Pulsar
PSR J1931+1428_P
Millisecond pulsar · binary system
A millisecond pulsar spinning 383 times per second: an old neutron star spun up again (“recycled”) by matter transferred from a companion. It shares a 4.36 h 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 | Aquila |
| Period | 2.610 ms (383 Hz) |
| Dispersion measure | 241.3 pc/cm³ |
| Distance | 6,226 pc (20.3 thousand ly) |
| Companion | helium white dwarf (estimated), ~0.29 M☉ |
| Orbital period | 4.36 h |
| Discovery | 2025 · fast_gpps |
| Source | ATNF Pulsar Catalogue |
| Right ascension (J2000) | 19h 31m 48.4s |
| Declination (J2000) | +14° 28′ 00″ |
In the sky
Visible from the whole Northern Hemisphere and south to latitude 76° S. North of latitude 76° 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 20 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 360 million years.