Check out today's astronomy picture of the day, featuring a numerical relativity visualization made by some folks i… https://t.co/Y4dMYs4LYp
In the 1st year of the period Chih-ho, the 5th moon, the day chi-ch'ou, a guest star appeared...
Yang Wei-T'e, Imperial Astronomer of the Sung Dynasty, 1054 A.D.
Starting July 4, 1054 A.D., the people of the world were treated to an astonishing spectacle. A new star appeared in the sky. For 23 days, it was visible even during daylight. The star gradually faded following its appearance on July 4. After a little more than a year, the event was over entirely. It could no longer be seen, even at night. Its brief glory was recorded by Chinese and Korean astronomers, as well as American Indians of the Southwest United States. The witnesses to that singular event in 1054 were seeing a Supernova.
We've seen that old stars use up their fuel, cool off, and settle down into a White Dwarf, Neutron Star, or Black Hole. This usually doesn't happen very peacefully, however. The cooling is like a chair being tipped over. It is steady until it reaches the tipping point. Once it passes that point, it goes faster and faster. Soon, however, the inner layers of the star — its most dense part — will be stopped from falling by electron or neutron degeneracy pressure as the core changes into a miniature White Dwarf or Neutron Star. The falling matter from above will suddenly crash into this inner layer, and change too. The fall and crash happens in just seconds. All this sudden crashing and changing gives off enormous amounts of energy. That energy heats up the outer layers of the star and blows them out into space with fantastic speed. At its peak, a typical supernova might shine ten billion times more brightly than our Sun! Luckily, we are usually far enough away that this isn't too bright.
With such sudden movements of matter, the intense warpage of spacetime will change drastically and quickly. It should not be surprising, then, if gravitational waves are given off by a supernova. In fact, gravitational waves will only come out if the supernova has some "asymmetry" — that is, only if the supernova has bumps. This will likely happen, for example, if the original star was rotating very quickly. Fortunately, we expect most supernovae to go off in this way. Then, the gravitational waves will come out as one big — though brief — burst.
Carl Sagan said, "We are star stuff." He meant that we are made of matter that came from the stars. The Oxygen we breathe, the Carbon found in every cell in our bodies, the Calcium in our bones... all of this was formed in stars. Without supernovae to blow all this star stuff into the wide cosmos, however, it would all still be trapped deep inside of those stars. These most violent of explosions breathe life into the Universe.