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An overview of derivatives and their application in kinematics. It explains how derivatives represent the rate of change of a function and demonstrates the calculation of derivatives for simple functions. Additionally, it applies these concepts to the motion of bodies with constant acceleration.
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Summary of Lecture 3 – KINEMATICS II
f x f a function that depends upon the argument. You should think of as a machine that gives you the value when you input .)
x f f x
f x x t
0
function. It tells us where a body is at different times.
t
x t t dx x dt Δ → t
0 lim (^ )^ ( ). t
x t t x t Δ → t
Δ x
Δ t
x t t x t t t
(^2 ) 2 2 2
0
we choose to be extremely small:
2 lim t 2
t x t t t t t t t t x (^) t t x dx t Δ → t dt
1 0
n n t
x t t dx x (^) nt dt t
− Δ →
0 0 2
x t
x t = x + t + at
0 0 0 v 1 (2 ) v 2 This clearly shows that v 0 (acceleration is constant)
dx (^) a t at dt d (^) a a dt
d (^) g dt
= ≈ m/sec. This is true provided we are fairly close to the earth, otherwise the value of g decreases as we go further away from the earth. Also, note that if we measured distances from the ground
2 2 2 2
up, then the acceleration would be negative.
d d dx d x d x dt dt dt dt dt x t x
with respect to.
t
r^ G^ = x t )ˆ ( )ˆ v ˆ^ ˆ v ˆ^ v ˆ Here the unit vectors ˆ^ and ˆare fixed, meaning that they do not dep
x y
i y t j dr dx (^) i dyj dt dt dt i j i j
end upon time.
cos You can think of: ( )( cos )
(length of ) (projection of on ) OR, ( )( cos ) (length of ) (projection of o
n ). Remember that for unit vectors ˆ ˆ^ ˆ^ ˆ^ 1 and ˆ^ ˆ 0.
i ⋅ i = j ⋅ j = i ⋅ j =
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