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Scientific principles
Einstein's General Theory of Relativity

Einstein's Theory of General Relativity

Albert Einstein developed the theory of general relativity in 1915. It is a gravitational theory that primarily involves a particle’s acceleration with respect to or relative to another. It describes the relationship of space, time, and matter. It is also a modified and improved alteration of Newton’s Law of Gravity. 
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Galileo’s Principles on Astronomy and Falling Bodies
Scientific principles
Galileo’s Principles on Astronomy and Falling Bodies
One of the significant contributions of Galileo Galilei to astronomy was his invention of the first telescope that is able to magnify up to thirty times. By using the telescope, he was able to study and observe heavenly bodies and images of the earth. His discoveries using his astronomical telescope have greatly helped preceding astronomers and scientists to understand and analyze the properties and attributes of different heavenly bodies.
His claims include discovering the uneven surface and craters of the moon. The reflected light that shines from the moon enabled him to observe the mountainous surfaces of the moon. He was able to observe the stars in the Milky Way galaxy by noticing from his telescope that the universe is made up of numerous stars.
Galileo observed planets. He was the one who discovered the four moons of the planet Jupiter which are now called the Galilean moons. He observed the oval shape of the planet Saturn. He studied the planet Venus and showed that it undergoes a set of phases that is similar to the moon. According to Galileo, the planet Venus can be viewed in its set of phases from the earth. These observations and theories by Galileo supported the Copernican system.
Galileo observed the dark patches on the sun through his telescope and these dark patches are what are scientifically termed today as sunspots. His observation of the motion of these sunspots indicated that the sun is rotating on its axis.
Galileo also had significant contributions in the field of mechanics.
Galileo discovered the law of falling bodies. His theory opposed the principles of Aristotle on falling bodies which states that when two objects with different masses are dropped at the same time from the same height, the heavier object will hit the ground first.
Galileo proposed that falling bodies fall with uniform acceleration as long as there is a negligible resistance of the medium through which the bodies are falling or when falling bodies are only influenced by gravity. When a body is falling through a vacuum, there is a negligible resistance of the medium. He observed that two objects with different weights hit the ground at the same time when these objects initially fall from the same height. When two objects of different weight initially falling from the same height will not hit the ground at the same time, this is caused by the air resistance or the resistance of the medium that the objects are falling through. His theories include that the speed or motion of a falling body does not depend on its weight, density, and size.
Galileo’s law of falling bodies is described in the statement that “The distance travelled by a falling body is directly proportional to the square of the time it took to travel.” He also stated a principle of inertia which states that “A body that is moving on a level surface will continue to move in the same direction with constant speed unless it is disturbed.”  His principle of inertia is associated with Newton’s first law which is the law of inertia.

Galileo’s Principles on Astronomy and Falling Bodies


One of the significant contributions of Galileo Galilei to astronomy was his invention of the first telescope that is able to magnify up to thirty times. By using the telescope, he was able to study and observe heavenly bodies and images of the earth. His discoveries using his astronomical telescope have greatly helped preceding astronomers and scientists to understand and analyze the properties and attributes of different heavenly bodies.
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Isaac Newton’s Laws of Motion
Scientific principles
Isaac Newton’s Laws of Motion
Isaac Newton’s Laws of Motion are the basic foundations of classical mechanics. These laws relate the forces that act upon a body to the motion of the body.
Newton's first law of Motion
The first law states that “An object at rest will remain at rest and an object in motion will remain in motion with the same speed and in the same direction unless acted upon by a net external force.” This law is also called as the law of inertia. This law means that a stationary object will remain stationary and not moving until a force will act upon it and a moving object will neither slow down nor move faster until an unbalanced force will act upon it. An unbalanced force or net external force is referred to as the vector sum of all forces acting on the body that is not equal to zero. As an example, consider a remote-controlled toy car. It does not move unless you attempt to move it. When it is already in motion, it moves in one direction unless you attempt to change its direction and it remains moving until you attempt to stop it.
Newton's Second law of Motion
The second law states that “The force applied to a body produces a proportional acceleration.” This law is described in the equation F=ma where F is force applied to the body, m is the mass of the body, and a is the acceleration of the body. The force applied to the body is equal to the vector sum of all  forces acting upon the body when many forces are acting upon the body in an instant. The direction of the applied force acting upon the body is the same as the direction of the acceleration of the body. This law also describes that the acceleration of the body is inversely proportional to the mass of the body. Applications of this law are easily observed in our everyday life. Consider again a toy car. When a net external force is applied to it, it accelerates but when you put something heavy on it, it needs more applied force to achieve the same acceleration. When the same force is applied on both, the one that is heavier will accelerate less.
Newton's Third law of Motion
The third law states that ''every action there is always an equal and opposite reaction.” This means that when a force is applied on an object, the object reacts with a force that is equal in magnitude to the force applied on it but it acts in the opposite direction. The force may be equal in magnitude but the acceleration of the one doing the action is not always the same as the acceleration of the one that is reacting because the mass of the two objects may not always have the same mass. Consider a jack in the box. When the top of the box is pushing the jack down, the jack is pushing the top of the box upward with the same amount of force that it is pushed by the top of the box. In the same way, when you press or push something, it will press or push you back with the same amount of force.
These three laws of motion are the basic principles in which the statics and dynamics of bodies are developed.

Isaac Newton’s Laws of Motion

Isaac Newton’s Laws of Motion are the basic foundations of classical mechanics. These laws relate the forces that act upon a body to the motion of the body.
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Kepler’s Laws of Planetary Motion
Scientific principles
Kepler’s Laws
Johannes Kepler stated the three laws of planetary motion. These laws are what are known today as Kepler’s laws and they describe the motion of the planets. He discovered these laws through the help of Tycho Brahe’s studies collections because he was in charge of them when Brahe died.
The first law states that “Every planet has an elliptical orbit with the Sun at one focus.” Having an elliptical orbit means that the sum of the distances of each orbital point to a point called the focus is constant. The first law states that the Sun is a focus of the orbit of every planet in the solar system. The claims of the Ptolemaic and Copernican systems stated that the orbits of the planets follow a circular path or a superposition of circular paths. Johannes Kepler discovered the elliptic path of the orbits of the planets after studying Tycho Brahe’s observations and study collections and he proved this through his calculations. The elliptical orbit of the planets is an effect of the force of gravity. Most of the planets follow an elliptical orbit with low eccentricity. Other heavenly bodies such as asteroids also follow an elliptical orbit, with high eccentricity, with the Sun at one of its foci. The eccentricity of an ellipse describes its shape, that is, an ellipse with low eccentricity has a geometric shape that is close to a circle and an ellipse with high eccentricity has a geometric shape that is close to an oval or a stretched circle.
The second law states that “For equal intervals of time, the line that joins the planet to the Sun sweeps out equal areas.” Consider that when the planet earth is following its elliptical orbit for one day or 24 hours, an area is covered by the earth’s path in its orbit and it is described by the line that joins the earth to the sun. The second law states that for a 24-hour time interval, this area is always the same wherever the earth on the point of its orbit is. Since the Sun is at one focus of the elliptical orbit of every planet, the planets move faster when they are closer to the sun because the areas that they sweep are the same when they are farther from the sun.
The third law states that “The square of the period of a planet’s orbit is directly proportional to the cube of the semi-major axis of the planet’s orbit.” This law is described by the equation P2=ka3 where P is the planet’s orbital period, k is the proportionality constant and a is the planet orbit’s semi-major axis. The proportionality constant is the same for all planets. This law implies that the time it takes the planet to orbit around the sun or what is known as its orbital period increases as its distance from the sun, which is directly related to its orbital path’s semi-major axis, also increases. Mercury, which is the nearest planet to the sun, takes the shortest time to orbit around the sun and Pluto, which is the farthest plant from the sun takes the longest time to orbit around the sun. The third law was what other scientists and astronomers used to calculate for orbital periods of satellites and other heavenly bodies.
Kepler’s Laws of Planetary Motion have been very useful for other scientists and astronomers to understand the orbital paths of the planets, satellites, and moons.

Kepler’s Laws of Planetary Motion

 

Johannes Kepler stated the three laws of planetary motion. These laws are what are known today as Kepler’s laws and they describe the motion of the planets. He discovered these laws through the help of Tycho Brahe’s studies collections because he was in charge of them when Brahe died. 
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Nikola Tesla’s Inventions and Principles
Scientific principles
Nikola Tesla’s Principles
The AC motors used in electrical power systems are mostly induction motors. Nikola Tesla invented the AC induction motor after first discovering the principle of rotating magnetic field.
The principle of rotating magnetic field is basically shown when two coils of wire perpendicular to each other can rotate a magnetic field if the coils are supplied with 90 degrees out of phase AC current.
The  Two-phase Induction Motor
Nikola Tesla’s two-phase induction motor consists of two sets of wire coils surrounding the core of a motor. The two sets of coils are perpendicular to each other. The coils act as electromagnets when alternating current passes through them. The polarity of the coil electromagnets changes when the direction of the current flow reverses. The current that passes through the first coil creates a magnetic field around the coil and this causes the coil to turn. When the direction of the current flow that passes through the first coil reverses, a magnetic field is produced around the second coil. This process produces a rotating magnetic field. This theory of operation of a rotating magnetic field makes up the induction motor with only the rotor moving.
The Tesla Coil
The Tesla coil, which is also one of Nikola Tesla’s inventions, is instrumental in developing wireless communication especially in radio communications. The Tesla coil is a type of an air-core transformer with the primary and secondary windings set at resonance. A resonance is a condition of an electrical circuit in which the combination of the alternating currents impedance values cancel out. The Tesla coil demonstrates properties of insulators and conductors in interaction with electric fields in high frequency.
The Tesla coil consists of a primary winding, a secondary winding, a transformer, and two high-voltage capacitors. The transformer consists of an iron core in which coils of copper wire are wound around its hollow center. The iron core inside the transformer acts as an electromagnet when an alternating current is passing through the transformer and this will produce a magnetic field around the primary winding. The electrical energy stored in the capacitors is then converted to magnetic energy. When the frequency in the primary winding is high enough, a magnetic field will be produced in the secondary winding.
The Tesla Turbine
One important contribution of Nikola Tesla to the area of energy conversion is his invention of what is known today as the Tesla Turbine. The Tesla turbine is a bladeless turbine that uses the boundary layer effect to cause the rotor disk of the turbine to move in the direction of the fluid. The boundary layer effect is defined as the interaction of a fluid with a solid surface with the boundary layer as the disk surface in which the thin layer of fluid is interacting with. The adhesive property of fluids causes fluid molecules to reduce speed and stick above the metal surface of the rotor disk. These molecules will cause the fluid flow above them to slow down. The viscous property of fluids causes the fluid molecules to keep from separating. This whole process creates a pulling force that causes the rotor disk to move in the direction of the fluid.

The Scientific work of Nikola Tesla

The AC motors used in electrical power systems are mostly induction motors. Nikola Tesla invented the AC induction motor after first discovering the principle of rotating magnetic field. 
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