Help physic to calculate btw satellite and earth

In summary, the conversation discusses the relationship between the orbital velocity of a satellite and the rotation rate of the earth. The question asks for the necessary height of the satellite above the earth's surface, given the radius and mass of the earth. The respondent suggests considering relevant equations to solve the problem.
  • #1
lovelycecila
2
0
the angular velocity of the satellite to be equal to the rotation rate of the earth.given that the radius of the Earth is 6380km and the mass Earth 5.98 * 10^24.how high the surface of Earth should satellite be placed
 
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  • #2
Hello lovelycecila!

It seems from the date you provided, and what result you want, that what you meant was "Orbital Velocity" rather than "angular velocity" .

On PF it is required that you show us some working and a reasonable attempt before we can offer any real help. We don't do the homework for you, after all. Think perhaps of some relevant equations, that should definitely help.
 
  • #3


To calculate the height at which a satellite should be placed above the surface of the Earth, we need to use the formula for centripetal force:

F = (mv^2)/r

Where F is the centripetal force, m is the mass of the satellite, v is the velocity of the satellite, and r is the distance between the satellite and the center of the Earth.

First, we need to find the velocity of the satellite. We know that the angular velocity of the satellite is equal to the rotation rate of the Earth, which is 1 revolution per day or 2π radians per day. We can convert this to radians per second by dividing by the number of seconds in a day (24 hours * 60 minutes * 60 seconds), giving us a value of 7.27 * 10^-5 radians per second.

Next, we need to find the mass of the satellite. This information is not provided in the question, so we will assume a standard satellite mass of 1000 kg.

Now, we can plug in these values into the formula:

F = (mv^2)/r

F = (1000 kg)(7.27 * 10^-5 radians/second)^2 / (6380 km)

F = 0.111 N

This is the force required to keep the satellite in orbit around the Earth. To find the height at which the satellite should be placed, we can use the equation for gravitational force:

F = (GmM)/r^2

Where F is the force of gravity, G is the gravitational constant, m is the mass of the satellite, M is the mass of the Earth, and r is the distance between the satellite and the center of the Earth.

We can rearrange this equation to solve for r:

r = √(GmM/F)

Plugging in the values, we get:

r = √(6.67 * 10^-11 N m^2/kg^2 * 1000 kg * 5.98 * 10^24 kg / 0.111 N)

r = 4.2 * 10^7 meters

This is the distance from the center of the Earth to the satellite, so we need to subtract the radius of the Earth (6.38 * 10^6 meters) to get the height above the surface:

Height = 4.2 * 10^7 meters - 6
 

1. How do we calculate the distance between a satellite and the Earth?

The distance between a satellite and the Earth can be calculated using the formula: distance = orbital radius + Earth's radius. The orbital radius is the distance between the center of the Earth and the satellite's orbital path. The Earth's radius is the distance from the center of the Earth to its surface.

2. Why is it important to calculate the distance between a satellite and the Earth?

Calculating the distance between a satellite and the Earth is important for a variety of reasons. It helps in determining the satellite's position, velocity, and acceleration, which are crucial for its proper functioning. It also helps in predicting and avoiding collisions with other satellites or debris in space.

3. How does satellite altitude affect the distance from the Earth?

The altitude of a satellite, or its distance from the Earth's surface, directly affects the distance between the satellite and the Earth. As the altitude increases, the distance between the satellite and the Earth also increases. This is because the satellite's orbital path becomes larger, resulting in a longer distance between the satellite and the Earth.

4. What is the difference between geostationary and polar orbiting satellites in terms of distance from the Earth?

Geostationary satellites have an orbital radius of approximately 36,000 kilometers and remain in a fixed position above the Earth's equator. Polar orbiting satellites, on the other hand, have a lower orbital radius and continuously move around the Earth's poles. This results in a varying distance between polar orbiting satellites and the Earth, while geostationary satellites maintain a relatively constant distance.

5. How does the Earth's gravity affect the distance between a satellite and the Earth?

The Earth's gravity plays a significant role in determining the distance between a satellite and the Earth. The stronger the gravitational pull, the closer the satellite will be to the Earth. This is why satellites in low Earth orbit have a shorter distance from the Earth compared to those in higher orbits.

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