PULSAR · NEUTRON STAR

A pulsar blinks only thanks to one geometric detail: its magnetic axis is tilted from its spin axis, so the beam sweeps around like a lighthouse. With that tilt at zero the pulses die out even though the star keeps turning. Spin periods run from radio pulsars at a few turns per second to millisecond pulsars like PSR B1937+21 at 642 turns per second, while a magnetar's 10¹⁴ to 10¹⁵ Gauss field brakes it into a slow spin.

▸ Compressing a massive star's core after a supernova → neutron star (~1.4 M☉ / ~20 km)…
▸ Spinning it up + flux conservation → ~10¹² Gauss magnetic field
▸ Building a magnetic axis TILTED from the spin axis + two beams at the magnetic poles
▸ Placing "Earth / receiver" to catch the lighthouse pulse beat
▸ Calibrating the radio pulse clock…
▸ Ready — Online. ✅
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Simulation room Pulsar

Pulsar · Neutron star
Online
lighthouse effect · sweeping beam
Observing
📡 Pulsar radio
Spin period—
Spin rate—
Magnetic tilt—
Magnetic field—
Type—
Received signal
—
Left-drag = rotate · right-drag = pan · scroll = zoom · double-click = neutron-star cross-section
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Radio pulse train over time — each peak = one beam sweep across Earth received pulse amplitude
About Pulsar

A pulsar blinks only thanks to one geometric detail: its magnetic axis is tilted from its spin axis, so the beam sweeps around like a lighthouse. With that tilt at zero the pulses die out even though the star keeps turning. Spin periods run from radio pulsars at a few turns per second to millisecond pulsars like PSR B1937+21 at 642 turns per second, while a magnetar's 10¹⁴ to 10¹⁵ Gauss field brakes it into a slow spin.

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