SUPERNOVA: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 jettison matter into space at some 9,000 to 25,000 miles (15,000 to 40,000 kilometers) per second. These blasts produce much of the material in the universe—including 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.
Few stars become supernovae. Many stars cool in later life to end their days as white dwarfs and, later, black dwarfs.
Star Fusion
But massive stars, 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—becoming ever denser and hotter.
White Dwarfs
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.
If a white dwarf takes on enough mass it reaches a level called the Chandrasekhar Limit. At this point the pressure at its center will become so great that runaway fusion occurs and the star detonates in a thermonuclear supernova.
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 (at least ten times the size of our sun) that 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.
COSMIC COLLISIONS:
For example, we most likely have a moon because a protoplanet about the size of Mars careened into early Earth, breaking off a glob of material that coalesced in orbit around us.
We also most likely have dominion over the planet because another huge object crashed the dinosaur's party about 65 million years ago, triggering the mass extinction that allowed mammals to flourish.Considering that it's happened before, astronomers are anticipating that catastrophic collisions with Earth might happen again, and there are people who have dedicated their lives to understanding the risks and thinking up solutions.
