1 00:00:10,260 --> 00:00:16,530 A black hole is a single point in space that has a lot of mass. One of the ways 2 00:00:16,530 --> 00:00:21,620 that we look for black holes is to develop new instruments 3 00:00:21,620 --> 00:00:25,560 and new technologies that can try to search for them. 4 00:00:30,300 --> 00:00:37,100 As we've observed black holes including the the supermassive black hole in the center of our galaxy, 5 00:00:39,280 --> 00:00:43,180 because it has such a strong gravity because it has lots of mass, 6 00:00:43,540 --> 00:00:46,540 stars will orbit black holes 7 00:00:46,740 --> 00:00:56,040 and as stars get closer and closer to the center of a black hole as it crosses over the Event Horizon, 8 00:00:56,340 --> 00:01:01,640 what will happen is that the material of these stars will get shredded apart, 9 00:01:02,180 --> 00:01:09,580 because the gravitational pull of a black hole is so strong that the material of the stars gets pulled apart. 10 00:01:11,220 --> 00:01:16,700 But there is an event horizon, which is the point at which the black hole's gravity 11 00:01:16,700 --> 00:01:20,220 starts to pull you so much that you can't escape. 12 00:01:20,720 --> 00:01:23,620 So as you approach the black hole, you'll feel its pull. 13 00:01:24,020 --> 00:01:29,852 But then as you get closer and closer and closer towards the event horizon, that's the point of no return so you couldn't 14 00:01:29,900 --> 00:01:30,720 escape past that. 15 00:01:32,340 --> 00:01:39,140 The easiest way to think of a black hole is just like anything that has mass so the Earth has mass 16 00:01:39,460 --> 00:01:43,460 And one of the reasons that the Moon orbits around the Earth 17 00:01:43,780 --> 00:01:50,480 is because the gravitational attraction of these two massive bodies. And so, Earth is distorting 18 00:01:50,900 --> 00:01:59,024 the space around the Moon and so that's what keeps the Moon in orbit. And so now take that to an extreme. So take 19 00:01:59,096 --> 00:02:01,900 something that's as massive as the Sun, 20 00:02:02,300 --> 00:02:06,700 or as massive as a million Suns and put it at a single point, 21 00:02:07,200 --> 00:02:14,200 and that distortion that you get is coming from that amount of mass in a single point. 22 00:02:19,160 --> 00:02:28,352 Black holes vary in size a lot. We know that black holes can be formed by massive stars exploding and then collapsing into 23 00:02:28,428 --> 00:02:29,860 the singular point. 24 00:02:30,140 --> 00:02:35,540 And those give us black holes that are about the mass of the Sun. So, those are solar mass black holes. 25 00:02:35,660 --> 00:02:40,960 However, we also know at the center of galaxies, like the Milky Way, 26 00:02:41,700 --> 00:02:47,100 there are supermassive black holes and these are millions or even billions of times the mass of the Sun. 27 00:02:47,280 --> 00:02:58,060 And how these form is actually a mystery. Studying black holes really gives us a fundamental insight 28 00:02:58,060 --> 00:03:01,580 into how gravity works because 29 00:03:01,720 --> 00:03:07,020 it's such a small physical scale, but it's a super massive object. 30 00:03:07,020 --> 00:03:11,100 And so understanding how black holes work and the 31 00:03:11,100 --> 00:03:18,261 interactions of black holes in other parts of the universe really give us a fundamental insight that we could then use to 32 00:03:18,331 --> 00:03:21,320 think about how our own solar system works. 33 00:03:22,180 --> 00:03:29,580 And so if we can understand how black holes work, they'll give us a key to really understanding our universe.