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Pulsar

PSR B0853-33 (J0855-3331)

Radio pulsar

A neutron star spinning once every 1.27 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
ConstellationPyxis
Period1.268 s
Period derivative6.3×10⁻¹⁵ s/s
Characteristic age3.2 million years
Magnetic field2.9×10¹² G
Spin-down luminosity1.2×10³² erg/s
Dispersion measure86.4 pc/cm³
Distance502 pc (1.6 thousand ly)
Discovery1978 · mol2, htru_pks, misc, pks70, pkshl
SourceATNF Pulsar Catalogue
Right ascension (J2000)8h 55m 38.4s
Declination (J2000)−33° 31′ 39″

In the sky

Visible from the whole Southern Hemisphere and north to latitude 56° N. South of latitude 56° S it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 389. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 29 million years.

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