Astronomy - Ch. 22: Neutron Star (3 of 17) What is Neutron Degeneracy?
Visit http://ilectureonline.com for more math and science lectures! To donate: http://www.ilectureonline.com/donate https://www.patreon.com/user?u=3236071 We will learn neutron degeneracy pressure can uphold a neutron star with a mass up to 0.7 time mass of our Sun. Two neutrons with the
From playlist THE "WHAT IS" PLAYLIST
Nuclear Fission; splitting the atom for beginners: from fizzics.org
There are notes to support this video here:https://www.fizzics.org/nuclear-fission/ Nuclear Fission is the splitting of the nucleus of an atom into two or more parts by hitting it with a small particle, almost always a neutron (a proton would be repelled from the positive nucleus and an el
From playlist My Top Videos
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From playlist Physics
Liquid Metal Embrittlement - Gallium vs. Aluminium
Bringing gallium and aluminium together has some interesting and occasionally rather explosive results, as Dan found out in this little tale from the prep room. Subscribe for regular science videos: http://bit.ly/RiSubscRibe Liquid metal embrittlement is a phenomenon where ductile metals,
From playlist Tales from the Prep Room
When a dying star is too massive to leave behind a white dwarf and not massive enough to leave behind a black hole, you get a neutron star (sometimes a pulsar). It's a very compact clump of neutrons surrounded by a very strong magnetic field. These things are crazy!! ______________________
From playlist Astronomy
Lec 1 | MIT 22.091 Nuclear Reactor Safety, Spring 2008
Lecture 1: Introduction and overview Instructor: Andrew Kadak View the complete course: http://ocw.mit.edu/22-091S08 License: Creative Commons BY-NC-SA More information at http://ocw.mit.edu/terms More courses at http://ocw.mit.edu
From playlist MIT 22.091 Nuclear Reactor Safety, Spring 2008
Lec 19 | MIT 3.091SC Introduction to Solid State Chemistry, Fall 2010
Lecture 19: Point & Line Defects Instructor: Donald Sadoway View the complete course: http://ocw.mit.edu/3-091SCF10 License: Creative Commons BY-NC-SA More information at http://ocw.mit.edu/terms More courses at http://ocw.mit.edu
From playlist MIT 3.091SC Introduction to Solid State Chemistry, Fall 2010
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From playlist Science Unplugged: Particle Physics
Astronomy - Ch. 22: Neutron Star (1 of 17) What is a Neutron Star?
Visit http://ilectureonline.com for more math and science lectures! To donate: http://www.ilectureonline.com/donate https://www.patreon.com/user?u=3236071 We will learn a neutron star is the remnant of the collapse of he core of a super massive star (greater than 8 times the of our Sun).
From playlist THE "WHAT IS" PLAYLIST
29. Nuclear Materials Science Continued
MIT 22.01 Introduction to Nuclear Engineering and Ionizing Radiation, Fall 2016 Instructor: Michael Short View the complete course: https://ocw.mit.edu/22-01F16 YouTube Playlist: https://www.youtube.com/playlist?list=PLUl4u3cNGP61FVzAxBP09w2FMQgknTOqu The lecture on nuclear materials and
From playlist MIT 22.01 Introduction to Nuclear Engineering and Ionizing Radiation, Fall 2016
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From playlist Chemistry
Lec 19 | MIT 3.091 Introduction to Solid State Chemistry
Defects in Crystals: Point Defects, Line Defects, Interfacial Defects, Voids View the complete course at: http://ocw.mit.edu/3-091F04 License: Creative Commons BY-NC-SA More information at http://ocw.mit.edu/terms More courses at http://ocw.mit.edu
From playlist MIT 3.091 Introduction to Solid State Chemistry, Fall 2004
27. Nuclear Materials — Radiation Damage and Effects in Matter
MIT 22.01 Introduction to Nuclear Engineering and Ionizing Radiation, Fall 2016 Instructor: Michael Short View the complete course: https://ocw.mit.edu/22-01F16 YouTube Playlist: https://www.youtube.com/playlist?list=PLUl4u3cNGP61FVzAxBP09w2FMQgknTOqu Prof. Short uses all the concepts int
From playlist MIT 22.01 Introduction to Nuclear Engineering and Ionizing Radiation, Fall 2016
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From playlist Chemistry
0:00 why do we care about diffusion and the axe body spray demo 6:00 diffusion concentration gradients 7:25 atomistic description of diffusion 18:15 Fick's First Law for steady-state diffusion 20:35 diffusion coefficient 40:44 Ficks Second Law for non-steady state diffusion 52:06 short cir
From playlist Introduction to Materials Science & Engineering Fall 2019
Have We Contaminated the Moon?
Humans are full of microbes. Humans also went to the Moon. Does that mean we left colonies over there? ---------- Dooblydoo thanks go to the following Patreon supporters -- we couldn't make SciShow without them! Shout out to Justin Ove, Justin Lentz, David Campos, Philippe von Bergen, Chri
From playlist SciShow Space
Neutron Star Collision and Gamma Ray Burst Discovery
From NASA Astrophysics and Goddard Space Flight Center. Every day or two, on average, satellites detect a massive explosion somewhere in the sky. These are gamma-ray bursts, the brightest blasts in the universe. They're thought to be caused by jets of matter moving near the speed of light
From playlist Violent Universe
Burj Khalifa | The Secrets of its incredibly Strong Foundation
How such a massive building able to stand strong on loose Dubai soil? Let's explore all the secrets of Burj Khalifa's foundation in this video. Please be a Lesics team member and get access to exclusive engineering contents: https://www.youtube.com/channel/UCqZQJ4600a9wIfMPbYc60OQ/join h
From playlist Civil Engineering
Get your free quote with Lumerit here: http://go.lumerit.com/realengineering/ Second Channel: https://www.youtube.com/channel/UCMet4qY3027v8KjpaDtDx-g Stress and strain is one of the first things you will cover in engineering. It is the most fundamental part of material science and it's
From playlist Real Engineering
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From playlist Science Unplugged: Neutrinos