Pulsar
PSR J1836-0150_P
Millisecond pulsar · binary system
A millisecond pulsar spinning 183 times per second: an old neutron star spun up again (“recycled”) by matter transferred from a companion. It shares a 51.490 days orbit with a helium white dwarf. Period, spin-down, distance and orbit come from the ATNF Pulsar Catalogue; the beam geometry is illustrative.
| Type | Pulsar |
|---|---|
| Constellation | Serpens |
| Period | 5.460 ms (183 Hz) |
| Dispersion measure | 199.4 pc/cm³ |
| Distance | 4,863 pc (15.9 thousand ly) |
| Companion | helium white dwarf (estimated), ~0.25 M☉ |
| Orbital period | 51.490 days |
| Discovery | 2025 · fast_gpps |
| Source | ATNF Pulsar Catalogue |
| Right ascension (J2000) | 18h 36m 05.8s |
| Declination (J2000) | −1° 49′ 59″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 88° N. 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 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 281 million years.