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Pulsar

PSR B2321-61 (J2324-6054)

Radio pulsar

A neutron star spinning once every 2.35 seconds; the beams from its magnetic poles sweep across Earth on every turn. Period, spin-down, distance and orbit come from the ATNF Pulsar Catalogue; the beam geometry is illustrative.

TypePulsar
ConstellationTucana
Period2.347 s
Period derivative2.6×10⁻¹⁵ s/s
Characteristic age14 million years
Magnetic field2.5×10¹² G
Spin-down luminosity7.9×10³⁰ erg/s
Dispersion measure15.2 pc/cm³
Distance1,348 pc (4.4 thousand ly)
Discovery1978 · mol2, misc
SourceATNF Pulsar Catalogue
Right ascension (J2000)23h 24m 27.1s
Declination (J2000)−60° 54′ 06″

In the sky

Visible from the whole Southern Hemisphere and north to latitude 29° N. South of latitude 29° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out 4,397 years ago. At that time the first farming villages were being founded; there was no writing yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 78 million years.

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