FP3.5 - Vectors
- Syllabus
- 2019
- Topic
- —
- Level
- A2
The vector product a×b is a vector perpendicular to both a and b. Its direction follows the right-hand orientation, while its magnitude records the area scale generated by the two vectors:∣a×b∣=∣a∣∣b∣sinθ,where 0≤θ≤π is the angle between them.
a×b=a2b3−a3b2a3b1−a1b3a1b2−a2b1
| Quantity | Vector expression | Geometric meaning |
|---|---|---|
| a×b | component formula above | Perpendicular vector; reversing order reverses its direction. |
| ∣a×b∣ | magnitude of the cross product | Area of the parallelogram on a,b. |
| 21∣a×b∣ | half the magnitude | Area of the triangle on the same two sides. |
| a⋅(b×c) | scalar triple product | Signed volume scale of a parallelepiped. |
| ∣a⋅(b×c)∣ | absolute triple product | Volume of the parallelepiped; divide by 6 for the corresponding tetrahedron. |
Order matters: b×a=−(a×b), whereas cyclic changes leave a scalar triple product unchanged. A zero cross product means the two non-zero vectors are parallel. A zero scalar triple product means the three vectors are coplanar, because the third vector has no component perpendicular to the plane of the first two.
Let a=(1,2,−1) and b=(3,0,2). Thena×b=(4,−5,−6),∣a×b∣=77.The triangle with adjacent sides a and b has area 77/2. If c=(0,1,1), then(a×b)⋅c=−11,so the parallelepiped volume is 11; the sign records orientation, not a negative physical volume.
A calculated cross product should satisfy (a×b)⋅a=0 and (a×b)⋅b=0. These two dot-product checks catch most component or sign errors before the result is used as a normal or area vector.
Do not treat the cross product as commutative, and do not use the signed scalar triple product directly as a volume. For a triangle use half the parallelogram area; for a tetrahedron use one sixth of the parallelepiped volume. Cross products here are three-dimensional.
A vector equation separates position from direction. A line through the point with position vector a and non-zero direction b may be writtenr=a+λbor equivalently(r−a)×b=0.The second form says exactly that the displacement from the fixed point is parallel to the line direction.
| Problem | Construction |
|---|---|
| Distance from point P to plane through A with normal n | d=∣n∣∣AP⋅n∣ |
| Line of intersection of non-parallel planes | Direction n1×n2; find one point satisfying both plane equations. |
| Shortest distance between skew lines r=a1+λb1 and r=a2+μb2 | d=∣b1×b2∣∣(a2−a1)⋅(b1×b2)∣ |
| Distance between parallel lines with common direction b | d=∣b∣∣(a2−a1)×b∣ |
Each distance formula is a projection. For a point and plane, the displacement is projected onto the unit normal. For skew lines, b1×b2 is perpendicular to both directions, so projecting any joining displacement onto this common normal gives the fixed perpendicular separation.
For the plane 2x−y+2z=6 and point P=(1,1,1), the normal is n=(2,−1,2). Substitution gives the signed residual 2−1+2−6=−3, sod=22+(−1)2+22∣−3∣=1.The absolute value is essential because distance is non-negative.
Forℓ1:r=λ(1,0,1),ℓ2:r=(0,1,0)+μ(0,1,1),the common normal is (1,0,1)×(0,1,1)=(−1,−1,1). With joining vector (0,1,0),d=3∣(0,1,0)⋅(−1,−1,1)∣=31.Solving the coordinate equations confirms the lines do not intersect, so the skew formula applies.
For two plane equations, first cross their normals to obtain the intersection-line direction. Then choose one coordinate conveniently and solve the two simultaneous linear equations for a point. Substitute the final parametric line into both plane equations: both identities must hold for every parameter value.
The skew-line denominator is zero for parallel directions, so use the parallel-line formula instead. A zero scalar triple product gives zero separation but does not by itself distinguish intersecting from coincident/parallel cases; classify the directions and solve for intersection. Direction vectors and normals may be rescaled by any non-zero constant without changing the geometry.
A plane is fixed by one point and two independent in-plane directions, or by one point and a non-zero normal. These descriptions produce equivalent parametric, vector-normal and Cartesian equations; converting between them reveals the geometry needed for intersections and angles.
| Form | Equation | Meaning |
|---|---|---|
| Parametric | r=a+sb+tc | Point a plus two non-parallel directions in the plane. |
| Normal | r⋅n=p | n is perpendicular to the plane and p=a⋅n. |
| Point-normal | (r−a)⋅n=0 | Every in-plane displacement from A is perpendicular to n. |
| Cartesian | Ax+By+Cz=D | Normal n=(A,B,C) and D=p. |
From a parametric form, calculate n=b×c and then p=a⋅n. From a Cartesian form, read off the normal and find any convenient point satisfying the equation; two independent vectors perpendicular to the normal may then serve as parametric directions.
A plane through A=(1,−1,2) with directions b=(1,2,0) and c=(0,1,1) hasn=b×c=(2,−1,1).Since a⋅n=2+1+2=5, its normal and Cartesian forms arer⋅(2,−1,1)=5,qquad2x−y+z=5.Substituting A and both direction displacements verifies the conversion.
If three non-collinear points A,B,C define a plane, use AB and AC as the two directions. Their cross product is a normal. If the cross product is zero, the points are collinear and do not determine a unique plane.
The acute angle θ between two planes is the acute angle between their normals:cosθ=∣n1∣∣n2∣∣n1⋅n2∣,0≤θ≤2π.The absolute value selects the acute angle because reversing a normal does not change its plane.
In r⋅n=p, p is a scalar, not necessarily the perpendicular distance from the origin; that distance is ∣p∣/∣n∣. The two parametric directions must be independent. Equivalent plane equations may differ by any non-zero scalar multiple, so compare all coefficients together rather than term by term.