The Ordered Universe Physical events Predictable Quantifiable Without the predictability of physical events the scientific method could not proceed. The Ordered Universe Stonehenge A Giant Calendar Built to Keep Track of Time Began in 2800 BC, Still Accurate Today The Ordered Universe As seen by: Ptolemy – 2nd century Copernicus - 16th century Brahe – late 16th century Kepler – early 17th century Galileo – early 17th century The Ordered Universe Galileo “The Father of Experimental Science” The Ordered Universe Experimentation collecting data using instruments and mathematical calculations The Ordered Universe Motion Speed = distance/time Velocity – speed in a specific direction Acceleration – rate of change in velocity The Ordered Universe Newton’s Laws of Motion 1st Law 2nd Law 3rd Law The Ordered Universe 1st Law of Motion – a moving object will continue moving in a straight line at a constant speed, and a stationary object will remain at rest, unless acted upon by an unbalanced force The Ordered Universe 2nd Law of Motion – the acceleration produced on a body by a force is proportional to the magnitude of the force and inversely proportional to the mass of the object The Ordered Universe 3rd Law of Motion – for every action there is an equal and opposite reaction The Ordered Universe Gravity = our #1 force “an attractive force between any 2 objects in the universe which is proportional to the masses of the objects and inversely proportional to the square of the distance between them” The Ordered Universe Weight force of gravity on an object in a particular place can change Mass amount of actual matter an object has stays constant The Ordered Universe Gravity “G” – universal constant, applies to any 2 masses in the universe “g” – gravity on the Earth’s surface only Question: If we drop two objects from the same distance above the surface of the Earth, which will fall faster, the heavier object or the lighter object?