Supernova

Background

A nova is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star that slowly fades over weeks or months.

Back in the 1950's all the science fiction novels which needed an earth-shattering kaboom would use a Nova. Star goes boom, incinerates the entire solar system, pretty apocalyptic. Astronomers didn't know anything about novae except they were huge, so science fiction author had free reign.

Nowadays we know that novae happen only in binary star systems. A normal star has the misfortune to be orbited by a white dwarf. Over the millennium the dwarf sucks hydrogen out of the normal star like a cosmic vampire. The dwarf starts burning the hydrogen using carbon-nitrogen-oxygen fusion reaction.

Sometimes the the white dwarf suffers a runaway reaction, and you get a nova.

The fact that a white dwarf is required made instantly obsolete all those science fiction stories about the sun going nova.

With each explosion only about one ten-thousandth of the white dwarf's mass is ejected. The point is that a vampire white dwarf can go nova multiple times. For instance, the star RS Ophiuchi has gone nova six times. The mass is ejected at velocities up to several thousand kilometers per second.

Astronomers estimate that about 30 to 60 novae occur in our galaxy per year.

A nova can reach an absolute magnitude of -8.8, or about 42.7 trillion times the luminosity of the sun. Nova emit about 10-7 Foe or about 10³⁷ joules.

Novae to eject enriched elements into the interstellar medium like red giant, supergiant stars, and supernovae do. But only a paltry amount. Supernovae emit 50 times as much, and red giant/supergiant stars emit 200 times as much.

Dwarf Nova are also called U Geminorum variable, being one of several types of cataclysmic variable star, consisting of a close binary star system in which one of the components is a white dwarf that accretes matter from its companion. Their increase in luminosity is not due to a fusion explosion. Rather it is a vampire white dwarf star whose accretion disk becomes unstable. Part of the disk suddenly collapse onto the white dwarf and releases large amounts of gravitational potential energy.

This only releases a tiny fraction of the energy of a full fledged nova, and would be difficult to detect from another solar system without a telescope. It is hardly apocalyptic.

It is only mentioned here in case you run across the term in your researches and get confused.

Luminous Red Nova is a stellar explosion believed to be caused by the merging of two stars. They are characterised by a distinct red colour, and a light curve that fades slowly with resurgent brightness in the infrared. Luminous red novae are not related to standard novae, which are explosions that occur on the surface of white dwarf stars.

Kilonova are caused when two neutron stars or a neutron star and a black hole merge. Kilonovae not only emit intense bursts of light, but also lots of gravitational waves. These mergers are thought to produce gamma-ray bursts and emit bright electromagnetic radiation, called "kilonovae", due to the radioactive decay of heavy r-process nuclei that are produced and ejected fairly isotropically during the merger process. The measured high sphericity of the kilonova AT2017gfo at early epochs was deduced from the blackbody nature of its spectrum.

Kilonovae emit about 10^-5 Foe (10³⁹ joules) to 10^-3 Foe (10⁴¹ joules).

A supernova (pl.: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova 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 completely destroyed to form a diffuse nebula. The peak optical luminosity of a supernova can be comparable to that of an entire galaxy before fading over several weeks or months. The word supernova has the plural form supernovae or supernovas and is often abbreviated as SN or SNe. It is derived from the Latin word nova, meaning 'new', which refers to what appears to be a temporary new bright star. Adding the prefix "super-" distinguishes supernovae from ordinary novae, which are far less luminous. The word supernova was coined by Walter Baade and Fritz Zwicky, who began using it in astrophysics lectures in 1931. Its first use in a journal article came the following year in a publication by Knut Lundmark, who may have coined it independently. Supernovae are divided into two basic physical types:
Type Ia
These result from some binary star systems in which a carbon-oxygen white dwarf is accreting matter from a companion. (What kind of companion star is best suited to produce Type Ia supernovae is hotly debated.) In a popular scenario, so much mass piles up on the white dwarf that its core reaches a critical density of 2 x 1⁰⁹ g/cm³. This is enough to result in an uncontrolled fusion of carbon and oxygen, thus detonating the star.
Type II
These supernovae occur at the end of a massive star's lifetime, when its nuclear fuel is exhausted and it is no longer supported by the release of nuclear energy. If the star's iron core is massive enough, it will collapse and become a supernova. However, these types of supernovae were originally classified based on the existence of hydrogen spectral lines: Type Ia spectra do not show hydrogen lines, while Type II spectra do. In general this observational classification agrees with the physical classification outlined above, because massive stars have atmospheres that are made of mostly hydrogen, while white dwarf stars are bare. However, if the original star was so massive that its strong stellar wind had already blown off the hydrogen from its atmosphere by the time of the explosion, then it too will not show hydrogen spectral lines. These supernovae are often called Type Ib supernovae, despite really being part of the Type II class of supernovae. Looking at this discrepancy between our modern classification, which is based on a true difference in how supernovae explode, and the historical classification, which is based on early observations, one can see how classifications in science can change over time as we better understand the natural world.

A hypernova is a very energetic supernova which is believed to result from an extreme core-collapse scenario. In this case, a massive star (>30 solar masses) collapses to form a rotating black hole emitting twin astrophysical jets and surrounded by an accretion disk. It is a type of stellar explosion that ejects material with an unusually high kinetic energy, an order of magnitude higher than most supernovae, with a luminosity at least 10 times greater. Hypernovae release such intense gamma rays that they often appear similar to a type Ic supernova, but with unusually broad spectral lines indicating an extremely high expansion velocity. Hypernovae are one of the mechanisms for producing long gamma ray bursts (GRBs), which range from 2 seconds to over a minute in duration. They have also been referred to as superluminous supernovae, though that classification also includes other types of extremely luminous stellar explosions that have different origins.

General Information

Name: Nova, Novae, Novas

Other Names: Dwarf Nova, Luminous Red Nova, Kilonova, Supernova, Hypernova

Origin: Real World

Appearance:

• Nova: Typically around 35 to 75 per year within the Milky Way Galaxy.
• Dwarf Nova: No found official recorded amount, though they normally appear within the Milky Way Galaxy.
• Luminous Red Nova: The Large Synoptic Survey Telescope repotedly observes 20-750 luminous red novaes per year.
• Kilonova: Extremely rare, with it being believed that only 10 such systems can have an event like this occur in the entire Milky Way Galaxy.
• Supernova: Typically once every 50 years in the Milky Way Galaxy.
• Hypernova: The data is harder to find on this as a hypernova is a massively amplified supernova, thus the supernovas observed can at times be hypernovas.

Classification: Stellar Explosions, Cataclysmic Variable

Environment: Outer Space

Result: Massive amount of luminosity energy that can be seen from telescopes, can also at times result in black holes.

Codex Statistics

Key: Nova | Luminous Red Nova | Kilonova | Supernova

Tiering System: Varies, normally High 5-B to Low 4-C, Lower with Dwarf Nova | Varies | Varies, normally 5-A to 4-C to High 4-C | Varies normally 4-B, Higher with Hypernova

Attack Potency: Varies (Novas vary depending on the star and white dwarf), normally Large Planet level (Novas can emit about 10^-7 Foe or about 10³⁷ joules) to Low Mass Star level (Each nova releases up to 100,000 times the annual energy output of our sun, with the sun producing 1.23x10³⁵ joules of energy in one year(1.23e40 Joules)), Lower with Dwarf Nova (Dwarf Novas release a tiny fraction of energy of a full-fledged nova) | Varies (Luminous Red Nova's carry luminosities between that of a nova and that of a supernova) | Varies (Kilonovas are caused from compact objects crashing together), normally Brown Dwarf level (Kilonovas are about 1000 times brighter than a nova(1e40 Joules)) to Star level to High Mass Star level (Kilonovas are also about 1/10th to 1/100th the brightness of a typical supernova(1e42 to 1e44 Joules)) | Varies, normally Solar System Level (Supernova explosions release energies of about 10⁴⁴ joules, the supernova is the event that helped determine the composition of the Solar System 4.5 billion years ago, and may even have triggered the formation of this system), Higher with Hypernova (Hypernovas release about 10^53 ergs or around 9.99e45 joules)

Attack Speed: Relativistic core collapse (Novas collapse inward at 70,000 kilometers per second or about 23% the speed of light), Relativistic+ with Gamma Ray Burst (Novas release a gamma ray, resulting in a minimum velocity of approximately 299,792,158 m/s (99.9999% the speed of light) being described as a particles accelerating near the speed of light), Speed of Light with Gravitational Waves (Core collapsing causes gravitational waves which travel at the speed of light)

Range: Varies, normally at least Stellar for typical nova explosions (Nova explosions normally produce so much light, they can be seen from distant solar systems without a telescope and can be seen from other galaxies), Interplanetary with Supernovas (The supernova is the event that helped determine the composition of the Solar System 4.5 billion years ago, and may even have triggered the formation of this system), Lower with Dwarf Novas (Dwarf Novas are difficult to detect from another solar system without a telescope)

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Powers and Techniques

Absorption, Light Manipulation & Fusionism (Novas happen when a white dwarf absorbs material from a binary companion, the hydrogen undergoes fusion which causes it to brighten up significantly causing up to 100,000 times more enery released into space), Extreme Heats (Novas absorbing from another star causes its surface temperature to reach temperatures up to 20 million kelvin causing the hydrogen to fuse), Radiation Manipulation (Novas release a gamma radiation, an electromagnetic radiation described in terms of astream of photons that are massless particles each traveling in a wave-line pattern and moving at the speed of light), Gravity Manipulation (Core collapsing causes gravitational waves), Black Hole Creation (Novas are the result of dying stars, which black holes can form before a nova or supernova through the collapse of a neutron star)

All previous Nova powers and abilities, Black Hole Creation & Explosion Manipulation (Kilonovas electromagnetic raidation blast can happen through two neutron stars colliding or a neutron star and a stellar-mass black hole colliding and merging)

All previous Nova powers and abilities, Explosion Manipulation (A supernova when a star runs out of fuel in its core and detonates with an enormous explosion)