Vectors – Scalars and Vectors


Figure 2.1 A signpost gives information about distances and directions to towns or to other locations relative to the location of the signpost. Distance is a scalar quantity. Knowing the distance alone is not enough to get to the town; we must also know the direction from the signpost to the town. The direction, together with the distance, is a vector quantity commonly called the displacement vector. A signpost, therefore, gives information about displacement vectors from the signpost to towns. (credit: modification of work by “studio tdes”/Flickr,

Chapter Outline

  • 2.1 Scalars and Vectors
  • 2.2 Coordinate Systems and Components of a Vector
  • 2.3 Algebra of Vectors
  • 2.4 Products of Vectors

Vectors are essential to physics and engineering. Many fundamental physical quantities are vectors, including displacement, velocity, force, and electric and magnetic vector fields. Scalar products of vectors define other fundamental scalar physical quantities, such as energy. Vector products of vectors define still other fundamental vector physical quantities, such as torque and angular momentum. In other words, vectors are a component part of physics in much the same way as sentences are a component part of literature.

In introductory physics, vectors are Euclidean quantities that have geometric representations as arrows in one dimension (in a line), in two dimensions (in a plane), or in three dimensions (in space). They can be added, subtracted, or multiplied. In this chapter, we explore elements of vector algebra for applications in mechanics and in electricity and magnetism. Vector operations also have numerous generalizations in other branches of physics.

2.1 Scalars and Vectors

Learning Objectives

By the end of this section, you will be able to:

  • Describe the difference between vector and scalar quantities.
  • Identify the magnitude and direction of a vector.
  • Explain the effect of multiplying a vector quantity by a scalar.
  • Describe how one-dimensional vector quantities are added or subtracted.
  • Explain the geometric construction for the addition or subtraction of vectors in a plane.
  • Distinguish between a vector equation and a scalar equation.

Many familiar physical quantities can be specified completely by giving a single number and the appropriate unit. For example, “a class period lasts 50 min” or “the gas tank in my car holds 65 L” or “the distance between two posts is 100 m.” A physical quantity that can be specified completely in this manner is called a scalar quantity. Scalar is a synonym of “number.” Time, mass, distance, length, volume, temperature, and energy are examples of scalar quantities.

Scalar quantities that have the same physical units can be added or subtracted according to the usual rules of algebra for numbers. For example, a class ending 10 min earlier than 50 min lasts 50min−10min=40min50min−10min=40min. Similarly, a 60-cal serving of corn followed by a 200-cal serving of donuts gives 60cal+200cal=260cal60cal+200cal=260cal of energy. When we multiply a scalar quantity by a number, we obtain the same scalar quantity but with a larger (or smaller) value. For example, if yesterday’s breakfast had 200 cal of energy and today’s breakfast has four times as much energy as it had yesterday, then today’s breakfast has 4(200cal)=800cal4(200cal)=800cal of energy. Two scalar quantities can also be multiplied or divided by each other to form a derived scalar quantity. For example, if a train covers a distance of 100 km in 1.0 h, its speed is 100.0 km/1.0 h = 27.8 m/s, where the speed is a derived scalar quantity obtained by dividing distance by time.

Many physical quantities, however, cannot be described completely by just a single number of physical units. For example, when the U.S. Coast Guard dispatches a ship or a helicopter for a rescue mission, the rescue team must know not only the distance to the distress signal, but also the direction from which the signal is coming so they can get to its origin as quickly as possible. Physical quantities specified completely by giving a number of units (magnitude) and a direction are called vector quantities. Examples of vector quantities include displacement, velocity, position, force, and torque. In the language of mathematics, physical vector quantities are represented by mathematical objects called vectors (Figure 2.2). We can add or subtract two vectors, and we can multiply a vector by a scalar or by another vector, but we cannot divide by a vector. The operation of division by a vector is not defined.

Figure 2.2 We draw a vector from the initial point or origin (called the “tail” of a vector) to the end or terminal point (called the “head” of a vector), marked by an arrowhead. Magnitude is the length of a vector and is always a positive scalar quantity. (credit “photo”: modification of work by Cate Sevilla)

Let’s examine vector algebra using a graphical method to be aware of basic terms and to develop a qualitative understanding. In practice, however, when it comes to solving physics problems, we use analytical methods, which we’ll see in the next section. Analytical methods are more simple computationally and more accurate than graphical methods. From now on, to distinguish between a vector and a scalar quantity, we adopt the common convention that a letter in bold type with an arrow above it denotes a vector, and a letter without an arrow denotes a scalar. For example, a distance of 2.0 km, which is a scalar quantity, is denoted by d = 2.0 km, whereas a displacement of 2.0 km in some direction, which is a vector quantity, is denoted by d⃗ →.

Suppose you tell a friend on a camping trip that you have discovered a terrific fishing hole 6 km from your tent. It is unlikely your friend would be able to find the hole easily unless you also communicate the direction in which it can be found with respect to your campsite. You may say, for example, “Walk about 6 km northeast from my tent.” The key concept here is that you have to give not one but two pieces of information—namely, the distance or magnitude (6 km) and the direction (northeast).

Displacement is a general term used to describe a change in position, such as during a trip from the tent to the fishing hole. Displacement is an example of a vector quantity. If you walk from the tent (location A) to the hole (location B), as shown in Figure 2.3, the vector D⃗ →, representing your displacement, is drawn as the arrow that originates at point A and ends at point B. The arrowhead marks the end of the vector. The direction of the displacement vector D⃗ → is the direction of the arrow. The length of the arrow represents the magnitude D of vector D⃗ →. Here, D = 6 km. Since the magnitude of a vector is its length, which is a positive number, the magnitude is also indicated by placing the absolute value notation around the symbol that denotes the vector; so, we can write equivalently that D≡∣∣D⃗ ∣∣. To solve a vector problem graphically, we need to draw the vector D⃗ → to scale. For example, if we assume 1 unit of distance (1 km) is represented in the drawing by a line segment of length u = 2 cm, then the total displacement in this example is represented by a vector of length d=6u=6(2cm)=12cm, as shown in Figure 2.4. Notice that here, to avoid confusion, we used D=6km to denote the magnitude of the actual displacement and d = 12 cm to denote the length of its representation in the drawing.

Figure 2.3 The displacement vector from point A (the initial position at the campsite) to point B (the final position at the fishing hole) is indicated by an arrow with origin at point A and end at point B. The displacement is the same for any of the actual paths (dashed curves) that may be taken between points A and B.

Figure 2.4 A displacement D⃗ → of magnitude 6 km is drawn to scale as a vector of length 12 cm when the length of 2 cm represents 1 unit of displacement (which in this case is 1 km).

Suppose your friend walks from the campsite at A to the fishing pond at B and then walks back: from the fishing pond at B to the campsite at A. The magnitude of the displacement vector D⃗ AB→ from A to B is the same as the magnitude of the displacement vector D⃗ BA→ from B to A (it equals 6 km in both cases), so we can write DAB=DBA. However, vector D⃗ AB→ is not equal to vector D⃗ BA→ because these two vectors have different directions: D⃗ AB≠D⃗ BA. In Figure 2.3, vector D⃗ BA→ would be represented by a vector with an origin at point B and an end at point A, indicating vector D⃗ BA→ points to the southwest, which is exactly 180°180° opposite to the direction of vector D⃗ AB→. We say that vector D⃗ BA→ is antiparallel to vector D⃗ AB→ and write D⃗ AB=−D⃗ BA→, where the minus sign indicates the antiparallel direction.

Two vectors that have identical directions are said to be parallel vectors — meaning, they are parallel to each other. Two parallel vectors A⃗ → and B⃗ → are equal, denoted by A⃗ =B⃗ , if and only if they have equal magnitudes ∣∣A⃗ ∣∣=∣∣B⃗ ∣∣. Two vectors with directions perpendicular to each other are said to be orthogonal vectors. These relations between vectors are illustrated in Figure 2.5.

Figure 2.5 Various relations between two vectors A⃗ → and B⃗ →. (a) A⃗ ≠B⃗  because A≠B. (b) A⃗ ≠B⃗  because they are not parallel and A≠B. (c) A⃗ ≠−A⃗  because they have different directions (even though ∣∣A⃗ ∣∣=∣∣−A⃗ ∣∣. (d) A⃗ =B⃗  because they are parallel and have identical magnitudes A = B. (e) A⃗ ≠B⃗ because they have different directions (are not parallel); here, their directions differ by 90° — meaning, they are orthogonal.


Two motorboats named Alice and Bob are moving on a lake. Given the information about their velocity vectors in each of the following situations, indicate whether their velocity vectors are equal or otherwise. (a) Alice moves north at 6 knots and Bob moves west at 6 knots. (b) Alice moves west at 6 knots and Bob moves west at 3 knots. (c) Alice moves northeast at 6 knots and Bob moves south at 3 knots. (d) Alice moves northeast at 6 knots and Bob moves southwest at 6 knots. (e) Alice moves northeast at 2 knots and Bob moves closer to the shore northeast at 2 knots.

Algebra of Vectors in One Dimension

Vectors can be multiplied by scalars, added to other vectors, or subtracted from other vectors. We can illustrate these vector concepts using an example of the fishing trip seen in Figure 2.6.

Figure 2.6 Displacement vectors for a fishing trip. (a) Stopping to rest at point C while walking from camp (point A) to the pond (point B). (b) Going back for the dropped tackle box (point D). (c) Finishing up at the fishing pond.

Suppose your friend departs from point A (the campsite) and walks in the direction to point B (the fishing pond), but, along the way, stops to rest at some point C located three-quarters of the distance between A and B, beginning from point A (Figure 2.6(a)). What is his displacement vector D⃗ AC when he reaches point C? We know that if he walks all the way to B, his displacement vector relative to A is D⃗ AB, which has magnitude DAB=6km and a direction of northeast. If he walks only a 0.75 fraction of the total distance, maintaining the northeasterly direction, at point C he must be 0.75DAB=4.5km away from the campsite at A. So, his displacement vector at the rest point C has magnitude DAC=4.5km=0.75DAB and is parallel to the displacement vector D⃗ AB. All of this can be stated succinctly in the form of the following vector equation:


In a vector equation, both sides of the equation are vectors. The previous equation is an example of a vector multiplied by a positive scalar (number) α=0.75. The result, D⃗ AC, of such a multiplication is a new vector with a direction parallel to the direction of the original vector D⃗ AB.

In general, when a vector A⃗  is multiplied by a positive scalar α, the result is a new vector B⃗  that is parallel to A⃗ :



The magnitude |B⃗ | of this new vector is obtained by multiplying the magnitude |A⃗ | of the original vector, as expressed by the scalar equation:



In a scalar equation, both sides of the equation are numbers. Equation 2.2 is a scalar equation because the magnitudes of vectors are scalar quantities (and positive numbers). If the scalar α is negative in the vector equation Equation 2.1, then the magnitude |B⃗ | of the new vector is still given by Equation 2.2, but the direction of the new vector B⃗  is antiparallel to the direction of A⃗ . These principles are illustrated in Figure 2.7(a) by two examples where the length of vector A⃗  is 1.5 units. When α=2, the new vector B⃗ =2A⃗  has length B=2A=3.0 units (twice as long as the original vector) and is parallel to the original vector. When α=−2, the new vector C⃗ =−2A⃗  has length C=|−2|A=3.0 units (twice as long as the original vector) and is antiparallel to the original vector.

Figure 2.7 Algebra of vectors in one dimension. (a) Multiplication by a scalar. (b) Addition of two vectors (R⃗ (is called the resultant of vectors A⃗ and B⃗ ). (c) Subtraction of two vectors (D⃗  is the difference of vectors A⃗  and B⃗ ).

Now suppose your fishing buddy departs from point A (the campsite), walking in the direction to point B (the fishing hole), but he realizes he lost his tackle box when he stopped to rest at point C (located three-quarters of the distance between A and B, beginning from point A). So, he turns back and retraces his steps in the direction toward the campsite and finds the box lying on the path at some point D only 1.2 km away from point C (see Figure 2.6(b)). What is his displacement vector D⃗ AD when he finds the box at point D? What is his displacement vector D⃗ DB from point D to the hole? We have already established that at rest point C his displacement vector is D⃗ AC=0.75. Starting at point C, he walks southwest (toward the campsite), which means his new displacement vector D⃗ CD from point C to point D is antiparallel to D⃗ AB. Its magnitude |D⃗ CD| is DCD = 1.2 km = 0.2 DAB, so his second displacement vector is D⃗ CD = −0.2D⃗ AB. His total displacement D⃗ AD relative to the campsite is the vector sum of the two displacement vectors: vector D⃗ AC (from the campsite to the rest point) and vector D⃗ CD (from the rest point to the point where he finds his box):



The vector sum of two (or more) vectors is called the resultant vector or, for short, the resultant. When the vectors on the right-hand-side of Equation 2.3 are known, we can find the resultant D⃗ AD as follows:



When your friend finally reaches the pond at B, his displacement vector D⃗ AB from point A is the vector sum of his displacement vector D⃗ AD from point A to point D and his displacement vector D⃗ DB from point D to the fishing hole: D⃗ AB = D⃗ AD+D⃗ DB (see Figure 2.6(c)). This means his displacement vector D⃗ DB is the difference of two vectors:



Notice that a difference of two vectors is nothing more than a vector sum of two vectors because the second term in Equation 2.5 is vector −D⃗ AD (which is antiparallel to D⃗ AD). When we substitute Equation 2.4 into Equation 2.5, we obtain the second displacement vector:



This result means your friend walked DDB = 0.45 DAB = 0.45(6.0km) = 2.7 km from the point where he finds his tackle box to the fishing hole.

When vectors A⃗  and B⃗  lie along a line (that is, in one dimension), such as in the camping example, their resultant R⃗ =A⃗ +B⃗  and their difference D⃗ = A⃗ −B⃗  both lie along the same direction. We can illustrate the addition or subtraction of vectors by drawing the corresponding vectors to scale in one dimension, as shown in Figure 2.7.

To illustrate the resultant when A⃗  and B⃗  are two parallel vectors, we draw them along one line by placing the origin of one vector at the end of the other vector in head-to-tail fashion (see Figure 2.7(b)). The magnitude of this resultant is the sum of their magnitudes: R = A + B. The direction of the resultant is parallel to both vectors. When vector A⃗  is antiparallel to vector B⃗ , we draw them along one line in either head-to-head fashion (Figure 2.7(c)) or tail-to-tail fashion. The magnitude of the vector difference, then, is the absolute value D = |A−B| of the difference of their magnitudes. The direction of the difference vector D⃗  is parallel to the direction of the longer vector.

In general, in one dimension — as well as in higher dimensions, such as in a plane or in space — we can add any number of vectors and we can do so in any order because the addition of vectors is commutative:



and associative:



Moreover, multiplication by a scalar is distributive:



We used the distributive property in Equation 2.4 and Equation 2.6.

When adding many vectors in one dimension, it is convenient to use the concept of a unit vector. A unit vector, which is denoted by a letter symbol with a hat, such as uˆ, has a magnitude of one and does not have any physical unit so that |uˆ| ≡ u =1. The only role of a unit vector is to specify direction. For example, instead of saying vector D⃗ AB has a magnitude of 6.0 km and a direction of northeast, we can introduce a unit vector uˆ that points to the northeast and say succinctly that D⃗ AB = (6.0km)uˆ = (6.0km). Then the southwesterly direction is simply given by the unit vector −uˆ. In this way, the displacement of 6.0 km in the southwesterly direction is expressed by the vector:



A Ladybug Walker

A long measuring stick rests against a wall in a physics laboratory with its 200-cm end at the floor. A ladybug lands on the 100-cm mark and crawls randomly along the stick. It first walks 15 cm toward the floor, then it walks 56 cm toward the wall, then it walks 3 cm toward the floor again. Then, after a brief stop, it continues for 25 cm toward the floor and then, again, it crawls up 19 cm toward the wall before coming to a complete rest (Figure 2.8). Find the vector of its total displacement and its final resting position on the stick.


If we choose the direction along the stick toward the floor as the direction of unit vector uˆ, then the direction toward the floor is +uˆ and the direction toward the wall is −uˆ. The ladybug makes a total of five displacements:


The total displacement D⃗  is the resultant of all its displacement vectors.

Figure 2.8 Five displacements of the ladybug. Note that in this schematic drawing, magnitudes of displacements are not drawn to scale. (credit “ladybug”: modification of work by “Persian Poet Gal”/Wikimedia Commons)


The resultant of all the displacement vectors is:


In this calculation, we use the distributive law given by Equation 2.9. The result reads that the total displacement vector points away from the 100-cm mark (initial landing site) toward the end of the meter stick that touches the wall. The end that touches the wall is marked 0 cm, so the final position of the ladybug is at the (100 – 32)cm = 68-cm mark.


A cave diver enters a long underwater tunnel. When her displacement with respect to the entry point is 20 m, she accidentally drops her camera, but she doesn’t notice it missing until she is some 6 m farther into the tunnel. She swims back 10 m but cannot find the camera, so she decides to end the dive. How far from the entry point is she? Taking the positive direction out of the tunnel, what is her displacement vector relative to the entry point?

Algebra of Vectors in Two Dimensions

When vectors lie in a plane—that is, when they are in two dimensions—they can be multiplied by scalars, added to other vectors, or subtracted from other vectors in accordance with the general laws expressed by Equation 2.1, Equation 2.2, Equation 2.7, and Equation 2.8. However, the addition rule for two vectors in a plane becomes more complicated than the rule for vector addition in one dimension. We have to use the laws of geometry to construct resultant vectors, followed by trigonometry to find vector magnitudes and directions. This geometric approach is commonly used in navigation (Figure 2.9). In this section, we need to have at hand two rulers, a triangle, a protractor, a pencil, and an eraser for drawing vectors to scale by geometric constructions.

Figure 2.9 In navigation, the laws of geometry are used to draw resultant displacements on nautical maps.

For a geometric construction of the sum of two vectors in a plane, we follow the parallelogram rule. Suppose two vectors A⃗  and B⃗  are at the arbitrary positions shown in Figure 2.10. Translate either one of them in parallel to the beginning of the other vector, so that after the translation, both vectors have their origins at the same point. Now, at the end of vector A⃗  we draw a line parallel to vector B⃗  and at the end of vector B⃗  we draw a line parallel to vector A⃗  (the dashed lines in Figure 2.10). In this way, we obtain a parallelogram. From the origin of the two vectors we draw a diagonal that is the resultant R⃗  of the two vectors: R⃗ = A⃗ +B⃗  (Figure 2.10(a)). The other diagonal of this parallelogram is the vector difference of the two vectors D⃗ = A⃗ −B⃗ , as shown in Figure 2.10(b). Notice that the end of the difference vector is placed at the end of vector A⃗ .

Figure 2.10 The parallelogram rule for the addition of two vectors. Make the parallel translation of each vector to a point where their origins (marked by the dot) coincide and construct a parallelogram with two sides on the vectors and the other two sides (indicated by dashed lines) parallel to the vectors. (a) Draw the resultant vector R⃗  along the diagonal of the parallelogram from the common point to the opposite corner. Length R of the resultant vector is not equal to the sum of the magnitudes of the two vectors. (b) Draw the difference vector D⃗ = A⃗ −B⃗  along the diagonal connecting the ends of the vectors. Place the origin of vector D⃗  at the end of vector B⃗  and the end (arrowhead) of vector D⃗  at the end of vector A⃗ . Length D of the difference vector is not equal to the difference of magnitudes of the two vectors.

It follows from the parallelogram rule that neither the magnitude of the resultant vector nor the magnitude of the difference vector can be expressed as a simple sum or difference of magnitudes A and B, because the length of a diagonal cannot be expressed as a simple sum of side lengths. When using a geometric construction to find magnitudes |R⃗ | and |D⃗ |, we have to use trigonometry laws for triangles, which may lead to complicated algebra. There are two ways to circumvent this algebraic complexity. One way is to use the method of components, which we examine in the next section. The other way is to draw the vectors to scale, as is done in navigation, and read approximate vector lengths and angles (directions) from the graphs. In this section we examine the second approach.

If we need to add three or more vectors, we repeat the parallelogram rule for the pairs of vectors until we find the resultant of all of the resultants. For three vectors, for example, we first find the resultant of vector 1 and vector 2, and then we find the resultant of this resultant and vector 3. The order in which we select the pairs of vectors does not matter because the operation of vector addition is commutative and associative (see Equation 2.7 and Equation 2.8). Before we state a general rule that follows from repetitive applications of the parallelogram rule, let’s look at the following example.

Suppose you plan a vacation trip in Florida. Departing from Tallahassee, the state capital, you plan to visit your uncle Joe in Jacksonville, see your cousin Vinny in Daytona Beach, stop for a little fun in Orlando, see a circus performance in Tampa, and visit the University of Florida in Gainesville. Your route may be represented by five displacement vectors A⃗ , B⃗ , C⃗ , D⃗ , and E⃗ , which are indicated by the red vectors in Figure 2.11. What is your total displacement when you reach Gainesville? The total displacement is the vector sum of all five displacement vectors, which may be found by using the parallelogram rule four times. Alternatively, recall that the displacement vector has its beginning at the initial position (Tallahassee) and its end at the final position (Gainesville), so the total displacement vector can be drawn directly as an arrow connecting Tallahassee with Gainesville (see the green vector in Figure 2.11). When we use the parallelogram rule four times, the resultant R⃗  we obtain is exactly this green vector connecting Tallahassee with Gainesville: R⃗ = A⃗ +B⃗ +C⃗ +D⃗ +E⃗ .

Figure 2.11 When we use the parallelogram rule four times, we obtain the resultant vector R⃗ = A⃗ +B⃗ +C⃗ +D⃗ +E⃗ , which is the green vector connecting Tallahassee with Gainesville.

Drawing the resultant vector of many vectors can be generalized by using the following tail-to-head geometric construction. Suppose we want to draw the resultant vector R⃗  of four vectors A⃗ , B⃗ , C⃗ , and D⃗  (Figure 2.12(a)). We select any one of the vectors as the first vector and make a parallel translation of a second vector to a position where the origin (“tail”) of the second vector coincides with the end (“head”) of the first vector. Then, we select a third vector and make a parallel translation of the third vector to a position where the origin of the third vector coincides with the end of the second vector. We repeat this procedure until all the vectors are in a head-to-tail arrangement like the one shown in Figure 2.12. We draw the resultant vector R⃗  by connecting the origin (“tail”) of the first vector with the end (“head”) of the last vector. The end of the resultant vector is at the end of the last vector. Because the addition of vectors is associative and commutative, we obtain the same resultant vector regardless of which vector we choose to be first, second, third, or fourth in this construction.

Figure 2.12 Tail-to-head method for drawing the resultant vector R⃗ =A⃗ +B⃗ +C⃗ +D⃗ . (a) Four vectors of different magnitudes and directions. (b) Vectors in (a) are translated to new positions where the origin (“tail”) of one vector is at the end (“head”) of another vector. The resultant vector is drawn from the origin (“tail”) of the first vector to the end (“head”) of the last vector in this arrangement.


Geometric Construction of the Resultant

The three displacement vectors A⃗ , B⃗ , and C⃗  in Figure 2.13 are specified by their magnitudes A = 10.0, B = 7.0, and C = 8.0, respectively, and by their respective direction angles with the horizontal direction α=35°, β=−110°, and γ=30°. The physical units of the magnitudes are centimeters. Choose a convenient scale and use a ruler and a protractor to find the following vector sums: (a) R⃗ = A⃗ +B⃗ , (b) D⃗ = A⃗ −B⃗ , and (c) S⃗ = A⃗ −3B⃗ +C⃗ .

Figure 2.13 Vectors used in Example 2.2 and in the Check Your Understanding feature that follows.


In geometric construction, to find a vector means to find its magnitude and its direction angle with the horizontal direction. The strategy is to draw to scale the vectors that appear on the right-hand side of the equation and construct the resultant vector. Then, use a ruler and a protractor to read the magnitude of the resultant and the direction angle. For parts (a) and (b) we use the parallelogram rule. For (c) we use the tail-to-head method.


For parts (a) and (b), we attach the origin of vector B⃗  to the origin of vector A⃗ , as shown in Figure 2.14, and construct a parallelogram. The shorter diagonal of this parallelogram is the sum A⃗ +B⃗ . The longer of the diagonals is the difference A⃗ −B⃗ . We use a ruler to measure the lengths of the diagonals, and a protractor to measure the angles with the horizontal. For the resultant R⃗ , we obtain R = 5.8 cm and θR ≈ 0°. For the difference D⃗ , we obtain D = 16.2 cm and θD=49.3°, which are shown in Figure 2.14.

Figure 2.14 Using the parallelogram rule to solve (a) (finding the resultant, red) and (b) (finding the difference, blue).

For (c), we can start with vector −3B⃗  and draw the remaining vectors tail-to-head as shown in Figure 2.15. In vector addition, the order in which we draw the vectors is unimportant, but drawing the vectors to scale is very important. Next, we draw vector S⃗  from the origin of the first vector to the end of the last vector and place the arrowhead at the end of S⃗ . We use a ruler to measure the length of S⃗ , and find that its magnitude is S = 36.9 cm. We use a protractor and find that its direction angle is θS=52.9°. This solution is shown in Figure 2.15.

Figure 2.15 Using the tail-to-head method to solve (c) (finding vector S⃗ , green).


Using the three displacement vectors A⃗ , B⃗ , and F⃗  in Figure 2.13, choose a convenient scale, and use a ruler and a protractor to find vector G⃗  given by the vector equation G⃗ = A⃗ +2B⃗ −F⃗ .

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