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Created with Fabric.js 1.4.5 Infographic Project Assessment By: Jack Hubbard Newton's 1st Law- An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force. Inertia is the resistance of any physical object to any change in its state of motion, including changes to its speed and direction. Newtons 2nd Law-The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object. Equation: F=ma Weight- the force exerted on a body by gravityEquation: W=mg Universal Law of Gravity- states that any two objects exert a gravitational force of attraction on each other Tides and Moon Phases- Tides and the moon phases have a direct correllation because the sea level rises and falls in relation to the sun and moon's gravitational pullSpring Tides- When the moon is full or new, the gravitational pull of the moon and sun are combined. At these times, the high tides are very high and the low tides are very low.Neap Tides- They occur during quarter moons and have a much smaller effect or wave. Projectile Motion- An object that is influenced by outside forces when active or in motion. Horizontal and Vertical Component- The horizontal component would include an obstacle like wind and the vertical componentis gravity dragging the projectile down.Free Fall Acceleration- the active motion or velocity of a projectile measured with the horizontal and vertical components Newton's 3rd Law- For every action, there is an equal or opposite reactionForce Pairs- the way to identify the two objects reacting off of eachother Momentum- the quantity of motion that an object hasImpulse- the quantity of force x timeElastic Collision- when objects collide and transfer energy but don't stickInelastic Collision- when objects collide and transfer energy and stickEquation- F1= -F2 Isaac Newton was born on January 4, 1643 in Woolsthorpe, England. He was an established physicist and mathematician who created the basic priciples for modern physics. He created one of the most influential books in physics history called Philosopiae Naturalis Principa Mathematica. He died on March 31, 1727.
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