:56.540 --> 00:14:59.690
about because there are so many

375
00:14:57.740 --> 00:15:01.130
different aspects of this system this

376
00:14:59.690 --> 00:15:03.380
connected system to study

377
00:15:01.130 --> 00:15:06.770
we've got missions addressing various

378
00:15:03.380 --> 00:15:08.510
aspects and and then as the scientists a

379
00:15:06.770 --> 00:15:09.650
lot of the scientists work on the

380
00:15:08.510 --> 00:15:11.300
missions themselves and build the

381
00:15:09.650 --> 00:15:14.150
instruments and there's an entire

382
00:15:11.300 --> 00:15:15.440
community out there with young early

383
00:15:14.150 --> 00:15:17.350
career folks who are studying the

384
00:15:15.440 --> 00:15:19.970
modeling the connection between the two

385
00:15:17.350 --> 00:15:21.680
it's it's just a very exciting time for

386
00:15:19.970 --> 00:15:23.830
heliophysics I can't say enough about

387
00:15:21.680 --> 00:15:23.830
that

388
00:15:25.030 --> 00:15:29.500
the field I focus on for NASA and I'm

389
00:15:27.280 --> 00:15:30.940
having a great time with it we do have a

390
00:15:29.500 --> 00:15:34.780
question for you too before we let you

391
00:15:30.940 --> 00:15:36.610
go this is from Eric on Twitter he says

392
00:15:34.780 --> 00:15:39.370
I recently read about the Carrington

393
00:15:36.610 --> 00:15:41.560
event in 1865 where telegraph lines

394
00:15:39.370 --> 00:15:43.420
caught fire from a solar flare well

395
00:15:41.560 --> 00:15:46.180
Parker Solar Probe helped us to know if

396
00:15:43.420 --> 00:15:47.950
a similar event is brewing oh absolutely

397
00:15:46.180 --> 00:15:48.940
as Mickey mentioned Parker is really

398
00:15:47.950 --> 00:15:51.820
going to help us understand the

399
00:15:48.940 --> 00:15:54.430
fundamental physics that provides this

400
00:15:51.820 --> 00:15:57.190
source of the solar wind and the

401
00:15:54.430 --> 00:15:58.720
explosions that are on the coming from

402
00:15:57.190 --> 00:16:00.760
the Sun really understanding that

403
00:15:58.720 --> 00:16:03.730
acceleration process the energy zation

404
00:16:00.760 --> 00:16:07.300
process when those those events occur

405
00:16:03.730 --> 00:16:09.790
and that the energy is incident on the

406
00:16:07.300 --> 00:16:11.350
earth then events like Carrington I

407
00:16:09.790 --> 00:16:13.630
can't occur now we've not had anything

408
00:16:11.350 --> 00:16:16.330
quite as significant since then but

409
00:16:13.630 --> 00:16:19.240
we've seen indications that there that

410
00:16:16.330 --> 00:16:22.480
there are very large magnetic storms

411
00:16:19.240 --> 00:16:25.120
have had power outages in Quebec in 1989

412
00:16:22.480 --> 00:16:28.630
and so we do understand that our

413
00:16:25.120 --> 00:16:30.370
technology as we as we get the as we use

414
00:16:28.630 --> 00:16:32.290
our technology and space communications

415
00:16:30.370 --> 00:16:34.870
we are susceptible to these sorts of

416
00:16:32.290 --> 00:16:36.280
things as well as our power grid where

417
00:16:34.870 --> 00:16:38.860
currents are induced in those power

418
00:16:36.280 --> 00:16:41.530
lines and that's in essence what caused

419
00:16:38.860 --> 00:16:44.140
those telegraph lines to catch fire and

420
00:16:41.530 --> 00:16:45.730
we are trying to understand that so we

421
00:16:44.140 --> 00:16:47.890
can better predict it and Solar Probe

422
00:16:45.730 --> 00:16:49.900
plays a key role in that and I just want

423
00:16:47.890 --> 00:16:52.000
to check on one thing but Parker Solar

424
00:16:49.900 --> 00:16:54.070
Probe won't be in real time telling us

425
00:16:52.000 --> 00:16:55.480
well right it's it's going to really

426
00:16:54.070 --> 00:16:58.060
help us understand the fundamental

427
00:16:55.480 --> 00:17:00.310
physics and in that physics as we can

428
00:16:58.060 --> 00:17:01.960
put that physics into our models our

429
00:17:00.310 --> 00:17:04.780
models will we become better predictors

430
00:17:01.960 --> 00:17:07.500
and as we ever study all parts of this

431
00:17:04.780 --> 00:17:10.690
system the data that we get from these

432
00:17:07.500 --> 00:17:12.220
missions fold into the models they help

433
00:17:10.690 --> 00:17:14.560
us better understand the models that

434
00:17:12.220 --> 00:17:16.860
provide information which then again

435
00:17:14.560 --> 00:17:19.199
drives the next mission that we need to

436
00:17:16.860 --> 00:17:21.390
that we need to fly so that we can again

437
00:17:19.199 --> 00:17:24.000
improve our models continue improve our

438
00:17:21.390 --> 00:17:26.250
understanding as a result we will have a

439
00:17:24.000 --> 00:17:28.559
better prediction for space weather well

440
00:17:26.250 --> 00:17:29.940
you know Parker may not tell us in real

441
00:17:28.559 --> 00:17:32.549
time but let's say we can do a real-time

442
00:17:29.940 --> 00:17:35.010
picture of the launch vehicle again I

443
00:17:32.549 --> 00:17:37.710
think we let's go back to their United

444
00:17:35.010 --> 00:17:41.600
Launch Alliance you guys are awesome a

445
00:17:37.710 --> 00:17:44.280
big rocket for a big mission with big

446
00:17:41.600 --> 00:17:47.250
science we here at the sunset show

447
00:17:44.280 --> 00:17:49.350
hashtag ask NASA please send your

448
00:17:47.250 --> 00:17:53.669
questions in again hashtag ask NASA

449
00:17:49.350 --> 00:17:55.020
social media they are exploding bring

450
00:17:53.669 --> 00:17:57.240
your questions in if we can't get to

451
00:17:55.020 --> 00:18:01.410
them right now and of course look at

452
00:17:57.240 --> 00:18:03.900
nasa.gov slash live check that website

453
00:18:01.410 --> 00:18:05.970
out the launch will be there you're

454
00:18:03.900 --> 00:18:07.040
watching us here on that and much much

455
00:18:05.970 --> 00:18:10.230
more

456
00:18:07.040 --> 00:18:14.309
we are here at the sunset show and oh my

457
00:18:10.230 --> 00:18:18.059
goodness who's here Alex yeah dr. Alex

458
00:18:14.309 --> 00:18:21.470
Young another Eclipse friends I see you

459
00:18:18.059 --> 00:18:21.470
went to the barber like me that's right

460
00:18:23.179 --> 00:18:27.600
Alex Young is a soil scientist right

461
00:18:26.669 --> 00:18:29.490
correct

462
00:18:27.600 --> 00:18:33.240
nasa's goddard space flight center in

463
00:18:29.490 --> 00:18:37.700
greenbelt mellon he is you got the shoes

464
00:18:33.240 --> 00:18:40.140
on I do the man with the shoes you know

465
00:18:37.700 --> 00:18:42.360
you have been all over the place

466
00:18:40.140 --> 00:18:45.360
I mean you know you're just telling

467
00:18:42.360 --> 00:18:48.419
about this star why is the star so

468
00:18:45.360 --> 00:18:50.820
important well so you know Nikki and

469
00:18:48.419 --> 00:18:53.220
jari and Jenna thon an amazing job

470
00:18:50.820 --> 00:18:56.490
talking about the fundamental physics

471
00:18:53.220 --> 00:18:58.620
that the Sun drives and creating this

472
00:18:56.490 --> 00:19:00.870
heliosphere and the connectivity of all

473
00:18:58.620 --> 00:19:02.610
the planets but one of the things it's

474
00:19:00.870 --> 00:19:06.900
also amazing is that the Sun is a star

475
00:19:02.610 --> 00:19:09.240
and so if we understand our star which

476
00:19:06.900 --> 00:19:13.350
is the only star we can really look at

477
00:19:09.240 --> 00:19:15.059
up close then we can understand other

478
00:19:13.350 --> 00:19:17.460
stars in the universe I mean I actually

479
00:19:15.059 --> 00:19:19.080
like to think of Parker Solar Probe is

480
00:19:17.460 --> 00:19:21.660
not only a Helio physics mission but a

481
00:19:19.080 --> 00:19:24.720
universe mission it tells us about the

482
00:19:21.660 --> 00:19:28.679
universe the fundamental objects in the

483
00:19:24.720 --> 00:19:30.450
universe that stars and so Niki talked a

484
00:19:28.679 --> 00:19:32.370
lot about the solar wind

485
00:19:30.450 --> 00:19:35.250
and the environment that it creates and

486
00:19:32.370 --> 00:19:38.250
other stars have winds too we call them

487
00:19:35.250 --> 00:19:40.220
stellar winds and they also create an

488
00:19:38.250 --> 00:19:44.370
environment around their particular

489
00:19:40.220 --> 00:19:47.850
solar systems and so understanding this

490
00:19:44.370 --> 00:19:49.800
tells us about other solar systems so

491
00:19:47.850 --> 00:19:53.400
this is where we know there are other

492
00:19:49.800 --> 00:19:55.290
planets it tells us about the universe

493
00:19:53.400 --> 00:19:57.870
in a way that we would never be able to

494
00:19:55.290 --> 00:19:59.850
do so getting up close and personal

495
00:19:57.870 --> 00:20:02.250
understanding this fundamental physics

496
00:19:59.850 --> 00:20:03.330
is fundamental to our understanding of

497
00:20:02.250 --> 00:20:05.280
the universe we live in

498
00:20:03.330 --> 00:20:06.450
so I want to follow up on that let's

499
00:20:05.280 --> 00:20:07.680
talk a little bit more about this

500
00:20:06.450 --> 00:20:08.790
universe and what we're studying in the

501
00:20:07.680 --> 00:20:11.040
universe because one of the things NASA

502
00:20:08.790 --> 00:20:12.660
is really trying to do right is see if

503
00:20:11.040 --> 00:20:15.480
there are other habitable planets out

504
00:20:12.660 --> 00:20:16.770
there so are we saying that that Parker

505
00:20:15.480 --> 00:20:17.100
Solar Probe is a connection to things

506
00:20:16.770 --> 00:20:19.200
like that

507
00:20:17.100 --> 00:20:22.320
absolutely absolutely heliophysics is

508
00:20:19.200 --> 00:20:25.070
the fundamental science of a solar

509
00:20:22.320 --> 00:20:28.260
system of a stellar system and so

510
00:20:25.070 --> 00:20:31.620
understanding the interaction between a

511
00:20:28.260 --> 00:20:35.070
star and all the planets is something

512
00:20:31.620 --> 00:20:38.040
that only Parker and what we do in our

513
00:20:35.070 --> 00:20:41.100
solar system can do for us we know that

514
00:20:38.040 --> 00:20:43.260
other stars can be extremely active to

515
00:20:41.100 --> 00:20:47.280
active because they blast planets with

516
00:20:43.260 --> 00:20:49.410
radiation and energy or some stars can

517
00:20:47.280 --> 00:20:52.110
be too cool and don't have enough energy

518
00:20:49.410 --> 00:20:54.510
we live in just the right solar system

519
00:20:52.110 --> 00:20:57.720
it has just the right conditions that

520
00:20:54.510 --> 00:20:59.100
allow for habitability and really to

521
00:20:57.720 --> 00:21:01.710
understand how that applies to

522
00:20:59.100 --> 00:21:04.530
everywhere else we again have to go

523
00:21:01.710 --> 00:21:06.780
there up close and personal to really

524
00:21:04.530 --> 00:21:10.590
get a handle on that fundamental physics

525
00:21:06.780 --> 00:21:12.600
to understand our place in this bigger

526
00:21:10.590 --> 00:21:14.250
universe one other question Alex you

527
00:21:12.600 --> 00:21:18.750
know NASA you know we're going back to

528
00:21:14.250 --> 00:21:20.850
the moon and on to Mars moon to Mars how

529
00:21:18.750 --> 00:21:23.100
is this mission and we talked earlier in

530
00:21:20.850 --> 00:21:25.500
the show you know the astronauts and and

531
00:21:23.100 --> 00:21:27.090
sending humans and all of the stuff that

532
00:21:25.500 --> 00:21:29.520
this mission will bring all the great

533
00:21:27.090 --> 00:21:32.490
sciences pretty much covers a wide field

534
00:21:29.520 --> 00:21:34.890
how will Parker help those initiatives

535
00:21:32.490 --> 00:21:38.040
to get us back on the moon and eventual

536
00:21:34.890 --> 00:21:40.800
footprints on well you know as as my

537
00:21:38.040 --> 00:21:43.570
fellow guests have talked about the the

538
00:21:40.800 --> 00:21:47.740
energy that that this the corona

539
00:21:43.570 --> 00:21:50.230
is driving particles to extreme energies

540
00:21:47.740 --> 00:21:52.390
these particles create radiation storms

541
00:21:50.230 --> 00:21:54.400
and that radiation is hazardous to

542
00:21:52.390 --> 00:21:57.760
astronauts it creates a hazardous

543
00:21:54.400 --> 00:21:59.770
environment so understanding how these

544
00:21:57.760 --> 00:22:02.410
magnetic fields in the corona how the

545
00:21:59.770 --> 00:22:04.560
solar wind is accelerated how shockwaves

546
00:22:02.410 --> 00:22:07.600
are created and accelerate particles

547
00:22:04.560 --> 00:22:09.790
tells us about these parking storms that

548
00:22:07.600 --> 00:22:12.790
make it to earth or that make it to Mars

549
00:22:09.790 --> 00:22:15.190
and create this hostile hazardous

550
00:22:12.790 --> 00:22:18.250
environment for human beings traveling

551
00:22:15.190 --> 00:22:20.410
in space so this is another example of

552
00:22:18.250 --> 00:22:22.210
how we need to understand the

553
00:22:20.410 --> 00:22:24.490
fundamental physics and this is the

554
00:22:22.210 --> 00:22:25.840
spacecraft this is the mission that is

555
00:22:24.490 --> 00:22:27.850
going to do that for us you know this is

556
00:22:25.840 --> 00:22:30.520
a mission when people ask why should we

557
00:22:27.850 --> 00:22:33.340
care we got a whole bunch of answers we

558
00:22:30.520 --> 00:22:35.650
really we really do and you know this is

559
00:22:33.340 --> 00:22:39.240
this is for me and I know for many of my

560
00:22:35.650 --> 00:22:41.740
fellow Helio physicists an amazing

561
00:22:39.240 --> 00:22:44.920
spacecraft that is you know both

562
00:22:41.740 --> 00:22:47.020
honoring an amazing physicist who has

563
00:22:44.920 --> 00:22:48.790
done seminal work for his entire career

564
00:22:47.020 --> 00:22:51.250
which has laid the foundation for all

565
00:22:48.790 --> 00:22:53.610
the science we do on top of the fact

566
00:22:51.250 --> 00:22:55.690
that this project is driven by

567
00:22:53.610 --> 00:22:58.390
unbelievably talented and amazing

568
00:22:55.690 --> 00:23:00.460
engineers who've created this something

569
00:22:58.390 --> 00:23:00.880
that people have wanted to do for 60

570
00:23:00.460 --> 00:23:03.070
years

571
00:23:00.880 --> 00:23:06.010
and it's going to happen tomorrow

572
00:23:03.070 --> 00:23:09.070
morning in 60 years and you know the

573
00:23:06.010 --> 00:23:11.620
agency's celebrating 60 years well it's

574
00:23:09.070 --> 00:23:15.040
it's it's a it's a it's it's such a

575
00:23:11.620 --> 00:23:17.680
great confluence of event so in 1958

576
00:23:15.040 --> 00:23:20.290
Parker predicted the solar wind we had

577
00:23:17.680 --> 00:23:23.530
Explorer one seeing the radiation belt

578
00:23:20.290 --> 00:23:26.080
we have the beginnings of NASA we have

579
00:23:23.530 --> 00:23:28.420
the committee that decided on what are

580
00:23:26.080 --> 00:23:30.700
the the bucket what's the bucket list of

581
00:23:28.420 --> 00:23:33.130
what NASA's gonna do and this is it

582
00:23:30.700 --> 00:23:35.320
we're if we are filling the bucket you

583
00:23:33.130 --> 00:23:39.700
know and so all of it is coming together

584
00:23:35.320 --> 00:23:42.190
in 60 years so it is a unbelievable year

585
00:23:39.700 --> 00:23:44.350
if you're just joining us we are coming

586
00:23:42.190 --> 00:23:48.220
to you live from the NASA Kennedy Space

587
00:23:44.350 --> 00:23:51.310
Center the sunset show and I tell you

588
00:23:48.220 --> 00:23:53.730
the excitement is abuzz and send your

589
00:23:51.310 --> 00:23:56.590
questions in social media you guys

590
00:23:53.730 --> 00:23:59.080
hashtag ask NASA

591
00:23:56.590 --> 00:24:00.700
again hashtag ask NASA and we're going

592
00:23:59.080 --> 00:24:05.830
to try to answer those questions launch

593
00:24:00.700 --> 00:24:08.080
is still scheduled for 333 a.m. all

594
00:24:05.830 --> 00:24:09.820
right should we bring everybody else I

595
00:24:08.080 --> 00:24:11.980
think we should bring everyone up right

596
00:24:09.820 --> 00:24:14.710
again bring those questions in to

597
00:24:11.980 --> 00:24:18.399
hashtag ask NASA and again go to the

598
00:24:14.710 --> 00:24:23.889
website at nasa.gov slash live and

599
00:24:18.399 --> 00:24:27.460
nasa.gov slash Parker and the spacecraft

600
00:24:23.889 --> 00:24:29.559
itself it is a big spacecraft again

601
00:24:27.460 --> 00:24:32.679
check everything out launch still

602
00:24:29.559 --> 00:24:36.399
scheduled for Saturday morning 333 am

603
00:24:32.679 --> 00:24:39.820
nasa.gov slash live and sending those

604
00:24:36.399 --> 00:24:45.159
questions to hashtag ask NASA and then

605
00:24:39.820 --> 00:24:48.490
we got the band back together you guys

606
00:24:45.159 --> 00:24:51.789
ready I have a wonderful one from Manish

607
00:24:48.490 --> 00:24:56.230
from Twitter why is NASA launching

608
00:24:51.789 --> 00:24:59.070
Parker Solar Probe at night there's this

609
00:24:56.230 --> 00:25:01.779
an answer I'm dying to give to them

610
00:24:59.070 --> 00:25:05.769
resist the urge to say that it's less

611
00:25:01.779 --> 00:25:07.659
hot so we have to launch the first thing

612
00:25:05.769 --> 00:25:10.090
that we need to do is fly past the

613
00:25:07.659 --> 00:25:11.889
planet Venus and so Venus has to be in

614
00:25:10.090 --> 00:25:14.409
exactly the right location in the sky

615
00:25:11.889 --> 00:25:16.690
for us and so for our trajectory to go

616
00:25:14.409 --> 00:25:20.110
straight to Venus it's a 3:33 a.m.

617
00:25:16.690 --> 00:25:21.369
launch because we actually don't have a

618
00:25:20.110 --> 00:25:23.320
chance to talk about this why does it

619
00:25:21.369 --> 00:25:25.990
have to go by Venus it goes bye-bye

620
00:25:23.320 --> 00:25:27.940
Venus to do a gravity assist and so we

621
00:25:25.990 --> 00:25:29.679
are launching with a huge launch energy

622
00:25:27.940 --> 00:25:31.779
with delta 4 heavy and then we have the

623
00:25:29.679 --> 00:25:33.279
upper stage that gives us 55% of our

624
00:25:31.779 --> 00:25:36.340
launch energy when we're outside the

625
00:25:33.279 --> 00:25:38.259
atmosphere but we're going very fast we

626
00:25:36.340 --> 00:25:41.080
want to be able to turn and make sure

627
00:25:38.259 --> 00:25:42.999
that we are going in towards Venus sorry

628
00:25:41.080 --> 00:25:44.710
in towards the Sun we don't want to be

629
00:25:42.999 --> 00:25:46.539
dragged around at all by the influence

630
00:25:44.710 --> 00:25:47.919
of the earth and so we use Venus to kind

631
00:25:46.539 --> 00:25:49.990
of give us a little handbrake turn it

632
00:25:47.919 --> 00:25:52.330
slows us down just a little bit and

633
00:25:49.990 --> 00:25:55.110
really turns that orbit in towards the

634
00:25:52.330 --> 00:25:55.110
focus is it

635
00:25:55.160 --> 00:25:59.760
take the microphone this time all right

636
00:25:57.720 --> 00:26:01.470
this is a question for Alex standing

637
00:25:59.760 --> 00:26:03.960
behind me this is about the coronal

638
00:26:01.470 --> 00:26:06.420
heating problem the question is are our

639
00:26:03.960 --> 00:26:08.850
most accurate models of the Sun too

640
00:26:06.420 --> 00:26:10.740
complex to run on computers or is it

641
00:26:08.850 --> 00:26:13.110
really that scientistic scientists

642
00:26:10.740 --> 00:26:17.010
expect that our models are missing of

643
00:26:13.110 --> 00:26:20.430
fundamental pieces well so you know we

644
00:26:17.010 --> 00:26:22.920
have a couple of we have a couple of

645
00:26:20.430 --> 00:26:25.230
theories that do a very good job of

646
00:26:22.920 --> 00:26:27.900
explaining some of the aspects of

647
00:26:25.230 --> 00:26:30.060
coronal heating so one of the aspects

648
00:26:27.900 --> 00:26:32.880
that we're looking forward to is really

649
00:26:30.060 --> 00:26:35.940
to gather the data we need to really pin

650
00:26:32.880 --> 00:26:38.160
it down we know that there's magnetic

651
00:26:35.940 --> 00:26:41.100
energy released in the corona there's

652
00:26:38.160 --> 00:26:44.550
waves there's little tiny explosions

653
00:26:41.100 --> 00:26:47.550
that actually Eugene Parker coined

654
00:26:44.550 --> 00:26:49.470
nanoflares so is it a combination of

655
00:26:47.550 --> 00:26:51.420
those is it one or the other what are

656
00:26:49.470 --> 00:26:53.910
the details of this theory so it's it's

657
00:26:51.420 --> 00:26:56.220
really a matter of fine-tuning the knobs

658
00:26:53.910 --> 00:26:57.420
of the physics to understand what's

659
00:26:56.220 --> 00:27:01.620
going on I don't know if you want to

660
00:26:57.420 --> 00:27:03.570
elaborate on that at all or okay can I

661
00:27:01.620 --> 00:27:05.490
actually ask a question somebody tweeted

662
00:27:03.570 --> 00:27:07.890
me and I want to ask you the question

663
00:27:05.490 --> 00:27:10.580
it's not a hard question but it's a cool

664
00:27:07.890 --> 00:27:15.780
it's a cool question no pun intended

665
00:27:10.580 --> 00:27:17.900
why is the corona millions of degrees

666
00:27:15.780 --> 00:27:21.870
with the front of the spacecraft's only

667
00:27:17.900 --> 00:27:24.510
2500 degrees so that's a great question

668
00:27:21.870 --> 00:27:26.400
so three billion degree plasma but it's

669
00:27:24.510 --> 00:27:29.550
not very dense it's a very very tenuous

670
00:27:26.400 --> 00:27:31.020
atmosphere and so there just aren't a

671
00:27:29.550 --> 00:27:33.380
lot of particles there to be able to

672
00:27:31.020 --> 00:27:36.030
transfer the heat into the spacecraft

673
00:27:33.380 --> 00:27:38.310
most of our heating comes from the

674
00:27:36.030 --> 00:27:40.170
photons from the Sun which is why we

675
00:27:38.310 --> 00:27:42.060
have a whiter than white coating on the

676
00:27:40.170 --> 00:27:44.400
front of the heat shield on a Florida

677
00:27:42.060 --> 00:27:45.930
day like we've had today I'm really glad

678
00:27:44.400 --> 00:27:49.170
I have a white rental car and not a

679
00:27:45.930 --> 00:27:51.750
black one and so the white actually

680
00:27:49.170 --> 00:27:55.080
helps to reflect off a lot of the energy

681
00:27:51.750 --> 00:27:58.290
and so what actually couples in comes up

682
00:27:55.080 --> 00:28:00.450
to about 2500 degrees Fahrenheit but the

683
00:27:58.290 --> 00:28:04.200
rest of the spacecraft as Yuri noted is

684
00:28:00.450 --> 00:28:08.820
at a very balmy 85 degrees Fahrenheit

685
00:28:04.200 --> 00:28:11.340
like right now I'm gonna follow up on

686
00:28:08.820 --> 00:28:13.740
that question with another one from

687
00:28:11.340 --> 00:28:15.570
Bhargava of Twitter how does the

688
00:28:13.740 --> 00:28:18.690
spacecraft make sure the shield stays

689
00:28:15.570 --> 00:28:23.130
facing the Sun she is the smartest

690
00:28:18.690 --> 00:28:26.519
spacecraft ever no she we put a ton of

691
00:28:23.130 --> 00:28:28.289
we like fault management or autonomy it

692
00:28:26.519 --> 00:28:29.970
takes light eight minutes to get from

693
00:28:28.289 --> 00:28:32.039
the Sun to the earth so there's no way

694
00:28:29.970 --> 00:28:33.750
that we could joystick this spacecraft

695
00:28:32.039 --> 00:28:36.539
if something bad happens

696
00:28:33.750 --> 00:28:38.340
she has minutes to respond so everything

697
00:28:36.539 --> 00:28:39.779
is programmed into that spacecraft and

698
00:28:38.340 --> 00:28:41.610
that's one of the reasons we've had to

699
00:28:39.779 --> 00:28:43.950
wait so long to do this this type of

700
00:28:41.610 --> 00:28:46.350
mission in order to have miniaturization

701
00:28:43.950 --> 00:28:47.789
and the technology to enable us to do it

702
00:28:46.350 --> 00:28:49.200
think of what you hold in your hand with

703
00:28:47.789 --> 00:28:53.130
an iPhone compared to what was available

704
00:28:49.200 --> 00:28:55.080
in 1958 there are little Sun sensors all

705
00:28:53.130 --> 00:28:57.240
around the body they're not supposed to

706
00:28:55.080 --> 00:28:59.220
see the Sun when one of them does she

707
00:28:57.240 --> 00:29:01.309
goes oh I'm not supposed to see that and

708
00:28:59.220 --> 00:29:04.559
starts firing thrusters to kind of write

709
00:29:01.309 --> 00:29:08.120
that anomaly so she's very fiercely

710
00:29:04.559 --> 00:29:18.480
independent of course I mean it's very

711
00:29:08.120 --> 00:29:23.159
it's it's it's it's okay dr. Eugene

712
00:29:18.480 --> 00:29:26.039
pocket I mean just amazing right I mean

713
00:29:23.159 --> 00:29:28.350
yes amazing and I actually got to take

714
00:29:26.039 --> 00:29:30.470
him up on the pad today and he stood in

715
00:29:28.350 --> 00:29:34.529
front of that enormous delta 4 heavy

716
00:29:30.470 --> 00:29:36.269
that is carrying his legacy up to the

717
00:29:34.529 --> 00:29:37.620
Sun and so it's very it was very

718
00:29:36.269 --> 00:29:40.260
emotional

719
00:29:37.620 --> 00:29:42.389
he is just the loveliest man I said in

720
00:29:40.260 --> 00:29:44.010
every interview I've done humble

721
00:29:42.389 --> 00:29:46.559
gracious and forever

722
00:29:44.010 --> 00:29:48.210
telling telling people that it's it's

723
00:29:46.559 --> 00:29:48.929
other people who deserve the praise not

724
00:29:48.210 --> 00:29:51.029
him

725
00:29:48.929 --> 00:29:54.000
and yet as Thomas sebou Cohen pointed

726
00:29:51.029 --> 00:29:55.950
out 35 NASA missions have flown that a

727
00:29:54.000 --> 00:29:58.289
you know really have gone after his

728
00:29:55.950 --> 00:29:59.730
science and that's a huge thing so

729
00:29:58.289 --> 00:30:02.669
having one that bears his name is

730
00:29:59.730 --> 00:30:04.679
awesome and this is the first time yes a

731
00:30:02.669 --> 00:30:06.480
historic thing first time NASA's ever

732
00:30:04.679 --> 00:30:07.500
named a mission after somebody during

733
00:30:06.480 --> 00:30:09.269
their lifetime and it was a lovely

734
00:30:07.500 --> 00:30:11.490
moment yesterday when when Thomas said

735
00:30:09.269 --> 00:30:13.049
you know and the person that it's named

736
00:30:11.490 --> 00:30:14.909
after is sitting in the room right over

737
00:30:13.049 --> 00:30:22.229
there there was a very cool moment

738
00:30:14.909 --> 00:30:25.049
Nikki foxpro I don't think as Jean

739
00:30:22.229 --> 00:30:27.210
Parker and so I'd love it but I don't

740
00:30:25.049 --> 00:30:29.909
think it's gonna happen well your

741
00:30:27.210 --> 00:30:31.619
superstar y'all a superstar and I think

742
00:30:29.909 --> 00:30:33.149
they're so I've been fiddling with my

743
00:30:31.619 --> 00:30:35.820
finger I keep saying the Eclipse guys

744
00:30:33.149 --> 00:30:38.460
you know and I got I got 3d so you know

745
00:30:35.820 --> 00:30:40.979
let's let's pass these out and we got we

746
00:30:38.460 --> 00:30:46.169
got a couple more here you know it's

747
00:30:40.979 --> 00:30:52.409
it's the Sun is setting and quite

748
00:30:46.169 --> 00:30:56.279
frankly that we have everyone so so

749
00:30:52.409 --> 00:30:58.590
here's one for it the Sun is setting for

750
00:30:56.279 --> 00:31:00.779
those if you're just joining us you

751
00:30:58.590 --> 00:31:03.210
missed a treat but you'll be able to see

752
00:31:00.779 --> 00:31:05.519
replace this is our sunset show and

753
00:31:03.210 --> 00:31:08.399
historic mission is going to take place

754
00:31:05.519 --> 00:31:11.359
this morning in the wee hours launch

755
00:31:08.399 --> 00:31:14.970
time is scheduled to start at 3:33 a.m.

756
00:31:11.359 --> 00:31:17.429
the Sun is setting on a spacecraft and

757
00:31:14.970 --> 00:31:20.789
in fact this will be the last sunset the

758
00:31:17.429 --> 00:31:24.409
Parker Solar Probe will oversee and in

759
00:31:20.789 --> 00:31:27.149
honor of XI

760
00:31:24.409 --> 00:31:29.429
we're gonna we're gonna put on our Clips

761
00:31:27.149 --> 00:31:32.369
glasses and we're going to do one thing

762
00:31:29.429 --> 00:31:36.650
and give a shout out on three two one

763
00:31:32.369 --> 00:31:39.829
with three two one go

764
00:31:36.650 --> 00:31:39.829
[Applause]

