2. Leaving The Earth Flashcards
I) How would you calculate the work done on an object with mass ‘m’ in a uniform gravitational field of strength ‘g’ through a height of ‘h’?
W = mgh
I) Why does an objects weight vary as it rises above the earth?
Since the earth has a radial gravitational field, the gravitational field strength fall off with the square of the distances an object moves further from the surface of the earth. This means that the objects weight is reduced as it gets further away from the earth’s centre of mass.
I) When are radial gravitational fields produced?
They are always produced by spherical or point masses.
I) Define gravitational potential (V).
The work done per unit mass to move a small object from infinity to that point.
At a distance r from the centre of a spherical object’s mass M:
V = -GM/r and is measured in J/Kg
I) What are equipotential lines and equipotential surfaces?
Equipotential lines - Lines connecting points of the same potential.
Equipotential surfaces - Surfaces (spheres) connecting pints of the same potential.
I) What work is done when an object is moved over an equipotential surface?
NONE
I) How is the escape velocity equation derived?
It is assumed that in order for an object to escape from the earth’s gravitational field, the total energy of that object must be greater than or equal to zero (ignoring air resistance).
Therefore gpe + ke = 0 is the critical point at which the object leaves the earth. You can then rearrange this equation to derive the escape velocity equation.
I) Define the escape velocity of an object.
The escape velocity of an object is the minimum speed needed for an object to “break free” from the gravitational attraction of a massive body.
I) What is the approximate escape velocity on earth?
11.2 kms^-1
I) How would you use the earth’s rotation to help achieve escape velocity?
The speed of the earth’s rotation is nearly 500 ms^-1 going from west to east at the equator.
Therefore, an object travelling tangentially from the equator in an easterly direction requires an initial velocity of about 10.7 kms^-1 relative to the surface of the earth in order to escape.
I) Why are space launch sites often located at the equator.
Since the surface velocity of the earth decreases with latitude launch sites are positioned at the equator where the surface velocity is greatest.
I) What is the schwarzschild radius and what are the consequences of it?
The radius of a sphere such that, if all the mass of an object were to be compressed within that sphere, the escape velocity from the surface of the sphere would equal the speed of light.
This means that these objects would not emit or reflex EM radiation appearing ‘black’.
These objects are known as black holes.
I) Why does the earth retain its atmosphere?
Because its escape velocity if much larger than the mean speed of air molecules at temperatures found on earth.
I) What is the energy of a satellite in orbit?
Its combined kinetic and potential energy.
Remember that the potential energy is negative since it is relative to infinity where the potential energy is zero.
I) What is the conservation of energy?
In any closed system the total energy remains constant although it may change form and internal work may also be done when one body interacts with another body.
I) Define momentum.
The product of an object’s mass and velocity (p = mv) and is a vector taking the direction of the velocity as its direction.
I) Define Impulse.
The product of the force and the time for which the force acts (Impulse = Ft).
Impulse is a vector and takes the same direction as the force.
It can also be defined as the change in momentum: mv-mu
I) What is newton’s third law?
For every action, there is an equal and opposite reaction.
Fa = -Fr
I) What is a perfectly elastic collision?
Collisions in which kinetic energy is conserved. In the macroscopic world these are very rare.