Two Physics problems related to gravitational energy

In summary, the required velocity for a rocket to reach a maximum height of 895 km above the surface of the Earth is 3920 m/s, and the required velocity for a rocket to reach an orbit with an altitude of 895 km is 8380 m/s. The approach for finding these velocities involves finding the energy needed for the rocket to end up with, and then determining what velocity corresponds to that energy.
  • #1
chroncile
35
0

Homework Statement


1.) How fast must a rocket leave the Earth’s surface to reach a maximum height of 895 km above the surface of the Earth (assume the rocket is simply going straight up)?

The answer is 3920 m/s

2.) How fast must a rocket leave the Earth’s surface to reach an orbit with an altitude of 895 km above the surface of the Earth?

The answer is 8380 m/s


Homework Equations


EG = -GMm / r


The Attempt at a Solution


For 1.)

Ek + EG = Ek' + EG'
0.5v2 = GM / r
V = square root ((2 * G * 5.97*x10^24)/895000+6370000)
V = 10,470 m/s

For 2.)

I have no idea
 
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  • #2
What you did for `1,' was you found the energy the rocket needed to end up with, then you figured out what velocity that corresponds to. You can do the same thing for `2,' just think: what's different about the final energy of the rocket in '2' as apposed to '1.'
 
  • #3
But I didn't even get the right answer in question 1.
 
  • #4
chroncile said:
But I didn't even get the right answer in question 1.
Good point. What is the initial potential energy? Then what is the final?
 
  • #5
how to solve this one.

For problem 2, you can use the equation for orbital velocity:

V = sqrt(GM / r)

Where:
V = orbital velocity
G = gravitational constant (6.67 x 10^-11 N*m^2/kg^2)
M = mass of the Earth (5.97 x 10^24 kg)
r = distance from the center of the Earth to the orbit (895,000 + 6,370,000 = 6,265,000 m)

Plugging in these values, we get:

V = sqrt((6.67 x 10^-11 N*m^2/kg^2 * 5.97 x 10^24 kg) / 6,265,000 m)
V = 7,910 m/s

Therefore, the rocket must leave the Earth's surface at a speed of 7,910 m/s to reach an orbit with an altitude of 895 km. This is significantly higher than the speed required in problem 1, as the rocket must overcome the Earth's gravity and also maintain enough velocity to stay in orbit.
 

FAQ: Two Physics problems related to gravitational energy

1. What is gravitational energy and how does it relate to physics?

Gravitational energy is the potential energy stored in an object due to its position in a gravitational field. This energy is related to physics because it is a fundamental concept in the study of gravity and its effects on objects.

2. Can you explain the difference between potential and kinetic energy in the context of gravitational energy?

Potential energy is the energy an object has due to its position or configuration, while kinetic energy is the energy an object has due to its motion. In the context of gravitational energy, potential energy is related to an object's position in a gravitational field, while kinetic energy is related to its motion within that field.

3. How is gravitational potential energy calculated in physics?

The formula for calculating gravitational potential energy is PE = mgh, where m is the mass of the object, g is the acceleration due to gravity, and h is the height or distance from the reference point. This formula assumes a constant gravitational field and neglects any other forces acting on the object.

4. What is the relationship between gravitational energy and the force of gravity?

The force of gravity is directly related to gravitational energy. The greater the gravitational energy of an object, the stronger the force of gravity it will experience. This is because gravitational energy is the potential to do work, and gravity is the force that causes objects to move and do work.

5. Can you provide examples of real-life applications of gravitational energy in physics?

Gravitational energy is a fundamental concept in many fields of physics, and it has numerous real-life applications. Some examples include understanding the orbits of planets and satellites, calculating the potential energy of objects in roller coasters and dams, and studying the formation and collapse of stars in astrophysics.

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