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Einstein's Theory of Relativity Made Easy!

Einstein’s Theory of Relativity Made Easy!

From what it is, to its impact on the world at large, join us as we explore Einstein’s Theory of Relativity made easy, and explain it so everyone can understand it. (Simplified)

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Watch Our “Wormhole Theory Explained – Breaking Spacetime!”

So where do we start with something as big and as complicated as the Theory of Relativity? I’m sure some of you wouldn’t even know what it is outside of its name, which is fine. But I’m sure you do know the man who came up with the idea, Albert Einstein. Einstein is revered as one of the smartest people to ever live, and he helped shape how we perceive both our world and our universe. So it might surprise you that this very brilliant man once started off as nothing more than a patent clerk. No, really, he did, and that’s part of the origin story to the Theory of Relativity.
Because one day, after doing his work at the patent office, he went on a trolley car to go home. And he would do this day after day after day. This is important because while he was on that car, he would think about the universe at large. He would ask himself questions and try to figure out the answers as best he could with the information he had. And one day, he was going away from a clock tower when he asked what would happen if the car he was on was going away from the clock tower…at the speed of light.
This may seem like an odd question to ask, but lightspeed travel is something that scientists are honestly trying to achieve right now, and these questions were truly the building blocks of this really happening. Anyway, back to the clock tower. Einstein theorized, as well as realized, that if he was moving the speed of light (which if you don’t know is 299,792,458 meters per second), the hands on the clock tower (meaning the minute hand and the hour hand) would quite literally appear to stop in place.
But, he also knew that while he himself was traveling at the speed of light and seeing everything stop more or less, everyone who was at the clock tower, and seeing things in “normal time” would not see them stop. The clock tower and its hands would keep ticking along as if nothing wrong.
Yet in this experiment, for Albert Einstein, time had literally slowed down, and it was at this moment that the “light bulb” went off in his head. Because it was through this experiment that he realized that if you go faster and faster through space, you’re actually causing time to go slower around you. But how was this possible if time was quite literally a constant force in the universe?
To try and answer this, Einstein would look to some of the other fathers of science to try and figure out the missing points in his equation. For example, he looked at the three laws of motion via Sir Isaac Newton. Newton notes that while objects do move at a certain speed, their values are never an absolute. Mainly because every speed we go at is based on a force imparted on something, or relative to something else. Such as how a car can go 65 miles per hour on a highway…but that’s only because the ground and friction ALLOW it to do so. No friction on the road? You’re not going that speed. Thus why he notes that every speed has to have “in respect to” another force or object that is allowing or perceiving that object’s speed.
However, in contrast, there is James Clark Maxwell, the father of electromagnetism, who notes that of all the things in the universe, it is light that is fixed. And as noted, light goes 299,792,458 meters per second. That will never change. That speed is another constant force in the universe. Anyone, anywhere in the world, or even anywhere in the universe will be able to determine that the speed of light is the same, it won’t change, and that’s part of the reason why the universe works like it does, because the speed of light is constant, right?
But therein lies the problem, or at least, Einstein realized that this was a problem. Because Newton said that no speed in the universe could be an absolute. But then Maxwell counters this by saving the speed of light is ALWAYS a constant. Which means that these two very universal and very accepted pieces of science are at a contradiction. Which is something you never want in the world of science, trust me.
If you’re still not getting the full picture of why this is a problem, here’s another thought experiment from Einstein to help explain it.
Imagine you are at a train station, and you are standing out on the platform when a storm comes. Then, out of the blue, two lightning bolts strike on either side of you. Because of your position in the middle of these lightning bolts, you perceive them at the exact same time, and the light reaches you at that same time.

Theory Of Relativity: Einstein’s Twin Paradox!

#InsaneCuriosity #Theory of Relativity #PhysicsHowTheUniverseWorks

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What’s On The Other Side Of A Black Hole?

What’s On The Other Side Of A Black Hole?

From what they are, to where they might go, and beyond! Join me as we explore the question of, “where do black holes lead to?”

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Before we dive into the potential pathways that Black Holes may have, it’s important to know exactly what they are. Because while you might have a loose definition as to what they are and what they do, they’re actually far more complex than you might realize. Which is why many people in NASA and other space programs are fascinated by them.
If you’re looking for a technical definition, this is how NASA describes Black Holes:
“A black hole is a place in space where gravity pulls so much that even light cannot get out. The gravity is so strong because matter has been squeezed into a tiny space. This can happen when a star is dying.”
This singularity as it is often called is a bit of a mystery in space, and for a very good reason. You see, black holes can form in large sizes, small sizes, and sometimes they don’t even need a fully fledged star to form at all! Which is scary in the sense that it means black holes can form in various ways.
Plus, since no light can actually escape them, it means that they can’t technically be seen by anyone. That being said, it’s easy to “see their work”, as the intense gravity of the Black Holes is enough to stretch objects from their “starting point” and slowly pull them to the Black Hole. This is known as spaghettification, because like a stretched piece of spaghetti, the object will get thinner and thinner until nothings exists but particles. And if you think that a Black Hole is limited in what it can absorb, you would be wrong. Very wrong in fact. If it is close enough, it’ll break down a star, a planet, multiple stars and planets at once, etc. It’s a question of range more than anything.
But there’s a catch to that, as you won’t be able to observe the spaghettification yourself. Why? Remember, no light escapes the void that is the Black Hole, so because of that, you’ll see the last known position of the object that light allows you to see. It’ll seem like they’re stuck in place and slowly going away until they’re gone. When in fact, they or it will be slowly pulled apart.
As we noted earlier, one of the main ways for a Black Hole to be born is to have a star collapse upon itself with such pressure that a Black Hole is a result. However, technically speaking, just about anything in the universe can become a Black Hole. How’s that for a scary thought?
It’s true though, and that’s one of the big “scaling” factors that you need to take into account when you’re talking about Black Holes. In fact, there’s actually a scarier thought that you need to consider, and that’s that black holes could technically be all around you right now. The only reason you’re not feeling their affects is that they’re not large enough to exert their own gravity.
The scale of a Black Hole is referred to as the Schwarzschild Radius. And becoming a Black Hole is impendent on you becoming so small and so dense that you can fit into this radius, and then potentially expand upon it. For example, a human being can become a Black Hole if condensed enough. However, the pressure needed to do that would not only be enormous, you could have to be shrunk 1 sextillion times smaller than a grain of sand. That’s REALLY small.

But that raises the question that we posed earlier, mainly, where do black holes lead to? I mean, if they can be of all sizes, and be anywhere from the size of a massive galaxy to the spec of sand on a beach, how can they lead to anywhere? How does that work? Would it work at all?
In the words of one scientist, “Who knows?”
“Falling through an event horizon is literally passing beyond the veil — once someone falls past it, nobody could ever send a message back,” he said. “They’d be ripped to pieces by the enormous gravity, so I doubt anyone falling through would get anywhere.”
Allow me to back up a little bit. Remember the whole “spagheticfication” thing I was talking about earlier? Well, the place that you would be “stretched to” is the horizon line of the black hole. Think of a black hole like a funnel. The big end of the funnel is the black hole that you “see” in space, and the rest of it is the core of the black hole that is hidden beneath its intense gravity. Now, if black holes DID lead somewhere, then like the funnel, you would have an access point through the core that you could go to. You get it?
The problem here is that most scientists believe based on their understanding of black holes that a horizon line is what awaits you at the end. So if you think about the funnel again, think about pinching the back end of it so that nothing could get out of said funnel. That’s what a lot of people think is in the center of a black hole, a literal end point. Which would be a problem for those who think it would lead anywhere…because it wouldn’t. It would end, o

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