Near the end of a star's life (a star similar to our own Sun), when the star has consumed most of its hydrogen by fusing the hydrogen into helium, the declining energy output of the star is no longer quite enough to keep the star's outer layers up against the star's gravity. So the star begins to collapse under its own gravity.
The gravitational collapse provides enough energy to kick the nuclear fusion reaction into overdrive, fusing the helium into carbon. The helium fusion releases far more energy, causing the star to explode abruptly.
Early observers watching the sky would occasionally observe a new star appearing suddenly where no star had been visible before. "New star" in latin is "nova stellarum"; so we call these ordinary stars dying "Nova". The "nova" stars shine brightly for weeks or months before fading into insignificance and disappearing again.
Now with powerful telescopes such as the 200-inch reflector at Mount Palomar, we can observe the stellar remnants. There is one in the constellation Orion, the Crab Nebula.
10000
10000 light years
It’s the bureau star
It’s the bureau star
the air pressure outside of the balloon decreases.
10000 10000 10000 10000 10000
20000-10000 = 10000
10,000,000,000,000,000
89/10000= 0.0089 * 10000/10000= 89/10000
0.50 percent of 10000 = 500.50% of 10000= 0.50% * 10000= 0.005 * 10000= 50
30 percent of 10000 = 300030% of 10000= 30% * 10000= 0.30 * 10000= 3000
10000 times 10000 equals 100000000.
45% of 10000= 45% * 10000= 0.45 * 10000= 4500
2.7% of 10000 = 2.7% * 10000 = 0.027 * 10000 = 270
It is 10000.
3300 * * * * * No. That is 33% of 10000. The question asked for 33%% of 10000 The correct answer is 33.
10000