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Galaxy Cluster Collision Created 1.6 Million Mile Shockwave
Space.com
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29/07/2024
NASA Chandra X-ray telescope data from galaxy cluster Abell 2146 shows a "shockwave that stretches for some 1.6 million miles," that was created by a collision with another cluster.
Credit: NASA/CXC/A. Hobart
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Tech
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00:00
Visit Chandra's beautiful universe.
00:05
Able 2146.
00:10
Galaxy clusters are among the largest structures in the universe,
00:14
containing hundreds of galaxies and huge amounts of hot gas and dark matter.
00:19
Sometimes these gigantic objects collide with one another,
00:23
and when they do, they release enormous amounts of energy,
00:27
unlike anything witnessed since the Big Bang.
00:30
These galaxy cluster collisions also provide scientists with physics laboratories
00:35
that are unavailable here on Earth.
00:38
A new study of the galaxy cluster collision, known as Able 2146,
00:43
uses a very long look, about 23 days' worth of observing time,
00:47
from NASA's Chandra X-ray Observatory.
00:51
X-rays are particularly important in studying galaxy clusters
00:55
because they detect the massive amounts of hot gas that fills the spaces between the galaxies themselves.
01:01
When researchers analyzed the Chandra data of Able 2146,
01:06
they found a shock wave that stretches for some 1.6 million miles.
01:11
The shock wave, which is similar to a sonic boom created by a jet plane,
01:16
was generated by the hot gas from one cluster pushing on the other.
01:22
There is also a second shock wave detected behind the collision.
01:26
Shock waves like those generated by a supersonic jet are collisional shocks,
01:31
meaning they involve direct collisions between particles.
01:35
Near sea level, the Earth's atmosphere is dense enough
01:39
so that gas particles typically travel only about 100 billionth of a meter
01:44
before colliding with another particle.
01:47
This is usually not the case in space.
01:50
In galaxy clusters and in the solar wind,
01:53
streams of particles blown away from the Sun,
01:56
direct collisions between particles occur too rarely to produce shock waves
02:00
because the gas has incredibly low density.
02:04
For example, in galaxy clusters,
02:07
particles typically must travel about 30,000 to 50,000 light-years before colliding.
02:13
Instead, the shocks in these cosmic environments are collisionless
02:18
and are generated by interactions between charged particles and magnetic fields.
02:24
Collisionless shock waves are important in several other fields of research beyond astrophysics.
02:30
For example, the radiation produced by shocks in the solar wind
02:34
can negatively impact commercial and military spacecraft operation,
02:39
as well as the safety of humans in space.
02:43
This study shows a deep connection between some of the largest, most energetic events
02:48
and much smaller ones closer to home.
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2:13
|
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