A plane in $\mathbb{R}^3$ and above is defined by one point $P$ contained in the plane and two direction vectors $\vec{a}$ and $\vec{b}$ that are not parallel.
A point $X$ in this plane is one such that $$X = P + s\cdot\vec{a}+t\cdot\vec{b}$$
For a certain $s,t \in \mathbb{R}$. This is called vectorial equation.
In $\mathbb{R}^3$ there is another way to define planes. With one point $P$ in the plane and only one direction vector $\vec{m}$, rather than two. This vector is perpendicular to the plane.
I'm guessing that the "vectorial equation" I described above does not apply in this scenario, as it requires two direction vectors and I only have one here.
I heard that in this case there is a "normal equation", however I am unsure how is it defined at all.
There is a definition in my book, but I don't quite grasp it:
All the points $(x,y,z)$ in a plane that contains $P = (p_1,p_2,p_3)$ and is perpendicular to the vector $\vec{n}=(a,b,c)$, are the only ones that satisfy:
$$ax+by+cz = d$$
Where $d = ap_1+bp_2+cp_3$.
Can you better explain this? I easily get the vectorial equation, but the normal equation is still fairly confusing to me.
The "vectorial" equation is of the parametric type. It means that by varying the two independent parameters, $s$ and $t$, you span the whole plane and get a double infinity of $X$ points.
The "normal" equation is of the implicit type. It means that for the whole space, only the points belonging to the plane do fulfill the given equation $\vec n.\vec X=d=\vec n.\vec P$, for some $P$ (belonging to the plane, as $X=P$ verifies the equation).
By the way, you can check the compatibility of the two representations by plugging $X$ from the vectorial equation into the normal equation:
$$\vec n.(\vec P+s.\vec a+t.\vec b)=\vec n.\vec P,$$ or $$s.\vec n.\vec a+t.\vec n.\vec b=0,$$ implying that both $\vec n.\vec a$ and $\vec n.\vec b$ are zero. $\vec n$ is perpendicular to $\vec a$ and $\vec b$.