What is the significance of the gravitational constant?

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SUMMARY

The gravitational constant, denoted as G and valued at 6.67 x 10-11 m3 kg-1 s-2, is crucial for calculating the gravitational force between two masses using the formula F = G(m1m2/r2). It is important to distinguish between G and the acceleration due to gravity on Earth, represented as little g (9.8 m/s2). The confusion often arises from mixing these two concepts, as G is a constant while little g is an acceleration experienced by objects near Earth's surface. The measurement of G was first accomplished by Henry Cavendish through a torsion balance setup.

PREREQUISITES
  • Understanding of Newton's Law of Universal Gravitation
  • Familiarity with the concepts of mass and distance in physics
  • Knowledge of basic physics formulas, particularly F = G(m1m2/r2)
  • Ability to differentiate between gravitational constant (G) and acceleration due to gravity (g)
NEXT STEPS
  • Research the historical context and experiments conducted by Henry Cavendish to measure G
  • Explore the implications of gravitational constant in astrophysics and cosmology
  • Learn about the differences between classical mechanics and general relativity regarding gravity
  • Investigate the applications of G in satellite motion and orbital mechanics
USEFUL FOR

Students of physics, educators teaching gravitational concepts, and anyone interested in the fundamental principles of gravity and its measurement.

GreatEscapist
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In my physics class, we learned that everything accelerates towards each other at 6.67 x 10-11. I'm not sure what about that doesn't make sense (We didn't talk about it much, but we're expected to know about it) but something doesn't. How can EVERYTHING accelerate at the gravity? Uhhh, wouldn't a bigger mass go faster? Earth goes 9.8 m/s2, so where does G come into play?
And how the crap did someone figure that out, anyway?
 
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GreatEscapist said:
In my physics class, we learned that everything accelerates towards each other at 6.67 x 10-11.
:confused: That's the gravitational constant G (in m3 kg-1 s-2), not the acceleration of anything.
 
GreatEscapist said:
In my physics class, we learned that everything accelerates towards each other at 6.67 x 10-11. I

This is incorrect. To find the force between 2 objects with respect to each other we use the following formula \ F=G \frac{m1*m2}{r^2}. Where m1 and m2 represent the mass of the objects and r is the distance between them.G is your gravitational constant which is not an acceleration . To find the acceleration on one of the objects at a certain distance from the other you take its mass out of the formula. The acceleration of object 2 at distance r from object 1 is \ a=G \frac{m1}{r^2} directed from 2 to 1
 
Last edited:
GreatEscapist said:
In my physics class, we learned that everything accelerates towards each other at 6.67 x 10-11. I'm not sure what about that doesn't make sense (We didn't talk about it much, but we're expected to know about it) but something doesn't. How can EVERYTHING accelerate at the gravity? Uhhh, wouldn't a bigger mass go faster? Earth goes 9.8 m/s2, so where does G come into play?
And how the crap did someone figure that out, anyway?
You may also be confusing little g with big G. The 9.8 m/s2 that you referred to is little g, and it is an acceleration. It is the acceleration that all objects fall at surface of the earth. Big G is as the previous posters described. You may find this page helpful: http://csep10.phys.utk.edu/astr161/lect/history/Newtongrav.html
 
Oh.
This would explain why my homework always comes out wrong.
 
G was measured by Henry Cavendish using a torsion setup , google it to get more precise details.
 

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