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m= mass of object

v= velocity

R= radius of the earth

h= height from the surface to the escape velocity

(mv2 )

______ = G MEM

R + h _____

(R+h)2

v2 =GME

______

(R +h)2

Ve = (√gR2 /(R+h)2 )

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What information can be learned from a position-time graph and from a speed-time graph?

A position time graph can show you velocity. As time changes, so does position, and the velocity of the object can be determined. For a speed time graph, you can derive acceleration. As time changes, so does velocity, and the acceleration of the object can be determined.If you are plotting velocity (speed) versus time, the slope is the acceleration.


What is the momentum and derive the formula for the momentum?

Momentum is the product of the mass and the velocity of an object. It's SI unit is kgms-1. Correct, but perhaps more easily interpreted as kgm/s.


How do you derive the formula of ozone layer?

Ozone layer has no formula. However there is a formula for ozone and that is O3.


What is a kinematics equation that uses acceleration final velocity distance and time but not initial velocity?

There is no ready equation, but you can derive one using the three known kinematic equations.Using the general notations:u = initial velocityv = final velocitya = accelerations = distancet = timev = u + atHence, u = v - atv2 = u2 + 2asHence, substituting the value of u from above,v2 = (v - at)2 + 2asv2 = v2 -2vat + a2t2 + 2asÂ?2vt = at2 + 2s Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? Â? .......(Cancelling v2 and dividing by a)


How do you calculate the formula for the shock absorber?

To calculate the formula for a shock absorber, you would typically need to consider factors such as the mass of the vehicle, the velocity at impact, the damping coefficient of the shock absorber, and the spring constant of the suspension system. You can use equations of motion and principles of physics to derive the formula that relates these parameters to determine the behavior of the shock absorber. This formula is crucial for predicting how the shock absorber will perform in various conditions to provide proper vehicle suspension and control.

Related Questions

How do you derive lateral displacement?

Lateral displacement can be derived using the formula: lateral displacement = initial velocity * time + 0.5 * acceleration * time^2. This formula takes into account the initial velocity, acceleration, and time taken for the object to undergo lateral displacement.


Describe the motion of a satellite relative to the direction of gravity at any moment in time?

Derive acceleration relative to time and plot the resultant velocity (centripetal and tangential) as a vector.


How do you derive units for acceleration?

Acceleration is the rate of change of velocity over time. By dividing a unit of velocity by a unit of time, we can derive the unit of acceleration. For example, if velocity is measured in meters per second (m/s) and time is measured in seconds (s), acceleration would be in meters per second squared (m/s^2).


How to derive the kinematic equations for motion in one dimension?

To derive the kinematic equations for motion in one dimension, start with the definitions of velocity and acceleration. Then, integrate the acceleration function to find the velocity function, and integrate the velocity function to find the position function. This process will lead to the kinematic equations: (v u at), (s ut frac12at2), and (v2 u2 2as), where (v) is final velocity, (u) is initial velocity, (a) is acceleration, (t) is time, and (s) is displacement.


When an object and acceleration is zero at some instant t in time its velocity is?

If an object's acceleration is zero at a specific instant in time, its velocity can either be zero or a constant non-zero value at that instant. This means that the object could be either at rest or moving with a constant velocity at that particular moment.


How can one derive the kinematic equations?

The kinematic equations can be derived by integrating the acceleration function to find the velocity function, and then integrating the velocity function to find the position function. These equations describe the motion of an object in terms of its position, velocity, and acceleration over time.


How do you derive the formula for cetripital acceleration?

That is done via calculus. Specifically, take the movement over a small distance, calculate the change in velocity divided by the time, and figure out what happens if the time interval gets smaller and smaller - as they say in calculus, "get the limit of the acceleration as the time tends towards zero".


Derive a formula for the speed of ocean waves in terms of Density acceleration of free fall depth and wavelength?

barn


How can you derive the formula for force (F) using the equation fma, which relates force (F), mass (m), and acceleration (a)?

To derive the formula for force (F) using the equation fma, you can rearrange the equation to solve for force. By dividing both sides of the equation by mass (m), you get F ma, where force (F) is equal to mass (m) multiplied by acceleration (a). This formula shows the relationship between force, mass, and acceleration.


How you can derive the velocity unit?

velocity=distance / time


What information can be learned from a position-time graph and from a speed-time graph?

A position time graph can show you velocity. As time changes, so does position, and the velocity of the object can be determined. For a speed time graph, you can derive acceleration. As time changes, so does velocity, and the acceleration of the object can be determined.If you are plotting velocity (speed) versus time, the slope is the acceleration.


How can one derive the escape velocity of an object from a celestial body?

To derive the escape velocity of an object from a celestial body, you can use the formula: escape velocity (2 gravitational constant mass of celestial body / distance from the center of the celestial body). This formula takes into account the gravitational pull of the celestial body and the distance of the object from its center. By calculating this value, you can determine the minimum velocity needed for an object to escape the gravitational pull of the celestial body.