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Revision: Mathematics >> Three-dimensional Geometry CUET (UG) Three-dimensional Geometry

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Definitions [6]

Definition: Co-ordinate Axes

The two mutually perpendicular number lines intersecting each other at their zeroes are called rectangular axes or coordinate axes, or axes of reference. 

Definition: Co-ordinates

The position of a point in a plane is expressed by a pair of numbers, one concerning the x-axis and the other concerning the y-axis. called co-ordinates. 

  • x → distance from y-axis (abscissa)

  • y → distance from x-axis (ordinate)

Definition: Direction Angles

If a directed line makes angles \[\alpha\], \[\beta\], and \[\gamma\] with the positive x-, y-, and z-axes respectively, then these are called the direction angles of the line.

Definition: Direction Cosines

The cosines of these angles are called the direction cosines of the line.

\[l = \cos \alpha, \quad m = \cos \beta, \quad n = \cos \gamma\]

So, the direction cosines are written as (l, m, n).

\[ \boxed{\,l^{2} + m^{2} + n^{2} = 1\,} \]

Definition: Direction Ratios

Any three numbers proportional to the direction cosines of a line are called the direction ratios of the line.

If (a, b, c) are direction ratios, then:

\[\frac{l}{a} = \frac{m}{b} = \frac{n}{c}\]
 
\[ \boxed{\,a : b : c = l : m : n\,} \]
Definition: Linear Equation

An equation of the form ax + by + c = 0 represents a straight line and is known as a linear equation.

Formulae [11]

Formula: Foundation of Coordinate Geometry
Sr. No. Name Condition Formula
i. Distance Formula Two points P(x₁, y₁), Q(x₂, y₂) \[\mathrm{d(PQ)}=\sqrt{\left(x_{2}-x_{1}\right)^{2}+\left(y_{2}-y_{1}\right)^{2}}\]
a. Internal Division P divides AB in the ratio m: n \[\mathrm{P\equiv\left(\frac{mx_{2}+nx_{1}}{m+n},\frac{my_{2}+ny_{1}}{m+n}\right)}\]
b. Midpoint Formula P is the midpoint of AB \[\mathrm{P}\equiv\left(\frac{x_{1}+x_{2}}{2},\frac{y_{1}+y_{2}}{2}\right)\]
c. External Division P divides AB externally in m: n \[\mathrm{P\equiv\left(\frac{mx_{2}-nx_{1}}{m-n},\frac{my_{2}-ny_{1}}{m-n}\right)}\]
iii. Centroid Formula Triangle with vertices A, B, C \[\left(\frac{x_1+x_2+x_3}{3},\frac{y_1+y_2+y_3}{3}\right)\]
Formula: For Sine of the Angle

If the direction ratios are \[(a_1, b_1, c_1)\] and \[(a_2, b_2, c_2)\], then:

\[\sin \theta = \frac{\sqrt{(a_1b_2 - a_2b_1)^2 + (b_1c_2 - b_2c_1)^2 + (c_1a_2 - c_2a_1)^2}}{\sqrt{a_1^2 + b_1^2 + c_1^2} \sqrt{a_2^2 + b_2^2 + c_2^2}}\]
Formula: If Direction Ratios are Given

If the direction ratios of two lines are:

First line: \[(a_1, b_1, c_1)\]

Second line: \[(a_2, b_2, c_2)\]

then the cosine of the angle \[\theta\] between them is:

\[\cos \theta = \left| \frac{a_1a_2 + b_1b_2 + c_1c_2}{\sqrt{a_1^2 + b_1^2 + c_1^2} \sqrt{a_2^2 + b_2^2 + c_2^2}} \right|\]
Formula: If Direction Cosines are Given

If the direction cosines of the two lines are

\[(l_1, m_1, n_1)\] and \[(l_2, m_2, n_2)\], then:

\[\cos \theta = |l_1l_2 + m_1m_2 + n_1n_2|\]
Formula: Distance between Skew Lines

If the lines are \[ \vec{r} = \vec{a}_{1} + \lambda\vec{b}_{1} \] and \[ \vec{r} = \vec{a}_{2} + \mu\vec{b}_{2}, \]

then \[ \vec{a}_{1}, \vec{a}_{2} \] are position vectors of points on the lines and \[ \vec{b}_{1}, \vec{b}_{2} \] are their direction vectors.

Vector Form: 

\[\mathbf{d}=\left|\frac{(\overline{\mathbf{b}}_{1}\times\overline{\mathbf{b}}_{2}).(\overline{\mathbf{a}}_{2}-\overline{\mathbf{a}}_{1})}{\left|\overline{\mathbf{b}}_{1}\times\overline{\mathbf{b}}_{2}\right|}\right|\]

Cartesian Form:

\[\mathbf{d}=\left|\frac{ \begin{vmatrix} x_2-x_1 & y_2-y_1 & z_2-z_1 \\ \mathbf{a}_1 & \mathbf{b}_1 & \mathbf{c}_1 \\ \mathbf{a}_2 & \mathbf{b}_2 & \mathbf{c}_2 \end{vmatrix}}{\sqrt{\left(\mathbf{a}_1\mathbf{b}_2-\mathbf{a}_2\mathbf{b}_1\right)^2+\left(\mathbf{a}_1\mathbf{c}_2-\mathbf{a}_2\mathbf{c}_1\right)^2+\left(\mathbf{b}_1\mathbf{c}_2-\mathbf{b}_2\mathbf{c}_1\right)^2}}\right|\]

Formula: Distance between Parallel Lines

\[SD=\left|\frac{\left(a_{2}-a_{1}\right)\times b}{\left|b\right|}\right|\]

Formula: Slope & Intercept

From general form:

  • Slope (m) = −a / b
  • Y-intercept = −c / b
Formula: Angle between Line and Plane

Vector Form:

\[\sin\theta=\left|\frac{\overline{\mathbf{b}}.\overline{\mathbf{n}}}{\left|\overline{\mathbf{b}}\right|.\left|\overline{\mathbf{n}}\right|}\right|\]

Cartesian Form:

\[\mathrm{sin}\theta=\frac{\mathrm{aa}_{1}+\mathrm{bb}_{1}+\mathrm{cc}_{1}}{\sqrt{\mathrm{a}^{2}+\mathrm{b}^{2}+\mathrm{c}^{2}}\sqrt{\mathrm{a}_{1}^{2}+\mathrm{b}_{1}^{2}+\mathrm{c}_{1}^{2}}}\]

Formula: Angle between Two Planes

Vector Form:

\[\cos\theta=\left|\frac{\overline{\mathbf{n₁}}.\overline{\mathbf{n₂}}}{\left|\overline{\mathbf{n₁}}\right|.\left|\overline{\mathbf{n₂}}\right|}\right|\]

Cartesian Form:

\[\cos\theta=\left|\frac{\mathrm{a}_{1}\mathrm{a}_{2}+\mathrm{b}_{1}\mathrm{b}_{2}+\mathrm{c}_{1}\mathrm{c}_{2}}{\sqrt{\mathrm{a}_{1}^{2}+\mathrm{b}_{1}^{2}+\mathrm{c}_{1}^{2}}\sqrt{\mathrm{a}_{2}^{2}+\mathrm{b}_{2}^{2}+\mathrm{c}_{2}^{2}}}\right|\]

Formula: Distance of a Point from a Plane

Vector Form:

\[\mathbf{d}=\frac{\left|\left(\overline{\mathbf{a}}.\overline{\mathbf{n}}\right)-\mathbf{p}\right|}{\left|\overline{\mathbf{n}}\right|}\]

Cartesian Form:

\[\mathbf{d}=\left|\frac{\mathbf{a}x_{1}+\mathbf{b}y_{1}+\mathbf{c}z_{1}+\mathbf{d}}{\sqrt{\mathbf{a}^{2}+\mathbf{b}^{2}+\mathbf{c}^{2}}}\right|\]

Formula: Angle between Two Lines

Vector:

Angle between two lines: \[\cos\theta=\left|\frac{\mathbf{b}_{1}\cdot\mathbf{b}_{2}}{|\mathbf{b}_{1}||\mathbf{b}_{2}|}\right|\]

If two lines are perpendicular: b₁ · b₂ = 0

If two lines are parallel: b₁ = λb₂

Cartesian: 

\[\cos\theta=\frac{|a_{1}a_{2}+b_{1}b_{2}+c_{1}c_{2}|}{\sqrt{a_{1}^{2}+b_{1}^{2}+c_{1}^{2}}\sqrt{a_{2}^{2}+b_{2}^{2}+c_{2}^{2}}}\]

If two lines are perpendicular: a₁a₂ + b₁b₂ + c₁c₂ = 0

If two lines are parallel: \[\frac{a_1}{a_2}=\frac{b_1}{b_2}=\frac{c_1}{c_2}\]

Key Points

Key Points: Co-ordinate Geometry

Sign Convention

  • Right of y-axis → +x

  • Left of y-axis → −x

  • Above x-axis → +y

  • Below x-axis → −y

Standard Line Results

  • x = 0 → y-axis

  • y = 0 → x-axis

  • x = a → line parallel to the y-axis

  • y = b → line parallel to the x-axis

Quadrant Reminder

Quadrant Sign of (x, y)
I (+, +)
II (−, +)
III (−, −)
IV (+, −)
Key Points: Direction Cosines and Direction Ratios of a Line
  • Direction Cosines (DCs) of a line: \[(l, m, n) = (\cos \alpha, \cos \beta, \cos \gamma)\].

  • Main identity: \[l^2 + m^2 + n^2 = 1\].

  • Direction Ratios (DRs): Are proportional to DCs.

  • Relation between DRs and DCs: If DRs are (a, b, c), then DCs are proportional to (a, b, c) divided by \[\sqrt{a^2 + b^2 + c^2}\].

  • DRs for two points: For points \[P(x_1, y_1, z_1)\] and \[Q(x_2, y_2, z_2)\], DRs are \[(x_2 - x_1, y_2 - y_1, z_2 - z_1)\].

Key Points: Equation of a Line in Space
  • Through point \(\vec a\) and parallel to \(\vec b\): \(\vec r = \vec a + \lambda \vec b\).

  • Parametric form: \(x = x_1 + \lambda a,; y = y_1 + \lambda b,; z = z_1 + \lambda c\).

  • Cartesian form: \(\frac{x-x_1}{a} = \frac{y-y_1}{b} = \frac{z-z_1}{c}\).

Key Points: Angle Between Two Lines
  • The angle between two lines depends only on their directions.

  • If lines do not pass through the origin, imagine parallel lines through the origin.

  • The dot-product formula is the main method for solving these questions.

  • In symmetric form, denominators give direction ratios.

  • Zero dot product means perpendicular lines.

  • Proportional direction ratios mean parallel lines.

  • The required angle is generally the acute angle.

Key Points: Shortest Distance Between Two Lines
  • Intersecting lines: SD = 0

  • Parallel lines: \[SD = \frac{|(\vec{a}_2 - \vec{a}_1) \times \vec{b}|}{|\vec{b}|}\]

  • Skew lines: \[SD = \frac{|(\vec{a}_2 - \vec{a}_1) \cdot (\vec{b}_1 \times \vec{b}_2)|}{|\vec{b}_1 \times \vec{b}_2|}\]

Key Points: Equation of a Plane
Case Vector Form Cartesian Form
1. Normal form (given normal vector) \[\overline{\mathbf{r}}.\hat{\mathbf{n}}=\mathbf{p}\] ax + by + cz + d = 0
2. Through a point (x₁, y₁, z₁) \[\begin{bmatrix} \mathbf{\overline{r}}-\mathbf{\overline{a}} \end{bmatrix}.\mathbf{\overline{n}}=\mathbf{0}\] a(x−x₁) + b(y−y₁) + c(z−z₁) = 0
3. Through point + parallel to two vectors \[\begin{bmatrix} \overline{\mathbf{r}}\overline{\mathbf{b}}\overline{\mathbf{c}} \end{bmatrix}= \begin{bmatrix} \overline{\mathbf{a}}\overline{\mathbf{b}}\overline{\mathbf{c}} \end{bmatrix}\] \[\begin{vmatrix} x-x_1 & y-y_1 & z-z_1 \\ \mathbf{b}_1 & \mathbf{b}_2 & \mathbf{b}_3 \\ \mathbf{c}_1 & \mathbf{c}_2 & \mathbf{c}_3 \end{vmatrix}=0\]
4. Through three non-collinear points \[(\mathbf{r-a})\cdot[(\mathbf{b-a})\times(\mathbf{c-a})]=0\] \[\begin{vmatrix} x-x_1 & y-y_1 & z-z_1 \\ x_2-x_1 & y_2-y_1 & z_2-z_1 \\ x_3-x_1 & y_3-y_1 & z_3-z_1 \end{vmatrix}=0\]
5. Through the intersection of two planes \[\left(\overline{\mathbf{r}}.\overline{\mathbf{n}}_1-\mathbf{d}_1\right)+\lambda\left(\overline{\mathbf{r}}.\overline{\mathbf{n}}_2-\mathbf{d}_2\right)=0\] (a₁x + b₁y + c₁z + d₁) + λ(a₂x + b₂y + c₂z + d₂) = 0

Equation of a Plane in Intercept form:

\[\frac{x}{a}+\frac{y}{b}+\frac{z}{c}=1\]

Distance of the Plane from Origin is

\[d=\frac{1}{\sqrt{\frac{1}{a^{2}}+\frac{1}{b^{2}}+\frac{1}{c^{2}}}}\]

Key Points: Equations of Line in Different Forms
Form Formula
X-axis y = 0
Y-axis x = 0
Parallel to the X-axis y = b or y = -b
Parallel to the Y-axis x = a or x = -a
Slope-point form y − y₁ = m(x − x₁)
Two-point form \[\frac{y-y_{1}}{y_{1}-y_{2}}=\frac{x-x_{1}}{x_{1}-x_{2}}\]
Slope-intercept form y = mx + c
Intercept form \[\frac{x}{\mathrm{a}}+\frac{y}{\mathrm{b}}=1\]
Normal form x cosα + y sinα = p
Parametric form \[\frac{x-x_{1}}{\cos\theta}=\frac{y-y_{1}}{\sin\theta}=r\]

Position of a Point:

For line: ax₁ + by₁ + c

  • If ax₁ + by₁ + c = 0 → Point lies on the line
  • If ax₁ + by₁ + c < 0 → Point lies on one side (origin side)
  • If ax₁ + by₁ + c > 0 → Point lies on other side
Key Points: Coplanarity of Two Lines

Vector Form:

Condition for coplanarity of two lines:

Two lines r = a₁ + λb₁ and r = a₂ + μb₂ are coplanar if

(a₁ − a₂) · (b₁ × b₂) = 0

Equation of the plane containing both lines:

\[\left(\overline{\mathbf{r}}-\overline{\mathbf{a}_1}\right).\left(\overline{\mathbf{b}_1}\times\overline{\mathbf{b}_2}\right)=\mathbf{0}\] or \[\left(\overline{\mathbf{r}}-\overline{\mathbf{a}_2}\right).\left(\overline{\mathbf{b}_1}\times\overline{\mathbf{b}_2}\right)=\mathbf{0}\]

Cartesian Form:

\[\begin{vmatrix} x_2-x_1 & y_2-y_1 & z_2-z_1 \\ \mathbf{a}_1 & \mathbf{b}_1 & \mathbf{c}_1 \\ \mathbf{a}_2 & \mathbf{b}_2 & \mathbf{c}_2 \end{vmatrix}=0\]

Key Points: Condition for Parallelism and Perpendicularity

Condition for Perpendicularity:

\[\overline{\mathbf{b}}=\lambda\overline{\mathbf{n}}\], λ is a parameter

\[\frac{\mathbf{a}_{1}}{\mathbf{a}}=\frac{\mathbf{b}_{1}}{\mathbf{b}}=\frac{\mathbf{c}_{1}}{\mathbf{c}}\]

Condition for Parallelism:

The line is parallel to the plane, if

\[\overline{\mathbf{b}}.\overline{\mathbf{n}}=0\]

aa₁ + bb₁ + cc₁ = 0

Key Points: Vector and Cartesian Equations of a Line
Case Vector Form Cartesian Form (Symmetric Form)
1. Through a point + parallel to vector r = a + λb x = x₁ + lλ y = y₁ + mλ z = z₁ + nλ
2. Through two points r = a + λ(b − a) x − x₁ / (x₂ − x₁) = y − y₁ / (y₂ − y₁) = z − z₁ / (z₂ − z₁)
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