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Astronomy

A dying star’s luminous shell

Shape an expanding stellar envelope from a round shell into bipolar lobes. Track its expansion age and the fading emission measure.

A dying star’s luminous shell — Actual application image
Actual application image

The model and its limits

Ballistic homologous shell and an n² emission proxy. Ionization, shocks and line ratios are not solved; colours represent an illustrative narrow-band composite.

Equations used in the module
Equations
R = vt; n ∝ t^(-3); ∫n²dV ∝ t^(-3)

Related experiments

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A star the size of a planet — Actual application image

Astronomy

A star the size of a planet

Add mass to a cold white dwarf and watch its radius shrink. Compare its density and surface redshift with the familiar scale of Earth.

A city-sized star — Actual application image

Astronomy

A city-sized star

Compress a stellar mass into a small radius. Compare compactness, surface redshift and the increasing fraction of the surface visible through light bending.

A star spills into its companion — Actual application image

Astronomy

A star spills into its companion

Expand the donor toward its Roche lobe. Watch the transfer stream switch on when the stellar surface reaches the critical radius.