Thanks!

You can also turn on the known asteroid population:

https://dahlend.github.io/ketev/#t=2026-11-12.9717&sel=2026%...

Everything runs in the browser, served as a static github pages so I don't have to think about hosting or anything.

I've always only ever seen diagrams of the Jupiter Trojans from a top down perspective so I never realized how much they stretched beyond the orbital plane of the solar system.

Do you know why they stretch so up and down relative to Jupiter? Is that sort 3d distribution shape typical for L4 and L5 Lagrangian points, and it's just amplified by the size of Jupiter or is there something else at play there?