What The Physics?!
Greg Gravity Death
updated
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See a new experiment (previous video) that, for the first time ever, shows how a ball can roll uphill:bit.ly/2TY1FX9
** PRODUCTION CREDITS
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Host, Producer: Greg Kestin
Filming: Daniel Thomson, Greg Kestin, Lauren Liebhaber, Yasmeen Ketcherside, Kelsey Tsipis, Tim Treuer
Research, Writing: Greg Kestin, Samia Bouzid
Editing, Animating: Greg Kestin
Editorial Input: Julia Cort, Ari Daniel
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From the producers of PBS NOVA
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The next video released will explain how the Anti-Gravity Cone actually works; what force overpowers the force of gravity?
** PRODUCTION CREDITS
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Host, Producer: Greg Kestin
Filming: Daniel Thomson, Greg Kestin, Lauren Liebhaber, Yasmeen Ketcherside, Kelsey Tsipis, Tim Treuer
Research, Writing: Greg Kestin, Samia Bouzid
Editing, Animating: Greg Kestin
Editorial Input: Julia Cort, Ari Daniel
Media: Shutterstock
Special thanks to Entire NOVA team
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
You may have heard that the Coriolis effect makes water in the bathtub spiral down the drain in a certain way, or that it determines the way that a toilet flushes. That’s actually wrong.
Although, as you may have noticed while tracking a hurricane on the news, storms in the Northern Hemisphere spin counterclockwise, while those in the Southern Hemisphere spin clockwise. Why do storms spin in different directions depending on their location? And why do they spin in the first place? The answer is the Coriolis effect.
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** PRODUCTION CREDITS
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- Host, Producer: Greg Kestin
- Filming: Greg Kestin
- Research, Writing: Greg Kestin
Samia Bouzid
- Editing, Animating: Samia Bouzid
Greg Kestin
- Editorial Input: Julia Cort, Ari Daniel
- Science consultants: David Holland, Louis Deslauriers, Kerry Emanuel, Daniel Jacob
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- Special thanks: Harvard Lecture Demonstration Group (Daniel Davis, Allen Crockett, Daniel Rosenberg)
- Special thanks: Entire NOVA team
- From the producers of PBS NOVA © WGBH Educational Foundation - Funding provided by FQXi
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DIY Particle Detector: youtu.be/wN_DMMQEhfQ
PRODUCTION CREDITS
Host, Producer: Greg Kestin
Research, Writing: Samia Bouzid, Greg Kestin
Editing, Animating: Daniel Thomson
Editorial Input from: Julia Cort, Ari Daniel
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation Funding provided by FQXi Music provided by APM
"How To Travel to Another Galaxy" will be out next week––subscribe so you won't miss it! bit.ly/2o2WYxD
PRODUCTION CREDITS
Host, Producer: Greg Kestin
Filming: Greg Kestin
Research, Writing: Greg Kestin, Samia Bouzid
Editing, Animating: Samia Bouzid, Lauren Liebhaber
Editorial Input from: Julia Cort, Ari Daniel
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation Funding provided by FQXi Music provided by APM
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Host, Producer: Greg Kestin
Filming: Greg Kestin
Research, Writing: Greg Kestin, Samia Bouzid
Editing, Animating: Daniel Thomson
Editorial Input from: Julia Cort, Ari Daniel
Science consultant: Susana Deustua
Media: Shutterstock, NASA, ESA
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation Funding provided by FQXi Music provided by APM
Music: APM
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Host, Producer: Greg Kestin
Filming: Greg Kestin
Research, Writing: Greg Kestin, Samia Bouzid
Editing, Animating: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Science consultant: Susana Deustua
Media: Shutterstock, NASA, ESA
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation Funding provided by FQXi Music provided by APM
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Host, Producer: Greg Kestin
Writing: Greg Kestin, Samia Bouzid
Editorial Input from: Julia Cort, Ari Daniel
Filming: Greg Kestin
Editing: Greg Kestin & Daniel Thomson
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation Funding provided by FQXi
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Host, Producer: Greg Kestin
Research and Writing: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Science Consultant: Murti Salapaka, Saurav Talukdar, Abu Sebastian
Filming, Editing, and Animation: Greg Kestin
Filming, Writing, & Editing Contributions from: Lauren Liebhaber, Daniel Thomson
Media: Shutterstock, CytoViva (Nanoparticles in water)
Brownian Motion Footage courtesy of Sam Snook of Latimer Arts College
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NOVA Wonders "What's the Universe Made of?" pbs.org/video/nova-wonders-whats-the-universe-made-of-2eyoyw
More information on electron orbitals: http://www.mesacc.edu/~kev2077170/supplements/Atoms&orbitals.pdf
Host, Producer: Greg Kestin
Research and Writing: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Science Consultant: Or Hen
Filming, Editing, and Animation: Greg Kestin
Media: Shutterstock
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From the producers of PBS NOVA © WGBH Educational Foundation
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Host, Producer: Greg Kestin
Research, Writing: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Filming, Editing, and Animation: Greg Kestin
Science consultant: Steven A. Rodney, Mark Trodden
Media courtesy of ESO, NASA
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
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Host, Producer: Greg Kestin
Research: Samia Bouzid, Greg Kestin, Peter Chang
Writing: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Filming, Editing, and Animating: Greg Kestin, Samia Bouzid
Scientific Consultants: Mark Hillery, Scott Aaronson
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
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Sound effects: Freesound.org
Silicone heart footage courtesy of ETH Zürich
Fireball animation courtesy of Videocopilot.net
There are three possible answers to this question...but they all break physics as we know it!
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Learn more in NOVA's two-hour special, "Black Hole Apocalypse": http://www.pbs.org/wgbh/nova/space/black-hole-apocalypse.html
CREDITS:
Host, Producer: Greg Kestin
Research: Samia Bouzid, Greg Kestin, and Peter Chang
Writing: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Filming, Editing, and Animation: Greg Kestin and Samia Bouzid
Scientific Consultants: Joe Polchinski, Netta Engelhardt, Steve Giddings
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
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Sound effects: Freesound.org
Images: MEDIODESCOCIDO (Stewie Griffin) and Paul Anderson (Grumpy Cat)
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Learn more in NOVA's two-hour special, "Black Hole Apocalypse": http://www.pbs.org/wgbh/nova/space/black-hole-apocalypse.html
CREDITS:
Host, Producer: Greg Kestin
Researchers: Samia Bouzid, Peter Chang
Writers: Samia Bouzid, Greg Kestin
Scientific Consultants: Joe Polchinski, Andrew Hamilton, Netta Engelhardt, Steve Giddings, Ethan Siegel, Janna Levin
Editorial Input from: Julia Cort, Ari Daniel
Filming and Editing: Greg Kestin
Animation: Greg Kestin and Francesco Castelnovo
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
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Learn more in NOVA's two-hour special, "Black Hole Apocalypse": http://www.pbs.org/wgbh/nova/space/black-hole-apocalypse.html
CREDITS:
Host, Producer: Greg Kestin
Researchers: Samia Bouzid, Peter Chang
Writers: Samia Bouzid, Greg Kestin
Scientific Consultants: Joe Polchinski, Andrew Hamilton, Netta Engelhardt, Steve Giddings, Ethan Siegel, Janna Levin
Editorial Input from: Julia Cort, Ari Daniel
Filming and Editing: Greg Kestin
Animation: Greg Kestin and Francesco Castelnovo
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
Links to unlisted videos along this adventure:
Push Greg into Black Hole: youtube.com/watch?v=Mpgw0oWLzS8
Jump into Black Hole: youtube.com/watch?v=YRPpwUA6nQA
Quantum Death: youtube.com/watch?v=SiutiEXlS60
Gravity Death: youtube.com/watch?v=QIsRZ0nNYcs
Greg Quantum Death: youtube.com/watch?v=hEEtfkclPDw
Greg Gravity Death: youtube.com/watch?v=u0VdQTkc-78
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LINKS AND DETAILS:
More details:
#1. Speed of sound: Unlike light, sound needs a medium to travel through, and its speed depends on characteristics of that medium like density and temperature. In the extreme environment of a neutron star’s core, sound can travel extremely fast. But knowing that sound can’t surpass the speed of light, physicists can narrow down their models of neutron stars to include only those where “extremely fast” is less than light speed.
For more: http://www.phys.utk.edu/news/archives/2015/speed-of-sound.pdf
#2. Invisibility: The invisibility lens pictured in the video was developed at the University of Rochester. For more on how it works: http://www.rochester.edu/newscenter/watch-rochester-cloak-uses-ordinary-lenses-to-hide-objects-across-continuous-range-of-angles-70592/
A more recent attempt at invisibility: ft.com/content/c6864c76-de7d-11e7-a0d4-0944c5f49e46
#3. Relativity rainbows: A team at MIT created a game called “A Slower Speed of Light” that lets you see the world as you would at near-light speeds. Their trailer: youtube.com/watch?v=uu7jA8EHi_0
#4. Acoustic levitation: A demo from Harvard Natural Sciences Lecture Demonstrations: youtube.com/watch?v=XpNbyfxxkWE
#5: Quantum cloning: A video from MinutePhysics on why quantum mechanics doesn’t allow cloning: youtube.com/watch?v=owPC60Ue0BE
CREDITS:
Host, Producer: Greg Kestin
Researchers: Greg Kestin, Samia Bouzid
Writers: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Filming: Greg Kestin
Editing: Greg Kestin, Samia Bouzid
Media: Hubble, NASA
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Ultrasonic Levitation video footage courtesy Harvard Natural Sciences Lecture Demonstrations
Ultrasonic Levitation still courtesy of Argonne National Laboratory
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Sound effects: Freesound.org
Today we’re remembering Stephen Hawking, who shone light on the darkest places in the universe.
Video about information paradox: youtu.be/jyFAsbBvZ70
Credits
Host, Producer: Greg Kestin
Researchers: Greg Kestin, Samia Bouzid
Writers: Samia Bouzid, Greg Kestin
Editorial Input from: Julia Cort, Ari Daniel
Black Hole Animations: Edgeworx
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
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*learn more about electron volts here: en.wikipedia.org/wiki/Electronvolt
Host, Producer: Greg Kestin
Researchers: Samia Bouzid, Drew Gannon, Peter Chang
Writers: Samia Bouzid, Greg Kestin
Fish voices: Tiffany Dill, Arlo Perez
Scientific Consultant: Alan Lightman, Curtis McCully
Editorial Input from: Julia Cort, Ari Daniel
Filming: Greg Kestin
Animation and Editing: Greg Kestin
Special thanks: Entire NOVA team
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Here is the research paper: nature.com/articles/nature25792
Authors: Judd D. Bowman, Alan E. E. Rogers, Raul A. Monsalve, Thomas J. Mozdzen & Nivedita Mahesh
This evidence seems to suggest that the dark matter is particles that are less than four times the mass of a proton and are moving at non-relativistic speeds. This is consistent with dark matter particles being so-called WIMPs: en.wikipedia.org/wiki/Weakly_interacting_massive_particles.
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Credits
Host, Producer: Greg Kestin
Researchers: Greg Kestin, Samia Bouzid
Writers: Greg Kestin, Samia Bouzid
Scientific Consultant: Douglas Finkbeiner
Editorial input from: Julia Cort, Ari Daniel
Filming: Greg Kestin
Animation and Editing: Greg Kestin
Special thanks: Avi Loeb, entire NOVA team
Media Courtesy of: NASA, ESO, and CERN
Dark matter halo footage courtesy of ESO/L. Calçada.
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CREDITS:
Host, Producer: Greg Kestin
Researcher: Samia Bouzid
Writers: Samia Bouzid, Greg Kestin
Scientific Consultants: Sabine Hossenfelder, Dave Goldberg
Editorial Input from: Julia Cort, Ari Daniel, David Condon
Filming: Greg Kestin, Peter Chang, Samia Bouzid
Animation and Editing: Greg Kestin
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
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Music provided by APM
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Three of the answers are related to previous videos:
- How to See Quantum with the Naked Eye: youtube.com/watch?v=YiZP6YpnMds
- Can We Measure Consciousness? youtube.com/watch?v=laOZjSFdj24
- 3 Things Faster than Light: youtube.com/watch?v=kNqf-FsUMww
Images courtesy of CERN and ATLAS.
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Check out youtube.com/user/EugeneKhutoryansky, who was kind enough to share his water wave animation with us.
ADVANCED SCIENTIFIC NOTE: Quantum mechanics would be much more obvious if we had very sensitive eyes. If your eyes identified each photon individually, you would see them land as described in the video, and only build up to this wave pattern. The pattern that we see can be explained classically by waves, it is *ultimately* a quantum phenomenon. The only reason it's hard to tell is because our light detectors (eyes) aren't quite sensitive enough.
CREDITS:
Host, Producer: Greg Kestin
Researcher: Samia Bouzid
Writers: Samia Bouzid, Greg Kestin
Scientific Consultant: Louis Deslauriers
Editorial Input from: Julia Cort, Ari Daniel
Animation and Editing: Greg Kestin
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Footage of bridge and man holding child: Videoblocks
Sound effects: Freesound.org
Watch "Black Hole Apocalypse" Here: http://www.pbs.org/wgbh/nova/space/black-hole-apocalypse.html
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Host, Writer, Producer: Greg Kestin
Scientific Consultant: Samir Mathur
Editorial Input from: Julia Cort
Animation: Edgeworx
Animation and Editing: Greg Kestin
Special thanks: Entire NOVA team
From the producers of PBS NOVA © WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
Watch "Black Hole Apocalypse" Here: http://www.pbs.org/wgbh/nova/space/black-hole-apocalypse.html
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Writer, Host, Producer: Greg Kestin
Cinematography: Brian Kantor and Ari Daniel
Editorial Input form: Julia Cort
Editor in Chief, Cook's Illustrated: Dan Souza
Senior Editor, Cook's Illustrated: Lan Lam
Scientific Consultants: Scott Kenyon
Animation: Edgeworx
Editing and Animation: Greg Kestin
Special thanks: Entire NOVA and Cook's Illustrated teams
From the producers of PBS NOVA © WGBH Educational Foundation
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b.) As much as a water molecule
c.) As much as a mosquito
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SCIENTIFIC NOTES:
* The relationship between information and energy comes from Landauer's Principle, which connects the erasure of information and energy. But, more generally changes in information (e.g. recording information) are related to changes in energy. I will talk more about this in a future episode about the physics of memory, and why you will forget everything you ever knew! en.wikipedia.org/wiki/Landauer%27s_principle
* The numbers calculated in this video give a lower limit on the energy to record a particular amount of information, but to create a more permanent storage of information would require more energy.
* Retina display resolution, as it's name implies, is similar to the eye's resolution.
CREDITS:
Host, Producer: Greg Kestin
Researcher: Samia Bouzid
Writer:
Samia Bouzid
Greg Kestin
Animation & Compositing:
Danielle Gustitus
Greg Kestin
Contributing Writer:
Lissy Herman
Scientific Consultants:
Frank Haist
Murti Salapaka
Filming, Writing, & Editing Contributions from:
Samia Bouzid
David Goodliffe
Brian Kantor
Guest Appearances:
Lindsey Chou
Ana Aceves
Drew Gannon
Editorial Input form:
Julia Cort
Anna Rothschild
Special thanks:
Ari Daniel
Allison Eck
Fernando Becerra
Gil Kaplan
Eric Brass
Lauren Miller
And the entire NOVA team
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
Neuron & Digital Brain footage: Pond5
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SCIENTIFIC NOTES:
* Simulation of animats (simulated beings) from generation to generation, showing increase of phi: http://integratedinformationtheory.org/animats.html
* Research paper on Integrated Information Theory 3.0: http://journals.plos.org/ploscompbiol/article?id=10.1371/journal.pcbi.1003588
* More on medical uses of IIT with EEG: http://stm.sciencemag.org/content/5/198/198ra105.short
* More on Behavioral Zombies and Philosophical Zombies: en.wikipedia.org/wiki/Philosophical_zombie#Types_of_zombies
* More on the relationship between consciousness and free will: http://www.scholarpedia.org/article/Integrated_information_theory
CREDITS:
Host, Writer, Producer: Greg Kestin
Animation & Compositing: Marquee Productions & Greg Kestin
Contributing Writer: Lissy Herman
Scientific Consultants:
Masafumi Oizumi
Larissa Albantakis
Christof Koch
Filming, Writing, & Editing Contributions from:
Samia Bouzid and David Goodliffe
Image Contributions from: Drew Ganon
Editorial Input form:
Julia Cort
Lauren Aguirre
Anna Rothschild
Special thanks:
Ari Daniel
Allison Eck
Fernando Becerra
Gil Kaplan
Bella Solanot
Eric Brass
Lauren Miller
And the entire NOVA team
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
Neuron & MRI footage: Pond5
Additional footage from: Rise of the Robots, find credits at
http://www.pbs.org/wgbh/nova/tech/rise-of-the-robots.html
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Scientific notes:
Stellar mass black holes vs. supermassive black holes
* Stellar mass black holes form from the collapse of massive stars at the ends of their lives, so they have roughly the same mass as a star. Supermassive black holes are physically identical to their smaller counterparts, except they are 10 thousand to a billion times the size of the sun. However, their formation is more of a mystery. They may form from the merging of smaller black holes.
http://astronomy.swin.edu.au/cosmos/S/Supermassive+Black+Hole
Supermassive black holes at the center of galaxies
* Almost every large galaxy has a supermassive black hole at its center, but researchers are not yet sure (https://jila.colorado.edu/research/astrophysics/black-holes-galaxies) why that’s the case, how they originate, and what their role is in the creation and evolution of galaxies.
Why are stars different colors?
* The color of a star depends on its temperature (http://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_colour.html). The hotter a star, the higher energy its light will be. Higher energy/temperature corresponds with the blue end of the visible spectrum and lower energy/temperature corresponds with the red end.
How does dark matter make stars spin faster?
* In the 1960s, astronomers Vera Rubin and Kent Ford noticed that stars at the edges of galaxies were moving just as fast as stars at the center, which surprised them: it appeared that the force of gravity causing stars to orbit the center of the galaxy was not weakening over distance. Their observation implied that something else, distributed throughout the galaxy, was exerting a gravitation pull. We now know that that “something else,” now named dark matter, accounts for about 85% of the matter in the universe. (It existence was inferred in the 1930s, when the astronomer Fritz Zwicky(http://www2.astro.psu.edu/users/rbc/a1/week_10.html) noticed that galaxies in clusters were moving faster than they should.)
Size of the universe
* The universe is only 13.8 billion years old, but has a radius of about 46 billion light-years. If nothing can travel faster than the speed of light, how can that be? The expansion of the universe, driven by dark energy, is causing distances between objects to grow. Note that it is not moving those objects apart; rather, it is increasing the amount of space between them. phys.org/news/2015-10-big-universe.html
Cosmic webs
* Galaxies are not distributed randomly (http://skyserver.sdss.org/dr1/en/astro/structures/structures.asp) in space; instead, clusters of galaxies form web-like patterns. These webs consist of filaments, where dark matter and ordinary (baryonic) matter are concentrated, and voids, where galaxies are scarce. Researchers believe that these large-scale structures grew out of minor fluctuations in density at the beginning of the universe.
Composition of the early universe
* Moments after the Big Bang, the universe formed the nuclei for what would be come the universe’s hydrogen and helium atoms, with one helium nucleus for every 10 or 11 hydrogen (http://umich.edu/~gs265/bigbang.htm). When the first stars formed, there were no heavier elements — those elements formed inside stars.
String Theory Landscape
* The String Theory Landscape is a theory that the universe we live in is one of many universes. It attempts to explain how certain constants of nature seem “fine-tuned” for life, which contradicts the anthropic principle, or the notion that we humans hold a special place in the universe. scientificamerican.com/article/multiverse-the-case-for-parallel-universe/%0A
Disintegration of the universe
* In the future Degenerate Era of the universe, as space-time expands and stars burn up, all of the matter in stars will be consumed by black holes. But even black holes are not forever. Stephen Hawking theorized that black holes will slowly radiate away their mass in what is now called Hawking radiation until they too dissipate away. http://www.nytimes.com/books/first/a/adams-universe.html
______
MEDIA CREDITS:
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Additional Animations:
- Galaxy within Universe: Edgeworx;
- Stars at center of Milky Way - NASA/NCSA University of Illinois Visualization by Frank Summers, Space Telescope Science Institute, Simulation by Martin White and Lars Hernquist, Harvard University
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SCIENTIFIC NOTES:
Explosive young stars
* The average lifetime of a star is about 10 billion years, but the bigger the star, the shorter its life. One rare type of star, called a hypergiant, can be tens, hundreds, or even a thousand times the mass of our sun. These stars burn out and explode into supernovae in just a few million years.
http://www.guide-to-the-universe.com/hypergiant-star.html
Black holes
* Black holes form from the collapse of a massive star at the end of its life, but this only happens in stars about three times as massive as the sun. http://burro.case.edu/Academics/Astr201/EndofSun.pdf
How big is the universe?
* Probably infinite. No one knows the size of the universe for sure, and we may never know, but the latest thinking is that it probably goes on forever. map.gsfc.nasa.gov/universe/uni_shape.html
Standard cosmological model
* According to the standard cosmological model, the universe started with a big bang, underwent rapid inflation within the first fraction of a second, and continues to expand, driven by a vacuum energy called dark energy. All of the structure we see in the universe has come from interactions between dark energy and dark matter (which accounts for about 85% of the universe’s matter). This model describes and predicts many phenomena in the universe but is not perfect. physics.aps.org/articles/v8/108
False vacuum model
* The false vacuum model is a real, albeit unlikely theory. All the fundamental forces of nature have corresponding fields (e.g., gravitational fields, magnetic fields, etc.), and we generally believe that the universe is at rest in a global minimum of the potentials of those fields. But if we are instead at rest in a local minimum, or a “false vacuum,” the universe could potentially be nudged, catastrophically, into a lower minimum.
Recycling stars into life
* Before the first stars, the universe was all hydrogen and helium. All heavier elements, including the building blocks of life, were forged in stars.
Dark matter and dark energy
* Only 5% of the universe is made up of matter we can see. The “missing mass” later dubbed dark matter was first noticed in the 1930s; dark energy was discovered in the 1990s. In both cases, their existence was inferred by their effect on objects they interact with. However, they are still not directly observable, so nobody knows yet what they are made of.
Leftover light from the Big Bang
* The theory of the Big Bang predicted the existence of cool radiation pervading the universe, left over from its beginning. In an accidental discovery, two New Jersey scientists discovered the cosmic microwave background, a nearly uniform bath of radiation throughout the universe at a temperature of about 3 Kelvin, or -454 degrees Fahrenheit.
Gravitational waves
* Albert Einstein predicted the existence of gravitational waves in his theory of general relativity in 1916. According to his theory, the acceleration of massive objects, like black holes, should send ripples through space-time at the speed of light. A century after his prediction, two merging black holes sent a ripple through space-time that was detected on Earth as a signal that stretched the 4-kilometer arms of a detector by less than 1/1,000 the width of a proton.
Cosmic dust
* Cosmic dust is cast off from stars at the end of their lives and hovers in galaxies as clouds. These clouds of dust absorb ultraviolet and visible light, obscuring much of what lies behind them. This makes it notoriously difficult to study things like the dusty center of our galaxy.
Fermi bubbles
* Enormous bubbles of gamma rays protruding above and below the center of the galaxy, roughly along its axis of rotation. http://www.skyandtelescope.com/astronomy-resources/understanding-fermi-bubbles
The observable universe
* The universe is 13.8 billion years old. Since the distance we can observe is limited by the time it takes light to travel to Earth, we can only ever observe a fraction of the universe: an expanding sphere around us that is now about 46 billion years in radius. However, the universe is much larger than what we can observe.
CREDITS:
Host, Writer, Producer: Greg Kestin
Animation & Compositing: Danielle Gustitus
Contributing Writers: Lissy Herman, HCSUCS
Filming, Writing, & Editing Contributions from:
Samia Bouzid and David Goodliffe
Creation of Sad Star Image: Drew Ganon
Special thanks:
Julia Cort
Lauren Aguirre
Ari Daniel
Anna Rothschild
Allison Eck
Fernando Becerra
And the entire NOVA team
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Music provided by APM
Sound effects: Freesound.org
Images: Big Bang – NASA
Additional Animations: Edgeworx
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More about the experiment:
Marissa Giustina’s research: http://arxiv.org/abs/1511.03190
Advanced scientific note about Doppler: If there is a light moving away from you at constant velocity in static flat (Minkowski) space-time, no matter how red it is, you will never conclude it is going faster than light. But, here I am discussing the conclusions one might come to if you mistakenly use Doppler in the context of the curved space-time of the universe (where there is expansion). Interpreting the huge redshift as a result of the doppler effect, could make one think that galaxies we see are moving away at speeds approaching light speed. And since what we are actually seeing is light from those galaxies from billions of years ago, and given that the universe is expanding, you might be tempted to say that they have since "accelerated" to faster than the speed of light. You might go further and say that there are more distant galaxies that we can't see which are moving away even faster. So you might conclude there are galaxies moving faster than light in the universe. But the redshift isn't from doppler and this "acceleration" of the expanding universe isn't actually causing a true increase in velocity.
Sometimes astronomers do say there is a faster than light "recession speed" by pretending the expansion of the universe is causing distant galaxies to move away from each other at a corresponding velocity, but that's misleading. In general relativity, you can actually have an increase in space between objects without causing a corresponding increase in the relatives velocities of those objects.
CREDITS:
Host, Writer, Animator, Editor:
Greg Kestin
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Special thanks:
Marissa Giustina
Nick Hutzler
Julie Elksy
Byron Drury
Jacob Barandes
Tyler Howe
Lissy Herman
Ari Daniel
Lauren Aguirre
Kristine Allington
Allison Eck
Anna Rotschild
MEDIA CREDITS:
Music provided by APM:
Deep_Science_No-perc
Mysteries_of_Science_B
Dreaming_of_the_Stars_a
Curiosity_Kills_the_Cat_2
Conundrum_a
Images:
Stars - Rene Barrios
Earth - Eirika
galaxy spiral (by coornio - diviantart)
Squirrel with scissors - 60811670 - Dollarphotoclub
Equations - 91613623 - Dollarphotoclub
Maxresdefault - Sean Stewart
Marissa Giustina - Lammerhuber
Tangled cat - David Swayze
Cat doll - Vicky Somma
Stock footage:
train-exits-tunnel - Pond5
Bin_pulsar_442 - Courtesy of Nasa
Expanding in space (40294) - Courtesy of Nasa
WMAP_archive - Courtesy of Nasa
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More about the experiment:
physics.aps.org/story/v16/st1
uam.es/personal_pdi/ciencias/jcuevas/Teaching/Pound-Rebka-PRL1960.pdf
CREDITS:
Host, Writer, Animator, Editor:
Greg Kestin
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Special thanks:
Tyler Howe
Ari Daniel
Paul Horowitz
Sara Tewksbury
Seeta Joseph
Karishma Desai
Lauren Aguirre
Kristine Allington
Allison Eck
Lauren Miller
Stuart McNeil
MEDIA CREDITS:
Music provided by APM:
Inside_The_Lab_A
Sound effects:
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ambulance-city-street-night - Pond5
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CREDITS:
Host, Writer, Animator, Editor:
Greg Kestin
Special thanks:
Tyler Howe
Julie Elsky
Lissy Herman
Patrick Mitran
Jerry Gibson
Lauren Aguirre
Kristine Allington
Anna Rothschild
Allison Eck
Ari Daniel
Lauren Miller
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
SCIENTIFIC NOTES:
- Messages can also be encoded by altering the phase of the signal being sent from the antenna.
- Phones use several (~8) frequencies at one time, and since there are limited frequencies (~100) for the tower to use, manages the sharing of them.
MEDIA CREDITS:
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Curio C
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Freesound.org
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Two tree cell towers (Devra)
Top of cell tower (Ervins Strauhmanis)
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digital-computer-brain-binary
bangkok-city-skyline-aerial-da
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Try a mini version of this at home: youtu.be/ho0o7H6dXSU
CREDITS:
Host, Writer, Animator, Editor:
Greg Kestin
From the producers of PBS NOVA
© WGBH Educational Foundation
Funding provided by FQXi
Special thanks:
Tyler Howe
Ari Daniel
Lissy Herman
Kurt Kolasinski
David Allara
Patrick Lake
Ryan Mckell
Lauren Aguirre
Kristine Allington
Anna Rothschild
Allison Eck
Lauren Miller
Peter Behroozi
Fred Behroozi
Daniel Rosenberg
Kesto Productions
MEDIA CREDITS:
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C'est La Vie
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Little Jynx
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Gangster Benjamin Franklin from Compton (Philip Taylor)
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sea_waves_prores - Pond5


