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To gain a better understanding of the velocity and acceleration vectors, imagine you are driving along a curvy road. If you do not turn the steering wheel, you would continue in a straight line and run off the road. The speed at which you are traveling when you run off the road, coupled with the direction, gives a vector representing your velocity, as illustrated in the following figure.

This figure represents a curving road. On the road is a car. At the car there are two vectors. The first vector is tangent to the back of the car. The second vector comes out of the front of the car in the direction the car is heading. Both of the vectors are labeled “velocity vectors”.
At each point along a road traveled by a car, the velocity vector of the car is tangent to the path traveled by the car.

However, the fact that you must turn the steering wheel to stay on the road indicates that your velocity is always changing (even if your speed is not) because your direction is constantly changing to keep you on the road. As you turn to the right, your acceleration vector also points to the right. As you turn to the left, your acceleration vector points to the left. This indicates that your velocity and acceleration vectors are constantly changing, regardless of whether your actual speed varies ( [link] ).

This figure is a car. The path the car is traveling is an increasing curve represented by a dotted line. The center of the car is labeled “tsub0” on the curve. From this point there are two vectors that are orthogonal to each other. The first vector is asubt and the second vector is asubn. In between these two vectors is a vector labeled “a”. It has angle theta between vector a and asubt.
The dashed line represents the trajectory of an object (a car, for example). The acceleration vector points toward the inside of the turn at all times.

Components of the acceleration vector

We can combine some of the concepts discussed in Arc Length and Curvature with the acceleration vector to gain a deeper understanding of how this vector relates to motion in the plane and in space. Recall that the unit tangent vector T and the unit normal vector N form an osculating plane at any point P on the curve defined by a vector-valued function r ( t ) . The following theorem shows that the acceleration vector a ( t ) lies in the osculating plane and can be written as a linear combination of the unit tangent and the unit normal vectors.

The plane of the acceleration vector

The acceleration vector a ( t ) of an object moving along a curve traced out by a twice-differentiable function r ( t ) lies in the plane formed by the unit tangent vector T ( t ) and the principal unit normal vector N ( t ) to C. Furthermore,

a ( t ) = v ( t ) T ( t ) + [ v ( t ) ] 2 κ N ( t ) .

Here, v ( t ) is the speed of the object and κ is the curvature of C traced out by r ( t ) .

Proof

Because v ( t ) = r ( t ) and T ( t ) = r ( t ) r ( t ) , we have v ( t ) = r ( t ) T ( t ) = v ( t ) T ( t ) . Now we differentiate this equation:

a ( t ) = v ( t ) = d d t ( v ( t ) T ( t ) ) = v ( t ) T ( t ) + v ( t ) T ( t ) .

Since N ( t ) = T ( t ) T ( t ) , we know T ( t ) = T ( t ) N ( t ) , so

a ( t ) = v ( t ) T ( t ) + v ( t ) T ( t ) N ( t ) .

A formula for curvature is κ = T ( t ) r ( t ) , so T ( t ) = κ r ( t ) = κ v ( t ) . This gives a ( t ) = v ( t ) T ( t ) + κ ( v ( t ) ) 2 N ( t ) .

The coefficients of T ( t ) and N ( t ) are referred to as the tangential component of acceleration    and the normal component of acceleration    , respectively. We write a T to denote the tangential component and a N to denote the normal component.

Tangential and normal components of acceleration

Let r ( t ) be a vector-valued function that denotes the position of an object as a function of time. Then a ( t ) = r″ ( t ) is the acceleration vector. The tangential and normal components of acceleration a T and a N are given by the formulas

a T = a · T = v · a v

and

a N = a · N = v × a v = a 2 a T 2 .

These components are related by the formula

a ( t ) = a T T ( t ) + a N N ( t ) .

Here T ( t ) is the unit tangent vector to the curve defined by r ( t ) , and N ( t ) is the unit normal vector to the curve defined by r ( t ) .

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Source:  OpenStax, Calculus volume 3. OpenStax CNX. Feb 05, 2016 Download for free at http://legacy.cnx.org/content/col11966/1.2
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