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Introductory Physics 9th Grade Science Mr. Wenger Click to continue Who is Isaac Newton? Scientific Notation Newton’s First Law of Motion Newton’s Third Law of Motion Click Here For Instructions! Newton’s Second Law of Motion Newton’s Law of Universal Gravitation Ready for the quiz? Click here! Newton’s First Law of Motion – The Law of Inertia An object as rest stays at rest, while an object in motion stays in motion with the same velocity and acceleration. This is true, unless an outside force acts onto such object. For example, if you set down your backpack on the floor, the backpack will not move unless you or something else picks it up or exerts another force on it. Return to Menu Newton’s Second Law of Motion Newton’s Second Law of motion can be summed up in an equation he created: F = ma. Where F is force, m is mass, and a is acceleration. This equation shows that Force is proportional to acceleration and in the same direction of the net force. So in short, this equation states that when a force acts onto a mass, acceleration is produced. Return to Menu Newton’s Third Law of Motion Newton’s third law is probably one of the most commonly heard laws. For every action, there is an equal and opposite reaction. This means, that for every force that is applied to anything, there is an equal and opposite reaction at that exact same point. For example, if you lean up against a wall, the wall is pushing up against you to keep you from falling over. Return to Menu Newton’s Law of Universal Gravitation This law also has a formula shown in the picture below. Where F is for force, m stands for masses of the two objects, and G is the gravitation constant. This law states that any two objects in the entire universe, as long as they have mass, are attracted to each other by a force! That’s right, the computer and yourself have an attraction to each other at any point in time, though the force may be infinitesimal, it’s still there! Return to Menu Who is Isaac Newton? Isaac Newton was and still is a very famous English physicist. He was also widely know for his mathematics in his own time. Newton was one of the first scientists to develop calculus. Newton’s calculus was eventually disregarded and proved wrong, but led to the calculus we use today. Newton is most widely known for his Laws of Motion, and his Law of Universal Gravitation which you will learn about in this activity. Return to Menu Scientific Notation Scientific notation is very important, it is a way to shorten the writing of numbers so we don’t need to take up an entire page writing one answer. For instance, the sun is 149600000000 meters away from the Earth. We can express this as so: 149.6 x 10^9, this means that you will move the decimal place over one place and if there isn’t a number currently there, add a zero to the end of the number. Return to Menu If the mass of the Earth is 5.972 x 10^24kg, and the mass of the sun is 1.989 x 10^30 kg. The distance between the Sun and the Earth is 149.6 x 10^9 meters, what is the force that the Sun and the Earth enact on each other? Also, use G = 6.67 x 10^-11 (m^3/kg s^2) Answers are expressed in unit of force Newtons (N) A) 5.30 x 10^33 N B) 3.54 x 10^22 N C) 5.31 x 10^32 N D) 17.8 x 10^-9 N A) 5.30 x 10^33 N Remember the equation for universal gravitation is F = G (m1 * m2)/r^2. Do not forget to square your distance from the Earth to the Sun, go ahead and give it another try! Return to Question B) 3.54 x 10^22 N Great job! Please continue to the next slide to finish this activity. Click to Continue C) 5.31 x 10^32 N Don’t forget the gravitation constant G in your formula! Remember that the formula is F = G(m1 * m2)/r^2. Return to Question D) 17.8 x 10^-9 N Woops, don’t forget the equation is F = G(m1 * m2)/r^2. Don’t forget to use both masses next time! Return to Question Instructions • Click the links on the menu to learn more about the designated topic. • Read about all the topics • When you are ready, proceed to the quiz which is accessed from the menu. • Finish the quiz and proceed to follow designated instructions. Return to Menu Congratulations! Now that you’re finished, please click the link to return to the title slide for the next person. Return to Title Slide