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Spider Pulsars Caught Destroying Nearby Stars - Explained
Space.com
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01/04/2025
Data from the Chandra X-ray Telescope has revealed spider pulsars, which are a group of dead stars, in globular cluster Omega Centauri "preying' on nearby stars. The Chandra team explains.
Credit: NASA/CXC/A. Hobart
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00:00
Music
00:04
Visit Chandra's beautiful universe. Omega Centauri
00:08
A horde of dead stars
00:12
known as spider pulsars are obliterating companion stars within their
00:16
reach. Data from NASA's Chandra X-ray Observatory
00:20
of the globular cluster Omega Centauri are helping astronomers
00:24
understand how these spider pulsars prey on nearby stars.
00:28
A pulsar is the spinning, dense core that remains
00:32
after a massive star collapses into itself. Rapidly
00:36
rotating neutron stars can produce beams of radiation.
00:40
Like a rotating lighthouse beam, the radiation can be observed as a powerful
00:44
pulsing source of radiation, or pulsar.
00:48
Some pulsars spin around dozens to hundreds of times per second,
00:52
and these are known as millisecond pulsars.
00:56
Spider pulsars are a special class of millisecond
01:00
pulsars and get their name from the damage they inflict on small
01:04
companion stars in orbit around them. Through winds of energetic
01:08
particles streaming from their surfaces, the spider pulsars
01:13
methodically strip the companion stars of their outer layers.
01:17
Astronomers recently discovered 18 millisecond pulsars in
01:21
Omega Centauri, located about 17,700 light-years
01:25
from Earth, using radio telescopes. A pair of
01:29
astronomers from the University of Alberta in Canada then looked at Chandra data
01:33
of Omega Centauri to see how many of the millisecond pulsars give off
01:37
X-rays. They found 11 millisecond pulsars
01:41
emitting X-rays, and five of those were spider pulsars, concentrated near the
01:45
center of Omega Centauri. The researchers next
01:49
combined the data of Omega Centauri with Chandra observations of
01:53
the energetic spider pulsars in 12 other globular clusters.
01:57
Spider pulsars are typically separated from their companions by only about
02:01
1 to 14 times the distance between the Earth and Moon.
02:05
This close proximity, cosmically speaking, causes the energetic
02:09
particles from the pulsars to be particularly damaging to their
02:13
companion stars.
02:17
Chandra's sharp X-ray vision is crucial for studying millisecond pulsars
02:21
in globular clusters, because they often contain large numbers of X-ray
02:26
sources in a small part of the sky, making it difficult to distinguish sources
02:30
from each other.
02:34
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