Three-dimensional geometry
A dot on a sheet of paper needs only two numbers to pin it down — its distance east and its distance north of some origin. But a fly buzzing around a room, or a satellite orbiting the Earth, needs a third number: height. Three-dimensional geometry is the coordinate toolkit for exactly that upgrade — locating any point in space by an ordered triple once three mutually perpendicular axes meet at an origin. This ISC Class 11 Section-B unit builds only what coordinates alone can give: the octants space is carved into, the distance between two points in space, and the section formula for a point dividing a segment in a given ratio. No vectors, no direction cosines — those wait for Class XII. Everything here is the 2-D coordinate geometry you already know, with one careful extra coordinate carried through every formula.
Three mutually perpendicular axes through an origin locate any point in space as an ordered triple , and every 2-D coordinate formula — distance, section, mid-point, centroid — extends by simply adding the matching -term.
The core idea
Axes, planes, octants. The -, - and -axes are mutually perpendicular lines through a common origin . Each pair of axes spans a coordinate plane: the -plane is every point with , the -plane is , and the -plane is . These three planes slice all of space into eight octants, distinguished purely by the signs of , , — the familiar positive quadrant of 2-D work becomes the octant where all three coordinates are positive. A point is written , where , , are its signed perpendicular distances from the -, -, and -planes respectively. Compare this with the plane: there, a point needed only its distances from two axes; here, a third perpendicular measurement — height above or below the -plane — is unavoidable, because the room a fly buzzes around genuinely has three independent directions, not two. The axes themselves are simply the three edges of a corner of a room meeting at the origin, each at right angles to the other two, and the coordinate planes are the three walls-plus-floor meeting at that corner. Just as the sign of and told you which quadrant a 2-D point sat in, the signs of , , together tell you which of the eight octants a 3-D point sits in. There is no separate name to memorise for each octant beyond the sign pattern itself — for instance has , so it sits in the octant where the first and third coordinates are positive and the second is negative, and no two octants share the same sign pattern.
Distance formula. For and ,
where: is the straight-line distance, and each squared term is the change in one coordinate. Setting at the origin gives the special case .
Section formula. If divides segment internally in the ratio , then
where: is read as " parts near , parts near " — multiplies 's coordinates and multiplies 's. For external division, flip the sign of the terms (equivalently use ratio ). Setting gives the mid-point, , and applying the formula to a triangle's median (ratio ) gives its centroid, .
The goal is to show that the 3-D distance between and is by applying the ordinary 2-D distance formula twice and the Pythagoras theorem once, so that the whole 3-D result rests on tools already familiar from plane coordinate geometry.
Step 1. Drop straight down onto the plane through parallel to the -plane, landing at the point — same and as , same as . The segment is vertical, of length , and it is perpendicular to the plane , hence perpendicular to every segment lying in that plane, including .
Step 2. Both and share the coordinate , so they lie in the same plane parallel to the -plane, and within that plane the problem is purely 2-D. The ordinary plane distance formula gives .
Step 3. Triangle has a right angle at , because is perpendicular to the plane containing . By the Pythagoras theorem, .
Step 4. Take the square root of both sides: . The 3-D formula is exactly the 2-D one with a third squared term appended, because the vertical drop from to is always perpendicular to the horizontal plane through and , whatever the coordinates.
Worked example
Show that the points , , are the vertices of a right-angled isosceles triangle.
Step 1. Apply the distance formula to each pair. .
Step 2. Similarly, , and .
Step 3. Compare the three squared lengths. Since , sides and are equal, so is isosceles. Also , so by the converse of the Pythagoras theorem the angle opposite — angle — is a right angle.
Answer: is right-angled at and isosceles, with and .
Competitive stretch
Find the point dividing and internally in the ratio . Here , so , , . The point is — the same section formula that produced the vertical drop in the derivation above, now used to split a segment rather than measure it. Notice each coordinate is computed independently by the identical rule: multiply the far point's coordinate by , the near point's by , add, and divide by — there is nothing extra to learn for the -coordinate once the - and -coordinates are understood.
Common traps
- Dropping the -term out of habit. Students fluent in 2-D formulas sometimes forget the third coordinate — check that , and all appear in every step.
- Misreading the octant from the coordinate signs. Three coordinates give eight sign combinations, not four; one careless sign flip puts a point in the wrong octant.
- Swapping and in the section formula. The formula is not symmetric in and : pairs with 's coordinates, with 's, in the order the ratio was written.
- Reaching for vectors or direction cosines. This Section-B unit is worked entirely with coordinates; direction cosines, direction ratios and vector equations belong to Class XII.
Ask the tutor: If keeping track of all three coordinates through a distance or section-formula calculation feels fiddly, ask the AI tutor to walk through one coordinate — , then , then — at a time.
Why does the 3-D distance formula just add one more squared term instead of something more complicated?
Because the extra dimension is perpendicular to the other two, not tangled up with them. Dropping a point straight down onto the plane of the other point turns the 3-D problem into an ordinary 2-D distance plus one vertical segment, and those two pieces meet at a right angle by construction. The Pythagoras theorem then combines them by squaring and adding — exactly the pattern the derivation walks through. Any number of mutually perpendicular directions would add in the same simple way.
Do I need to know direction cosines or vectors for this ISC Section-B chapter?
No. This unit — Section B, "Introduction to Three-Dimensional Geometry" — is built entirely from coordinates: axes, coordinate planes, octants, the distance formula and the section formula, including its mid-point and centroid special cases. Direction cosines, direction ratios, and the vector or Cartesian equations of lines and planes are Class XII tools and are outside this chapter's scope, even though they return to the same coordinate axes.
How is the 3-D section formula different from the 2-D version I already know?
It is not really different — it is the same formula with a -coordinate line added. You still compute and exactly as in the plane, and now also using the same and . The mid-point formula () and the centroid formula (from the median ratio) carry over the same way, just with a third coordinate averaged alongside the first two.