~astro-craze~

Some stars behave as if it's better to burn out than to fade away. These stars end their evolutions in massive cosmic explosions known as supernovae.

When supernovae explode they produces matter into space at some 15,000 to 40,000 kilometers per second. These blasts produce much of the material in the universe. These includes some elements, like iron, which make up our planet and even ourselves. Heavy elements are only produced in supernovae, so all of us carry the remnants of these distant explosions within our own bodies.

Supernovae add enriching elements to space clouds of dust and gas, further interstellar diversity, and produce a shock wave that compresses clouds of gas to aid new star formation.

But only a select few stars become supernovae. Many stars cool in later life to end their days as white dwarfs and, later, black dwarfs.

As for massive stars, which some of them maybe many times larger than our own sun, may create a supernova when their core's fusion process runs out of fuel. Star fusion provides a constant outward pressure, which exists in balance with the star's own mass-driven, inward gravitational pull. When fusion slows, outbound pressure drops and the star's core begins to condense under gravity. It becomes ever denser and hotter!

To outward appearances, such stars begin growing, swelling into bodies known as red supergiants, which I posted in earlier posts. But at their cores shrinking continues, making a supernova imminent. Imminent here means overhanging, or in another word, it’s jutting out.

When a star's core contracts to a critical point a series of nuclear reactions is unleashed. This fusion staves off core collapse for a time—but only until the core is composed largely of iron, which can no longer sustain star fusion.

In a microsecond, the core may reach temperatures of billions of degrees Celsius. 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.

Supernovae also occur in binary star systems. Smaller stars, up to eight times the mass of our own sun, typically evolve into white dwarves. A star condensed to this size, about that of Earth, is very dense and thus has strong enough gravitational pull to gather material from the system's second star if it is close enough.

A supernova can light the sky up for weeks, and the massive transfer of matter and energy leaves behind a very different star.

Typically only a tiny core of neutrons, a spinning neutron star, is left to evidence a supernova. Neutron stars give off radio waves in a steady stream or, as pulsars, in intermittent bursts.

If a star was so massive, as in like ten times the size of our sun, it leaves behind a large core, a new phenomenon will occur. Because such a burned-out core has no energy source to fuse, and thus produces no outward pressure, it may become engulfed by its own gravity and turn into a cosmic sinkhole for energy and matter—a black hole, which I already post it before.

In my next post, I will tell you more about white dwarf and red dwarves.

for extra info, please log on to

= science.nationalgeographic.com/science/space/.../cosmic-explosion.html

= en.wikipedia.org/wiki/Supernova