Universal gravitational problem

In summary, the gravity on Earth is 9.81 and the gravity of Planet X is 19.6. The radius of Planet X is 2 times bigger than the radius of Earth.
  • #1
anna sung
46
0

Homework Statement



Planet X has a mass 8 times that of Earth and the acceleration due to gravity at its surface is 19.6 m/s2. The radius of the planet x compared to Earth is:

The answer is 2times bigger

Homework Equations



Fg = gm1m2 / r^2

The Attempt at a Solution



Is Earth's gravity 9.8 and the gravity of planet x is 19.6.
Where would I put these values in ?


 
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  • #2
Check your relevant equation what do each of the variables and constants mean?

In particular, f=Gmm/r^2 where G is what?
 
  • #3
jedishrfu said:
Check your relevant equation what do each of the variables and constants mean?

In particular, f=Gmm/r^2 where G is what?

Isn't g universal gravitational constant which is 6.67 x 10^-11?
Or is this where the 19.6m/s^2 should go into?
 
  • #4
G*m_1 is the acceleration due to gravity for a body
 
  • #5
anna sung said:
Isn't g universal gravitational constant which is 6.67 x 10^-11?
Or is this where the 19.6m/s^2 should go into?

Denote the universal gravitational constant by G. People use the notation g for the gravitational acceleration on the surface of the Earth: g≈9.81 m/s2

According to the law of universal gravitation, the force of gravity on an object of mass m is F=GmM/R2 at the surface of the Earth. M is the mass of Earth (5.97 x 10^24 kg) and R is the Radius of Earth (6.37 x 10^6 m).
The gravitational acceleration is F/m=g=GM/R2. Plug in the data: it is 9.81 m/s2

19.6 m/s2 is the gravitational acceleration at the surface on an other planet. How does it related to the radius and mass of the planet?

ehild
 
  • #6
So f=mg=GmM/r^2
Then say the mass of Earth is 2. Planet x is 8 times of the earth, so then 16.
Earth has gravity 9.8 and planet x has gravity 19.6.
Then the equation is really this: g=m/r^2
So Earth is square root ( 2/9.8)=0.45
planet x is square root (16/19.6) = 0.903
Oh, okay yeah and it's twice larger.
Okay I get it,
Thank you so much.^_^
 
  • #7
You are welcome :smile:

ehild
 

What is the Universal Gravitational Problem?

The Universal Gravitational Problem is a fundamental scientific concept that explains the force of gravity between all objects in the universe. It states that all objects with mass are attracted to each other by a force known as gravity.

Who developed the Universal Gravitational Problem?

The Universal Gravitational Problem was developed by Sir Isaac Newton in the late 17th century. He published his findings in his famous work "Principia Mathematica" in 1687.

What is the equation for the Universal Gravitational Problem?

The equation for the Universal Gravitational Problem is F = G * (m1 * m2)/r^2, where F is the gravitational force, G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between them.

How does the Universal Gravitational Problem apply to celestial bodies?

The Universal Gravitational Problem applies to celestial bodies such as planets, stars, and galaxies. It is responsible for keeping these objects in orbit around each other and for the formation of larger structures in the universe.

What are some real-world applications of the Universal Gravitational Problem?

The Universal Gravitational Problem has many practical applications, including determining the trajectory of space objects, calculating the force needed for spacecraft to escape Earth's gravity, and predicting the orbits of planets and satellites. It also plays a crucial role in understanding the dynamics of our solar system and the universe as a whole.

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