Is the Given Answer for the Classical Mechanics Problem on Earth Correct?

In summary, to achieve a free fall of $0\,m/s^2$ at a given radius $r$, the centripetal acceleration $\omega^2 r$ must be equal to the acceleration due to gravity $\frac{GM}{r^2}$. Solving for $r$, we get $r=4.3\cdot 10^7\,m$. However, it is possible that the given values for the angular velocity and mass have a higher precision, resulting in a slightly different value for $r$.
  • #1
WMDhamnekar
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  • #2
We are given the angular velocity $\omega = 7\cdot 10^{-5}\,rad/s$ and the mass $M=6\cdot 10^{24}\,kg$.
To achieve a free fall of $0\,m/s^2$ at radius $r$ we need that the centripetal acceleration is equal to the acceleration due to gravity,
Note that $v=\omega r$, so the centripetal acceleration is $\frac{v^2}{r}=\omega^2 r$.
The acceleration due to gravity is $\frac{GM}{r^2}$, where $G=6.67\cdot 10^{-11}$ is the gravitational constant (leaving out the unit while assuming SI units).
So:
$$\omega^2 r = \frac{GM}{r^2}$$
Solve for $r$.
 
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  • #3
Klaas van Aarsen said:
We are given the angular velocity $\omega = 7\cdot 10^{-5}\,rad/s$ and the mass $M=6\cdot 10^{24}\,kg$.
To achieve a free fall of $0\,m/s^2$ at radius $r$ we need that the centripetal acceleration is equal to the acceleration due to gravity,
Note that $v=\omega r$, so the centripetal acceleration is $\frac{v^2}{r}=\omega^2 r$.
The acceleration due to gravity is $\frac{GM}{r^2}$, where $G=6.67\cdot 10^{-11}$ is the gravitational constant (leaving out the unit while assuming SI units).
So:
$$\omega^2 r = \frac{GM}{r^2}$$
Solve for $r$.
Hi,
So, we get $r^3 =8.172587755e22m^3/rad^2$ So,$r=43396349.43332m/\sqrt[3]{rad^2}$. Is this answer correct?
 
  • #4
Dhamnekar Winod said:
Hi,
So, we get $r^3 =8.172587755e22m^3/rad^2$ So,$r=43396349.43332m/\sqrt[3]{rad^2}$. Is this answer correct?
I get the same answer.
Do note that $rad$ is not an actual physical unit, but it's a ratio. When we multiply the angular velocity (rad/s) with the radius (m), the rad unit is effectively eliminated and we get m/s.
So properly we have $r=4.3\cdot 10^7\,m$.

It means that answer 2 should be the correct answer.
Admittedly it's a bit strange that it is given as $4.4\cdot 10^7\,m$ instead of $4.3\cdot 10^7\,m$.
Since we're talking about earth, perhaps they used a mass and angular velocity with a higher precision than the ones given in the problem statement.
EDIT: Hmm... in that case we would actually get $r=4.2\cdot 10^7\,m$, so that can't be it after all.
 
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Related to Is the Given Answer for the Classical Mechanics Problem on Earth Correct?

1. What is classical mechanics?

Classical mechanics is a branch of physics that deals with the motion of macroscopic objects, such as planets, cars, and baseballs. It describes how these objects move and interact with each other under the influence of forces.

2. Who is considered the father of classical mechanics?

Sir Isaac Newton is considered the father of classical mechanics. He developed the three laws of motion and the law of universal gravitation, which laid the foundation for classical mechanics.

3. What are the three laws of motion?

The three laws of motion, as stated by Newton, are:
1. An object will remain at rest or in motion with a constant velocity unless acted upon by an external force.
2. The force acting on an object is equal to its mass multiplied by its acceleration.
3. For every action, there is an equal and opposite reaction.

4. How does classical mechanics differ from quantum mechanics?

Classical mechanics deals with the behavior of macroscopic objects, while quantum mechanics describes the behavior of subatomic particles. Classical mechanics follows deterministic laws, while quantum mechanics involves probability and uncertainty.

5. What are some real-world applications of classical mechanics?

Classical mechanics has numerous practical applications, including the design of bridges and buildings, the motion of satellites and spacecraft, and the development of vehicles and machines. It is also used in fields such as astronomy, engineering, and sports.

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