What are two possible results of a supernova explosion?
After the supernova, the following is possible:
- A compact residue (supernova remnants), such as a pulsar or black hole.
- Expanding external shock wave.
- Secondary wave propagating in the interstellar medium and in dense supernova emissions.
What types of star can explode in a supernova?
The companion can be any other type of star, like a red giant, main sequence star, or even another white dwarf. In a Type Ia supernova, a white dwarf (left) draws matter from a companion star until its mass hits a limit which leads to collapse and then explosion.
What causes the supernova to blow up?
What causes a star to blow up? Gravity gives the supernova its energy. For Type II supernovae, mass flows into the core by the continued formation of iron from nuclear fusion. Once the core has gained so much mass that it cannot withstand its own weight, the core implodes.
What is a neutron star left after a supernova explosion?
What Is Left After A Supernova? Answer: A neutron star that is left-over after a supernova is actually a remnant of the massive star which went supernova. Once the neutron star is over the mass limit, which is at a mass of about 3 solar masses, the collapse to a black hole occurs in less than a second.

What is the meaning of supernova explosion?
1 : the explosion of a star in which the star may reach a maximum intrinsic luminosity one billion times that of the sun. 2 : one that explodes into prominence or popularity also : superstar.
What happens after a supernova explodes?
The remnants of the stellar core which are left after the supernovae explosion will follow one of two paths: neutron star or black hole.
Can a supernova destroy Earth?
A supernova is a spectacular explosion of a massive star. If our sun exploded as a supernova, the resulting shock wave probably wouldn't incinerate the entire Earth, but the side of Earth facing the sun would boil away.
What is a supernova made of?
Iron atoms become crushed so closely together that the repulsive forces of their nuclei create a recoil of the squeezed core—a bounce that causes the star to explode as a supernova and give birth to an enormous, superheated, shock wave.
What happens if a supernova hit Earth?
Both types are extremely powerful, sending energetic radiation and blast waves of ejected gas far into space. If a supernova explosion were to occur within about 25 light-years of Earth, our planet would probably lose its atmosphere, and all life would perish.
How long do supernovas last?
The explosion of a supernova occurs in a star in a very short timespan of about 100 seconds. When a star undergoes a supernova explosion, it dies leaving behind a remnant: either a neutron star or a black hole.
Can you survive a supernova?
Can life survive? There is no way for life to survive on the surface of a planet witnessing a supernova. As shown above, a habitable planet orbiting Betelgeuse will lose at least 4 km of its surface, vaporized to space.
Can a planet survive a supernova?
In some cases even a portion of a planetary biosphere (deep in planet's crust) can survive. However, if a star loses too much mass, a planet would leave. Also, if star's collapse is asymmetric then the star itself can leave the planetary system.
Will our sun ever go supernova?
No supernova, no black hole Our sun isn't massive enough to trigger a stellar explosion, called a supernova, when it dies, and it will never become a black hole either. In order to create a supernova, a star needs about 10 times the mass of our sun.
How powerful is a supernova?
A supernova is an explosion of a massive supergiant star. It may shine with the brightness of 10 billion suns! The total energy output may be 1044 joules, as much as the total output of the sun during its 10 billion year lifetime.
Can a supernova destroy a galaxy?
At a certain distance, even a small supernova represents a threat to life on Earth. Supernovas are created during the last moments of a star's life. These gigantic explosions can wipe out galaxies and the planets inside them.
How hot is a supernova?
1,000,000,000 degrees CelsiusA supernova can light the sky up for weeks. The temperature in a supernova can reach 1,000,000,000 degrees Celsius. This high temperature can lead to the production of new elements which may appear in the new nebula that results after the supernova explosion.
Can a supernova destroy a galaxy?
At a certain distance, even a small supernova represents a threat to life on Earth. Supernovas are created during the last moments of a star's life. These gigantic explosions can wipe out galaxies and the planets inside them.
Do supernovae create black holes?
Overview. Failed supernovae are thought to create stellar black holes by the collapsing of a red supergiant star in the early stages of a supernova.
What happens after a star explodes?
So what happens to the parts that aren't blown away? CAITY: So the core of a star collapses when the rest of it is exploding outward. So that core will continue to collapse under its own gravity and it can form one of two objects. It can become something called a neutron star or it can form into a black hole.
How long would it take a supernova to reach Earth?
The supernova is about 13,000 light-years away. A light-year is the distance that light can travel in a year -- about 6 trillion miles (10 trillion kilometers). Because the supernova is 13,000 light-years away, it took 13,000 years for light from the exploded star to reach Earth.
Observation history
The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.
Discovery
Early work on what was originally believed to be simply a new category of novae was performed during the 1920s. These were variously called "upper-class Novae", "Hauptnovae", or "giant novae". The name "supernovae" is thought to have been coined by Walter Baade and Fritz Zwicky in lectures at Caltech during 1931.
Naming convention
Supernova discoveries are reported to the International Astronomical Union 's Central Bureau for Astronomical Telegrams, which sends out a circular with the name it assigns to that supernova. The name is formed from the prefix SN, followed by the year of discovery, suffixed with a one or two-letter designation.
Classification
Astronomers classify supernovae according to their light curves and the absorption lines of different chemical elements that appear in their spectra. If a supernova's spectrum contains lines of hydrogen (known as the Balmer series in the visual portion of the spectrum) it is classified Type II; otherwise it is Type I.
Current models
In the galaxy NGC 1365 a supernova (the bright dot slightly above the galactic center) rapidly brightens, then fades more slowly.
Other impacts
Supernovae are a major source of elements in the interstellar medium from oxygen through to rubidium, though the theoretical abundances of the elements produced or seen in the spectra varies significantly depending on the various supernova types. Type Ia supernovae produce mainly silicon and iron-peak elements, metals such as nickel and iron.
Milky Way candidates
The next supernova in the Milky Way will likely be detectable even if it occurs on the far side of the galaxy. It is likely to be produced by the collapse of an unremarkable red supergiant and it is very probable that it will already have been catalogued in infrared surveys such as 2MASS.
History of supernova observations
Various civilizations recorded supernovae long before the telescope was invented. The oldest recorded supernova is RCW 86, which Chinese astronomers saw in A.D. 185. Their records show that this "guest star" stayed in the sky for eight months, according to NASA.
Star death
On average, a supernova will occur about once every 50 years in a galaxy the size of the Milky Way. Put another way, a star explodes every second or so somewhere in the universe, and some of those aren't too far from Earth.
Type II supernovae
Let's look at the more exciting Type II first. For a star to explode as a Type II supernova, it must be at several times more massive than the sun (estimates run from eight to 15 solar masses). Like the sun, it will eventually run out of hydrogen and then helium fuel at its core. However, it will have enough mass and pressure to fuse carbon.
Caught in the act
Recent studies have found that supernovas vibrate like giant speakers and emit an audible hum before exploding.
What is Supernova Explosion?
Gamma rays released in the Supernova Explosion are harmful for life. (Credit: NASA)
History of supernova Explosion
The supernovae in any galaxy are not too frequent and there are normally two to three supernovae observed per century. The supernovae occurred in our galaxy were observed in the past by Chinese, European and Islamic astronomers.
Types of Supernova Explosion
The nature of all the supernovae are not same, they have different light spectrum which indicate the presence of different elements. Light spectrum is obtained by passing the light of supernova from prism which splits the light into its component just like rainbow. The pattern obtained after passing through prism is called light spectrum.
Type Ia Supernova due to Thermonuclear runaway
Thermonuclear runaway supernova occurs in binary stars in which one of them has become white dwarf. As we have learned in earlier post “ stellar evolution ” that the core of stars which have mass less than 1.4 times the mass of sun end up their life into white dwarf. This limit of 1.4 times of solar mass is also known as Chandrasekhar Limit.
Type II Supernova due to Core Collapse
Core collapse supernova occurs when the mass of core of star is more than 1.4 times the solar mass. As we have learned that in the massive star the chain of nuclear reaction stops at iron. As the iron has highest stability and the conversion of iron into higher element do not produce energy instead they requires input of energy.
Impact of Supernova Explosion
Supernovae play an important role in the evolution of universe. The supernova distributes the heavy elements in the interstellar medium. The shock waves originated by supernova also helps in the formation of new stars. Supernova can also affect the biosphere of any planet having life if the distance of supernova from planet is not large.
Formation of heavy elements
The energy released in the supernova is so large that the hydrogen in the upper layer undergo nuclear chain reaction and give rise to element heavier than iron like copper, gold, silver and even uranium etc. The supernova throws these newly formed heavier elements into the interstellar medium.

Overview
A supernova is a powerful and luminous explosion of a star. It has the plural form supernovae /-viː/ or supernovas, and is abbreviated SN or SNe. This transient astronomical event occurs during the last evolutionary stages of a massive star or when a white dwarf is triggered into runaway nuclear fusion. The original object, called the progenitor, either collapses to a neutron star or black hole, or is comp…
Observation history
Compared to a star's entire history, the visual appearance of a supernova is very brief, sometimes spanning several months, so that the chances of observing one with the naked eye is roughly once in a lifetime. Only a tiny fraction of the 100 billion stars in a typical galaxy have the capacity to become a supernova, being restricted to those having high mass and rare kinds of binary stars contai…
Naming convention
Supernova discoveries are reported to the International Astronomical Union's Central Bureau for Astronomical Telegrams, which sends out a circular with the name it assigns to that supernova. The name is formed from the prefix SN, followed by the year of discovery, suffixed with a one or two-letter designation. The first 26 supernovae of the year are designated with a capital letter from A …
Classification
Astronomers classify supernovae according to their light curves and the absorption lines of different chemical elements that appear in their spectra. If a supernova's spectrum contains lines of hydrogen (known as the Balmer series in the visual portion of the spectrum) it is classified Type II; otherwise it is Type I. In each of these two types there are subdivisions according to the presence of lines from other elements or the shape of the light curve (a graph of the supernova's apparen…
Current models
Supernova type codes, as summarised in the table above, are taxonomic: the type number is based on the light observed from the supernova, not necessarily its cause. For example, type Ia supernovae are produced by runaway fusion ignited on degenerate white dwarf progenitors, while the spectrally similar type Ib/c are produced from massive stripped progenitor stars by core collapse.
External impact
Supernovae events generate heavier elements that are scattered throughout the surrounding interstellar medium. The expanding shock wave from a supernovae can trigger star formation. Galactic cosmic rays are generated by supernova explosions.
Supernovae are a major source of elements in the interstellar medium from ox…
Milky Way candidates
The next supernova in the Milky Way will likely be detectable even if it occurs on the far side of the galaxy. It is likely to be produced by the collapse of an unremarkable red supergiant and it is very probable that it will already have been catalogued in infrared surveys such as 2MASS. There is a smaller chance that the next core collapse supernova will be produced by a different type of massi…
See also
• Kilonova – Supernova formed from a neutron star merger
• List of supernovae
• List of supernova remnants
• Quark-nova – Hypothetical violent explosion resulting from conversion of a neutron star to a quark star
How The Term “Nova” Was invented?
Catastrophic Nuclear Explosion
What Causes A Nova?
What Is A Supernova Explosion?
- A supernova is a stellar explosion that can outshine an entire galaxy for a brief period of time. The amount of energy, that is radiated in this explosion, is as much as the Sun or any other ordinary star is expected to emit over its entire lifespan, but this radiation is over a brief burst. The supernova explosion gradually fades from view over a ...
How Supernova Was Discovered?
Supernova Is Extremely Rare
How It Is expressed?