Calculating Gravitational Acceleration at a Planet's Surface

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SUMMARY

The discussion focuses on calculating gravitational acceleration at a planet's surface using the formula \( a = \frac{GM}{r^2} \), where \( G \) is the gravitational constant, \( M \) is the mass of the planet, and \( r \) is the radius of the planet. Participants emphasize the importance of the \( r^2 \) term in determining how a planet's size influences an object's weight. The correct answer to the posed problem is identified as option D, highlighting the relationship between mass and gravitational force.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation
  • Familiarity with the gravitational constant (G)
  • Knowledge of basic physics equations related to force and acceleration
  • Concept of mass and radius in gravitational calculations
NEXT STEPS
  • Study the derivation of the gravitational force equation \( F = \frac{Gm_1m_2}{r^2} \)
  • Learn how to calculate gravitational acceleration using different planetary masses and radii
  • Explore the implications of gravitational acceleration on weight variations on different planets
  • Investigate the role of the gravitational constant in astrophysics and its applications
USEFUL FOR

Students studying physics, educators teaching gravitational concepts, and anyone interested in understanding the effects of planetary size on gravitational acceleration.

dinhjeffrey
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Homework Statement



http://img26.imageshack.us/i/1113001.jpg/

#13

Homework Equations


m=F/a
F=g(m1m2)/r^2

The Attempt at a Solution



well, the answer is D, but I am not sure how a planet's size can affect an object's weight on there. I am guessing you have to use the gravitational constant. I am guessing you plug in the planets weight and the objects weight into m1 and m2 of gravitational constant?
 
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dinhjeffrey said:

Homework Statement



http://img26.imageshack.us/i/1113001.jpg/

#13

Homework Equations


m=F/a
F=g(m1m2)/r^2

The Attempt at a Solution



well, the answer is D, but I am not sure how a planet's size can affect an object's weight on there. I am guessing you have to use the gravitational constant. I am guessing you plug in the planets weight and the objects weight into m1 and m2 of gravitational constant?
It is all about that r^2 term. If you know M (mass of planet) but don't know r (the radius of the planet - distance from centre to the surface), how do you find a (= GM/r^2) at the surface?

AM
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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