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Pulsar

PSR B1828-60 (J1833-6023)

Radio pulsar

A neutron star spinning once every 1.89 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
ConstellationPavo
Period1.889 s
Period derivative2.7×10⁻¹⁶ s/s
Characteristic age111 million years
Magnetic field7.2×10¹¹ G
Spin-down luminosity1.6×10³⁰ erg/s
Dispersion measure35.0 pc/cm³
Distance1,336 pc (4.4 thousand ly)
Discovery1978 · mol2, pks70, pkssw
SourceATNF Pulsar Catalogue
Right ascension (J2000)18h 33m 14.8s
Declination (J2000)−60° 23′ 04″

In the sky

Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out 4,357 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 77 million years.

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