Pulsar
PSR B1817-13 (J1820-1346)
Radio pulsar
A neutron star spinning once every 0.921 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.
| Type | Pulsar |
|---|---|
| Constellation | Serpens |
| Period | 921.5 ms |
| Period derivative | 4.5×10⁻¹⁵ s/s |
| Characteristic age | 3.3 million years |
| Magnetic field | 2.1×10¹² G |
| Spin-down luminosity | 2.3×10³² erg/s |
| Dispersion measure | 771.0 pc/cm³ |
| Distance | 5,837 pc (19.0 thousand ly) |
| Discovery | 1986 · jb2, htru_pks, pks1, pksmb |
| Source | ATNF Pulsar Catalogue |
| Right ascension (J2000) | 18h 20m 19.8s |
| Declination (J2000) | −13° 46′ 15″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 76° N. South of latitude 76° 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 19 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 338 million years.