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Sources: • Stirling Bridge & Falkirk 1297-98 (Pete Armstrong). ISBN: 978-1-84176-510-5 • Robert the Bruce, King of Scots (Ronald McNair Scott). ISBN: 978-1-78211-177-1 • A Great and Terrible King: Edward I and the Forging of Britain (Marc Morris). ISBN: 978-0-091-79684-6 • The Hammer of the Scots: Edward I and the Scottish Wars of Independence (David Santiuste). ISBN: 978-1-78159-012-6 • Edward I (Michael Prestwich). ISBN: 978-0-300-07157-3 • William Wallace: Brave Heart (James MacKay). ISBN: 9781780574288
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🚩 Over the past decade, Bulgarian armies under Samuel had conquered much of the European possessions of the Byzantine Empire. In 986, Basil II led the campaign personally with 30,000 soldiers. This much larger than average Roman field army showed the importance the Emperor placed on the threat from Bulgaria and the intent to subdue the Bulgarians with one strike…
🚩 On June 24th, 1812, the French Emperor Napoleon led 450 thousand men across the Niemen River into Russia, beginning one of the most notorious military disasters in history. Throughout this 6-month campaign, both French and Russian commanders would struggle with forces far greater than any army: politics, logistics and of course, nature.
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📢 Narrated by David McCallion
🎼 Music: EpidemicSound.com Filmstro
📚 Sources: Chandler D. The Campaigns of Napoleon. Weidenfeld & Nicolson Ltd 1966. Griess T ed. Atlas for the Wars of Napoleon. Avery Publishing Group Inc 1986. Hartley J, Keenan P, Lieven D eds. Russia and the Napoleonic Wars. Palgrave MacMillan 2015. Lieven D. Russia Against Napoleon. Viking 2010. Nafziger G. Napoleon’s Invasion of Russia. Presidio 1988. Black J. The French Revolution and Napoleonic Wars. Rowman & Littlefield 2022. Nester W. Napoleon and the Art of Diplomacy. Savas Beatie 2012. Voelcker T. Admiral Saumarez versus Napoleon. The Boydell Press 2008. Lunde H. A Warrior Dynasty. Casemate 2014. [Charles XII] Marvin Girelli
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🚩 The Battle of Tifernum (297 BC) was an important battle of the Third Samnite War, fought between the Romans and the Samnites near the modern town of Città di Castello in central Italy. The outcome of this clash would lead to the decisive Battle of Sentinum in 295 BC…
📚 Sources: Cassius Dio, Roman History Diodorus Siculus, Library of History Dionysius of Halicarnassus, Roman Antiquities Frontinus, Stratagems Livy, From the Founding of the City Polybius, Histories Zonaras, Epitome of Histories Bradley, G. 2020: Early Rome to 290 BC: The Beginnings of the City and the Rise of the Republic, Edinburgh. Cornell, T. 2017: ‘The “Samnite Wars,” 343-290 BC, in M. Whitby & H. Sidebottom (eds.), The Encyclopedia of Ancient Battles, Malden MA, Oxford & Chichester, West Sussex, 2.469-479. Forsyth, G. 2006: A Critical History of Early Rome: From Prehistory to the First Punic War, Berkeley. Oakley, S. P. 1997-2005: A Commentary on Livy, Books VI-X, Oxford.
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🚩 On June 24th, 1812, the French Emperor Napoleon led 450 thousand men across the Niemen River into Russia, beginning one of the most notorious military disasters in history. Throughout this 6-month campaign, both French and Russian commanders would struggle with forces far greater than any army: politics, logistics and of course, nature.
🚩 Support HistoryMarche on Patreon and for as little as $1 per video you get ad-free early access to our videos: https://www.patreon.com/historymarche
📢 Narrated by David McCallion
🎼 Music: EpidemicSound.com Filmstro
📚 Sources: Chandler D. The Campaigns of Napoleon. Weidenfeld & Nicolson Ltd 1966. Griess T ed. Atlas for the Wars of Napoleon. Avery Publishing Group Inc 1986. Hartley J, Keenan P, Lieven D eds. Russia and the Napoleonic Wars. Palgrave MacMillan 2015. Lieven D. Russia Against Napoleon. Viking 2010. Nafziger G. Napoleon’s Invasion of Russia. Presidio 1988. Black J. The French Revolution and Napoleonic Wars. Rowman & Littlefield 2022. Nester W. Napoleon and the Art of Diplomacy. Savas Beatie 2012. Voelcker T. Admiral Saumarez versus Napoleon. The Boydell Press 2008. Lunde H. A Warrior Dynasty. Casemate 2014. [Charles XII] Marvin Girelli
🚩 Keep exploring at http://brilliant.org/HistoryMarche/. Get started for free, and hurry—the first 200 people get 20% off an annual premium subscription. 👇 Push down for more cool stuff 👇
🚩The Second Battle of Mohács was part of the 1683-1699 Great Turkish War, which pitted the Ottomans against one of the several “Holy Leagues” thrown together over the decades to try to counter them. The Battle of Mohacs was one of the turning points that swung the war in favor of the Habsburgs.
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📢 Narrated by David McCallion
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Sources: Finkel, Caroline. Osman’s Dream: The History of the Ottoman Empire. Hachette UK, 2007. Szita, László. THE BATTLE OF SZÁRSOMLYÓ MOUNTAIN (1687) (Hungary, 1987) Abbott, J. History of the Habsburg Empire (Madison & Adams Press, 2018). Childs, J. C. R., & Childs, J. Armies and warfare in Europe, 1648-1789. (Manchester University Press, 1982). Charles Joseph. The Life of Prince Eugene, of Savoy: From His Own Original Manuscript. Vol. 3. J. Davis, 1812. Šegvić, Filip Šimetin, and Tomislav Branđolica. “The age of heroes in historiography: the example of Prince Eugene of Savoy.” Austrian History Yearbook 44 (2013): 211-233. Wheatcroft, Enemy at the Gate
Prince Eugene Playlist: Episode 1: https://youtu.be/XPmPiww_4o0 Episode 2: Coming soon Episode 3 and beyond: Working on it
🚩 The Second Turkish Siege of Vienna in 1683 was followed by a Habsburg offensive, during which Prince Eugene of Savoy became its foremost luminary. The siege of Buda in 1686 was fought between the Holy League and the Ottoman Empire, ending almost 150 years of Turkish rule. Although Eugene played a minor role in the siege, it was during these early encounters of the Long Turkish War that he made a name for himself and rose through the ranks.
🚩 Support HistoryMarche on Patreon and for as little as $1 per video you get ad-free early access to our videos: https://www.patreon.com/historymarche
📢 Narrated by David McCallion
🎼 Music: EpidemicSound.com Filmstro
📚 Sources: Abbott, J. History of the Habsburg Empire (Madison & Adams Press, 2018). Childs, J. C. R., & Childs, J. Armies and warfare in Europe, 1648-1789. (Manchester University Press, 1982). Charles Joseph. The Life of Prince Eugene, of Savoy: From His Own Original Manuscript. Vol. 3. J. Davis, 1812. Šegvić, Filip Šimetin, and Tomislav Branđolica. “The age of heroes in historiography: the example of Prince Eugene of Savoy.” Austrian History Yearbook 44 (2013): 211-233. Wheatcroft, Enemy at the Gate, 216-225 A historical description of the glorious conquest of the city of Buda pp. 20–23, especially 9 July
🚩 The Battle of the Catalaunian Plains, (AD 451), battle fought between the Huns under Attila and a mixed Roman and Visigoth force under Aetius and Theodoric I; checked the Hunnic advance in Europe. The battle, long-remembered for its ferocity, resulted in Attila’s defeat, though the casualty figures in traditional accounts are probably exaggerated. The Huns’ defeat prevented the widespread destruction and spoliation of Gaul, but it is unlikely that Attila’s horde could have made any deep impression upon the Latin and urban character of the country.
🚩 I combined all parts of our “Battle of the Catalaunian Plains” mini-series for easier viewing. This video was chosen by my Patrons. Thank you so much for your likes and comments ❤️. If you enjoy my videos please consider subscribing.
The Coriolis effect says that anytime you’re rotating—whether it’s on a playground toy or your home planet—objects moving in straight lines will appear to curve. This bizarre phenomenon affects many things, from the paths of missiles to the formation of hurricanes.
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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Are wormholes real or are they just magic disguised as physics and maths? And if they are real how do they work and where can we find them?
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You’ve probably seen atoms like this emoji ⚛ everywhere from science textbooks to the logo for The Big Bang Theory. But what does an atom really look like? The truth is much stranger.
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What if the Earth were swallowed by a black hole? Would humanity’s legacy be gone forever? Or could you somehow get back that information from behind the event horizon?
There are three possible answers to this question…but they all break physics as we know it!
Have you ever wondered what it would be like to fall into a black hole? Take a 360° adventure to find out!
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#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.
#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: https://www.youtube.com/watch?v=uu7jA8EHi_0
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: https://en.wikipedia.org/wiki/Weakly_interacting_massive_particles.
Is String Theory the final solution for all of physic’s questions or an overhyped dead end?
This video was realised with the help of Dr. Alessandro Sfondrini and it was funded by SNSF under Agora Grant n. 171622 and through the NCCR SwissMAP: The Mathematics of Physics.
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We did something a little different in this episode and answered questions from you, our viewers. If you have a questions about the universe, past videos, or life as a scientist, leave a comment below!
How can you train yourself to be a quantum detector? Quantum interactions happen at impossibly small scales. But the life-size effects are all around you. You can detect quantum mechanics all over — if you know how to look for it.
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.
NOVA has teamed up with Cook’s Illustrated to cook up a recipe for stars and black holes – a culinary “course” on how the most mysterious objects in the universe are created.
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! https://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.
What makes a brain or machine conscious? Will robots become more conscious than we are? One theory, which can actually calculate consciousness, is beginning to provide some answers.
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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. https://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. https://www.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
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MEDIA CREDITS:
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Sound effects: Freesound.org
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– 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
What if everything in the universe came to your doorstep…in a box?! What The Physics is BACK! Future episodes will explore the universe—but first, let’s unbox it.
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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. https://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. https://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.
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
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Ari Daniel
Anna Rothschild
Allison Eck
Fernando Becerra
And the entire NOVA team
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Designer babies, the end of diseases, genetically modified humans that never age. Outrageous things that used to be science fiction are suddenly becoming reality. The only thing we know for sure is that things will change irreversibly.
Thanks to Volker Henn, James Gurney and (prefers anonymity) for help with this video!
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SOURCES AND FURTHER READING:
The best book we read about the topic: GMO Sapiens