A Type II supernova (plural: supernovae or supernovas) results from the rapid collapse and violent explosion of a massive star. A star must have at least 8 times, and no more than 40–50 times, the mass of the Sun (M☉) for this type of explosion. It is distinguished from other types of supernovae by the presence of hydrogen in its spectrum. Type II supernovae are mainly observed in the spiral arms of galaxies and in H II regions, but not in elliptical galaxies.
Stars generate energy by the nuclear fusion of elements. Unlike the Sun, massive stars possess the mass needed to fuse elements that have an atomic mass greater than hydrogen and helium, albeit at increasingly higher temperatures and pressures, causing increasingly shorter stellar life spans. The degeneracy pressure of electrons and the energy generated by these fusion reactions are sufficient to counter the force of gravity and prevent the star from collapsing, maintaining stellar equilibrium. The star fuses increasingly higher mass elements, starting with hydrogen and then helium, progressing up through the periodic table until a core of iron and nickel is produced. Fusion of iron or nickel produces no net energy output, so no further fusion can take place, leaving the nickel-iron core inert. Due to the lack of energy output creating outward pressure, equilibrium is broken.
Types of Supernova - Type I and Type II explained - Universe Sandbox 2
Patreon page:
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Hello and welcome to What Da Math!
In this video, we will talk about the two main types of supernovae - supernova type 1 and type 2 - and describe the main differences between them.
Enjoy and please subscribe.
Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
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published: 08 May 2016
Astronomy: The Supernova (8 of 10) What is a Type 2 Supernova Explosion?
Visit http://ilectureonline.com for more math and science lectures!
In this video I will explain what is a type 2 supernova explosion.
published: 21 Jul 2014
Type II Supernova Short Animation
Here's a motion graphics piece I did this year in After Effects.
Directed, edited, narrated by Christian Rush
published: 09 May 2012
Type II Supernova - Sixty Symbols
After last week's excitement (see our astronomy sister channel at http://www.youtube.com/DeepSkyVideos for more details), we turn our attention to types of supernova.
Featuring Professor Mike Merrifield.
Deep Sky Videos on last week's Type II can be found at:
http://www.youtube.com/watch?v=_GEyAsaWB4k
http://www.youtube.com/watch?v=x5zo5449wHU
As usual, here is Mike explaining the Atlas of Creation on his shelf: http://www.youtube.com/watch?v=Dylv1EiMejI
Visit our website at http://www.sixtysymbols.com/
We're on Facebook at http://www.facebook.com/sixtysymbols
And Twitter at http://twitter.com/#!/periodicvideos
This project features scientists from The University of Nottingham
Sixty Symbols videos by Brady Haran
published: 29 Mar 2012
Types of Supernova Explosions | Supernovae Explained
News(23.02.2021): At the center of SN1987a, a type 2 supernova have a Neutron Star.
This video is all about different types of supernova and how it happens.
Supernovae is a spectacular event occur at the end of supermassive stars. Every supernova explosion is unique. All the naturally occurring elements are created during a supernova explosion. The very elements which are the basic ingredients of stars, planets and all the living beings including us.
Links to the previous videos on this series:
1. Stellar Evolution : https://youtu.be/Sk_n0jiLfaw
2. Inside of a dying star (core) : https://youtu.be/gzNy8w4ToME
0:00 Introduction
0:12 Supernova explosion
0:33 Types of supernovae & how they are classified
1:00 Type II Supernova
1:47 Type Ib & Ic intro
1:54 Condition for Core Collapse Su...
published: 19 Feb 2021
Type-II Supernova (15 Solar Mass Star) [720p]
This movie shows the visualization of supercomputer simulations of the birth of a neutron star and the onset of the supernova explosion of a star with 15 times the mass of the Sun.
The neutron star is as an extremely compact object that forms in the deep interior of the dying massive star when the stellar core collapses under the pull of its own gravity within fractions of a second. It encompasses more than a solar mass in finally the volume of a big city and is visible first as whitish, then blue, intransparent sphere at the center. A shock wave (discernable as surface of a sharp transition between yellow/red and blueish colors) is launched when the infalling stellar matter (visible as extended blue cloud around the neutron star) crashes supersonically onto the surface of the nascent n...
published: 25 Jan 2010
SuperNova Type 2 DAWID ALLAH WON
published: 25 May 2020
Type II supernova (a.k.a,, core collapse supernova)
Type II supernova (a.k.a., core collapse supernova)
AstroPictionary
Astronomy Vocabulary
Patreon page:
https://www.patreon.com/user?u=2318196&ty=h
Hello and welcome to What Da Math!
In this video, we will talk about the two main types of supernova...
Patreon page:
https://www.patreon.com/user?u=2318196&ty=h
Hello and welcome to What Da Math!
In this video, we will talk about the two main types of supernovae - supernova type 1 and type 2 - and describe the main differences between them.
Enjoy and please subscribe.
Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
Patreon page:
https://www.patreon.com/user?u=2318196&ty=h
Hello and welcome to What Da Math!
In this video, we will talk about the two main types of supernovae - supernova type 1 and type 2 - and describe the main differences between them.
Enjoy and please subscribe.
Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
After last week's excitement (see our astronomy sister channel at http://www.youtube.com/DeepSkyVideos for more details), we turn our attention to types of supe...
After last week's excitement (see our astronomy sister channel at http://www.youtube.com/DeepSkyVideos for more details), we turn our attention to types of supernova.
Featuring Professor Mike Merrifield.
Deep Sky Videos on last week's Type II can be found at:
http://www.youtube.com/watch?v=_GEyAsaWB4k
http://www.youtube.com/watch?v=x5zo5449wHU
As usual, here is Mike explaining the Atlas of Creation on his shelf: http://www.youtube.com/watch?v=Dylv1EiMejI
Visit our website at http://www.sixtysymbols.com/
We're on Facebook at http://www.facebook.com/sixtysymbols
And Twitter at http://twitter.com/#!/periodicvideos
This project features scientists from The University of Nottingham
Sixty Symbols videos by Brady Haran
After last week's excitement (see our astronomy sister channel at http://www.youtube.com/DeepSkyVideos for more details), we turn our attention to types of supernova.
Featuring Professor Mike Merrifield.
Deep Sky Videos on last week's Type II can be found at:
http://www.youtube.com/watch?v=_GEyAsaWB4k
http://www.youtube.com/watch?v=x5zo5449wHU
As usual, here is Mike explaining the Atlas of Creation on his shelf: http://www.youtube.com/watch?v=Dylv1EiMejI
Visit our website at http://www.sixtysymbols.com/
We're on Facebook at http://www.facebook.com/sixtysymbols
And Twitter at http://twitter.com/#!/periodicvideos
This project features scientists from The University of Nottingham
Sixty Symbols videos by Brady Haran
News(23.02.2021): At the center of SN1987a, a type 2 supernova have a Neutron Star.
This video is all about different types of supernova and how it happens.
S...
News(23.02.2021): At the center of SN1987a, a type 2 supernova have a Neutron Star.
This video is all about different types of supernova and how it happens.
Supernovae is a spectacular event occur at the end of supermassive stars. Every supernova explosion is unique. All the naturally occurring elements are created during a supernova explosion. The very elements which are the basic ingredients of stars, planets and all the living beings including us.
Links to the previous videos on this series:
1. Stellar Evolution : https://youtu.be/Sk_n0jiLfaw
2. Inside of a dying star (core) : https://youtu.be/gzNy8w4ToME
0:00 Introduction
0:12 Supernova explosion
0:33 Types of supernovae & how they are classified
1:00 Type II Supernova
1:47 Type Ib & Ic intro
1:54 Condition for Core Collapse Supernovae
2:00 Type Ib
2:28 Type Ic
2:52 What to thermal runaway?
3:09 Type Ia Supernovae
5:07 conclusion
Content in this video is originally created by Talk Sci team. Few public domain images of NASA/ESA is used here as examples of supernovae. Credit for the same is given in the bottom left corner of the image while it appears.
News(23.02.2021): At the center of SN1987a, a type 2 supernova have a Neutron Star.
This video is all about different types of supernova and how it happens.
Supernovae is a spectacular event occur at the end of supermassive stars. Every supernova explosion is unique. All the naturally occurring elements are created during a supernova explosion. The very elements which are the basic ingredients of stars, planets and all the living beings including us.
Links to the previous videos on this series:
1. Stellar Evolution : https://youtu.be/Sk_n0jiLfaw
2. Inside of a dying star (core) : https://youtu.be/gzNy8w4ToME
0:00 Introduction
0:12 Supernova explosion
0:33 Types of supernovae & how they are classified
1:00 Type II Supernova
1:47 Type Ib & Ic intro
1:54 Condition for Core Collapse Supernovae
2:00 Type Ib
2:28 Type Ic
2:52 What to thermal runaway?
3:09 Type Ia Supernovae
5:07 conclusion
Content in this video is originally created by Talk Sci team. Few public domain images of NASA/ESA is used here as examples of supernovae. Credit for the same is given in the bottom left corner of the image while it appears.
This movie shows the visualization of supercomputer simulations of the birth of a neutron star and the onset of the supernova explosion of a star with 15 times ...
This movie shows the visualization of supercomputer simulations of the birth of a neutron star and the onset of the supernova explosion of a star with 15 times the mass of the Sun.
The neutron star is as an extremely compact object that forms in the deep interior of the dying massive star when the stellar core collapses under the pull of its own gravity within fractions of a second. It encompasses more than a solar mass in finally the volume of a big city and is visible first as whitish, then blue, intransparent sphere at the center. A shock wave (discernable as surface of a sharp transition between yellow/red and blueish colors) is launched when the infalling stellar matter (visible as extended blue cloud around the neutron star) crashes supersonically onto the surface of the nascent neutron star. The shock-heated stellar gas envelopes the neutron star as a red and orange shell.
The intense flux of neutrinos, weakly interacting elementary particles that are abundantly radiated from the neutron star, further heats the postshock layers to higher temperatures and thus triggers the onset of violent convective overturn. Roughly a tenth of a second after its launch the shock develops ronounced asphericity, partly due to the convective perturbations, partly because of a generic instability to nonradial deformation (visible by dipolar oscillations of the shock). More infalling stellar gas (blue) is channelled towards the neutron star in downflows while heated gas (red and yellow) is rising against the infalling matter due to buoyancy. Thus the shock is pushed to larger and larger radii. Finally, the flow arranges itself into two huge, inflating polar lobes that are alternatingly fed by powerful waves of fresh, neutrino-heated gas from equator-near downflows. By the end of the movie the largely aspherical shock rushes outward with a speed of 10,000 kilometers per second (requiring a zoom-out in the movie) and is going to expell the outer layers of the dying star in the supernova explosion.
credit: M.Rampp (RZG)
source: http://www.rzg.mpg.de/visualisation/scientificdata/rzgprojects/type-ii-supernova-simulations
This movie shows the visualization of supercomputer simulations of the birth of a neutron star and the onset of the supernova explosion of a star with 15 times the mass of the Sun.
The neutron star is as an extremely compact object that forms in the deep interior of the dying massive star when the stellar core collapses under the pull of its own gravity within fractions of a second. It encompasses more than a solar mass in finally the volume of a big city and is visible first as whitish, then blue, intransparent sphere at the center. A shock wave (discernable as surface of a sharp transition between yellow/red and blueish colors) is launched when the infalling stellar matter (visible as extended blue cloud around the neutron star) crashes supersonically onto the surface of the nascent neutron star. The shock-heated stellar gas envelopes the neutron star as a red and orange shell.
The intense flux of neutrinos, weakly interacting elementary particles that are abundantly radiated from the neutron star, further heats the postshock layers to higher temperatures and thus triggers the onset of violent convective overturn. Roughly a tenth of a second after its launch the shock develops ronounced asphericity, partly due to the convective perturbations, partly because of a generic instability to nonradial deformation (visible by dipolar oscillations of the shock). More infalling stellar gas (blue) is channelled towards the neutron star in downflows while heated gas (red and yellow) is rising against the infalling matter due to buoyancy. Thus the shock is pushed to larger and larger radii. Finally, the flow arranges itself into two huge, inflating polar lobes that are alternatingly fed by powerful waves of fresh, neutrino-heated gas from equator-near downflows. By the end of the movie the largely aspherical shock rushes outward with a speed of 10,000 kilometers per second (requiring a zoom-out in the movie) and is going to expell the outer layers of the dying star in the supernova explosion.
credit: M.Rampp (RZG)
source: http://www.rzg.mpg.de/visualisation/scientificdata/rzgprojects/type-ii-supernova-simulations
Patreon page:
https://www.patreon.com/user?u=2318196&ty=h
Hello and welcome to What Da Math!
In this video, we will talk about the two main types of supernovae - supernova type 1 and type 2 - and describe the main differences between them.
Enjoy and please subscribe.
Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
After last week's excitement (see our astronomy sister channel at http://www.youtube.com/DeepSkyVideos for more details), we turn our attention to types of supernova.
Featuring Professor Mike Merrifield.
Deep Sky Videos on last week's Type II can be found at:
http://www.youtube.com/watch?v=_GEyAsaWB4k
http://www.youtube.com/watch?v=x5zo5449wHU
As usual, here is Mike explaining the Atlas of Creation on his shelf: http://www.youtube.com/watch?v=Dylv1EiMejI
Visit our website at http://www.sixtysymbols.com/
We're on Facebook at http://www.facebook.com/sixtysymbols
And Twitter at http://twitter.com/#!/periodicvideos
This project features scientists from The University of Nottingham
Sixty Symbols videos by Brady Haran
News(23.02.2021): At the center of SN1987a, a type 2 supernova have a Neutron Star.
This video is all about different types of supernova and how it happens.
Supernovae is a spectacular event occur at the end of supermassive stars. Every supernova explosion is unique. All the naturally occurring elements are created during a supernova explosion. The very elements which are the basic ingredients of stars, planets and all the living beings including us.
Links to the previous videos on this series:
1. Stellar Evolution : https://youtu.be/Sk_n0jiLfaw
2. Inside of a dying star (core) : https://youtu.be/gzNy8w4ToME
0:00 Introduction
0:12 Supernova explosion
0:33 Types of supernovae & how they are classified
1:00 Type II Supernova
1:47 Type Ib & Ic intro
1:54 Condition for Core Collapse Supernovae
2:00 Type Ib
2:28 Type Ic
2:52 What to thermal runaway?
3:09 Type Ia Supernovae
5:07 conclusion
Content in this video is originally created by Talk Sci team. Few public domain images of NASA/ESA is used here as examples of supernovae. Credit for the same is given in the bottom left corner of the image while it appears.
This movie shows the visualization of supercomputer simulations of the birth of a neutron star and the onset of the supernova explosion of a star with 15 times the mass of the Sun.
The neutron star is as an extremely compact object that forms in the deep interior of the dying massive star when the stellar core collapses under the pull of its own gravity within fractions of a second. It encompasses more than a solar mass in finally the volume of a big city and is visible first as whitish, then blue, intransparent sphere at the center. A shock wave (discernable as surface of a sharp transition between yellow/red and blueish colors) is launched when the infalling stellar matter (visible as extended blue cloud around the neutron star) crashes supersonically onto the surface of the nascent neutron star. The shock-heated stellar gas envelopes the neutron star as a red and orange shell.
The intense flux of neutrinos, weakly interacting elementary particles that are abundantly radiated from the neutron star, further heats the postshock layers to higher temperatures and thus triggers the onset of violent convective overturn. Roughly a tenth of a second after its launch the shock develops ronounced asphericity, partly due to the convective perturbations, partly because of a generic instability to nonradial deformation (visible by dipolar oscillations of the shock). More infalling stellar gas (blue) is channelled towards the neutron star in downflows while heated gas (red and yellow) is rising against the infalling matter due to buoyancy. Thus the shock is pushed to larger and larger radii. Finally, the flow arranges itself into two huge, inflating polar lobes that are alternatingly fed by powerful waves of fresh, neutrino-heated gas from equator-near downflows. By the end of the movie the largely aspherical shock rushes outward with a speed of 10,000 kilometers per second (requiring a zoom-out in the movie) and is going to expell the outer layers of the dying star in the supernova explosion.
credit: M.Rampp (RZG)
source: http://www.rzg.mpg.de/visualisation/scientificdata/rzgprojects/type-ii-supernova-simulations
A Type II supernova (plural: supernovae or supernovas) results from the rapid collapse and violent explosion of a massive star. A star must have at least 8 times, and no more than 40–50 times, the mass of the Sun (M☉) for this type of explosion. It is distinguished from other types of supernovae by the presence of hydrogen in its spectrum. Type II supernovae are mainly observed in the spiral arms of galaxies and in H II regions, but not in elliptical galaxies.
Stars generate energy by the nuclear fusion of elements. Unlike the Sun, massive stars possess the mass needed to fuse elements that have an atomic mass greater than hydrogen and helium, albeit at increasingly higher temperatures and pressures, causing increasingly shorter stellar life spans. The degeneracy pressure of electrons and the energy generated by these fusion reactions are sufficient to counter the force of gravity and prevent the star from collapsing, maintaining stellar equilibrium. The star fuses increasingly higher mass elements, starting with hydrogen and then helium, progressing up through the periodic table until a core of iron and nickel is produced. Fusion of iron or nickel produces no net energy output, so no further fusion can take place, leaving the nickel-iron core inert. Due to the lack of energy output creating outward pressure, equilibrium is broken.
... and Type II at the end of a stars life ... Two months later, they detected light from the same region of the galaxy, that’s unusual since it is very unusual for a Type II supernova to repeat itself.
A neutron star in the remnants of a supernova ...Around 168,000 years ago, a star in the Large Magellanic Cloud exploded in a spectacular Type II supernova ... This image is of a rare type of gravitational ...
The last time astronomers observed this phenomenon was in 1987 when a Type II supernova (SN1987A) appeared suddenly in the Large Magellanic Cloud (LMC), roughly 168,000 light-years from Earth.
Massive stars about eight times more massive than the Sun explode as supernovae at the end of their lives ... These types of supernovae are called core-collapse supernovae, also known as Type II ... Artist’s impression of a Type II supernova explosion.
How do the various isotopes produced by supernovae drive the ... For example, Type II supernovae, also known as core-collapse supernovae are known to produce Titanium-44, which is an unstable isotope.
According to the study, the metallicity of HE 2315−4240, together with its abundances of magnesium and silicon suggest that the star formed from the gas enriched by a Type II supernova explosion.
... abundance of supernova explosions ... In this image, Hubble examined the surroundings of the Type II SN 2004G, seeking to study the kinds of stars that end their lives as this kind of supernova.
The Moon meets Spica Saturday night. Credit... credit ... A spectroscopic binary with a companion star in a close orbit, Spica is one of the closest stars to our solar system with the potential to explode as a Type II supernova in the next few million years.
Supernovae are classified into two types. Type I and Type II, with each being broken down into various subtypes based on their appearances or chemical compositions. Additionally, remnants of supernovae ...
They added that the enhancement in alpha elements like silicon, magnesium or titanium, suggest an old age of the cluster's stellar population, which likely formed at early epochs from a gas mainly enriched by Type II supernovae.
Designated SN 2023adsy, the newfound stellar explosion is the most distant Type Ia supernova so far detected ... Type I (no hydrogen in their spectra) and Type II (showcasing hydrogen spectral lines).
An international team of astronomers have performed photometric and spectroscopic observations of a Type Ibn supernova, known as SN 2023fyq ... Type I SNe lack hydrogen in their spectra, while those of Type II showcase spectral lines of hydrogen.
The data for this Hubble image came from a study of Type-II supernovae host galaxies ... The supernova which brought UGC 9684 to Hubble's attention occurred in 2020 ... Remarkably, the 2020 supernova isn't ...
Artist’s impression of a Type II supernova explosion, which involves the destruction of a massive supergiant star. When stars explode as supernovae, they eject matter into space, potentially polluting nearby companion stars.
Although they acknowledge an alternative explanation of the grain coming from a nova, Nevill and co-authors think it is far more likely the source was a hydrogen-burning supernova, a rare kind of Type II supernova.
