Chandra X-ray Observatory | Tour: Colossal Collisions Linked to Solar System Science @ChandraXray | Uploaded June 2022 | Updated October 2024, 5 days ago.
Galaxy clusters are among the largest structures in the Universe, containing hundreds of galaxies and huge amounts of hot gas and dark matter. Sometimes, these gigantic objects collide with one another, and, when they do, they release enormous amounts of energy unlike anything witnessed since the Big Bang. These galaxy cluster collisions also provide scientists with physics laboratories that are unavailable here on Earth.
A new study of the galaxy cluster collision known as Abell 2146 uses a very long look — about 23 days' worth of observing time — from NASA's Chandra X-ray Observatory. X-rays are particularly important in studying galaxy clusters because they detect the massive amounts of hot gas that fills the spaces between the galaxies themselves.
When researchers analyzed the Chandra data of Abell 2146, they found a shockwave that stretches for some 1.6 million miles. The shock wave, which is similar to sonic boom created by a jet plane, was generated by the hot gas from one cluster pushing on the other. There is also a second shock wave detected behind the collision.
Shock waves like those generated by a supersonic jet are collisional shocks, meaning they involve direct collisions between particles. Near sea level, the Earth's atmosphere is dense enough so that gas particles typically travel only about 100 billionth of a meter before colliding with another particle. This is usually not always the case in space. In galaxy clusters and in the solar wind — streams of particles blown away from the Sun — direct collisions between particles occur too rarely to produce shock waves because the gas has incredibly low density. For example, in galaxy clusters particles typically must travel about 30,000 to 50,000 light-years before colliding. Instead, the shocks in these cosmic environments are "collisionless," and are generated by interactions between charged particles and magnetic fields.
Collisionless shock waves are important in several other fields of research beyond astrophysics. For example, the radiation produced by shocks in the solar wind can negatively impact commercial and military spacecraft operation, as well as the safety of humans in space. This study shows a deep connection between some of the largest, most energetic events and much smaller ones closer to home.
More at: https://chandra.si.edu/photo/2022/a2146/
Galaxy clusters are among the largest structures in the Universe, containing hundreds of galaxies and huge amounts of hot gas and dark matter. Sometimes, these gigantic objects collide with one another, and, when they do, they release enormous amounts of energy unlike anything witnessed since the Big Bang. These galaxy cluster collisions also provide scientists with physics laboratories that are unavailable here on Earth.
A new study of the galaxy cluster collision known as Abell 2146 uses a very long look — about 23 days' worth of observing time — from NASA's Chandra X-ray Observatory. X-rays are particularly important in studying galaxy clusters because they detect the massive amounts of hot gas that fills the spaces between the galaxies themselves.
When researchers analyzed the Chandra data of Abell 2146, they found a shockwave that stretches for some 1.6 million miles. The shock wave, which is similar to sonic boom created by a jet plane, was generated by the hot gas from one cluster pushing on the other. There is also a second shock wave detected behind the collision.
Shock waves like those generated by a supersonic jet are collisional shocks, meaning they involve direct collisions between particles. Near sea level, the Earth's atmosphere is dense enough so that gas particles typically travel only about 100 billionth of a meter before colliding with another particle. This is usually not always the case in space. In galaxy clusters and in the solar wind — streams of particles blown away from the Sun — direct collisions between particles occur too rarely to produce shock waves because the gas has incredibly low density. For example, in galaxy clusters particles typically must travel about 30,000 to 50,000 light-years before colliding. Instead, the shocks in these cosmic environments are "collisionless," and are generated by interactions between charged particles and magnetic fields.
Collisionless shock waves are important in several other fields of research beyond astrophysics. For example, the radiation produced by shocks in the solar wind can negatively impact commercial and military spacecraft operation, as well as the safety of humans in space. This study shows a deep connection between some of the largest, most energetic events and much smaller ones closer to home.
More at: https://chandra.si.edu/photo/2022/a2146/
