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Mathematics · Ch 11 — Three-Dimensional Geometry

Equation of a Line Through a Given Point and Parallel to Given Vector

11.3.1

Equation of a Line Through a Given Point and Parallel to Given Vector

Equation of a Line Through a Given Point and Parallel to a Given Vector

The fundamental problem is to find the equation of a line when we know one point it passes through and its direction. In three-dimensional space, a line is completely determined by a point on it and a vector parallel to it. This vector gives the line its orientation, while the point fixes its location.

Vector Form of the Equation

Let OO be the origin of the rectangular coordinate system. Let AA be the given point on the line, with position vector a⃗\vec{a}. Let b⃗\vec{b} be a given vector parallel to the line ll. Now consider any arbitrary point PP on the line ll, with position vector r⃗\vec{r}.

The vector AP→\overrightarrow{AP} is the vector from point AA to point PP. Since the line passes through AA and PP, and the line is parallel to b⃗\vec{b}, the vector AP→\overrightarrow{AP} must also be parallel to b⃗\vec{b}. Therefore, there exists some real number λ\lambda such that:

AP→=λb⃗\overrightarrow{AP} = \lambda \vec{b}

But we can express AP→\overrightarrow{AP} in terms of position vectors:

AP→=OP→−OA→=r⃗−a⃗\overrightarrow{AP} = \overrightarrow{OP} - \overrightarrow{OA} = \vec{r} - \vec{a}

Equating these two expressions gives:

r⃗−a⃗=λb⃗\vec{r} - \vec{a} = \lambda \vec{b}

Rearranging, we obtain the vector equation of the line:

r⃗=a⃗+λb⃗\vec{r} = \vec{a} + \lambda \vec{b}

Here, λ\lambda is a parameter that can take any real value. For each distinct value of λ\lambda, this equation gives the position vector of a different point PP on the line. When λ=0\lambda = 0, we get the given point AA itself.

Vector equation of a line through point a⃗\vec{a} parallel to b⃗\vec{b}:

r⃗=a⃗+λb⃗,λ∈R\vec{r} = \vec{a} + \lambda \vec{b}, \quad \lambda \in \mathbb{R}

Note

If b⃗=ai^+bj^+ck^\vec{b} = a\hat{i} + b\hat{j} + c\hat{k}, then the numbers aa, bb, cc are called the direction ratios of the line. Conversely, if aa, bb, cc are the direction ratios of a line, then the vector b⃗=ai^+bj^+ck^\vec{b} = a\hat{i} + b\hat{j} + c\hat{k} is parallel to that line. Do not confuse b⃗\vec{b} with its magnitude ∣b⃗∣|\vec{b}|.

Cartesian Form of the Equation

We now derive the Cartesian (or scalar) form from the vector equation. Let the coordinates of the given point AA be (x1,y1,z1)(x_1, y_1, z_1). Let the direction ratios of the line be aa, bb, cc. Let the coordinates of any point PP on the line be (x,y,z)(x, y, z).

Then we can write the position vectors as:

r⃗=xi^+yj^+zk^\vec{r} = x\hat{i} + y\hat{j} + z\hat{k}

a⃗=x1i^+y1j^+z1k^\vec{a} = x_1\hat{i} + y_1\hat{j} + z_1\hat{k}

b⃗=ai^+bj^+ck^\vec{b} = a\hat{i} + b\hat{j} + c\hat{k}

Substituting these into the vector equation r⃗=a⃗+λb⃗\vec{r} = \vec{a} + \lambda \vec{b}:

xi^+yj^+zk^=(x1i^+y1j^+z1k^)+λ(ai^+bj^+ck^)x\hat{i} + y\hat{j} + z\hat{k} = (x_1\hat{i} + y_1\hat{j} + z_1\hat{k}) + \lambda(a\hat{i} + b\hat{j} + c\hat{k})

xi^+yj^+zk^=(x1+λa)i^+(y1+λb)j^+(z1+λc)k^x\hat{i} + y\hat{j} + z\hat{k} = (x_1 + \lambda a)\hat{i} + (y_1 + \lambda b)\hat{j} + (z_1 + \lambda c)\hat{k}

Equating the coefficients of i^\hat{i}, j^\hat{j}, and k^\hat{k} on both sides gives the parametric equations of the line:

x=x1+λax = x_1 + \lambda a

y=y1+λby = y_1 + \lambda b

z=z1+λcz = z_1 + \lambda c

These are called parametric equations because the coordinates xx, yy, zz are expressed in terms of the parameter λ\lambda.

›Proof

Derivation of the Cartesian equation by eliminating λ\lambda:

From the parametric equations, we can solve for λ\lambda in each case:

From x=x1+λax = x_1 + \lambda a: λ=x−x1a\lambda = \frac{x - x_1}{a}, provided a≠0a \neq 0

From y=y1+λby = y_1 + \lambda b: λ=y−y1b\lambda = \frac{y - y_1}{b}, provided b≠0b \neq 0

From z=z1+λcz = z_1 + \lambda c: λ=z−z1c\lambda = \frac{z - z_1}{c}, provided c≠0c \neq 0

Since λ\lambda is the same in all three equations, we equate these expressions:

x−x1a=y−y1b=z−z1c\frac{x - x_1}{a} = \frac{y - y_1}{b} = \frac{z - z_1}{c}

This is the Cartesian equation of the line. …

Figure 11.3A line l in space passing through point A with position vector a, parallel to direction vector b, and an arbitrary point P with position vector r drawn from the origin of the X, Y, Z axes.
Fig. 11.3 — A line l in space passing through point A with position vector a, parallel to direction vector b, and an arbitrary point P with position vector r drawn from the origin of the X, Y, Z axes.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

Fig 11.3 is the foundational picture for the entire topic of lines in 3D. It shows a standard rectangular coordinate system with axes XX, YY, ZZ meeting at the origin OO. The key object is a straight line ll (drawn in indigo, with arrows on both ends to show it extends infinitely in both directions) that does not pass through OO. Instead, it sits somewhere in space, offset from the origin.

Two points are marked on this line. Point AA is a fixed, given point on ll. Its position vector from OO is labelled a⃗=OA→\vec{a} = \overrightarrow{OA}. Point PP is an arbitrary (any) point on the same line, with position vector r⃗=OP→\vec{r} = \overrightarrow{OP}. The figure also shows a separate arrow labelled b⃗\vec{b}, drawn floating above the line (not attached to OO or AA). This arrow represents the direction vector of the line — it is parallel to ll and gives the line its orientation in space.

The physical idea is simple: to describe every point on ll, you start at AA and move some distance along the direction b⃗\vec{b}. The vector from AA to PP is AP→=r⃗−a⃗\overrightarrow{AP} = \vec{r} - \vec{a}. Since AP→\overrightarrow{AP} lies along the line, it must be parallel to b⃗\vec{b}. That means AP→\overrightarrow{AP} is a scalar multiple of b⃗\vec{b}: r⃗−a⃗=λb⃗\vec{r} - \vec{a} = \lambda \vec{b}, where λ\lambda is a real number (the parameter). Rearranging gives the central result.

r⃗=a⃗+λb⃗\vec{r} = \vec{a} + \lambda \vec{b}

This is the vector equation of a line through point AA (position a⃗\vec{a}) parallel to direction b⃗\vec{b}. Every value of λ\lambda gives a different point PP on ll: λ=0\lambda = 0 gives AA itself, λ>0\lambda > 0 gives points on one side of AA, and λ<0\lambda < 0 gives points on the other side.

From this vector form, the textbook derives the Cartesian form. If A=(x1,y1,z1)A = (x_1, y_1, z_1) and b⃗=ai^+bj^+ck^\vec{b} = a\hat{i} + b\hat{j} + c\hat{k} (where a,b,ca, b, c are the direction ratios), then equating components of r⃗=xi^+yj^+zk^\vec{r} = x\hat{i} + y\hat{j} + z\hat{k} with a⃗+λb⃗\vec{a} + \lambda\vec{b} gives the parametric equations:

x=x1+λa,y=y1+λb,z=z1+λcx = x_1 + \lambda a, \quad y = y_1 + \lambda b, \quad z = z_1 + \lambda c

Eliminating λ\lambda yields the symmetric Cartesian form:

x−x1a=y−y1b=z−z1c\frac{x - x_1}{a} = \frac{y - y_1}{b} = \frac{z - z_1}{c} …