1 00:00:06,630 --> 00:00:03,350 when a star like our sun begins to die 2 00:00:08,870 --> 00:00:06,640 it expands into a bloated red giant star 3 00:00:10,310 --> 00:00:08,880 shedding mass by puffing off its outer 4 00:00:12,709 --> 00:00:10,320 layers 5 00:00:15,110 --> 00:00:12,719 this change alters the gravitational 6 00:00:17,830 --> 00:00:15,120 influence the star has on its planetary 7 00:00:20,310 --> 00:00:17,840 system the gravity of the remaining 8 00:00:22,870 --> 00:00:20,320 large planets can disrupt the orbits of 9 00:00:25,429 --> 00:00:22,880 small objects like asteroids comets and 10 00:00:27,910 --> 00:00:25,439 moons scattering them like pinballs in 11 00:00:29,349 --> 00:00:27,920 an arcade game into exaggerated oval 12 00:00:31,589 --> 00:00:29,359 orbits 13 00:00:34,389 --> 00:00:31,599 as the red giant star runs out of its 14 00:00:37,350 --> 00:00:34,399 nuclear fuel it begins to contract 15 00:00:38,790 --> 00:00:37,360 creating a compact white dwarf star no 16 00:00:40,869 --> 00:00:38,800 larger than earth 17 00:00:43,270 --> 00:00:40,879 the exaggerated orbits of the wayward 18 00:00:45,510 --> 00:00:43,280 objects may bring them very close to the 19 00:00:47,910 --> 00:00:45,520 star where they experience powerful 20 00:00:50,549 --> 00:00:47,920 tidal forces that tear them apart 21 00:00:52,950 --> 00:00:50,559 creating a gas and dust disk around the 22 00:00:55,029 --> 00:00:52,960 white dwarf that eventually falls onto 23 00:00:57,270 --> 00:00:55,039 the star's surface 24 00:00:58,869 --> 00:00:57,280 five billion years from now when our sun 25 00:01:01,430 --> 00:00:58,879 is at the end of its life 26 00:01:03,830 --> 00:01:01,440 mercury venus and earth will likely be 27 00:01:05,350 --> 00:01:03,840 completely vaporized as the sun becomes 28 00:01:07,270 --> 00:01:05,360 a red giant 29 00:01:09,990 --> 00:01:07,280 the orbits of asteroids in the main 30 00:01:11,830 --> 00:01:10,000 asteroid belt will be altered eventually 31 00:01:13,750 --> 00:01:11,840 falling onto the white dwarf that our 32 00:01:15,590 --> 00:01:13,760 sun will become 33 00:01:18,230 --> 00:01:15,600 this scenario is exactly what is 34 00:01:19,710 --> 00:01:18,240 happening to a nearby white dwarf star 35 00:01:23,190 --> 00:01:19,720 named 36 00:01:25,910 --> 00:01:23,200 g23844 the star's death throws have so 37 00:01:28,310 --> 00:01:25,920 violently disrupted its planetary system 38 00:01:30,630 --> 00:01:28,320 that it is actively siphoning off debris 39 00:01:32,069 --> 00:01:30,640 from both the system's inner and outer 40 00:01:34,230 --> 00:01:32,079 reaches 41 00:01:36,390 --> 00:01:34,240 using archival data from hubble and 42 00:01:38,469 --> 00:01:36,400 other nasa space observatories 43 00:01:40,710 --> 00:01:38,479 astronomers have for the first time 44 00:01:44,149 --> 00:01:40,720 observed a white dwarf star consuming 45 00:01:46,630 --> 00:01:44,159 both rocky metallic and icy material 46 00:01:49,190 --> 00:01:46,640 the findings are intriguing because icy 47 00:01:52,149 --> 00:01:49,200 bodies are credited with irrigating dry 48 00:01:54,069 --> 00:01:52,159 rocky planets billions of years ago 49 00:01:56,789 --> 00:01:54,079 comets and asteroids are thought to have 50 00:01:58,950 --> 00:01:56,799 hit our planet delivering water and 51 00:02:00,630 --> 00:01:58,960 sparking the conditions necessary for 52 00:02:02,630 --> 00:02:00,640 life as we know it 53 00:02:04,789 --> 00:02:02,640 the makeup of the bodies raining onto 54 00:02:06,870 --> 00:02:04,799 the white dwarf implies that icy 55 00:02:08,949 --> 00:02:06,880 reservoirs might be common among 56 00:02:11,029 --> 00:02:08,959 planetary systems 57 00:02:13,030 --> 00:02:11,039 this white dwarf provides a unique 58 00:02:14,949 --> 00:02:13,040 opportunity to take distant planets 59 00:02:16,790 --> 00:02:14,959 apart and see what they were made of 60 00:02:17,750 --> 00:02:16,800 when they were first formed around the 61 00:02:19,910 --> 00:02:17,760 star 62 00:02:22,020 --> 00:02:19,920 letting us better understand what makes