Forces and Motion Scripted - UTeach Outreach
... The modern equations of motion proposed by Sir Isaac Newton (1643 – 1727) in 1686 form the basis of classical mechanics, the body of knowledge still used to predict the behavior of physical systems today. For movement very slow compared to the speed of light (about 670 million miles per hour), these ...
... The modern equations of motion proposed by Sir Isaac Newton (1643 – 1727) in 1686 form the basis of classical mechanics, the body of knowledge still used to predict the behavior of physical systems today. For movement very slow compared to the speed of light (about 670 million miles per hour), these ...
Centripetal force
... Assessment 1. A race car is moving with a speed of 200 km/h on a circular section of a race track that has a radius of 400 m. The race car and driver have a mass of 1400 kg. a) What is the magnitude of the centripetal acceleration felt by the driver? Asked: a ...
... Assessment 1. A race car is moving with a speed of 200 km/h on a circular section of a race track that has a radius of 400 m. The race car and driver have a mass of 1400 kg. a) What is the magnitude of the centripetal acceleration felt by the driver? Asked: a ...
Notes - UMD Physics
... released from rest with the string vertical and its top end tied to a fixed bar. Show that (a) the tension in the string is one-third the weight of the disk, (b) the magnitude of the acceleration of the CM is 2g/3, and (c) the speed of the CM is (4gh/3)1/2 after the disk has descended through distan ...
... released from rest with the string vertical and its top end tied to a fixed bar. Show that (a) the tension in the string is one-third the weight of the disk, (b) the magnitude of the acceleration of the CM is 2g/3, and (c) the speed of the CM is (4gh/3)1/2 after the disk has descended through distan ...
Chapter 4- wrap up
... If F is greater than f, the object must accelerate with a net force of F – f. If f is greater than F, the object won't move at all. If f = F then the object is moving at a constant speed (or is at rest) as the net force on the object is zero. n f ...
... If F is greater than f, the object must accelerate with a net force of F – f. If f is greater than F, the object won't move at all. If f = F then the object is moving at a constant speed (or is at rest) as the net force on the object is zero. n f ...
Physics - Rotational Motion and Astrophysics: Numerical Examples
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... Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. Any enquiries regarding this document/publication should be sent to us at ...
Rotational Motion and Astrophysics_tcm4-726390
... Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. Any enquiries regarding this document/publication should be sent to us at ...
... Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. Any enquiries regarding this document/publication should be sent to us at ...
TEKS 8.7 A
... to articulate them, then much of the ways things move become clear. Otherwise, the world can be a bewildering place in which objects move in seemingly bizarre ways. It is imperative that the student be led to observe and to analyze the way things actually move. The “Laws” of motion are laws only in ...
... to articulate them, then much of the ways things move become clear. Otherwise, the world can be a bewildering place in which objects move in seemingly bizarre ways. It is imperative that the student be led to observe and to analyze the way things actually move. The “Laws” of motion are laws only in ...
Mass versus weight
In everyday usage, the mass of an object is often referred to as its weight though these are in fact different concepts and quantities. In scientific contexts, mass refers loosely to the amount of ""matter"" in an object (though ""matter"" may be difficult to define), whereas weight refers to the force experienced by an object due to gravity. In other words, an object with a mass of 1.0 kilogram will weigh approximately 9.81 newtons (newton is the unit of force, while kilogram is the unit of mass) on the surface of the Earth (its mass multiplied by the gravitational field strength). Its weight will be less on Mars (where gravity is weaker), more on Saturn, and negligible in space when far from any significant source of gravity, but it will always have the same mass.Objects on the surface of the Earth have weight, although sometimes this weight is difficult to measure. An example is a small object floating in a pool of water (or even on a dish of water), which does not appear to have weight since it is buoyed by the water; but it is found to have its usual weight when it is added to water in a container which is entirely supported by and weighed on a scale. Thus, the ""weightless object"" floating in water actually transfers its weight to the bottom of the container (where the pressure increases). Similarly, a balloon has mass but may appear to have no weight or even negative weight, due to buoyancy in air. However the weight of the balloon and the gas inside it has merely been transferred to a large area of the Earth's surface, making the weight difficult to measure. The weight of a flying airplane is similarly distributed to the ground, but does not disappear. If the airplane is in level flight, the same weight-force is distributed to the surface of the Earth as when the plane was on the runway, but spread over a larger area.A better scientific definition of mass is its description as being composed of inertia, which basically is the resistance of an object being accelerated when acted on by an external force. Gravitational ""weight"" is the force created when a mass is acted upon by a gravitational field and the object is not allowed to free-fall, but is supported or retarded by a mechanical force, such as the surface of a planet. Such a force constitutes weight. This force can be added to by any other kind of force.For example, in the photograph, the girl's weight, subtracted from the tension in the chain (respectively the support force of the seat), yields the necessary centripetal force to keep her swinging in an arc. If one stands behind her at the bottom of her arc and abruptly stops her, the impetus (""bump"" or stopping-force) one experiences is due to acting against her inertia, and would be the same even if gravity were suddenly switched off.While the weight of an object varies in proportion to the strength of the gravitational field, its mass is constant (ignoring relativistic effects) as long as no energy or matter is added to the object. Accordingly, for an astronaut on a spacewalk in orbit (a free-fall), no effort is required to hold a communications satellite in front of him; it is ""weightless"". However, since objects in orbit retain their mass and inertia, an astronaut must exert ten times as much force to accelerate a 10‑ton satellite at the same rate as one with a mass of only 1 ton.On Earth, a swing set can demonstrate this relationship between force, mass, and acceleration. If one were to stand behind a large adult sitting stationary on a swing and give him a strong push, the adult would temporarily accelerate to a quite low speed, and then swing only a short distance before beginning to swing in the opposite direction. Applying the same impetus to a small child would produce a much greater speed.