How Can I Ace My Physics Test on Newton's Laws and Gravitation?

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SUMMARY

The discussion focuses on strategies to excel in a Grade 11 physics test centered on Newton's three laws and the universal law of gravitation. Key recommendations include mastering free body diagrams, identifying forces accurately, and practicing numerous problems. A specific proportionality problem illustrates how to calculate weight changes on different planets using the formula for gravitational force, demonstrating that an object weighing 500 N on Earth would weigh 1500 N on a planet with 300 times Earth's mass and 10 times its radius.

PREREQUISITES
  • Understanding of Newton's three laws of motion
  • Familiarity with free body diagrams
  • Knowledge of gravitational force calculations
  • Basic algebra for solving proportionality problems
NEXT STEPS
  • Practice drawing and analyzing free body diagrams
  • Study gravitational force calculations using the formula F = GmM/r²
  • Explore problems involving proportionality in gravitational contexts
  • Review examples of Newton's laws applied to real-world scenarios
USEFUL FOR

Students preparing for physics exams, educators teaching Newton's laws and gravitation, and anyone seeking to strengthen their understanding of classical mechanics.

Ameer Bux
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Hi guys. I am planning to get 100 percent for my upcoming physics test in two days time. I am i grade 11. The test is based on Newtons 3 laws and universal law of gravitation.

What are some of the best tips you can offer from your experience to help me achieve my goal?
 
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Ameer Bux said:
Hi guys. I am planning to get 100 percent for my upcoming physics test in two days time. I am i grade 11. The test is based on Newtons 3 laws and universal law of gravitation.

What are some of the best tips you can offer from your experience to help me achieve my goal?
Do lots of practice problems. :smile:
 
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Ameer Bux said:
Hi guys. I am planning to get 100 percent for my upcoming physics test in two days time. I am i grade 11. The test is based on Newtons 3 laws and universal law of gravitation.

What are some of the best tips you can offer from your experience to help me achieve my goal?
> master the art of drawing free body diagrams
> identify all forces acting in that diagram and apply Newton 1 for bodies in equilibrium (at rest or moving at constant velocity) or Newton 2 for accelerating bodies, with the wisdom to know the difference
> Do not confuse Newton 3 with Newton 1 or Newton 2. Newton 3 refers to equal and opposite forces acting on different bodies, whereas Newton 1 and 2 refer to net forces acting on the same body.

(I like your Avitar. Sort of like "Now that my house has burned down, I have a better view of the moon").
 
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berkeman said:
Do lots of practice problems. :smile:
Did 40 problems so far on Newtons first 3 laws. Going to start with universal law of gravitation in 30 mins.
 
PhanthomJay said:
> master the art of drawing free body diagrams
> identify all forces acting in that diagram and apply Newton 1 for bodies in equilibrium (at rest or moving at constant velocity) or Newton 2 for accelerating bodies, with the wisdom to know the difference
> Do not confuse Newton 3 with Newton 1 or Newton 2. Newton 3 refers to equal and opposite forces acting on different bodies, whereas Newton 1 and 2 refer to net forces acting on the same body.

(I like your Avitar. Sort of like "Now that my house has burned down, I have a better view of the moon").
Thanks a lot. Do you guys know a quick way to solve a proportionality problem in Newtons law of gravitation? I need some steps/method to follow. I don't know how to approach these kind of problems.

Example of a problem like that is as follows : A large planet has a radius 10x that of the Earth and a mass of 300x that of the earth.
a.) if the weight of a body is 500N on Earth what will be the weight on this planet?
b.) compare strenght of gravitational fields at the surface of the 2 planets.
 
The weight of an object on the surface of a particular planet is GmM/r^2, where G is the universal gravitational constant, m is the mass of the object, M is the mass of the planet, and r is the radius of the planet. So weight varies directly linearly with the planet mass, and inversely as the square of its radius. So in comparison to earth, if the planet mass increases 300 fold, and the planet's radius increases by 10 fold, then the object's weight increases by 300/10^2 = 300/100, that is, by a factor of 3. So the 500 N body weight on Earth will weigh 1500 N on that planet. So the gravitational field increases by 3.

You should note that since Weight = mg, then using the above formula yields g = GM/r^2, which , on planet earth, works out to g = 9.8 m/s^2, the acceleration of gravity. On the massive planet, g would be 9.8(3) or 29.4 m/s^2.
 

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