Compared to a supernova, a nuclear bomb would be like a puff of breath in a hurricane. Even a SMALL star is the equivalent of millions of hydrogen bombs PER SECOND, and a supernova is billions of times more powerful.
However, a nuclear explosion IS like one grain of sand out of the center of a star; with a temperature of millions of degrees for a tiny fraction of a second.
There is no way of knowing which star will next go "supernova".However, closer to home, Betelgeuse is the most likely to produce a supernova - within humanities lifetime.
When a single high mass star explodes, it undergoes a supernova event. The core collapses inwards and then rebounds explosively, sending out a shockwave that ejects the outer layers of the star into space. This explosion can outshine an entire galaxy for a short period of time.
Something short-lived or passing is called ephemeral.
When the core of a super giant collapses, it can trigger a supernova explosion. The intense heat and pressure leads to the fusion of heavier elements and the release of a tremendous amount of energy, resulting in a massive explosion that can outshine entire galaxies for a short period of time. This explosion also disperses newly formed elements and enriches the surrounding space, playing a key role in the creation of new stars and planets.
There aren't really any comparisons to be made to a supernova. Let's try one; a supernova is as much brighter than the Sun is as the Sun is to a flashlight. A supernova will release as much energy in an hour as a regular star does in its entire 10-billion year life.
There is no way of knowing which star will next go "supernova".However, closer to home, Betelgeuse is the most likely to produce a supernova - within humanities lifetime.
Long-lived stars are typically lower in mass, shine less brightly, and have longer lifespans compared to short-lived stars. Short-lived stars tend to be more massive, burn through their fuel more rapidly, and have shorter lifespans before evolving or ending in a supernova explosion.
When a star explodes, it releases an immense amount of energy, creating a supernova. This explosion can outshine an entire galaxy for a short period of time. Supernovae are crucial for the formation of heavy elements and can also cause the star to collapse and form a black hole or neutron star.
A short circuit is what usually causes a switchboard explosion.
When a single high mass star explodes, it undergoes a supernova event. The core collapses inwards and then rebounds explosively, sending out a shockwave that ejects the outer layers of the star into space. This explosion can outshine an entire galaxy for a short period of time.
TNT (the dynamite that caused the explosion) pop (the sound a small explosion might make)
SUPERNOVAE * A rare celestial phenomenon involving the explosion of most of the material in a star, resulting in an extremely bright, short-lived object that emits vast amounts of energy. * A supernova shines typically for several weeks to several months with a luminosity between 2 × 108 and 5 × 109 times that of the Sun, then gradually fades away. Each explosion ejects from one to several tens of solar masses at speeds ranging from thousands to tens of thousands of kilometers per second.
Yes, the presence of certain radioactive isotopes with short half-lives in meteorites suggests that the solar system formed shortly after a nearby supernova explosion, as these isotopes would have been formed in the supernova and then incorporated into the early solar system material. This timeline is supported by both astronomical observations and isotopic dating of meteorites.
An object further away will appear less bright than the same object closer to us. However, a supernova can emit the same brightness as our Sun does in it's whole lifetime, in a very short period of time - a nova on the other hand, at maximum brightness is only about 100,000 times that of the Sun.
Short-lived Ministry was created in 1746.
Short-lived Ministry ended in 1746.
It was because they were short-lived. Their love outlasted their lives.