You might recall those arrows of a certain length from the highschool algebra, or you might have already tinkered with vectors in a 3D package where they seem to be used to denote points in space. We will only be dealing with 3D vectors, in the form

`[x, y, z]`

where `x`

, `y`

and `z`

are single-precision floating point numbers (basically decimals with limited precision – and it's good to always keep that in mind), that describe a *position offset*in space in the context of the corresponding axes. In MAXScript, they are represented by the Point3 value.

However, it's important not to treat vectors as a list of numbers or coordinates only – especially since they are not really point coordinates per se. And since showing beats telling every time, let's have a look at this, first of all:

What can we say about it? Well, for one, it is defined by two points. And yet, it's not acutally one vector, it doesn't matter that the point labels are the same. Actually, at each frame we see a different vector. It's not the labelling that defines a it, it's the direction and its length. The vectors on the following images are all identical:

You might have seen the concept described as a directed magnitude and while that's definitely more exact, I want you to think about the 3D vectors we will be using primarily as

*position offsets*.

What does it mean? Different things in different contexts:

- when used for point positions in world space, a vector describes the position offset from the scene origin,
- in local space it's a position offset from the center of the object's coordinate system,
- for a pair of points it's a direction and distance to get from one to the other,
- and sometimes, like for example with normal vectors, we care mostly only about the direction part.

And as vectors are position-less, i.e. you can move a vector all around and it's still the same vector, let's respect the convention of placing the starting point at the origin:

You might remember that adding vectors graphically amounts to sticking a starting point of one vector to the end point of the other one, optionally adding other vectors iteratively, and in the end connecting the starting point of the first one with the end point of the last one. The order is arbitrary and doesn't matter.

That's true and lends itself nicely to the notion of vectors as position offsets in space, but let's have a look at another way to look at it. As I've said before, I will stick to the convention of placing vector starting points at the origin, and I do that for a reason:

The difference from the previous image is that here all the vectors are placed so that they start at the

`[0,0]`

point. Instead of putting the other vector in the addition to the end of the first one, let's draw a thin dashed line. As you can see, for both vectors, the end point of the dashed line ends up in the same place, at the end of the diagonal of the parallelogram created by the vectors. This diagonal is the resulting vector.Try and move the vertex handles around, and you will see that when both the vectors are of the same magnitude (length), their sum is a vector that halves their angle. If one of them is bigger, it drags the resulting vector more towards itself.

When expressed numerically, matching pairs of coordinates are added together:

[1, 0, 5] + [-10, 2, 0] = [-9, 2, 5]What can you use that for?

- With more vectors of the same length, the resulting vector will point in their average direction (unless they cancel out each other).
- When their lengths are different, the result is a weighted average (used in weighted normals where small faces contribute a smaller amount).

Since the axis vectors come handy pretty often, there are predefined MAXScript globals

`x_axis`

, `y_axis`

and `z_axis`

that contain the values `[1,0,0]`

, `[0,1,0]`

and `[0,0,1]`

respectively.Vector subtraction follows exactly the same rules, only flipping the vector that's negated. For a pair of vectors, it helps to think about it as the other diagonal of the parallelogram, the one that connects the end points of the two vectors when they share the same starting point (which is true for example for all positions in space measured from the origin point). The direction of the resulting vector depends on whether we are subtracting

*A*from

*B*or

*B*from

*A*.

In the next example,

*A*is the vector that is subtracted from

*B*, and as such becomes the new 'origin' point for the resulting vector. Whenever you find yourself deciding what to subtract from what, ask yourself what you want to treat as the

*origin*– the subtracted position effectively becomes one. Grab the vector handles and see how the result changes:

You can also think of it this way: subtracting

`[0,0,0]`

from any position gives you the position difference that needs to be added to the origin `[0,0,0]`

to get to that given position. The line *AB*is described by points

*A*and

*B*, and if you subtract

*A*from both of them, the first one is suddenly

`[0,0,0]`

– and the other one is *(B - A)*– our new vector.

by Vojtěch Čada (noreply@blogger.com) at April 27, 2017 08:37 AM