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Pulsar

PSR B2148+52 (J2150+5247)

Radio pulsar

A neutron star spinning once every 0.332 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
ConstellationCygnus
Period332.2 ms
Period derivative1.0×10⁻¹⁴ s/s
Characteristic age521 thousand years
Magnetic field1.9×10¹² G
Spin-down luminosity1.1×10³⁴ erg/s
Dispersion measure148.9 pc/cm³
Distance3,610 pc (11.8 thousand ly)
Discovery1985 · gb2, gb3, lotaas, fast_gpps
SourceATNF Pulsar Catalogue
Right ascension (J2000)21h 50m 37.8s
Declination (J2000)+52° 47′ 50″

In the sky

Visible from the whole Northern Hemisphere and south to latitude 37° S. North of latitude 37° N it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out 12 thousand 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 209 million years.

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