Light, time, and the rules that hold no matter how you are moving.
Ordinary matter makes up about 5% of the universe’s total mass and energy. The visualisation follows that share into smaller categories, showing where stars, planets and other familiar objects fit.
What a star leaves behind is fixed almost entirely by what it weighed when it was born, and the heaviest ones leave nothing at all.
Whatever falls into a black hole, all that survives of it is a weight and a spin, and those two numbers fix every layer of the thing left behind.
Light takes time to travel. This limits how soon we can learn about a distant event, and how soon anything we do can affect it. A light-cone diagram helps us explore both.