Hulse–Taylor pulsar
Pulsar · Pulsar in the constellation Aquila
About the Hulse–Taylor pulsar
The Hulse–Taylor pulsar is about 17,110 light-years from the Sun, so the light we see from it left about 17,110 years ago.
It is 20,684 light-years from the centre of the Milky Way.
The map lists it as a pulsar and shows it among the stars around the Sun, drawn on the plane of the Milky Way.
Its shrinking orbit gave the first evidence for gravitational waves (Nobel Prize 1993).
Key numbers
| Distance | 17,110 light-years (5.25 kpc) |
|---|---|
| Distance from the Galactic centre | 20,684 light-years |
| Galactic coordinates | l = 49.97°, b = +2.12° |
| Spin period | 59 ms |
| Distance method | estimated from dispersion measure (uncertain by ~2×) |
Data: ATNF Pulsar Catalogue v2.9.0.
Where it is
Its place in the universe, from the inside out: Sagittarius–Carina Arm › Milky Way › Local Group › Virgo Supercluster › Laniakea Supercluster › Observable universe.
Zoom out to see it in context: Local Arm, a view about 12,000 light-years across.
From Wikipedia
The Hulse–Taylor pulsar is a binary star system composed of a neutron star and a pulsar which orbit around their common center of mass. It is the first binary pulsar ever discovered.
Excerpt from the Wikipedia article Hulse–Taylor pulsar, licensed CC BY-SA 4.0.
Nearby on the map
- SS 433 Black hole
- SGR 1935+2154 Neutron star
- NGC 6791 Open star cluster
- Scutum–Centaurus Arm Galactic structure
- Solar circle Galactic structure
- V404 Cygni Black hole