Hoy descubriremos la ciencia involucrada en el proceso de depilación con laser.
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El láser que se usa tiene una longitud de onda de 1064 nanómetros es decir que es radiación infrarroja, invisible para nuestros ojo.
Los ojos oscuros, la piel y el cabello contienen una molécula llamada melanina que absorbe una amplia gama de longitudes de onda de luz, especialmente en la parte ultravioleta del espectro, y crea un escudo ideal contra los rayos dañinos del sol. Es por esto que te bronceas cuando tomas sol.
Ese es tu cuerpo que produce y libera más melanina en la piel.
Pero la idea con la depilación láser es hacer que los cabellos oscuros absorban la luz laser sin que la piel alrededor absorba mucha energía.
Entonces, funciona mejor si tienes cabellos oscuros y piel clara.

Un agradecimiento especial a Laser Away en Santa Mónica por ayudar a que esto suceda, ¡Su staff fue increíble! http://bit.ly/VeLaserAway

Además, quiero agradecer a Darren, sin BeyondSlowMotion nunca podríamos haber hecho esto. http://bit.ly/VeBeyondSlowMo

Investigación y filmación de Raquel Nuno y Aaron White.
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Traductora: Paula Salomone
Voz de doblaje: Pato Lago, Diego Rivas, Julia Gonzalez Biondini
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Edición y post-producción de video: Juan Caille Tornquist
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La teoría del Caos significa que los sistemas deterministas pueden ser impredecibles.
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¿Quiere saber más sobre la teoría del caos y los sistemas dinámicos no lineales?
Echa un vistazo: https://ve42.co/chaos-math
Hace tiempo que quería hacer un video sobre el caos. Fue desde que leí el fantástico libro de James Gleick, Chaos. Espero que este video dé una idea del espacio fásico: una imagen de los sistemas dinámicos en los que cada punto representa completamente el estado del sistema.
Para un péndulo, el espacio fásico es solo bidimensional y se pueden obtener órbitas (en el caso de un péndulo no amortiguado) o una espiral interna (en el caso de un péndulo con fricción).
Con las ecuaciones de Lorenz necesitamos tres dimensiones para mostrar el espacio fásico. Se dice que el atractor que encuentras para estas ecuaciones es extraño y caótico porque no hay un bucle (loop), solo curvas infinitas que nunca se cruzan. Esto explica por qué el movimiento es tan impredecible: dos condiciones iniciales diferentes que están muy juntas pueden terminar arbitrariamente separadas.

Imágenes de mariposa, cortesía de Phil Torres y The Jungle Diaries: https://ve42.co/monarch
Sistema solar, animaciones de 3 cuerpos e impresión de Jonny Hyman
Algunas animaciones hechas con Universe Sandbox: https://universesandbox.com/
Un agradecimiento especial al Prof. Mason Porter en UCLA, a quien entrevisté para este video.

Música de https://epidemicsound.com "The Longest Rest" "A Sound Foundation" "Seaweed"
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Se ha predicho que un planeta podría estar orbitando al Sol con un período de 10,000 años y una masa 5 veces mayor que la de la Tierra, en una órbita altamente elíptica e inclinada. ¿Qué evidencia respalda la existencia de un objeto tan extraño en el borde de nuestro sistema solar? SUSCRÍBETE ahora para ver todos nuestros videos:
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Escuché sobre el Planeta 9 durante mucho tiempo, pero me preguntaba qué tipo de evidencia podría apoyar esa afirmación tan audaz: un planeta en los límites de nuestra capacidad para detectarlo, tan lejos que su período es 60 veces el de Neptuno. La hipótesis del planeta 9 ayuda a explicar la agrupación de órbitas de objetos distantes del cinturón de Kuiper. También explica cómo algunos de estos objetos tienen órbitas muy inclinadas, hasta 90 grados, en relación con el plano del sistema solar. Incluso algunos orbitan en reversa. El hecho de que el perihelio esté tan alejado sugiere que otra fuente de gravedad era esencial para sus órbitas peculiares.

Muchas gracias a:
Prof. Konstantin Batygin, Caltech
Prof. David Jewitt, UCLA
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Einstein's classic thought experiment involves sitting on a train travelling at the speed of light. If you hold a mirror in front of your face, will you see your reflection in a mirror? How could light from your face reach the mirror if the mirror is travelling away from you? But it would be a pretty spooky train if you couldn't see your reflection so Einstein felt this solution wasn't realistic. On the other hand if you could see your reflection, it would mean light was travelling at the speed of light inside the train. But that meant the same light observed from outside the train would be going twice the speed of light. This again seems inconsistent. So Einstein resolved that you must see your reflection but that light must travel at the same speed inside and outside the train. The only way this is possible is if space and time are perceived differently by observers inside and outside the train.

How much would it take for you to risk $10?
Check out Audible: http://bit.ly/AudibleVe
Can you solve this? http://bit.ly/248Ve
Regression to the mean: http://bit.ly/VeRTTM

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Psychological literature shows that we are more sensitive to small losses and than small gains, with most people valuing a loss around 1.5-2.5 times as much as a gain. This means that we often turn down reasonable opportunities for fear of the loss. However over the course of our lives we will be exposed to many risks and opportunities and this invariably means that taking every small reasonable bet will leave us better off than saying no to all of them.

NOTE: The video is not saying to accept every bet, only those with reasonable odds (preferably in your favour), and those which if you lose would not cause significant financial or other damage. In those cases it is wise to be loss averse!

Filmed by Adrian Tan

Thanks to Physics Girl for suggestions on previous versions of this video. https://www.youtube.com/physicswoman

Why does time appear to speed up as we get older? Can we slow it down?
Thanks to the National Geographic Channel for sponsoring this video!
The new season of Brain Games starts Sunday, February 14th at 9/8c - http://po.st/90S7Ow

Brain Games is an Emmy-nominated TV series that explores the inner workings of the human mind through experiments and interactive games. Did you know it's estimated that you have more than a dozen senses in addition to the standard five? One of those is a sense of time or chronoception. Tune in to the new season of Brain Games to learn about all of your senses, and more, starting Sunday, February 14 at 9/8c

References:

Ageing and duration judgement:
http://bit.ly/1TRN0cr

Nerve conduction velocity slowing with age:
http://bit.ly/23Wq6oE

Experiments with rats suggest time perception is distributed across brain:
http://bit.ly/1T6IjdO

Time perception with repeated stimuli:
http://bit.ly/1TRNbo5

Energy usage in brain with age:
http://bit.ly/1nXliOU

Time perception in moments of fear / danger:
http://bit.ly/1RoK7Ps
http://1.usa.gov/1TRNa3w
http://bit.ly/1Q8tDvW

Attention’s relation to time perception and recollection of perceived time:
http://bit.ly/20odeD8
http://bit.ly/1TRNfEf

The merging of two neutron stars was detected by gravitational waves and then by telescopes in all parts of the electromagnetic spectrum. This is a historic detection as it demonstrates:
- the first gravitational waves detected from inspiraling neutron stars
- the first joint observation by gravitational wave and electromagnetic wave astronomy
- identification of a gamma ray burst in conjunction with merging neutron stars
- how gravitational waves and gamma rays can be used together to locate their source

All evidence so far indicates that the data support General Relativity.

Special thanks to Patreon supporters:
Tony Fadell, Donal Botkin, Curational, Jeff Straathof, Zach Mueller, Ron Neal, Nathan Hansen, Corvi

Support Veritasium on Patreon: http://ve42.co/patreon

Graphics from:
Jets and Debris from a Neutron Star Collision
This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817. They include gravitational waves (pale arcs); a near-light-speed jet that produced gamma rays (magenta); expanding debris from a "kilonova" that produced ultraviolet (violet), optical and infrared (blue-white to red) emission; and, once the jet directed toward us expanded into our view from Earth, X-rays (blue).
Credit: NASA's Goddard Space Flight Center/CI Lab

Virgo Helps Localize Gravitational-Wave Signals
Sky localizations of gravitational-wave signals detected by LIGO beginning in 2015 (GW150914, LVT151012, GW151226, GW170104), and, more recently, by the LIGO-Virgo network (GW170814, GW170817). After Virgo came online in August 2017, scientists were better able to localize the gravitational-wave signals. The background is an optical image of the Milky Way. The localizations of GW150914, LVT151012, and GW170104 wrap around the celestial sphere, so the sky map is shown with a translucent dome.
Credit: LIGO/Virgo/NASA/Leo Singer (Milky Way image: Axel Mellinger)

Variety of Gravitational Waves and a Chirp
The signal measured by LIGO and Virgo from the neutron star merger GW170817 is compared here to previously detected binary black hole mergers. All signals are shown starting at 30 Hertz, and the progression of GW170817 is shown in real time, accompanied by its conversion to audio heard at the end of the movie. GW170817 was observable for more than 30 times longer than any previous gravitational-wave signal.
Credit: LIGO/University of Oregon/Ben Farr

LIGO is funded by the NSF, and operated by Caltech and MIT, which conceived of LIGO and led the Initial and Advanced LIGO projects. Financial support for the Advanced LIGO project was led by the NSF with Germany (Max Planck Society), the U.K. (Science and Technology Facilities Council) and Australia (Australian Research Council) making significant commitments and contributions to the project.

More than 1,200 scientists and some 100 institutions from around the world participate in the effort through the LIGO Scientific Collaboration, which includes the GEO Collaboration and the Australian collaboration OzGrav. Additional partners are listed at http://ligo.org/partners.php

The Virgo collaboration consists of more than 280 physicists and engineers belonging to 20 different European research groups: six from Centre National de la Recherche Scientifique (CNRS) in France; eight from the Istituto Nazionale di Fisica Nucleare (INFN) in Italy; two in the Netherlands with Nikhef; the MTA Wigner RCP in Hungary; the POLGRAW group in Poland; Spain with the University of Valencia; and the European Gravitational Observatory, EGO, the laboratory hosting the Virgo detector near Pisa in Italy, funded by CNRS, INFN, and Nikhef.

Do negative air ions improve mood, anxiety, depression, alertness?
Part of this video was sponsored by LastPass, click here to find out more: http://bit.ly/2RZZTZk

Special thanks to Prof. Jack Beauchamp and Dr. Nathan Dalleska from Caltech for all their help running these experiments and discussing the research. For more, check out the links below:
http://www.cce.caltech.edu/peo....ple/jesse-l-jack-bea
http://beckmaninstitute.caltech.edu/eac.shtml

If you want to dig into the research on negative ions yourself, I suggest starting with the review studies:

Air ions and mood outcomes: a review and meta-analysis.
Perez V, Alexander DD, Bailey WH.
BMC Psychiatry. 2013 Jan 15;13:29.
https://www.ncbi.nlm.nih.gov/pubmed/23320516

Air ions and respiratory function outcomes: a comprehensive review
Dominik D Alexander, William H Bailey, Vanessa Perez, Meghan E Mitchell, and Steave Su
J Negat Results Biomed. 2013; 12: 14.
https://www.ncbi.nlm.nih.gov/p....mc/articles/PMC38485

Exposure of laboratory animals to small air ions: a systematic review of biological and behavioral studies.
Bailey WH, Williams AL, Leonhard MJ.
Biomed Eng Online. 2018 Jun 5; 17(1):72.
https://www.ncbi.nlm.nih.gov/pubmed/29866122

Thumbnail photography by Raquel Nuno

VFX by Alan Chamberlain

Sound recording by Whitney Clavin

Motion Graphics by Charlie Kilman

Music from Epidemic Sound: http://epidemicsound.com "Capture a Picture 1" and "Seaweed"

There is a common perception that weight and mass are basically the same thing. This video aims to tease out the difference between mass and weight by asking people what makes a car difficult to push. The standard answer is that it is difficult to push because it's heavy. But heaviness is a measure of weight, the gravitational pull of the Earth attracting the car to Earth's center. When the car is pushed on a flat road, the force of gravity does not oppose the motion. Instead the resistance felt is an indication of the car's mass which determines its inertia. Inertia is the property of matter that means it tends to resist acceleration - the greater the mass, the less the acceleration for a given amount of force.

Want to help plant 20M trees by 2020? Go to https://teamtrees.org #teamtrees
Huge thanks to all the YouTubers who organized this. My apologies for the repost.
These videos are from 2012 so my interest in trees goes back a long ways. I think these videos discuss two of the most interesting and amazing facts about our leafy friends: they are made mostly of CO2 (which comes from us breathing out amongst other sources) and they can transport water up a tube higher than any we can currently manufacture. So trees are out to get you. But we do much worse to them so we owe it to them to plant some more. 20 mil is a good start.

When a grape is cut nearly in half and placed in a microwave, plasma is produced. Please use caution if attempting this experiment: don't leave the microwave on for too long, make sure the area is well ventilated, and stand back. Remember the contents will be very hot afterwards.

A quote by Einstein: A human being is a part of the whole, called by us "Universe", a part limited in time and space. He experiences himself, his thoughts and feelings as something separated from the rest — a kind of optical delusion of his consciousness. This delusion is a kind of prison for us, restricting us to our personal desires and to affection for a few persons nearest to us. Our task must be to free ourselves from this prison by widening our circle of compassion to embrace all living creatures and the whole of nature in its beauty. Nobody is able to achieve this completely, but the striving for such achievement is in itself a part of the liberation and a foundation for inner security.

We put aerogel to the test vs 'not-a-flamethrower', a huge 2000°C flame to a large fiberglass blanket infused with silica aerogel - formerly the lightest solid (that title is now held by graphene aerogel).

Special thanks to:
Aerogel Technologies: https://ve42.co/aerogeltech
Aspen Aerogels: https://ve42.co/aspen
Ben: @BenScho999999
Dr. Stephen Steiner and the Aerogel Technologies team

The footage of aerogel materials in cold environments was provided courtesy of Aspen Aerogels. Their product, cryogel, was shown to be flexible in liquid nitrogen while preventing cold burns to the hand. They are the manufacturer of the blanket used in the main portion of this video.

This is the finale of my three-part series on aerogel. I'll put links to the other parts below:
World's Lightest Solid: https://youtu.be/AeJ9q45PfD0
I Waterproofed Myself With Aerogel: https://youtu.be/GcdB5bFwio4

Huge thanks to Patreon supporters:
Alfred Wallace, Arjun Chakroborty, Bryan Baker, Chris Vargas, Chuck Lauer Vose, Dale Horne, Donal Botkin, Eric Velazquez, halyoav, James Knight, Jasper Xin, Joar Wandborg, Kevin Beavers, kkm, Leah Howard, Lyvann Ferrusca, Michael Krugman, Mohammed Al Sahaf, Noel Braganza, Philipp Volgger, Pindex, Ron Neal, Sam Lutfi, Stan Presolski, Tige Thorman

This is an educational video demonstrating scientific experiments performed by professionals. It should not be attempted by viewers.

Music from Epidemic Sound: http://epidemicsound.com "Running Against the Clock" "Dangerous Forests"

Scientific research has shown that heterosexual males and females find members of the opposite sex more attractive when they wear the colour red. This is a subconscious preference that seems to have some evolutionary basis. We attempted to replicate these findings in Sydney but our methods were much less controlled and the results achieved were not statistically significant.

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Everyone has played with a mixture of corn starch and water (or at least I hope they have). This was one of my favorite experiments as a kid. Your hand slides into the slime easily when moving slowly but the mixture behaves as a solid if you hit it quickly. That is what is meant by 'non-Newtonian' - the fluid's properties change depending on its relative motion. These properties can be exploited to dramatic effect as has been shown on speaker cones before. Here I wanted to understand what is going on, what frequencies and amplitudes work best so I used a slow-mo camera.

Thanks to everyone at the YouTube Space LA for helping me film this. I couldn't have done it without you.

Music licensed from http://www.cuesongs.com
Love Lost (Instrumental) by Temper Trap
A Life in the Day by Ghost of Otis
Fortune's Fool Instrumental by Hiatus & Shura
The Man by Audio Android

Right after leaving the platform, the only significant force acting on the bungy jumper is his weight. This causes him to speed up from rest. His speed increases every second by nearly 10 m/s. This is not the maximum acceleration experienced by a bungy jumper, however.

A short a cappella tribute to experimentalists. It is sung while performing three simple experiments with household items: Mentos dropped in diet Coke, a tea bag emptied and burned, and a ping pong ball floating in the air stream of a hair dryer.

Three space travelers including record-setting astronaut Christina Koch return home from the International Space Station.

Christina Koch wrapped up a 328-day extended mission on her first spaceflight, having spent more time in space on a single mission than any other woman. Koch, along with station Commander Luca Parmitano of ESA (European Space Agency), and Soyuz commander Alexander Skvortsov of the Russian space agency Roscosmos departed the station in a Soyuz spacecraft that made a parachute-assisted landing at 4:12 a.m. EST southeast of Dzhezkazgan, Kazakhstan.

Koch's extended mission will provide researchers the opportunity to observe effects of long-duration spaceflight on a woman, as we prepare for Artemis missions to the Moon and human exploration of Mars.

AI SpaceFactory's "MARSHA" Mars Habitat just won NASA's 3-D Printed Habitat Challenge. Compared to others, their design looks downright luxurious. It has multiple floors, spacious living quarters, and plenty of windows to gaze upon the Martian horizon.

MORE SPACE CONTENT:
Elon Musk's Multibillion Dollar Mars Rocket, Explained
https://www.youtube.com/watch?v=FIn6r9RKVVM
NASA’s 4-Year Twin Experiment Takes Us Closer To Mars Than Ever Before
https://www.youtube.com/watch?v=ZVRft7r8-Ds
Why Are NASA Spacesuits White?
https://www.youtube.com/watch?v=damoYDG9rmk

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The Mars Homes That NASA Awarded $500k

Here are all the photos flying through interstellar space on Voyager's Golden Record. http://www.vox.com/2015/11/11/....9702090/voyager-gold

Help us make more ambitious videos by joining the Vox Video Lab. It gets you exclusive perks, like livestream Q&As with all the Vox creators, a badge that levels up over time, and video extras bringing you closer to our work! Learn more at http://bit.ly/video-lab

Sources:
http://voyager.jpl.nasa.gov/spacecraft/scenes.html
http://www.amazon.com/Pale-Blu....e-Dot-Vision-Future/
http://www.amazon.com/Murmurs-....Earth-Carl-Sagan-ebo

When Voyager 1 and Voyager 2 launched into space in 1977, their mission was to explore the outer solar system, and over the following decade, they did so admirably.

With an 8-track tape memory system and onboard computers that are thousands of times weaker than the phone in your pocket, the two spacecraft sent back an immense amount of imagery and information about the four gas giants, Jupiter, Saturn, Uranus, and Neptune.

But NASA knew that after the planetary tour was complete, the Voyagers would remain on a trajectory toward interstellar space, having gained enough velocity from Jupiter's gravity to eventually escape the grasp of the sun. Since they will orbit the Milky Way for the foreseeable future, the Voyagers should carry a message from their maker, NASA scientists decided.

The Voyager team tapped famous astronomer and science popularizer Carl Sagan to compose that message. Sagan's committee chose a copper phonograph LP as their medium, and over the course of six weeks they produced the "Golden Record": a collection of sounds and images that will probably outlast all human artifacts on Earth.

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