-
So, today we're going to make a big leap,
-
because today you're going to understand
-
how planets move around the Sun.
-
That's a mega problem, right?
-
The little ms you put in the equation
-
are not mass of a pulley or a plane,
-
but mass of Jupiter or mass of the Sun.
-
So, you're doing something of cosmological proportions.
-
And you don't need to know too much more to do that.
-
You're almost there.
-
So, I'm going to just tell you the one missing thing.
-
So, what Newton had done is to realize that