Earth's centripetal acceleration around the Sun

In summary, the Earth has a mass of 6 x 10^24kg and orbits the sun at a constant circular distance of 1.5 x 10^11 m in 3.15 x 10^7 seconds. The Earth's centripetal acceleration around the Sun can be calculated using the formula a = v^2/r or a = ω^2r, with the latter being more appropriate in this scenario.
  • #1
hrice
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Homework Statement


The Earth has a mass of 6 x 10 24kg and orbits the sun in 3.15 x 10 7 seconds at a constant circular distance of 1.5 x 10 11 m. What is the Earth's centripetal acceleration around the Sun?


Homework Equations





The Attempt at a Solution

 
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  • #2
hrice said:

Homework Statement


The Earth has a mass of 6 x 10 24kg and orbits the sun in 3.15 x 10 7 seconds at a constant circular distance of 1.5 x 10 11 m. What is the Earth's centripetal acceleration around the Sun?


Homework Equations





The Attempt at a Solution


What are the two most common formulae/expressions for centripetal acceleration? One of them is more appropriate for the date you are working with.
 

What is Earth's centripetal acceleration around the Sun?

Earth's centripetal acceleration around the Sun refers to the rate at which Earth's velocity changes as it orbits around the Sun. It is caused by the gravitational force between Earth and the Sun.

How is Earth's centripetal acceleration calculated?

Earth's centripetal acceleration can be calculated using the formula a = v^2/r, where a is the centripetal acceleration, v is the velocity of the orbiting object, and r is the distance between the object and the center of the orbit.

What is the value of Earth's centripetal acceleration around the Sun?

The value of Earth's centripetal acceleration around the Sun is approximately 0.0059 meters per second squared. This is significantly smaller than Earth's gravitational acceleration, which is approximately 9.8 meters per second squared.

Does Earth's centripetal acceleration change throughout its orbit?

Yes, Earth's centripetal acceleration changes throughout its orbit. This is because the distance between Earth and the Sun changes, causing the velocity and therefore the centripetal acceleration to change as well.

What would happen if Earth's centripetal acceleration were to suddenly stop?

If Earth's centripetal acceleration were to suddenly stop, Earth would no longer be able to stay in orbit around the Sun. It would continue to move in a straight line, away from the Sun, until it was either pulled back by the Sun's gravitational force or collided with another object in space.

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