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Pulsar

PSR B1933+17 (J1935+1745)

Radio pulsar

A neutron star spinning once every 0.654 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
ConstellationSagitta
Period654.4 ms
Period derivative3.8×10⁻¹⁶ s/s
Characteristic age27 million years
Magnetic field5.0×10¹¹ G
Spin-down luminosity5.3×10³¹ erg/s
Dispersion measure214.6 pc/cm³
Distance4,845 pc (15.8 thousand ly)
Discovery1975 · ar1, palfa, fast_gpps
SourceATNF Pulsar Catalogue
Right ascension (J2000)19h 35m 30.0s
Declination (J2000)+17° 45′ 12″

In the sky

Visible from the whole Northern Hemisphere and south to latitude 72° S. North of latitude 72° 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 16 thousand years ago. At that time Homo sapiens was spreading out of Africa; there was no farming yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 280 million years.

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