The Intergalactic Medium: A Cosmic Web Connecting Galaxies
These structures, resembling tree roots, consist primarily of hydrogen and helium filaments that flow into galaxies, providing the raw material for star formation.
Supermassive black holes, fueled by accretion disks, can emit energy that reshapes or destroys entire galaxies, profoundly impacting cosmic evolution.
These structures, resembling tree roots, consist primarily of hydrogen and helium filaments that flow into galaxies, providing the raw material for star formation.
These cosmic engines blast out huge jets of matter and radiation, completely reshaping or even killing the galaxies around them.
In the 1950s, astronomers detected mysterious, loud radio waves emanating from point-like objects scattered across the sky.
These objects were initially named 'quasi-stellar radio sources,' or quasars, because they appeared as dots like stars but were observed through radio waves rather than visible light.
Subsequent observations revealed that quasars were billions of light-years away, a discovery that explained their seemingly extreme speeds, which were actually a result of the universe's expansion.
During this period, early galaxies were still relatively small, yet quasars produced light thousands of times brighter than the entire Milky Way, indicating their immense energy output.
Black holes are the most efficient engines in the universe for converting matter into energy, achieving an efficiency 60 times greater than nuclear fusion in stars.
As gas particles in the accretion disk rub against each other due to friction and particle collisions, the disk heats up to hundreds of thousands of degrees, causing it to glow brightly.
This process allows quasars to consume between 1 and 100 Earth masses of gas every minute, fueling their prodigious energy output.
They release massive plumes of energy that can extend for hundreds of thousands of light-years, increasing the kinetic energy of atoms in galactic gas.
This heating prevents gas from collapsing under gravity, a necessary condition for star formation, as new stars can only ignite in cold gas.
Additionally, quasars physically push gas out of the galaxy, thereby depleting the raw materials required for future star creation.
While quasars are destructive, their regulatory effect on star formation might prevent conditions that are hazardous to life, such as frequent supernovae.
Excessive star formation can lead to numerous massive stars exploding, creating dangerous radiation environments, which quasar activity may help to mitigate.
Galactic evolution involves a delicate balance: although quasars eject gas, the shock waves they generate can also compress gas and trigger localized bursts of new star formation.
Galactic mergers typically force supermassive black holes to the center of the new galaxy, creating violent events that can also trigger star formation.
Currently, Sagittarius A* is dormant, but a future merger with the Andromeda galaxy, predicted to occur in a few billion years, could provide a fresh influx of gas that would reactivate it into a quasar.
However, there is no certainty regarding if or when such a dramatic event will unfold in our local galactic group.
This violent process stirs up vast amounts of dust and stars, ejecting them in every direction and creating stunning cosmic events.
Future civilizations might witness these spectacular phenomena, though the video suggests that human curiosity should remain focused on understanding the present universe.
Kurzgesagt has partnered with Brilliant.org to develop a series of educational lessons designed to elevate scientific understanding.
These lessons expand on popular video topics such as mammalian metabolism and climate science, providing in-depth explanations.
Specific modules are available that cover the formation and behavior of black holes, offering a comprehensive look at these cosmic phenomena.
The Brilliant platform employs an interactive, hands-on learning approach, which is likened to personalized tutoring for effective knowledge acquisition.
Brilliant offers thousands of additional lessons across a wide range of subjects, from math-based topics like algebra and probability to courses in programming and data science.
A new course, 'How Technology Works,' delves into topics such as password security and satellite GPS, explaining the underlying principles of modern technology.
Viewers can access a 30-day free trial by visiting brilliant.org/nutshell, and the first 200 individuals to sign up will receive a 20% discount on an annual membership.
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