Gravitational Forces Flashcards
what is the fundamental law of gravity
every particle with mass attracts every other particle with mass
relating to the fundamental law of gravity, how are bodies such as planets or stars formed
- as particles with mass attract each other, they begin to clump together
- the clumps of matter attract other clumps, forming larger bodies of material each time
- these large bodies end up becoming planets or stars
how does the speed of clumping change throughout this process
- initially it is very slow
- as the acceleration generated by the particles is small
- but as the clumps become larger the strength of their gravitational pull becomes more pronounced
- leading to quicker rates of clumping
what do all particles with mass generate around themselves
a gravitational field
what kind of force is gravity
- a distant force
- thats always attractive
what is the basic equation for the force a body, with mass m, feels within the gravitational field of another body
- F = mg
- with g being the gravitational field strength of the ‘exerter’
why doesnt this equation hold true in most realistic cases involving gravitational forces, like with the earth and moon
- because the body having a gravitational force exerted on it is also exerting a gravitational force on the ‘exerter’
- so the net gravitational force wouldnt just be the product of one bodys g force
what is the true equation for the gravitational force between two masses
F = Gm1m2 / r^2
what are each of the variables in F = Gm1m2 / r^2
- F = g force
- G = 6.67x10-11 Nm2kg-2
- m1 and m2 = masses 1 and 2
- r = distance of separation from the centres of gravity of m1 and m2
what is the equation for centripetal force
F = m2 v^2 / r
what is that m2 referring to
- the body experiencing the centripetal force
- between the earth and moon, it would be the moon
what do you need to know about the relationship between gravitational force between two objects and the centripetal force an object is experiencing
- they are equal
- so Gm1m2 / r^2 = m2 v^2 / r
where does that equation for centripetal force come from
- F = ma
- a = v^2 / r from circular motion
- so F = m v^2 / r
what is the equation for the speed of an body orbiting another body and why
- v = 2 pi r / T
- comes from v = x / t
- where x is the circumference of the orbit (pi D = pi 2r)
- and T is the time it takes for one full revolution (s)
what is usually the difference between m1 and m2
- m1 is the bigger object
- it is usually the main ‘exerter’