Pulsar
PSR J1701-3006H
Millisecond pulsar · in the globular cluster M62
A millisecond pulsar spinning 270 times per second: an old neutron star spun up again (“recycled”) by matter transferred from a companion. It shares a 3.19 h orbit with a very-low-mass companion. Period, spin-down, distance and orbit come from the ATNF Pulsar Catalogue; the beam geometry is illustrative.
| Type | Pulsar |
|---|---|
| Constellation | Ophiuchus |
| Period | 3.705 ms (270 Hz) |
| Period derivative | 3.8×10⁻²⁰ s/s |
| Characteristic age | 1.6 billion years |
| Magnetic field | 3.8×10⁸ G |
| Spin-down luminosity | 2.9×10³⁴ erg/s |
| Dispersion measure | 114.7 pc/cm³ |
| Distance | 4,851 pc (15.8 thousand ly) |
| Location | in the globular cluster M62 |
| Companion | very-low-mass companion (estimated), ~0.003 M☉ |
| Orbital period | 3.19 h |
| Discovery | 2024 · misc |
| Source | ATNF Pulsar Catalogue |
| Right ascension (J2000) | 17h 01m 13.8s |
| Declination (J2000) | −30° 06′ 25″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 60° N. South of latitude 60° 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 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.