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Peter Apps
Kashvi Panjolia
Peter Apps
Kashvi Panjolia
A vector field gives, as a function of position (and perhaps time), the value of a physical quantity that is described by a vector.
Key Concept: Vector Field - the assignment of a vector to each point in a portion of space. A vector field can be visualized as a collection of arrows with a given magnitude and direction, each attached to a point in the plane. ⬇️
Key Concept: Uniform Circular Motion - the motion of an object in a circle at a constant speed that is accelerating due to a change in direction.
Remember that there does not have to be a change in speed for there to be acceleration. Acceleration can be caused by a change in direction as well. A car making a turn at a constant speed is still accelerating because its direction is constantly changing. 🚗
In UCM there are four typical forces you will deal with: Tension, Friction, Gravity, and Normal. These forces are the cause of centripetal force. Centripetal force is not a new force; it is just a name for the force directed toward the center of the circle that is causing acceleration.
It is important to note that the centrifugal force is not a real force. This is a common misconception held by many students. The centrifugal force is an apparent force that is observed in a rotating reference frame. It is the result of the inertia of an object moving in a circular path, which makes it seem as though there is a force pushing it away from the center of rotation.
Equation: Fc = mv^2/r, where Fc is Centripetal Force in Newtons, m is mass in kilograms, v is the velocity in m/s, and r is the radius in meters.
The centripetal force is the name for the net force. Let’s dive into how the equation for centripetal force is derived: Newton’s second law gives us the equation F =ma, which can also be adapted for net force. Acceleration in a uniform circular motion is given as a = v^2/r, so Centripetal Force is simply mass times v^2/r or mv^2/r. Remember not to include the centripetal force on any free-body diagrams because it is not a force, but rather the net force.
The idea of using a field of vectors to represent the gravitational attraction between two objects is beyond the scope of AP Physics 1, so we use a simplified version of a vector field to represent this interaction.
The distance between the Earth and the moon is calculated using the distance between their centers of mass to simplify calculations. The two vectors are used to represent the magnitude and direction of the gravitational force between two objects.
🎥Watch: AP Physics 1 - Unit 3 Streams
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Peter Apps
Kashvi Panjolia
Peter Apps
Kashvi Panjolia
A vector field gives, as a function of position (and perhaps time), the value of a physical quantity that is described by a vector.
Key Concept: Vector Field - the assignment of a vector to each point in a portion of space. A vector field can be visualized as a collection of arrows with a given magnitude and direction, each attached to a point in the plane. ⬇️
Key Concept: Uniform Circular Motion - the motion of an object in a circle at a constant speed that is accelerating due to a change in direction.
Remember that there does not have to be a change in speed for there to be acceleration. Acceleration can be caused by a change in direction as well. A car making a turn at a constant speed is still accelerating because its direction is constantly changing. 🚗
In UCM there are four typical forces you will deal with: Tension, Friction, Gravity, and Normal. These forces are the cause of centripetal force. Centripetal force is not a new force; it is just a name for the force directed toward the center of the circle that is causing acceleration.
It is important to note that the centrifugal force is not a real force. This is a common misconception held by many students. The centrifugal force is an apparent force that is observed in a rotating reference frame. It is the result of the inertia of an object moving in a circular path, which makes it seem as though there is a force pushing it away from the center of rotation.
Equation: Fc = mv^2/r, where Fc is Centripetal Force in Newtons, m is mass in kilograms, v is the velocity in m/s, and r is the radius in meters.
The centripetal force is the name for the net force. Let’s dive into how the equation for centripetal force is derived: Newton’s second law gives us the equation F =ma, which can also be adapted for net force. Acceleration in a uniform circular motion is given as a = v^2/r, so Centripetal Force is simply mass times v^2/r or mv^2/r. Remember not to include the centripetal force on any free-body diagrams because it is not a force, but rather the net force.
The idea of using a field of vectors to represent the gravitational attraction between two objects is beyond the scope of AP Physics 1, so we use a simplified version of a vector field to represent this interaction.
The distance between the Earth and the moon is calculated using the distance between their centers of mass to simplify calculations. The two vectors are used to represent the magnitude and direction of the gravitational force between two objects.
🎥Watch: AP Physics 1 - Unit 3 Streams
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