MHB Calculating Acceleration on the Surface of Venus

Click For Summary
SUMMARY

The acceleration due to gravity on the surface of Venus can be calculated using the formula g' = GM/R², where M is the mass of Venus and R is its radius. Given that the mass of Venus is 81.5% of Earth's mass (4.86×1024 kg) and its radius is 94.9% of Earth's radius (6.05×106 m), the derived acceleration is approximately 8.87 m/s². Additionally, a rock weighing 75.0 N on Earth would weigh approximately 63.5 N on Venus, calculated using the ratio of gravitational forces.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation
  • Familiarity with gravitational acceleration formulas
  • Basic knowledge of mass and weight relationships
  • Ability to perform unit conversions and calculations
NEXT STEPS
  • Study the derivation of gravitational acceleration formulas in detail
  • Learn about the differences in gravitational forces on different celestial bodies
  • Explore the implications of gravity on weight and mass in varying environments
  • Investigate the physical characteristics of Venus compared to Earth
USEFUL FOR

Students in physics, astronomers, and anyone interested in planetary science and gravitational calculations will benefit from this discussion.

SantiagoHill
Messages
1
Reaction score
0
Friends, hello everyone!
Please help with this calculation.

The mass of Venus is 81.5% that of the earth, and its radius is 94.9% that of the earth.
(a) Compute the acceleration due to gravity on the surface of Venus from these data.
(b) If a rock weighs 75.0 N on earth, what would it weigh at the surface of Venuse?
 
Mathematics news on Phys.org
SantiagoHill said:
Friends, hello everyone!
Please help with this calculation.

The mass of Venus is 81.5% that of the earth, and its radius is 94.9% that of the earth.
(a) Compute the acceleration due to gravity on the surface of Venus from these data.
(b) If a rock weighs 75.0 N on earth, what would it weigh at the surface of Venuse?
a) You probably already have a formula for g' (the acceleration due to gravity) but here is the derivation anyway:
[math]F = \dfrac{GMm}{R^2} = m g'[/math]

[math]g' = \dfrac{GM}{R^2}[/math]

So if the mass of Venus is [math]M = 0.815 M_E[/math] and [math]R = 0.949 R_E[/math] then what is g'?

b) On Earth w = mg. So find m. On Venus w' = mg'...

-Dan
 
a) The mass of Venus MV represent 81.5% of the of the Earth. So, the mass of Venus is
MV=(81.5%)ME
(1)
Where ME is the mass of the Earth. Plug the mass of Earth into equation (1), so we can get MV by
MV=(0.815)ME=(0.815)(5.97×1024kg)=4.86×1024kg
The radius of Venus represent 94.9% of the radius of the Earth. So, the radius of Venus is
RV=(94.9%)RE
(2)
Where RE is the radius of the Earth. Plug the radius of Earth into equation (2), so we can get RV by
RV=(0.949)(6.38×106m)=6.05×106m
The weight w of a body is the total gravitational force exerted on it by all other bodies in the univerce where this gravitational force F is given by Newton`s general law of gravity by
F=GMVmRV2
(3)
Where RV is the radius of Venus, m is the mass of the body. As we mentioned above, this gravitational force equals the weight of the body which is mg, so using equation (3) we get the acceleration on Venus by
mg=GMVmRV2
gv=GMVRV2
(4)
Now, we plug values for RV, MV and G into equation (4) to get gv
gv=GMVRV2
=(6.67×10−11N⋅m2÷kg2)(4.86×1024kg)(6.05×106m)2
 
WestleyColeman said:
a) The mass of Venus MV represent 81.5% of the of the Earth. So, the mass of Venus is
MV=(81.5%)ME
(1)
Where ME is the mass of the Earth. Plug the mass of Earth into equation (1), so we can get MV by
MV=(0.815)ME=(0.815)(5.97×1024kg)=4.86×1024kg
The radius of Venus represent 94.9% of the radius of the Earth. So, the radius of Venus is
RV=(94.9%)RE
(2)
Where RE is the radius of the Earth. Plug the radius of Earth into equation (2), so we can get RV by
RV=(0.949)(6.38×106m)=6.05×106m
The weight w of a body is the total gravitational force exerted on it by all other bodies in the univerce where this gravitational force F is given by Newton`s general law of gravity by
F=GMVmRV2
(3)
Where RV is the radius of Venus, m is the mass of the body. As we mentioned above, this gravitational force equals the weight of the body which is mg, so using equation (3) we get the acceleration on Venus by
mg=GMVmRV2
gv=GMVRV2
(4)
Now, we plug values for RV, MV and G into equation (4) to get gv
gv=GMVRV2
=(6.67×10−11N⋅m2÷kg2)(4.86×1024kg)(6.05×106m)2
You are missing some division operators but otherwise correct.

Here's a bit of a shortcut.

Define [math]g' = \dfrac{GM_V}{R_V^2}[/math] and [math]g = \dfrac{GM_E}{R_E^2}[/math]. We know that [math]M_V = 0.815 M_E[/math] and [math]R_V = 0.949 R_E[/math]. Then
[math]g' = \dfrac{GM_V}{R_V^2} = \dfrac{G (0.815 M_E)}{(0.949 R_E)^2} = \dfrac{0.815}{0.949^2} \dfrac{G M_E}{R_E^2} = \dfrac{0.815}{0.949^2} \cdot g[/math]
and now you can use g = 9.81 m/s^2.

-Dan
 
topsquark said:
You are missing some division operators but otherwise correct.

Here's a bit of a shortcut.

Define [math]g' = \dfrac{GM_V}{R_V^2}[/math] and [math]g = \dfrac{GM_E}{R_E^2}[/math]. We know that [math]M_V = 0.815 M_E[/math] and [math]R_V = 0.949 R_E[/math]. Then
[math]g' = \dfrac{GM_V}{R_V^2} = \dfrac{G (0.815 M_E)}{(0.949 R_E)^2} = \dfrac{0.815}{0.949^2} \dfrac{G M_E}{R_E^2} = \dfrac{0.815}{0.949^2} \cdot g[/math]
and now you can use g = 9.81 m/s^2.

In order to get a better and more complete explanation of the solution of this problem, I advise you to go to https://plainmath.net/38641/the-mas...-the-earth-and-its-radius-is-94-9%-that-of-th and read the information here. In addition, you can find other useful information here.

Thanks for the advice.
 

Similar threads

  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 6 ·
Replies
6
Views
1K
Replies
54
Views
4K
Replies
9
Views
16K
  • · Replies 9 ·
Replies
9
Views
5K
  • · Replies 22 ·
Replies
22
Views
5K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 40 ·
2
Replies
40
Views
7K