1 00:00:00,020 --> 00:00:12,020 Music 2 00:00:12,040 --> 00:00:16,040 Narrator: In this activity, you'll model and measure the collapse of a large star to 3 00:00:16,060 --> 00:00:20,060 understand the important role of density in black holes. You'll need a 4 00:00:20,080 --> 00:00:24,080 latex balloon, blown-up to 6-8 inches in diameter, a few 5 00:00:24,100 --> 00:00:28,140 sheets of aluminum foil, a digital scale, 6 00:00:28,160 --> 00:00:32,200 a flexible tape measure, 7 00:00:32,220 --> 00:00:36,250 and a pair of scissors, or another sharp implement. 8 00:00:36,270 --> 00:00:40,320 Completely wrap the balloon in the aluminum foil, when you're done wrapping, you don't 9 00:00:40,340 --> 00:00:44,400 want to see any of the balloon peeking out. It may take a few sheets of foil to 10 00:00:44,420 --> 00:00:48,480 do this, depending on the size of the balloon, so use whatever you need. This 11 00:00:48,500 --> 00:00:52,520 foil-wrapped balloon represents a large star. 12 00:00:52,540 --> 00:00:56,560 Measure the circumference of the balloon with the tape measure and weigh the balloon on the scale. Record your 13 00:00:56,580 --> 00:01:00,600 baseline measurements. Gently squeeze the balloon, here 14 00:01:00,620 --> 00:01:04,710 you are the giant "hands" of gravity and the balloon should resist being squeezed 15 00:01:04,730 --> 00:01:08,790 because of the air pressure within the balloon. This is similar to what happens 16 00:01:08,810 --> 00:01:12,860 during the normal life a star, when gravity is balanced by fusion energy 17 00:01:12,880 --> 00:01:16,870 created at the core of the star. Now you're ready to simulate the end of the star's 18 00:01:16,890 --> 00:01:20,900 life as it runs out of fuel and that balance is broken. Pop the balloon 19 00:01:20,920 --> 00:01:25,040 carefully, trying not to crush the aluminum foil as you pop it. 20 00:01:25,060 --> 00:01:29,070 Be the hands of gravity again and gently squeeze the aluminum ball. 21 00:01:29,090 --> 00:01:33,090 This time, it doesn't push back. Make it about an inch smaller, 22 00:01:33,110 --> 00:01:37,140 keeping it as round as possible. Again, measure its circumference and weight, 23 00:01:37,160 --> 00:01:41,180 and record your new measurements. You'll repeat 24 00:01:41,200 --> 00:01:45,220 those steps a few more times, crushing down the foil ball about an inch more between measurements. 25 00:01:45,240 --> 00:01:49,250 For you final measurement, crush the ball as much as you possibly can, 26 00:01:49,270 --> 00:01:53,280 while keeping it round. Take one final measurement of its circumference and weight. 27 00:01:53,300 --> 00:01:57,320 You'll see that even though the size of the ball changed, its mass did not. 28 00:01:57,340 --> 00:02:01,350 This means that it just got more and more dense, like when a star collapses 29 00:02:01,370 --> 00:02:03,370 into a black hole. 30 00:02:03,390 --> 00:02:15,265 Music