1 00:00:00,366 --> 00:00:04,166 Accretion. In short, accretion means growth by accumulation. 2 00:00:04,500 --> 00:00:08,100 Land on Earth can form from accretion of soil deposited by rivers or sea. 3 00:00:08,500 --> 00:00:11,900 Planetary bodies can also grow from accretion as gravitational forces 4 00:00:11,900 --> 00:00:14,100 attract debris and other matter. 5 00:00:14,100 --> 00:00:16,366 But we want to talk about accretion in astronomy. 6 00:00:16,366 --> 00:00:18,666 Accretion is one way we can see black holes. 7 00:00:18,966 --> 00:00:21,066 Black holes have intense gravitational mass, 8 00:00:21,066 --> 00:00:23,833 pulling in everything in the vicinity, including light. 9 00:00:24,200 --> 00:00:27,533 Without that light, we can't see black holes, but we can see 10 00:00:27,533 --> 00:00:30,633 the disk-shaped flow of gas and dust that forms around some black holes. 11 00:00:30,900 --> 00:00:33,133 We call these accretion disks, and they can form around 12 00:00:33,133 --> 00:00:36,033 black holes of any size, as well as around some stars. 13 00:00:36,600 --> 00:00:40,700 Material in black hole accretion disks is really hot, like millions of degrees. 14 00:00:41,066 --> 00:00:42,233 This is caused by the collision 15 00:00:42,233 --> 00:00:45,433 of particles in the accretion disk as they are pulled into their black hole. 16 00:00:46,200 --> 00:00:49,200 These collisions can cause accretion disks to release X-rays, 17 00:00:49,366 --> 00:00:51,400 which can allow us to locate some black holes.