Light-speed Asteroids, Chicxulub Dinosaur Impact, Terraforming, and Hyper-giants | ASMR Whisper

all right so again this is in real time so the the flood has now wiped out the entire southeastern United States that would be terrifying but yeah there's lots of other things to be terrified about so let's find out what they are let's see let's zoom out to fly all right flying into Uranus in 3 2 1 cue someone walking in your room what did you guys just click on I'm sorry all right that was just a that was just a little Icebreaker to get us started here so for anybody who doesn't know the Universe Sandbox is an incredibly interesting game because you can well a because there's no plot to it but B you can C gives you a very realistic idea of the physics of the cosmos and not just the physics but the um you could see the gravity of the planets pulling the Sun a little bit which is exaggerated in this game of course you can slow time down you can manipulate things you can see the true distances between the planets as we zoom out here you see just how tight the orbits of the inner planets are relative to the outer planets you can see the incline I can get it right you can see the incline the true incline of Pluto that's this orange line here and just how exaggerated it is off the solar plane relative to the other planets is why Pluto is uh and all the dwarf planets are no longer in that category you can see the distances between the planets the size of the planets um so there's lots of things to do you can uh simulate impacts you and well as I was trying to just fool around to come up with some ideas for this video I realized a good starting place might be a tutorial so that's what we're going to do today we are going to take a couple tutorials and get used to get familiar with um it'll be a good rer pressure for me and a way for you guys to get familiar with the game itself if you aren't already but before we do throw five moons into Earth's orbit I want to take a moment to shout out the sponsor the um brand I partnered with today for this video into the am legitimately the most comfortable shirts I think I've ever worn so um I got this graphic te I thought this one was pretty sweet with the astronaut there actually some really cool designs on their website um my go-to is kind of basic plane and definitely with the pockets cuz I always have a pen yeah and it's just the most comfortable shirt you guys are ever going to wear these t-shirts are awesome so yeah I'll have links in the description I'll have it pinned it'll be the first comment you see down there so if you guys are in the Market please yeah look at this I really like this one in the back so into the am M code's going to be let's find out and you'll get a discount when you go there check them out please up here and then we can terraform some planets um replace our son with a black hole see what the dinosaur Chul impact would really uh fairly realistically look like so I thought this tutorial was pretty fun too so let's walk through it together and uh we'll see exactly what this game's all about and hopefully learn some things and we'll blow some things up along the way so this is Earth in Carl San's voice home to everything you know every sinner every saint who has ever lived has lived on this Earth carry down his or her life on this beautiful pale blue dot in the cosmos so naturally let's launch uh the largest object series the largest object in the asteroid build at it and see what happens all right let me zoom in a little more okay uh oh I launched to so what would you like to happen let's explore what would happen but there's other ways we can destroy Earth too I guess I zoomed out too far for that one let's uh we didn't get quite to the impact there so I love the the actual impact physics we'll check it out in a second here and it shows you what would happen shows you how the the propagation of energy and kinetic energy uh would wrap itself around the earth it's really cool so let's check it out let's put a moon really really close look at that it's already shredding apart from the title Forks effects title effects forces let's put a couple you could see just how devastating it would be and now mind you I guess I gotta mention the time steps of this game so every second in real in real time is an hour in the game so this would be taking course over days right now there would be a few hours there where some sections of the planet would still be safe and just see these these uh you know 2,000 mile wide molten balls of metal and silica whatever the moon's made of just orbiting in its sky that would be terrifying but yeah there's lots of other things to be terrified about so let's find out what they are so we can pause the game Let's choose a different object ahead let's choose tight now let's give the Earth five Titans let's put one here one out here zoom out a little bit let's press play so we are wreaking Celestial havoc in the universe right now so it's going to reset the game and now we have a 100 moons colliding with Earth all right you know what I'm going to go off script here because that's never fun to stay on script too much is it let's uh can zoom in and out this is cool yeah the reason I wanted to do to do these was because uh it explains to you some of the you know more the Lesser known features of the game I guess you can make double all their characteristics the radius uh the mass the velocity the temperature you can add different elements to the planets to terraform them something we're going to do you can change the age of the Earth I just that was the first time I ever noticed that one that's funny okay so let's make it two times larger now all the moons are being pulled into it you can see instantly the Earth is now obviously obviously it's heating up it's gaining mass it's pulling everything in it can also the tutorial says teach us about Earth's climate the importance of our sun and lasers I wonder what that means let's check it out let's explore the importance of what that's PR of our sun so the sun is the most important it's the primary source of light energy which Downstream of that in the chain the cycle of life and other processes on Earth is the um it's the the fundamentally the only source of energy other than the geothermal energy from our molden core so naturally what if we got rid of it let's just poop it out of existence tools D hit the sun there we go now look what happens it's interesting that mercury is the closest in orbits the fastest so it's ejected the fastest they all maintain their exact velocity just in a straight Direction now with no no more angular velocity it's immediately translated I don't know the actual physics of it but it is now linear and you see Neptune Uranus is they barely change much they're not moving a whole lot because their angular velocities are so much slower than the interior inner planets without the Sun our entire solar system is unstable unbalanced and lacks any input of energy look what would happen to our Earth we got to snowball Earth right now so we can check out Earth's properties here let's check it out a full list of editable properties which I've been looking into I want to do a video um on the true expanse of time from blank time all the way to the the uh the age of the universe and future projections of the age of the universe of how far into the future physics um we can project currently known physics to see how the universe is going to evolve part of that was understanding what we know about the Earth and how it's evolved and it's interesting how many how many large temperature fluctuations the Earth has been through and that uh it's been a snowball like this they think almost everything two massive glaciers aice C the north and south southern poles leaving essentially just the equator without ice for millions of years in the past and uh it's just fascinating how how remarkable it is how how special um unique of a time we're living in right now and the fact that we're technically also in in in Ice Age so uh yeah just food for that so we can see how the temperature is changing across earth Earth's surface here you can look at data views and check out the surface temperature the elevation gas pressure depth ice thickness all right see the surface temperature is pretty low so it's going to prompt us to bust out a laser see if we can warm up Africa here and remember this is one hour every second so if we slowed it down to real time you would see this propagating on a much more comprehensible scale I guess which I think is pretty cool so we'll check that out in a little bit okay but look at that you can see exactly on the surface temperature map over here where I'm firing the laser but the Earth is still cooling because it has no external heat Source from its from its mother stor so let's add another what is there we going to add another St let's add we're g to add another star let's check it out rigel the blue super giant rajel now I've let these planets drift pretty far away let's see what happens yeah you can see Earth is all the way out here and let's see how far Mercury went it's pretty far away let's see what happens if I get roughly right in the middle rajel is 23 times more massive than our sun so it's going to have that much more gravity what is let's see gravitational force okay okay gravitational force formula okay it changes inversely as the distance squared okay all right but it is directly proportional to the Mass of the Sun so okay so it will be 23 times look at that so it's already starting to make the planets to a U-turn it's gravitational force should be enough to bring back and heat up the earth now look how much further the Earth is than it was and now we're instead of an hour per second run days per second let's zoom into Earth here let's see if it heats up oh yeah looks like its atmosphere is completely gashes now so the planets are being sucked in the Earth is much too hot maybe we so maybe we made some mistakes ruined our solar system by deleting the Sun but that's okay there's always something to learn from an experiment even one that ends in disaster so and it reminds you you can not only terraform existing planets but you can create your own planet from scratch a life sustaining world and watch it evolve so here is going to walk us through terraforming Mars let's check it out let's see what happens so we're going to add water using the planet scaping tool Planet Escape liquid water oh chemical water um okay let's add it to the let's add it to Olympus Mons see if it gets gravity right okay yeah it does I guess the waterers the water is uh pooling around the base of it but it's also looks like it's evaporating the time scale here is 1 hour per second so all right now we can increase the amount of water per click that we're adding to the planet so let check that out let's check that out quad the radius of the Dual by selecting two times multiplier okay let's see select that twice aim at the planet press the whole all right so okay here we go lot more water now that's add it everywhere we definitely get a a feel for where the con contents would be which is another aspect of this game that's really cool you can it has real data about the elevation of the planets so when you do mess around with the atmospheres the climate the the geology of it you get a feel for just how they would look you know cuz we have liquid water on Earth to give us a baseline elevation measurement even though it's a little higher at the equator I believe okay now let's sorry my chair's clicking a lot I promise it's the chair all right let's see what what we got here we're gonna increase and watch it evolve and watch the water evolve over years one year per second did anything happen it wasn't enough water to cover to wrap around the entire planet so it was just uh stayed on one side of the planet and the water we added started to freeze because Mars of where it is and the relative to the sun we can try to give Mars a shorter days it says so one side doesn't get too hot or cold so we're going to make it spin faster tools of force so here we go oh and you can change the Tilt too oh okay all right we're making it go way too fast now it's got too much we accelerated it it's just ripping it apart all right so that was a a waste of time this is a pretty cool aspect where it tells you the habitable zones this is obviously colorcoded where red is hot blue is gold green is just right 4 L years away trapist one is actually a real star that jwsd has looked at and I think it's a brown dwarf or it's a really dim small much smaller than the Sun so all these planets the Cil lockone the the orbital distance from the Sun that uh or from trapist the star that would be heal the corrected the right amount of just the right amount of energy to allow life to form and water not to evaporate or freeze uh is much closer to it than than our our son's goldilock so so we're going to select it open its properties double the mass so now we disrupted all the planets it's a chaos all right so now we have galaxies can even fly beond the edge of the Milky Way to watch what happens when the Galaxies Collide and we have two black holes that simulate the center super massive black holes of our galaxies and they just merge but you can see the time step here now dramatically increased to 1 million years per second so let's see all right so it says here we go it's showing us how many different simulations it it has pre-programmed that we can open up cool let's see what we got here Saturn with rings yeah this one's pretty cool when you can watch the simulation how well this one's just more beautiful I guess how a moon or a large body thrown into Saturn's rings would destabilize them and warp them that's pretty neat let me see if I can do it just right here we go planets oh we're gonna add Neptune that's pretty massive yeah we're gonna add Neptune okay let's check it out to find out what Neptune does it is hard to tell all right here we go guys let's see what Neptune does here that's hard to tell how far okay there we go so I did get it close enough now watch three dimensionally what happens here so Neptune is throwing the Rings out and pulling it in pulling it up and down as it uh as its orbit you know crosses the plane of the the uh rings and now it's throwing you out like that's pretty cool sucking a lot of the particles into itself it's just completely disrupting the ring system a lot like you see galaxies in well in the pictures but also the simulations to try to understand the physics of uh what goes on when galaxies merge they they fling entire tals of billions of stars out which is that that fact is that's hard to comprehend you know thinking about one star is hard enough the size the energy the the the force the distance is between stars and then you think about billions of those Stars being flung out into inner Galactic space when galaxies start merging I had something to think about okay so one last note assist the tutorial while we watch the results of our experiment go home click the back arrow click the back arrow the guys see what else if you ever want to learn more about using Universe Sandbox just select a topic from here and then it sends us off with a nice farewell so I want to plan Escape let's check it out actually you know what let's let's do some let's just do some fun stuff we'll plan Escape in a minute all right so we got the Earth Moon system and for me let's take the trails off so don't have that disrupting us although it's useful to pinpoint where the moon's at I just wanted to look at just how far just how far away the moon really is maybe we'll try to superimpose it on the Galaxy back there all right so just look at this I will let it we'll put the moon on the other side just look at how far away the moon really is the moon was actually out this morning she a little bit after sunrise and when you look up you know you don't you don't realize the moon isn't just floating you know about this far away it's to really think about where that moon is it just seems so large in the sky it gives you an idea of how massive how large how large the diameter of the Moon really is if it seems so large in the sky yet is this far away let's see let's look above it okay we're zooming all the way into Earth and now I'm going to slow zoom out and watch how long it takes before the moon comes into frame right there it's like you would normally think I used I guess I won't speak for you but I really used to think the moon was maybe here CU When you're speaking on the scale of planets you know a couple Earth diameter seems pretty uh pretty far away you know 50 100,000 miles but it's like 30 30 Earth diameters I think it's still not in frame there we go that is how far the Apollo Astronauts had to travel it's incredible all right so let's throw an asteroid into the Earth here's what I want to do I want to first I want to look up the dinosaur asteroid oh look at that look at that would you look at that guys you type in chulu been an asteroid flies across the screen that really happened it sure did that's funny cute okay so Chul Loop was 120 mil in diameter it's an impact crater buried underneath the Yucatan Peninsula in Mexico its Center is offshore but the crater is named after the onshore community of chulu weblo 66 million years ago 10 kilm wait oh oh the craters 120 miles so 10 km which would be about 6 miles wide the uh was it yeah 1 km is6 miles I think so all right let's check it out now if we had let's see minor bodies it's surprising they wouldn't have a Cho Loop wonder if I searched for it could I find it there open no okay that's weird you would think they would have that all right I'm going to have to write them a letter then guys won't I now I love this game this is plenty cool because you can just create your own if you really want so that's what we're going to do let's check it out we got all right so let's check out our random asteroid I think we're going to have to custom make ch R Rock particle asteroid I think asteroids probably our best bet all right so we're gonna launch it we're going here come over here launch it launch it in and there we go so it's stationary now so let's X out of this configuration oh where' it go there it goes all right wait what's going on oh hope we got launched so we got days per second let's scale that way back oh okay let's redo that let's redo that all right so okay maybe I launched it wa too quick let's reset that okay all right so we're gonna We increase the time step to something like 10 minutes per second let's go ahead and add our asteroid random asteroid we're g to launch it launch velocity let's see how fast Kul Kul Loop Kul Loop hit hit the Earth stru diameter age coverage let's hit the dark reader mode for you guys so I can show you this without blinding you okay so 12 miles depth six miles across wow the crater was 12 miles deep that's a 12 miles deep there's a really cool video that I'd like to just maybe maybe like comment on or something like that one time in sometime soon that is a someone made maybe a lot of you guys have seen it but someone made um of the impact of real time impact it's a six hour video going over a couple minutes leading up to it and then the six hours around it after the impact and just how you can see the the wall that's a cool video wow there's a lot of really cool videos the sunam me in real time is this is this it maybe it is um in real time I got the sound turned way up this this is amazing um the air pressure gives you a breakdown of the air pressure the um you know the heat the shock wave the the different types of shock waves of uh the the ejector how high into the sky they would have gone How deep the impact the Air Blast velocity here so in the center we got mach five Hypersonic um you can see how deep it went the eject of the tsunami effects of course just taking out all of where I am all of uh the land surrounding the gulf let's see okay so Air Blast pressure Air flast Blast velocity so just a couple minutes after impact you have what less than 10 less than 10 minutes nine minutes after impact you have a category five hurricane radiating all it's already gone across the entire United States I mean this video is just awesome I this isn't the one I I saw I think but um yeah it's incredible what really happened so anyways um yeah I'd like to do a breakdown of this itself it is incredible you have you know regions that are just set on fire thousands of miles away so yeah Mount Everest look at the the bottom of the crater rebounds at 500 meters per second 500 m/ second the I mean it's got to be molten at that point the rock is just moving it impacted and then rebounding up look at that God and there you go wow that's real time look at that what is what is that though seismic wave FP wave is a prismic noise so God so you're already getting a pressure W okay anyways that's fascinating let's create our own impact now let's find what how fast it was going almost lost track of what I was what I was doing um discover is it here this is definitely a question you can look up was it an asteroid the only second largest impact structure on Earth and the only one whose Peak ring is intact directly accessible for the scientific for scientific research really Peak ring is that right so the Bak ring is on the tip of the Yucatan Peninsula right on it looks like it's right on the shore it's literally right on the shore of you that ghost Chu no way and the time scale of that too was at a relatively steep angle between 45 and 60° 20 kilomet per second okay what was the speed of the CH this is just turning into a chuu episod and if it's pronounced a different way let me know in the comments just going I've never heard it pronounced 1 m/ second 10 m High it would have hit Europe and Africa with a 10 meter high wave 100 foot wave or no that's a 30 foot wave that's still a massive wall of water traveling what three four 5,000 miles that's incredible okay so oh we got to pause that all right two km per second okay we got to delete that delete that let's see random asteroid K second okay let's add our own launch velocity let's 10x that 2x so here we go all right launch it oh we got to launch it at a steep angle that's right okay so clearly we gota start with a empty simulation we'll add an earth then we'll enter Chul Loop and then we'll launch that sucker and watch it go so add Planet there's our Earth okay all right we got the Yucatan ready to go is there a sun no just just got the lighting like there is okay so now what we got to do is add our asteroid let's check it out let's make it happen random asteroid okay launch um laun right at it I hope that uh that's an accurate launch okay so let's select it change the speed change the diameter where are we okay speed all right change the diameter 5 km 10 km okay I'll knock it down get precise with it okay see they're going to be comically I'm either going to have screwed up or not I don't know let's find out if I screwed this up maybe and look how small it looks when you back out okay well there it is 3 hours per second that's our time stamp so let's Okay that's really fast let's do a couple minutes per second that's still really fast wow this thing is moving with some speed okay well I guess it's way further away than I I thought so it's we'll speed it up look at that thing just imagine thank God we we're experimenting with Technologies to uh deflect asteroids man look at it that's pretty pretty precise shot isn't it all right that suckers know what we got to do I just remembered oh look at this thing the gravity Earth's gravity is sucking it in too all right we have to um rename this we got to give it a proper name don't we all right okay it is going to be named here we go why it still going the same speed I guess it looked like it sped up so maybe that makes sense if it's falling into Earth all right actually that'd be curious that'd be cool to see if it heats up would it let's find out if it does that let's find out how much maybe maybe it's it loses Mass maybe we can see the atmospheric effects of it all right that's six seconds per second slow this way down look at this sucker going that was a direct hit I'm pleasingly surprised I did not I think it would be that direct of a hit okay look at that suck okay so it's going it's temperature is still way up so so we're going at half speed right now4 seconds per real real time second it temperature is -273 C it's radius it's Mass isn't changing just real time let's see what it would look like in real time okay let's get the best view here I think a a wide angle view might be best oh okay the game literally wouldn't let me pause it that's funny wow okay let's check out what happens with Earth let's see what happens with Earth here so now we let's do real time here let's slow it down Okay so we're roughly in real time and we could see the shock wave traveling out at an incredible speed that is ridiculous how fast it's going so it's already going out it's already traveled 500 miles in the first couple seconds here um is Earth's temperature going to increase I mean that's its average temperature but let's see the view of all these different properties here you can see the gas pressure liquid depth um surface temperature we have one ridiculously hot spot at the impact site it looks like it beat it might have already beat at something like 1300° C all right so let's speed it up a little bit we G see what other effects so look at the tsunami effects it's already having it's going up Mexico Central America's wiped out the gulf the Southern United States hasn't hit Florida yet given a couple seconds Florida's going to get taken out too I'm hanging on hanging in there guys we see the gas pressure the bubble is expanding oh there it goes yeah the whole Southeast Eastern United States okay that's 3 XP that's actually incredibly fast this is something else to witness this is on pars is on 1 second per second and it's literally just 1 second per second that's frightening how fast the shock wave is traveling up the entire region around the gulf the entire Southeastern or Southern United States is underwater now and now we have I mean what is this debris oh yeah I haven't even got the 3D view yet look at that look at the three-dimensional view of the ejecta all the crust Earth's crust that would have ejected into space and all from from that little you know something six six miles wide that's not even a third as wide as Lake okobi here with the energy it had let's see if I can zoom in get a better see how do I do this now there we go go look at that oh there we go sorry I'm getting used to navigating with the keyboard here you can tilt it B left right in and out and then I can use the mouse to look up actually kind of want to see here I love I love the time manipulation aspect let's reverse it real quick all right I just want to see what it looks like after impact wow that for all right let's go to one second per second here let's check it out let's see just how terrible this impact crator was this asteroid impact was it's fascinating that on this scale right here it's so it's so uh it seems like it's moving so slowly and then once we get really close you're going to see just how fast it is and just how devastating a little six mile wide grater can be on a 10,000 mile wide earth planet so we'll speed it up to get a little closer but um to watch the effects yeah we do we do like 3x or 2x some nice even numb so I can quickly get back to where we're trying to go at cosmically it's like you can barely if I take the trail off you wouldn't even be able to see it from this scale if the game didn't make a point to enlarge objects for for the sake of you know visualizing it because it is a visual medium here this is so incredible yeah maybe that's a good angle I have right there all right we are approaching it in real time now it's not exactly where I wanted it to hit but it's pretty darn close so we're going to see just how devastating this was just imagine just imagine imagine looking up and seeing this thing coming being on the North and the Americas oh we just lost it we lost our POV because we lost the asteroid all we're going to zoom in here you can just see how devastating it is instantly within seconds the shock wave has already traveled hundreds of miles let's zoom out here here we go the effects of the impact on planets they for some reason keep propagating even when you mess with the time so trying my best to to give us a good view here all right trying to give us a good threedimensional view of just how high these fragments these what are called ejecta fragments are being launched into the air look at these and I imagine that this is similar to what it would be like if God forbid an asteroid ever hit earth again and we're not able to deflect it um just look how high this is going it's going hundreds if not thousands of miles in the air beyond the air out of the atmosphere and the site is it's propagating it's already swallowed up all of South Central America you could see and the wave has already covered Mexico Texas Louisiana Florida and it's Rippling oh there we go it's better it's Rippling it's fried I assume the you know the heat wave the the gas pressure bubble supersonic way faster than sound gas pressure shock wave in the ground I guess the one in the ground would be f than the one the atmospheric shock wave but yeah look how devastating Florida's already already about 70 now approaching 80% just wiped out um Louisiana's flooded Central America has been wiped out I'm assuming that's yeah the atmospheric shock wve right there then the water is coming right kind of in front of it obviously this isn't super you know exact exact and realistic but it's pretty darn realistic all right let's I just want to yeah try to get threedimensional views of how high these these fragments are shooting in the air because that's you got to remember a huge part of the devastation is the fragments that rain back down on Earth I'm still I don't game I'm definitely never gamed with the PC so I'm still trying to figure out how to manipulate the uh the keyboard and the mouse controls at the same time all right so again this is in real time the devastation is so the the flood has now wiped out the entire southeastern United States um it's working its way up into Mexico which I understand a lot of central Mexico was actually pretty high elevation so the right here the uh the Rockies and that are going to take a while to to actually be uh flooded out let's look at Earth and I don't know what's going on here now but um let's open the properties of Earth and check out the the Heat map see what's going on with that composition let's check out the layers oh we see Earth is already heating up the minimum temperature is rapidly increasing the maximum temperature is decreasing ing from I think about 1300° at the impact site overview um the average temperature is 12.9 that's going to be increasing the impact site is obviously you see the gas pressure expanding look at that I'm not sure what that is if that's fragments coming back down or what what's going on with that oh there we go I'm finally learning how to use this all right and look at these these are well earth's earth's radius is about diameter is about with 8,000 um so Earth's diameter is about 8,000 miles so it's radius half of it is 4,000 miles there and uh so that's about 2,000 miles I'd say it's a qu of the diameter enter the ejecta launched into the atmosphere Beyond well beyond the atmosphere I guess in reality so let's check out the rest just think about that that's a that's so incredibly High into the air that's so powerful that's there's there's chunks hundreds of feet across I'm sure we using Freedom Units by the way guess I'll stick with Miles and feet and um being ejected you have stadiums of material being ejected thousands of miles into the into space and then Earth's gravity will pull it back [Music] down across the entire planet so let's see let's see how the planet's doing here okay so half of Mexico about half of the United States is taking out it's underwater right now and the average temperature of the entire planet has raised a degree just minutes after the impact now let's increase it it's 2x the speed here now will 4X it just to get a real understanding of it and you can watch this watch this temperature here you're going to see you're going to see this temperature increase and that is so incredible all right so look at the the fragments going to far here there fragments ejected are now you know 4,000 they're doubling their distance and it looks like the simulation's simulating the uh fragments falling back down onto the impact site and around it I set this up so the impact happen to brighten early in the morning so oh what did I just do here I don't know what that does c I just hit the letter c I don't know what kind of shortcut that was but the r right into the The Fray yeah look at that you can see everything oh that's awesome you can see the whole planet now okay let me zoom out how do I zoom out of this there we go okay now I'm zooming out to the whole planet on these Maps here we can see what is that one cold spot what is that random cold spot oh there we go that's kind of cool 2D profile composition composition oh I real I could do all that that's pretty neat see if the elevation got changed is it all right so it's wiped down I haven't even been paying attention to what what's actually going on so is that is that Alaska I didn't randomly get out move over to the Pacific did I yeah there's Newland Eastern Canada there wow um let's just look at the map okay the entire North American continent is underwater right now it doesn't look like the elevation changed so I'm assuming you know that doesn't mean that I'm assuming that means that you know the land Beyond you know whatever like 100 mile radius of the impact isn't actually affected it's just the atmosphere and the water the water washing over everything is um is what's causing the uh the ocean to increase that is incredible and again remember one thing that this isn't showing is the look how much it's I don't new feeling sits pretty high up too look at the water just it's still coming up all this is going to be burnt there's going to be a massive wall of of hot ionized gas essentially almost plasma I guess that is concentrically propagating out like the world's you know the largest ever nuclear explosion and it's just devastating Burns increases the temperature 13.7 it burns the entire planet and within hours that's uh all right we're doing 25x now so now we can see the Earth rotating in real time or not you know we can see look at that we can see the fragments Landing the ejective fragments landing on the other side of the Earth China Australia Indonesia that is nuts imagine that imagine being in Australia or uh you know somewhere else it's just the middle of the night and you just see you don't have any sense of an impact you have no tsunami maybe the the atmosphere is lighting up with auroras or something but uh you have no other warning sign and you just started getting Sky just starts lighting them up with football field size chunks raining down let's let's fast forward to see if anything else happens oh man surface temperature oh no okay I just want to see the impact site let's see okay now look at that we're already hitting Africa it's getting swallowed up now all the entirety of North and South America is just gone byebye that is incredible to think about that let's 10x that let's have that just 5 exit so if we watch our map up here that uh that one little asid I did all that and paved the way and killed out such a huge chunk let's lock on to Earth huge chunk of the uh what do you call it the um the biosphere surface lock there we go all right I wonder how long it would take we jumped it up to you know days per second I guess it's still water is still eating away at the planet I just wonder how long it would take to for the continents north for the Americas to come back you see the climate shifting it's 14 basically two weeks per second now two weeks per second okay let's just go crazy how many years does it take look at that we have years where it's just the green is just died out oh it became a snowball what what happened there okay I guess maybe that's just because we don't have a sun that's funny okay fair enough maybe we should add one let's it I think I already have there we go U scy is the largest known star and we are going to put it we're going to put it 100 120 Au that's the edge it's the boundary where our Sol wind stops it's the boundary of our solar systems basically our solar bubble so to speak let's put it there and see what happens to Earth days per second let's go back down to minutes per second all right it's been 200 years since we started the simulation I love that here we go all right let's see what happens we're at basically a half hour every second let's see what happens to Earth as it orbits this massive star now that sun right there this new Sun you scy oh okay it just jumped us right there didn't it is was only nine times the mass of the sun it's only nine times but its radius is eight times the if we can do that in Souls it's eight times the distance 70 720 million miles miles wide that that's baffling that poggles the Mind 700 million miles across into that's 2.4 2 million yeah two million times wider than the sun two million times wider than the sun I have a weird deck where I have to type the word sometimes I have I'm I'm compelled diam versus so the sun is um I'm I'm confused that would mean you Good's like a billion miles across or more so the sun is 860,000 Miles that's you know over 3/4 of a million miles across in diameter I'm not the first one to look look this up obviously the U SC has a diameter of 2.38 billion kilomet I don't mind it not being in Freedom Units because it's you such a large number now but that would be uh roughly four four billion miles across 1700 times the size of the sun what 1700 times the size of the sun I guess my MTH was way off I thought yeah it was e to the six oh I let the simulation run over here oh no it's not okay cool we should see its temperature start to increase now but yeah anyways I guess my the point of all that was who that um let's get off Surface lock here to just try to put in perspective how massive this object is U SC it's 120 times in this simulation further than the Sun so from this perspective we would be inside UI scutty right now if it were where the sun is if it were the same distance if it's Center point I guess it would be was at the same distance as the from Earth as the sun's Center and um but instead it's 120 times further from Earth than the sun is and it still looks I don't know what like 10 times larger which makes sense that's about multiply those that's about 1,700 times it's on the the same magnitude as it's how much larger it is it's 1700 fold increase from the Sun okay so it's average temperature Let's uh there we go we can see it start to increase now so we're changing it from let's do days per second so one day every second and we see that in that temperature increase now look at that nice nice warm glow that that light that star gives off that's amazing let's go back down well maybe not so we have our poor impacted Earth Africa is just an ocean now so is Western Europe where's North America I don't even know North and South America still just they're just buried under ice nice nice ocean okay let's see if we surface lock this although we miss out on that beautiful UI scutty glow but we can see there let's just increase it let's go crazy little strob of here okay there we go and now we see how rapidly so it's I got to change that Target Sim speed Auto there we go I wish the units would oh there we go okay thank you literally was just asking for the same the exact feature that was available that was nice thanks Universe hbox developers okay so we're at like 20x speed or something like that no we're we're at like 500x speed 5 minutes 8 minutes per second 60 seconds time 8 480 yeah something like that we can see the Earth is it's still warming up but I love the geologic time scales on this too how accurate it is because it would have to be you know we have an accurate distance we have accurate times accurate energies um or sorry accurate distance and size accurate energies accurate um lots of accuracies I guess the point I'm getting that but we also have accurate geologic time here it shows how long it would actually take for atmospheric changes to happen if you were to replace our sun and put it or replace our solar system with one U SC was at the center of yeah that's actually that just reminded me to check out the goldilock Zone if you watch scy let's give it a shot so let's Go ZO way way way way way out there we are VI I forget how you do that habitable zone maybe I think that's how you do it oh look at that that is so incredible that gives you an idea of the habitable zone so Earth is going to get burnt inevitably it is well within the uh within the danger zone see right there that's an example of just how how much larger they they they exaggerate the size of Earth from larger distances so that you're able to um you know still make it out you're not just Flying Blind but in reality Earth would still be even this far away would be a pin pinpoint you wouldn't be able to see it but let's see how it's doing how it's starting to heat up but to give you guys a perspective again it's all about relativity otherwise this just you know it's meaningless if we add a sun you can see it's h Zone too so in just like it's actually probably going to be a really great perspective um what did I just what is going on did I just add a bunch of planets did I just add a solar system okay just added a solar system on accident that's funny all right but yeah okay that's that's a great name still a good uh demonstration here let's highlight the sun okay look at the Sun's habitable zone which um is would Jupiter get blown up or that's okay it's just inaccurate all its moods there that's awesome those really all Jupiter's moons no way I know it has like 60 moons but that's is that 60 that's insane that is so that just seems like a lot it's got its four main Galilean moons the ones that Galileo saw 500 years ago I anim jopa and kalista anyways I should have named this channel I digress okay so here's the Sun and we zoom in oh I'm sorry and we zoom in and we check out we check out its habitable zone which Earth and Mars Earth is just in the habitable zone Venus looks like it's just out of it and Mercury is well out of it and Mars is actually looks like it's perfectly in it I'm G to go down here and add a GD again to help us get perspective here so Au is the distance 90 million miles about between the Earth and the Sun and on distances on the level of the solar system smaller than Interstellar and Intergalactic distances Au is one of the biggest uh one of the primary units you count in so for the distance from the Sun to the Earth is One AU and then Mars is about 2 Au sun to Jupiter is about seven or eight Au I think something like that so when you zoom out there we have Mercury Venus Earth Mars you keep going we have Jupiter Saturn about 7 to 10 Au if we keep going out if it lets us then we have Uranus and Neptune at roughly 20 to 30 Au and just there's Pluto Neptune right there so that's Pluto marks the beginning of the Kyper belt the edge of the solar system is about as many edges but the end of the solar bubble essentially the boundary at which the interstellar forces start to overcome the winds that stabilize the interior environment of our solar system and at about three times the distance of the sun to Neptune and Pluto they're about the same distance from the Sun and so that's 3 * 30 Au about 90 to 120 3 to four times the distance and then here it's only at about the entire diameter or the diameter of the entire solar system that we can see uy scy becomes um that we start being able to make out the habitable zone of UI scutty it's funny that our entire solar system seems to be orbiting just fine maybe I need to increase the time steps here maybe that's my issue um seems to be doing just fine though orbiting this star so yeah the the entire solar bubble that we opened our last episode about the birth of the solar system with explaining can fit won't even begin to break the the minimal boundary for the habitable zone of uy scy so that's that's incredible and we can see zooming out you can hardly even make out as we zoom out and start seeing the red green habitable zones you can hardly make out our entire solar system and looks like 668 Au is roughly probably between five and 900 Au here 800 Au is uh what's habitable it's where we would have to put Earth to not fry around you why scy okay so we return to the solar system now the regular no no U wife scy involved I wanted to mess around with some more impacts because it's fun to blow stuff up it's I think it's really fun to imagine what would be like to see an asteroid fall from from the sky all right it's in orbit now okay that's an orbit I don't want that now La one right here 3 km per second let's see I think the average Earth is going 30 kilm per second 17 to 20 so 30 50 17 to 25 kilm per second let's see average as asteroids the most common type of impactor slam into the Earth that an average velocity of at an average velocity of 18 kilm per second short period common impacts with the Earth are less common but have higher impact velocities 30 kilm per second look at this there lter impact long period comets are up are up in the 50 to 70 kilometer per second range that would devastate Earth even at what like a few hundred feet across so obviously it's it's a high priority for us to figure out exactly how to get to asteroids spot them before getting to them asteroids and and comets in particular but uh I guess asteroids are much more in our blind spots than comets are because they uh maybe because they they offcast more so they're more phys regardless the asteroids are the what populate most of the inner solar system so way way more likely to get hit by an asteroid I'd imagine um okay so let's play this out here we got two asteroids coming to hit Earth all right so we got this one oh this one's ping a sneak attack it's going to hit Earth at night how I don't know how how large these guys oh that one's already about to hit large this guy 103 kilm what it's masses kog 103 this is just a rock particle are we not calling this an asteroid why not okay so Earth is about to get destroyed by this quote unquote Rock particle which is going to be nuts look at this thing in real time it's it's about to destroy Earth imagine looking up and seeing this thing just go into the Sha Shadows like that oh my God imagine being you know oh look at that 100 miles from it and just seeing it disappear get closer and closer until it looks like it's obvious it's going to hit Earth and then it just disappears Over the Horizon all right let's see what the other one's doing has it hit yet no it is not this one's way behind let's see what this one does I already cleared out the atmosphere 15 minutes per second and the impact site is just witnessing dawn it's a new day over there where's the other one so it hit what uh where it is just the middle of the Pacific I guess did the other one already hit I'm confused where the other one all right let's let's restart I'm going to send a massive uh we're going to go five miles across let's go ahead and zoom right into Earth all right all right random asteroid you are up let's impact in the middle of the ocean we're going to make it let's see was six miles across let's make it 100 miles across or 50 let's not go too crazy they don't have miles okay okay okay that's about 50 miles across that's nuts that's we're going to go to 20 kilm per second 50 miles across I want to do this nice and slow so that we see all right let's bring it down twoes per second all it's at half speed right now this sucker is headed for the middle of the Atlantic let's go to one second real time and just again that's terrifying this is a there's no angle of incident so it's a direct maybe a 90° angle Bleak was the word orthogonal slightly off maybe 15° off let's see all right so here we go here's the impact in real time 20,000 miles hour in real time and there it goes couching out the Earth this is a 116 kilometer wide asteroid impacting the Earth in the middle of the Atlantic in real time and its shock wave this already 500 Miles easily in diameter okay let's see how it impacts how quick just like you know from from out here it doesn't look that quick definitely from out here but when you zoom in and recognize realize how large of an area that really is how devastating that would be all right so all right I just want to see how it's going to affect Europe and Africa here all right so we're going to do exit and then you see just in real time again isn't like you know um TV or you know any really good quality I guess for 2024 but the graphics still get the the point across I think okay you just see this massive so I guess that's the rebound right there it's going to displace just hundreds of thousands of square well thousands of square miles or at least hundreds of square miles I guess displacement it's forming a greater ring and obviously the shock wave it's just devastating everything um the entire Western Northern Hemisphere right now all right so if we so if we speed it up we can see all the ejected fragments now raining back down on Earth there's one destroying the Africa West Africa one nearly missed Madagascar there there's a couple raining down right there that looks like it's a to right for New Zealand if we speed this up we can see just what that uh no doesn't look like it's expanding it's going to say what that shock waves doing but look at it Glow just the black body radiation of it it's just glowing as it goes into night oh that's incredible all right let's go to the uh surface lock oh I can just do it from up there all right cool okay well it didn't it's not propagating like I expected it to so we're going to have to we're going to have to reset this and do something bigger I want to see true destruction and watch how the planet interacts all right so abandoned all um attempts to try to impact the Earth with small objects but then I thought all right why don't I explore not just increasing the size but increasing the velocity so we increased it from for the Chulo is it Chulo I feel like that's the wrong pronunciation but um Chul Loop crater we increased it to six miles wide increased the speed from like two to 20 kilometers per second but now I forgot that you can increase you can play around with light speed in this game so that's what I want to do I want to take an idea that I got from great still plays he he's a really funny YouTuber who messes around occasionally on Universe Sandbox let's try to Let's decrease the time make a tiny tiny object but mess around with the overall energy the kinetic energy it delivers upon impact by increasing its speed so we're at two minutes per second here I can launch this slow it down let's see the perspective is hard to get sometimes because there it is okay cool you forget how uh all right let's make this little guy a really little guy a tiny guy all right let's go let's Zoom right on half a kilometer let's go 75 m 3 m just a real tiny guy all right so that's 10 feet across but even that's still pretty big it's the size of a car let's make it three CM all right some of you out there would say that's still pretty big no that's a that's what we're going with all right so three almost four CM um those are 2 and a half cm per inch so it's like two Ines across obviously it's not going to do anything but now if we change the where did the earth go What's Happening Here we're in darkness now if we change the speed then we're gonna start finding some interesting ideas okay so we're at 6% speed of light let's find out what happens when we hit play in real time so light goes around the earth I think seven times per second that's you know roughly what is it 300,000 meters per second or kilometers per second I always get that one mixed up a lot of you guys know that let's find out 6% speed of light a three a two inch wide meteor now in reality I'm curious whether or not it would get disintegrated in the atmosphere if it was traveling and punctured punctured through it going that fast where did it hit India I guess I wasn't even paying attention to where it at yeah India oh oh my okay that was a lot of fragments that got knocked off there okay okay so now we're going to increase it from six two i' say We'll double it every time 10% maybe we'll do 20% so if we increase it 10 km across increase the speed 80% the speed of light decrease our simulation speed what is it going to do what is it going to do what are you going to do okay let's find out let's follow we're going to follow you right into Earth all right we are going to go in out down there we go down and out all right we're going to decrease that simulation speed there we go that's better let's decrease it a little more I want to see what we to be like a ground zero getting hit by a 50 kilometer wide asteroid traveling at 90% the speed of life let's find out guys here we go into the atmosphere we have entered the atmosphere and the planet there we go oh it has ripped all right let's zoom out a little bit get some perspective and remember this is 05 milliseconds per second this is on this order of Nan seconds it's like 50 50 NS per second it's happening pretty fast it's happening pretty fast all right one milliseconds 110,000 of a second that has happened on the order of 1,000 of a second per second let's see what happened on the back side oh it's just the whole earth okay I think we opened up a hole in the earth there and the earth looks pretty devastated oh look at that that's awesome that's pretty cool oh nice you can make that bigger that's awesome I didn't know you could do that [Music] yeah okay well all right that's about that we have a 50,000 degree Earth finally got some results that was a little a little disappointing uh having to having to ramp up the parameters that much okay last thing I want to do well second to last thing is uh yeah there we go look at that solar system is something along the lines of this I want to play around with objects in disrupting the solar system look at that Jupiter Beetle Juice is so big that it would essentially expand its surface would be all the way out to Jupiter oh so you just they just open the simulate well I guess that's all you could do the red super Giant Beetle Juice see Uranus like taco Tuesday like the the night after Taco Tuesday Uranus is heating up guys all right so Beetle Juice is a red super giant Mercury Venus Earth and Mars all have orbits smaller than Beetle juices radius so they would have already immediately been inside and Jupiter soon follows being swallowed up Beetle juices higher gravity PS in the rest of the solar system planets where is it 11 times the Sun's mass but even Beetle Juice isn't as large as you scutty look at that I really like the idea of replicating like what it would be like to live on a a planet with to Suns especially dim Suns because something like about dim Suns just seems really you know appealing in a in a fascinating sci-fi kind of way so if we we're g to put Earth out here way out here that's 78 you well let's check out the habitable zone that's we could attempt we could at least attempt to have a habitable Earth so habitable zone okay the beetle juic is 120 a again that's about the the extent of the actual solar systems of the actual solar system proper I guess before it start to get swamped by the interstellar winds so we're gonna add we got Earth way out here maybe in orbit it appears to be in orbit let's see well let's slow it down let's slow things down a little bit all right so the red super Giants there something yeah just so uh calm and fascinating and comforting at the same time this weird mix of I guess what I'm trying to do with my channel um about you know orbiting really far it's like you zoom in and you look and you ban across although them let me get rid of the habitability the habitable gas over [Music] here and to look at Beetle Juice that's so incredible so if we were to put the sun where Beetle Juice is it would look like a star it would be so far away it' be three no four times further from Earth than the Sun is from Pluto actually so let's do it let's see what it would look like so we got the sun right there so 10 a 12 a and let's see the luminosity the sun would give Earth it's flying to it wow almost nothing that's really interesting let me make sure the view is right so it's realistic lighting yeah realistic that's really interesting so let's find out what the let's find out how dim the sun actually looks yeah look at that it basically looks like a like a really bright star all right so I want to do I want to put the sun where it would actually be where's the Earth all right okay there's F chip okay the sun is oh wow look at this what what's going on here why does it look so close yeah that's that gives you an idea of just how you know exaggerated the planet sizes are really cuz this one Au is how close Sun actually is to Earth and the Luminosity will be pretty realistic okay all right there we go all right let's check it out look at the difference though Beetle Juice has to be 120 times further away than the Earth is from from the Sun for uh for the earth to be in its habitable zone all right and now we see the true Luminosity look at that that's like a an Amber reading light it's kind of like the the setting I have right now it's wild to think that being on an exoplanet or you know Planet orbiting Beetle Juice in its habitable zone even though it's impossible because Beetle Juice is a super giant and as a short lifespan you would never you wouldn't have time enough to evolve intelligent life there but if the planet happened to be habitable then maybe you could have you could colonize the planet so imagine living on a planet that dim and then look at the brightness that the Earth has to really blasted with light when you think about it and check out the apparent brightness from a distance of 1 Au about 90 million miles away it's way smaller but way brighter relative to Beetle Juice it's red super giant now if we delete this so we delete this planet delete or that sun we put UI Scotty out here or Canis Major is even larger it 12 we got put this one 800 a something like that probably out here 200 I'll put it in 120 now look at this be juice is massive kenis Majoris is kis maurus so red that a hyper giant it's only 1,400 light years from Earth wow that's awesome that's an actual picture of canis maurus right there Kess matures that's on the the star's been known since for over 3,000 years that's I love that that we used to humans have evolved staring at the stars not only using them objectively as guides in the night but as projections of our our our stories out to the sky one of the few things that it's over the span of even hundreds of generations of humans is fixed in nature RV y okay that was not I guess the constellation's been known for 3,000 years VY Canis Major is the stars in extreme oxygen rich red hyper giant it's one of the most luminous and massive red super Giants it's one of the most luminous stars in the about 17 times the mass of the Sun surrounded by a circumstellar envelope it's part of a star that has a roughly spherical shape and is not gravitationally bound to the car star core usually circumstellar envelopes are formed from the dense Stellar Wind and they are present before the formation of the star caused by its mass loss was one of the first radio masers ever discovered it's embedded in a large molecular cloud so it seems like it's way too chaotic to have any any planets with any possibility of life around those that star in that cloud the radius is roughly 1,400 times that of the sun which is close to the modeled maximum the Hayashi limit a volume nearly three billion times that of the Sun a volume of three billion times the sun wow speed of light would take six hours to go circumnavigate its surface compared to 14 seconds for for the sun look at it's discover I wonder if he had just quite to see it that's funny all right if you didn't know that was that was funny apparently have to talk to my talk myself out of out of crying at how bad my jokes are all right what I did want to see was I look at the uh the ball this immediately took when I put that right there the Earth's just GNA get sucked right into it oh whoa what an interesting orbit wow okay let's slow down here before anything crazy happens because this is exactly what I wanted I didn't I didn't plan this I'm not I'm not that sophisticated um oh yeah of course the Earth is a a ball of 300° gas but whatever I wanted to look at its sky just imagine being in a system like that and looking up at the sky and seeing two red hyper Giants it's not exactly Tatooine but I think it's still pretty cool the magnitude of things out in the universe always stunts me what I wanted to finish up with though there's a lot of cool little you know simulations pre-made simulations and a couple tutorials that we could do but I did want to now let's let's check out the one the constellation tutorial I did want to do that one okay here we go all right check it out so the stars and constellations may look like they are situated nested with you know in proximity to each other but um this one here in which Beetle Juice is actually a part of is a is a simulation but it's an accurate depiction of three-dimensional you know GD uh system showing you the spatial separation between the stars and a very popular constellation and it's going to show us how evolves so there's beet juice right there here's a hint constellations available visible in both the northern and the southern hemispheres and here it is so rajel is a pretty big star in Beetle Juice is the top left corner top left shoulder I guess for you guys it would be this one right of the Orion Nebula select expand oh steings to turn on the constellation labels now it says o constellations are only symbols images created from stars from the perspective of the Earth or the Sun if you're you know averaging distances there in the cosmos so if we lived in a different part of the Galaxy the tutorials saying we you know the constellations would be viewed these stars and they're not star groups they're just groups us projecting three dimensions onto a are projecting a two I guess a 2d surface on which from our perspective all stars appear to lie on but in reality they're really way further apart than uh than I you know used to guess and now it's going to re fast forward and watch how these Stars given their current known velocities which is a fascinating feat of human you know intellect now they discovered velocities of stars given that over any short span of just even years the Stars positions do not perceptibly change so how the hell do we know what the velocities are and I think it has something to do with Doppler shifts um has something to do with Statistics but I don't know much more than that off the cuff it's fascinating though other they're able to predict at least what these star Stellar velocities are so and they project them extrapolate them into the future when we get this let's press play and we see from our perspective this is how the stars are going to evolve it'll take about 350,000 years for oion to become unrecognizable but even then the four main stars really it still has roughly the same shape and I know the sword down here is a star forming region so maybe there'll be maybe some of that gas will have dispersed and cleared out and it'll seem like it's brighter maybe or maybe dimmer I don't know if the gas is not no longer reflecting any of the light but the Stars aren't physically related to each other just like one of you corrected me on the birth of the solar system video I know we formed within a constellation of stars or you know a group of stars the sun did the sun in our in US ultimately formed you know five to 10 five to seven billion years ago I guess um but the orbits around the Galaxy we've made about 20 orbits around the Milky Way core since then so all the stars since then have as they go they've drifted away dispers so it's interesting how stars do you know especially uh the Dynamics the galactic Dynamics how how it affects Stars how arms can form and you have star forming regions within galaxies you have bright bands you have denser cores denser regions of arms looser you have more eccentric orbits more um inclined orbits That Vary off the plane but still most of them are within the orbital Galactic plan even though constellations aren't physically significant they're still helpful for finding a way around the sky try loading the complete set of Western constellations and watch how their position their positions change over thousands of years oh there we go who let's back out here where are we look at that so if we Zoom all the way out now we can see this guy's coming towards us that's really interesting look at that oh okay we just I guess some are going to explode can we reverse that all right we can cool let's reverse it give back into your normal shape there there we go something like that nice okay oh there it is all right that is really interesting oh okay that's the Sun and we can see slowly how the position of all the Orion stars are changing over time over 10,000 years per second maybe we have visited some of those Stars before they even reach their positions right now that's cool in the threedimensional you looks like this this one's far away for so what do we are like your that's 100 light years that's a thousand possibility of interstellar Travelers so uh it's really fascinating I like it's also something interesting to think about just what kind of new technologies if we don't wipe ourselves out with AI or nuclear weapons what we will have achieved in just just the next 100 years and then and put that two three 400 years into the future I have no doubt in my mind that we'll have unlocked fundamental patterns and relations between matter and energy in the universe to be able to manipulate the space around us to put humans in another star system on another star systems Planet I habitable one hopefully okay well this has been fun I hope you guys enjoyed this really off-script Adventure in the universe sandb and I want to give into the am another shout out and thanks again for supporting the video today we partnered up because I really enjoy their shirts so I know you guys will too so go ahead and go click that link in the description or the comments for 10% off sitewide everything you see they have lots of really cool designs lots of really cool graphics and styles and like I said before their shirts are seriously comfortable so give them some love and thanks again into the am thanks for watching guys thanks as always for joining thanks for the love thanks for all the comments thanks for the support um you guys are always super super positive and encouraging and um I hope hope you guys enjoyed this one let me know what you did or didn't like let me know if you want Another Universe Sandbox video because I can make it happen there's still Lots left to [Music] explore I had fun hope you did too take you e for e e e e e e