3D Geometry Concepts and Formulas

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Vocabulary flashcards covering core 3D geometry definitions, direction cosines, internal division, and line distances from the lecture notes.

Last updated 7:25 AM on 9/21/26
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7 Terms

1
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Direction Cosines (DCs) of Vector A\mathbf{A}

The ratios l=a∣A∣l = \frac{a}{|\mathbf{A}|}, m=b∣A∣m = \frac{b}{|\mathbf{A}|}, and n=c∣A∣n = \frac{c}{|\mathbf{A}|} for a vector A=ai+bj+ck\mathbf{A} = a\mathbf{i} + b\mathbf{j} + c\mathbf{k}, which satisfy the identity l2+m2+n2=1l^2 + m^2 + n^2 = 1 and can also be expressed as −l,−m,−n-l, -m, -n.

2
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Direction Angles Identity for Sine

The trigonometric identity sin⁡2(α)+sin⁡2(β)+sin⁡2(γ)=2\sin^2(\alpha) + \sin^2(\beta) + \sin^2(\gamma) = 2, where α\alpha, β\beta, and γ\gamma are the direction angles made by a line or vector with the coordinate axes.

3
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Internal Division Formula in 3D

The coordinates of point PP dividing the line segment between (x1,y1,z1)(x_1, y_1, z_1) and (x2,y2,z2)(x_2, y_2, z_2) internally in the ratio m:nm:n, given by (mx2+nx1m+n,my2+ny1m+n,mz2+nz1m+n)\left( \frac{mx_2 + nx_1}{m+n}, \frac{my_2 + ny_1}{m+n}, \frac{mz_2 + nz_1}{m+n} \right).

4
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Angle Between Two Lines (Direction Cosines)

The cosine of the angle θ\theta between two lines with direction cosines (l1,m1,n1)(l_1, m_1, n_1) and (l2,m2,n2)(l_2, m_2, n_2), given by cos⁡(θ)=l1l2+m1m2+n1n2\cos(\theta) = l_1 l_2 + m_1 m_2 + n_1 n_2.

5
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Angle Between Two Lines (Direction Ratios)

The cosine of the angle θ\theta between two lines with direction ratios DR1\mathbf{DR}_1 and DR2\mathbf{DR}_2, given by cos⁡(θ)=DR1⋅DR2∣DR1∣∣DR2∣\cos(\theta) = \frac{\mathbf{DR}_1 \cdot \mathbf{DR}_2}{|\mathbf{DR}_1| |\mathbf{DR}_2|}.

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Distance Between Parallel Lines

The shortest distance dd between two parallel lines r=a+λb\mathbf{r} = \mathbf{a} + \lambda \mathbf{b} and r=c+μb\mathbf{r} = \mathbf{c} + \mu \mathbf{b}, given by d=∣(c−a)×b∣∣b∣d = \frac{|(\mathbf{c} - \mathbf{a}) \times \mathbf{b}|}{|\mathbf{b}|}.

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Distance Between Skew Lines

The shortest distance dd between two non-parallel, non-intersecting lines r=a+λb\mathbf{r} = \mathbf{a} + \lambda \mathbf{b} and r=c+μd\mathbf{r} = \mathbf{c} + \mu \mathbf{d}, given by d=∣[a−c,b,d]∣∣b×d∣d = \frac{|[\mathbf{a} - \mathbf{c}, \mathbf{b}, \mathbf{d}]|}{|\mathbf{b} \times \mathbf{d}|}.