Fourth year of secondary education
The force of gravity
José Luis San Emeterio Peña
 F G 
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Gravity beyond the earth

 

   All bodies attract each other according to Newton's principle of universal gravitation:

   Where F is the force of attraction, M and m the mass of the bodies, and r is the distance between them. G is the universal gravitational constant.

   This force is what permits us to put satellites into orbit, governs the tides and controls the movement of the planets around the sun.

   If you want to revise the corresponding experiments, click on their name:

  Satellites, tides, solar system 

 

  

 

 

 

 

  

   

 

  

Objectives of the teaching unit
Falling bodies
Free fall in a vacuum
Free fall in the air
Falling kinematics
Conclusions
The mass and weight of bodies
The weight of bodies
The difference between mass and weight
Conclusions
Measuring the intensity of g
A simple measuring device
g is not a true constant
Conclusions
Gravity beyond the earth
The force of the tides
The movement of satellites
The solar system
Conclusions
Evaluation