Crab Pulsar
Pulsar · Pulsar in the constellation Taurus

About the Crab Pulsar
The Crab Pulsar is about 6,523 light-years from the Sun, so the light we see from it left about 6,523 years ago.
It is 33,475 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.
Key numbers
| Distance | 6,523 light-years (2,000 pc) |
|---|---|
| Distance from the Galactic centre | 33,475 light-years |
| Galactic coordinates | l = 184.56°, b = -5.78° |
| Spin period | 33.4 ms |
| Distance method | independent (parallax or association) |
Data: ATNF Pulsar Catalogue v2.9.0.
Where it is
Its place in the universe, from the inside out: Perseus 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 Crab Pulsar is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054. Discovered in 1968, the pulsar was the first to be connected with a supernova remnant.
Excerpt from the Wikipedia article Crab Pulsar, licensed CC BY-SA 4.0.
Nearby on the map
- Crab Nebula Supernova remnant
- Rosette Nebula Nebula
- Eskimo Nebula Planetary nebula
- M67 Open star cluster
- Horsehead Nebula Nebula
- Flame Nebula Nebula