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How Can We See the Big Bang? | Brian Cox

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Clips are provided by PowerfulJRE
Music provided by WaterTower Music
Track Name : Interstellar Official Soundtrack | Cornfield Chase – Hans Zimmer | WaterTower
Disclaimer: The video and audio content used in this video is for educational purposes only and does not belong to me. I have given credit to the respective owners and creators of the content. This video is intended to provide information and knowledge to its viewers, and no copyright infringement is intended. I have made every effort to ensure that the content used in this video is properly credited and used in accordance with fair use guidelines. If you are the owner of any content used in this video and have any concerns, please contact me.
How Can We See the Big Bang? | Brian Cox
The Big Bang happened nearly 13.8 billion years ago, but remarkably, we can still observe its afterglow in the present day. In this discussion, Brian Cox explains how modern astronomy allows us to look back in time and witness the early moments of the universe. The key to this lies in the cosmic microwave background radiation (CMB)—the faint remnant heat from the Big Bang, which permeates the universe and serves as the oldest observable light. Using powerful telescopes like the James Webb Space Telescope (JWST) and radio observatories, scientists can detect this radiation, providing a direct window into the universe’s infancy.
Since light takes time to travel, looking at distant galaxies is like looking into the past. The farther away a galaxy is, the older the light we see. Some of the earliest galaxies, formed just hundreds of millions of years after the Big Bang, are now visible thanks to advancements in observational technology. The phenomenon of redshift—where light from ancient galaxies is stretched due to the expansion of the universe—allows astronomers to determine their distance and age, further confirming our models of cosmic evolution.
Brian Cox delves into how the Large Hadron Collider (LHC) also helps us understand the Big Bang by recreating extreme conditions similar to those in the universe’s first fractions of a second. By smashing particles together at high speeds, physicists can study the fundamental forces that shaped the cosmos.
Ultimately, our ability to "see" the Big Bang is not through direct observation of the explosion itself, but through the relics it left behind—faint radiation, distant galaxies, and subatomic particles that still carry the signatures of the universe’s origins. Each discovery brings us closer to answering one of the biggest questions in physics: How did everything begin?
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Clips are provided by PowerfulJRE
Music provided by WaterTower Music
Track Name : Interstellar Official Soundtrack | Cornfield Chase – Hans Zimmer | WaterTower
Disclaimer: The video and audio content used in this video is for educational purposes only and does not belong to me. I have given credit to the respective owners and creators of the content. This video is intended to provide information and knowledge to its viewers, and no copyright infringement is intended. I have made every effort to ensure that the content used in this video is properly credited and used in accordance with fair use guidelines. If you are the owner of any content used in this video and have any concerns, please contact me.
How Can We See the Big Bang? | Brian Cox
The Big Bang happened nearly 13.8 billion years ago, but remarkably, we can still observe its afterglow in the present day. In this discussion, Brian Cox explains how modern astronomy allows us to look back in time and witness the early moments of the universe. The key to this lies in the cosmic microwave background radiation (CMB)—the faint remnant heat from the Big Bang, which permeates the universe and serves as the oldest observable light. Using powerful telescopes like the James Webb Space Telescope (JWST) and radio observatories, scientists can detect this radiation, providing a direct window into the universe’s infancy.
Since light takes time to travel, looking at distant galaxies is like looking into the past. The farther away a galaxy is, the older the light we see. Some of the earliest galaxies, formed just hundreds of millions of years after the Big Bang, are now visible thanks to advancements in observational technology. The phenomenon of redshift—where light from ancient galaxies is stretched due to the expansion of the universe—allows astronomers to determine their distance and age, further confirming our models of cosmic evolution.
Brian Cox delves into how the Large Hadron Collider (LHC) also helps us understand the Big Bang by recreating extreme conditions similar to those in the universe’s first fractions of a second. By smashing particles together at high speeds, physicists can study the fundamental forces that shaped the cosmos.
Ultimately, our ability to "see" the Big Bang is not through direct observation of the explosion itself, but through the relics it left behind—faint radiation, distant galaxies, and subatomic particles that still carry the signatures of the universe’s origins. Each discovery brings us closer to answering one of the biggest questions in physics: How did everything begin?
#space #spacexelonmusk #viral #nasa #spacex ##viralvideo #astronomy #spacetechnology
#shorts #shortsfeed #shortvideos #shortvideo #shortsvideo #shortsyoutube #shortsviral #viralshortsvideo #viralshorts #viral #viralvideo #viralvideos
#space #deepspace #spaceship #spacelovers #spacesuit #spaceexploration #spacecraft #telescope #spacex #spacestation #universe #cosmos #nasa #viral #viralvideo #viralvideos #science #technology #physics #astronomy #astrophysics #astrophotography #cosmology #cosmos #jwst #jameswebbspacetelescope #jameswebb #hubble #hubbletelescope #video #videos #interstellar #neildegrassetyson #neil #tyson #michiokaku #kaku #briancox
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