The Crab
Pulsar
PSR B0531+21
The heart of a star that Chinese astronomers watched explode in 1054. It turns thirty times a second.
03 / 06
- Catalogue
- PSR B0531+21
- Type
- Pulsar
- We listen at
- 1400.000 MHz
- Period
- 33.7 ms
- Distance
- ≈ 6,500 light-years
- Discovered
- 1968 (the explosion: 4 July 1054)
- By
- David Staelin & Edward Reifenstein, Green Bank
- Position
- 05h 34m 31.9s
+22° 00′ 52″ - From Stilledal
- Circumpolar, just. Lowest at dawn.
In the summer of 1054 a new star appeared in Taurus, bright enough to see in daylight for three weeks. The court astronomers of the Song dynasty wrote it down. The Crab Nebula is what is left, and at its centre is this.
Thirty rotations a second is too fast to hear as clicks. In the headphones it becomes a tone, a buzz well below the lowest string of a cello.
Now and then it throws a giant pulse, hundreds of times brighter than the rest. When one arrives during a Listening Night, the astronomer on duty rings a bell.
{What it sounds like}
A low buzz, like a moth against glass.
{Headphones help. The sound is synthesized from the real period and profile.}
{Next station/} 04 / 06 · 1400.000 MHz