BINARY STAR SYSTEM

In the Algol system the lighter star is the older one — a paradox until astronomers realised it had already poured most of its mass onto its companion. Seen edge-on, the pair eclipse each other and the light curve carries alternating deep and shallow dips. Gas spills through the L1 point of the Roche lobe in a stream curved by the Coriolis effect and strikes the disk rim as a hot spot, while the gas piling up on the white dwarf eventually ignites as a nova.

▸ Loading sample systems: Algol · Sirius A+B · cataclysmic variable · contact…
▸ Placing the two stars on orbits around the shared barycenter
▸ Building Roche lobes & the L1 Lagrange point
▸ Enabling the mass-transfer stream & accretion disk (Coriolis)…
▸ Calibrating the eclipsing light curve
▸ Ready — Online. ✅
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Simulation room Binary star system

Binary Star System
Online
barycenter · Roche · light curve
Selected system
👁️ Algol
System type—
Mass—
Temperature (gainer/donor)—
Period—
Brightness—
Magnitude drop—
Eclipse status
—
Left-drag = rotate · right-drag = pan · scroll = zoom · click a STAR = Roche lobe
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Light curve — total brightness over time (dip = eclipse) brightness
About Binary Star System

In the Algol system the lighter star is the older one — a paradox until astronomers realised it had already poured most of its mass onto its companion. Seen edge-on, the pair eclipse each other and the light curve carries alternating deep and shallow dips. Gas spills through the L1 point of the Roche lobe in a stream curved by the Coriolis effect and strikes the disk rim as a hot spot, while the gas piling up on the white dwarf eventually ignites as a nova.

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