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g = 9 . 80 m/s 2 . size 12{g=9 "." "80 m/s" rSup { size 8{2} } } {}

Although g size 12{g} {} varies from 9 . 78 m/s 2 size 12{9 "." "78 m/s" rSup { size 8{2} } } {} to {} 9 . 83 m/s 2 size 12{9 "." "83 m/s" rSup { size 8{2} } } {} , depending on latitude, altitude, underlying geological formations, and local topography, the average value of 9 . 80 m/s 2 size 12{9 "." "80 m/s" rSup { size 8{2} } } {} will be used in this text unless otherwise specified. The direction of the acceleration due to gravity is downward (towards the center of Earth) . In fact, its direction defines what we call vertical. Note that whether the acceleration a size 12{a} {} in the kinematic equations has the value + g size 12{+g} {} or g size 12{ - g} {} depends on how we define our coordinate system. If we define the upward direction as positive, then a = g = 9 . 80 m/s 2 size 12{a= - g= - 9 "." "80 m/s" rSup { size 8{2} } } {} , and if we define the downward direction as positive, then a = g = 9 . 80 m/s 2 size 12{a=g=9 "." "80 m/s" rSup { size 8{2} } } {} .

One-dimensional motion involving gravity

The best way to see the basic features of motion involving gravity is to start with the simplest situations and then progress toward more complex ones. So we start by considering straight up and down motion with no air resistance or friction. These assumptions mean that the velocity (if there is any) is vertical. If the object is dropped, we know the initial velocity is zero. Once the object has left contact with whatever held or threw it, the object is in free-fall. Under these circumstances, the motion is one-dimensional and has constant acceleration of magnitude g size 12{g} {} . We will also represent vertical displacement with the symbol y size 12{y} {} and use x size 12{x} {} for horizontal displacement.

Kinematic equations for objects in free-fall where acceleration = - g

v = v 0 gt size 12{v=v rSub { size 8{0} } + ital "gt"} {}
y = y 0 + v 0 t 1 2 gt 2 size 12{y=y rSub { size 8{0} } +v rSub { size 8{0} } t+ { {1} over {2} } ital "gt" rSup { size 8{2} } } {}
v 2 = v 0 2 2 g y y 0 size 12{v rSup { size 8{2} } =v rSub { size 8{0} } rSup { size 8{2} } +2g left (y - y rSub { size 8{0} } right )} {}

Calculating position and velocity of a falling object: a rock thrown upward

A person standing on the edge of a high cliff throws a rock straight up with an initial velocity of 13.0 m/s . The rock misses the edge of the cliff as it falls back to Earth. Calculate the position and velocity of the rock 1.00 s, 2.00 s, and 3.00 s after it is thrown, neglecting the effects of air resistance.

Strategy

Draw a sketch.

Velocity vector arrow pointing up in the positive y direction, labeled v sub 0 equals thirteen point 0 meters per second. Acceleration vector arrow pointing down in the negative y direction, labeled a equals negative 9 point 8 meters per second squared.

We are asked to determine the position y size 12{y} {} at various times. It is reasonable to take the initial position y 0 size 12{y rSub { size 8{0} } } {} to be zero. This problem involves one-dimensional motion in the vertical direction. We use plus and minus signs to indicate direction, with up being positive and down negative. Since up is positive, and the rock is thrown upward, the initial velocity must be positive too. The acceleration due to gravity is downward, so a size 12{a} {} is negative. It is crucial that the initial velocity and the acceleration due to gravity have opposite signs. Opposite signs indicate that the acceleration due to gravity opposes the initial motion and will slow and eventually reverse it.

Since we are asked for values of position and velocity at three times, we will refer to these as y 1 size 12{y rSub { size 8{1} } } {} and v 1 size 12{v rSub { size 8{1} } } {} ; y 2 size 12{y rSub { size 8{2} } } {} and v 2 size 12{v rSub { size 8{2} } } {} ; and y 3 size 12{y rSub { size 8{3} } } {} and v 3 size 12{v rSub { size 8{3} } } {} .

Solution for Position y 1 size 12{y rSub { size 8{1} } } {}

1. Identify the knowns. We know that y 0 = 0 size 12{y rSub { size 8{0} } =0} {} ; v 0 = 13 . 0 m/s size 12{v rSub { size 8{0} } ="13" "." "0 m/s"} {} ; a = g = 9 . 80 m/s 2 size 12{a= - g= - 9 "." "80 m/s" rSup { size 8{2} } } {} ; and t = 1 . 00 s size 12{t=1 "." "00 s"} {} .

2. Identify the best equation to use. We will use y = y 0 + v 0 t + 1 2 at 2 size 12{y=y rSub { size 8{0} } +v rSub { size 8{0} } t+ { {1} over {2} } ital "at" rSup { size 8{2} } } {} because it includes only one unknown, y size 12{y} {} (or y 1 size 12{y rSub { size 8{1} } } {} , here), which is the value we want to find.

3. Plug in the known values and solve for y 1 size 12{y rSub { size 8{1} } } {} .

y 1 = 0 + 13 . 0 m/s 1 . 00 s + 1 2 9 . 80 m/s 2 1 . 00 s 2 = 8 . 10 m size 12{y"" lSub { size 8{1} } =0+ left ("13" "." "0 m/s" right ) left (1 "." "00 s" right )+ { {1} over {2} } left ( - 9 "." "80"" m/s" rSup { size 8{2} } right ) left (1 "." "00 s" right ) rSup { size 8{2} } =8 "." "10"`m} {}
Practice Key Terms 2

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Source:  OpenStax, College physics for ap® courses. OpenStax CNX. Nov 04, 2016 Download for free at https://legacy.cnx.org/content/col11844/1.14
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