What is a SuperNova?
A SuperNova is a natural phenomena in the nature of stars and space which takes place when a very big star known as the neutron star explodes! this explosion is so great that its effects will stay for 100 thousand years, it is so great that if it took place in our galaxy the brightness of the explosion will blind every eye on earth.
A supernova is the catastrophic death of a star, characterized by a massive output of energy. In the Milky Way, supernovae are relatively rare, with a few notable incidences of historical supernovae recorded as far back as 185 CE. Many previous supernovae were probably topics of conversation and concern among the people who witnessed them. Around the universe, several hundred are observed and recorded each year, providing information about the formation of the universe and the objects within it. There are two basic types of supernova, although each type is broken up into subtypes. In the case of a Type One, an instability arises in the chemical makeup of the star, leading to a thermonuclear explosion of formidable power. The core temperature of the star rises as a result of pressure and the imbalance, ultimately igniting the star in an explosion which can sometimes be visible with the naked eye from Earth. A Type Two supernova involves the collapse of the core of a star, triggering a c
A supernova (plural: supernovae) is a stellar explosion. They are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months. During this short interval, a supernova can radiate as much energy as the Sun could emit over its life span.[1] The explosion expels much or all of a star’s material[2] at a velocity of up to a tenth the speed of light, driving a shock wave[3] into the surrounding interstellar medium. This shock wave sweeps up an expanding shell of gas and dust called a supernova remnant. Several kinds of supernovas exist that may be triggered in one of two ways, running out of fuel or. After the core of an aging massive star ceases to generate energy from nuclear fusion, it may undergo sudden gravitational collapse into a neutron star or black hole, releasing gravitational potential energy that heats and expels the star’s outer layers. Alternatively, a white dwarf star may accumulate suff
