1 00:00:00,000 --> 00:00:08,942 The Milky Way galaxy: a swirling disk of dust and gas. 2 00:00:09,509 --> 00:00:14,614 Dust makes up less than one percent of the Milky Way's total visible matter 3 00:00:14,748 --> 00:00:19,319 but is widespread throughout the galaxy. 4 00:00:19,419 --> 00:00:23,990 Scientists think many elements that make up dust 5 00:00:24,591 --> 00:00:27,560 originate from exploding stars. 6 00:00:30,130 --> 00:00:33,099 In some regions of the galaxy, gas and dust collect into denser blobs. 7 00:00:36,903 --> 00:00:41,541 These blobs have enough matter to gravitationally collapse 8 00:00:42,876 --> 00:00:44,811 sparking the formation of young stars 9 00:00:44,811 --> 00:00:46,413 surrounded by disks of gas 10 00:00:46,413 --> 00:00:48,081 and dust that could eventually form planets. 11 00:00:49,749 --> 00:00:55,588 By studying the dust strewn between stars, scientists can learn about 12 00:00:55,655 --> 00:01:02,629 the galaxy-wide recycling of elements from star birth to star death.