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Astronomy

The cosmic web

Grow a primordial displacement field. Watch sheets and filaments emerge as initially separated matter streams approach one another.

The cosmic web — Actual application image
Actual application image

The model and its limits

Zel’dovich first-order Lagrangian displacement in a periodic cube. The approximation ceases to describe bound structures after shell crossing; brightness is illustrative.

Equations used in the module
Equations
x(q,D) = q - D∇Φ(q); ρ/ρ₀ = 1/|det(∂x/∂q)| before shell crossing

Related experiments

Back to catalogue
Stars cross the spiral arms — Actual application image

Astronomy

Stars cross the spiral arms

Follow a marked star through a rotating spiral pattern. Move the corotation radius and see where the star overtakes the arms.

A galaxy’s light profile — Actual application image

Astronomy

A galaxy’s light profile

Change the balance of disk and bulge. View the resulting three-dimensional galaxy and compare the exponential disk’s enclosed light with a Sérsic bulge.

Inside an active galaxy — Actual application image

Astronomy

Inside an active galaxy

Open the viewing cone of a dusty torus. Compare an unobscured view of the central engine with a line of sight passing through the dust.