Do you know how our solar system came to be? Well, I didn't either until I learned of the Solar Nebula Theory. It sounds boring but bear with me; basically these suuuuper smart guys named Emanuel Swedenborg, Pierre-Simon Laplace, and Immanuel Kant theorized about how the sun and all of our solar system (including other solar systems, duh) came to existence. To simplify the Solar Nebula Theory, a small gravitational collapse of a giant molecular cloud occurred; then poof here we are. Just kidding, that gravitational collapse allowed materials from all over to come together and eventually that formed a star. From there on our solar system formed just like you learn in science class, which I’m totally not currently in. The gravity that came with our sun forming attracted asteroids, rocks, and basically all the remnants of the gravitational collapse that didn’t go into the sun. These remnants eventually formed planets. What we know is that there are two types of planets, terrestrial and Jovian. Stay with me here, it gets interesting when Jupiter comes into the mix. So, terrestrial planets are rocky and such, much like Earth, Mars, Mercury, etc… Jovian planets; however, are much larger, like, huge. Think of Jupiter, that’s the only one we care about, right? Well when Jupiter had formed, there were a ton of asteroids and rocks just floating around the sun and planets. Jupiter wasn't having all that. That planet basically said go away and went on a monstrous rampage and cleaned up the solar system; all that cleaning, and Jupiter being so nice to all of us, we are still here and we don’t have meteorites raining down on us all of the time.
Speaking of meteorites and gravity and all, Earth has gravity; in case you didn’t know. An incredible scientist told us about this, his name is Isaac Newton. We don’t care about the apple and gravity thing, we aren't here for that. What we’re here for are his three laws of motion.
1. An object in motion will stay in motion (Inertia)
This law tells us that if you move something, it will keep moving. Well, I tried that and it didn't work. It didn't work because of an unbalanced force. Unbalanced forces allow for objects to stop moving, start moving, or keep an object stationary. This unbalanced force is friction. Friction occurs when two objects rub against each other, it essentially stops an object from moving. To sum it all up, with Newton’s first law, everything that moved would keep moving for eternity; but, that doesn't happen due to unbalanced forces (friction).
2. The force of an object is the same as its mass x acceleration F=ma
The genius’ second law is all about how much force an object has and how to calculate it. If there is a gigantic rock weighing 9,000kg hits your house accelerating at 30mph, chances are it has enough force to destroy your house. In order to figure out the force of this rock, multiply 9,000 by 30. Go ahead, do the math. Good job. Obviously you can reverse this F=ma if you have the force and mass but not acceleration, or vice versa for mass and acceleration.
3. For every action, there is an opposite reaction
Say you push on a wall with 50 lbs of pressure, that wall pushes back with the same force. If two people are on a rope, both hold on tightly, and they run away from each other. By the time the rope is at its fullest length they should have already realized that it wasn't a good idea. When the rope becomes stiff and cannot go any further out, it will snap both of the runners back a few feet. For that motion of the rope snapping into place, it snapped backwards. That’s an opposite reaction of the first reaction.
Unfortunately for you, we aren’t done yet. Since I know how much all of you love this blog, I’ve decided to go and research Kepler’s three laws (wow things come in threes a lot). I’ll make this quick and sweet for all of you dedicated readers, all two of you. To be short and sweet about it (don’t hold me to this, it won’t be either of these things), Kepler had three laws of planetary motion.
1. The Law of Ellipses
All of the paths of the planets are in an elliptical shape. An elliptical shape is basically an oval; but, hey, fancy science words make for an intelligent blog post. The planets move far away from the focus of the elliptical, in this case the sun, then get sucked back by the star’s gravitational pull. They then zoom by the sun and go far out again. The process repeats itself over and over and over and over and over again. It has happened more than over and over and over and over; one elliptical is a year. The Earth has traveled this path many times.
2. The Law of Equal Areas
This rule is a bit difficult to understand for the weaker minded of you two fabulous readers, but, I’ll do my best. If you somehow are able to see the Earth’s whole elliptical, then set a timer for 1 month and mark down where the Earth was at every 1 month interval. Draw a line from the sun to each marking of the Earth. Due to the elliptical pathway, there will be wider and narrower triangles throughout the markings. All of these triangles have the same area. The wider triangles are where the Earth moved much slower and the narrower triangles are where the Earth moved much faster, also, that is where the Earth was much farther away from the sun than when the triangles were wide.
3. The Law of Harmonies
As physicsclassroom.com states “The ratio of the squares of the periods of any two planets is equal to the ratio of the cubes of their average distances from the sun. “ This law helps us determine what period and how far away all planets are individually from the sun. The formula to determine all of this is T^2/R^3. To use this effectively, find the yearly period (how long it takes for a planet to make a full rotation around the sun) or a planet, in this case Earth, 1.00 yr, and the average distance the planet is from the sun in astronomical units, 1.00 au. plug this into the formula with the yearly rotation as T and the average distance as R (1.00^2/1.00^3). This is easiest because the T^2/R^3 comes out as 1.00. All information for other planets may be found online or in a planetary motion textbook.
See guys? Was that so bad? Oh, it was. If you didn't like it then HAHA! I've wasted your time! However, if you did like it, you’re amazing and I personally love you. Gosh don’t be so sensitive, I’m just fooling around. Whether you enjoyed it or not I appreciate you reading this.
Thanks for reading!See guys? Was that so bad? Oh, it was. If you didn't like it then HAHA! I've wasted your time! However, if you did like it, you’re amazing and I personally love you. Gosh don’t be so sensitive, I’m just fooling around. Whether you enjoyed it or not I appreciate you reading this.
By Garrett Boyce
P.S. I apologize for the white background of most of this last paragraph. I do not know how to adjust it to the normal background of common text.
