Pulsar
PSR B1729-41 (J1732-4128)
Radio pulsar
A neutron star spinning once every 0.628 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 | Scorpius |
| Period | 628.0 ms |
| Period derivative | 1.3×10⁻¹⁴ s/s |
| Characteristic age | 775 thousand years |
| Magnetic field | 2.9×10¹² G |
| Spin-down luminosity | 2.0×10³³ erg/s |
| Dispersion measure | 195.3 pc/cm³ |
| Distance | 7,234 pc (23.6 thousand ly) |
| Discovery | 1978 · mol2, htru_pks, pksmb |
| Source | ATNF Pulsar Catalogue |
| Right ascension (J2000) | 17h 32m 50.0s |
| Declination (J2000) | −41° 28′ 48″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 49° N. South of latitude 49° 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 24 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 419 million years.