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Pulsar

PSR B2022+50 (J2023+5037)

Radio pulsar

A neutron star spinning once every 0.373 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
Period372.6 ms
Period derivative2.5×10⁻¹⁵ s/s
Characteristic age2.4 million years
Magnetic field9.8×10¹¹ G
Spin-down luminosity1.9×10³³ erg/s
Dispersion measure33.0 pc/cm³
Distance2,059 pc (6.7 thousand ly)
Discovery1985 · gb2, lotaas, fast_gpps
SourceATNF Pulsar Catalogue
Right ascension (J2000)20h 23m 42.0s
Declination (J2000)+50° 37′ 35″

In the sky

Visible from the whole Northern Hemisphere and south to latitude 39° S. North of latitude 39° N it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out 6,716 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 119 million years.

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