1 00:00:08,780 --> 00:00:06,440 using nasa's spitzer space telescope 2 00:00:12,350 --> 00:00:08,790 we've looked at many nearby stars to 3 00:00:14,900 --> 00:00:12,360 look for orbiting dust and asteroids and 4 00:00:17,870 --> 00:00:14,910 comets orbiting debris leftover from the 5 00:00:19,639 --> 00:00:17,880 process of planet formation we saw 6 00:00:21,800 --> 00:00:19,649 something very unusual that we hadn't 7 00:00:25,790 --> 00:00:21,810 seen around any other star we saw 8 00:00:27,950 --> 00:00:25,800 evidence for a massive collision when 9 00:00:31,130 --> 00:00:27,960 the two objects collide everything 10 00:00:33,200 --> 00:00:31,140 happens very quickly in the animation 11 00:00:35,840 --> 00:00:33,210 things have been slowed down to allow 12 00:00:38,510 --> 00:00:35,850 you to see the impacting shockwave 13 00:00:41,650 --> 00:00:38,520 propagate across the surface of this 14 00:00:43,720 --> 00:00:41,660 devastated planet 15 00:00:46,150 --> 00:00:43,730 starting from the point of impact and 16 00:00:49,240 --> 00:00:46,160 circulate into the backside causing 17 00:00:51,730 --> 00:00:49,250 waves on the surface the entire planet 18 00:00:53,560 --> 00:00:51,740 becomes molten meanwhile tremendous 19 00:00:55,690 --> 00:00:53,570 amounts of material are ejected from the 20 00:00:57,640 --> 00:00:55,700 planet both outside of the system and 21 00:00:59,560 --> 00:00:57,650 some falls back under the system itself 22 00:01:01,810 --> 00:00:59,570 depending on the details of the 23 00:01:03,729 --> 00:01:01,820 collision whether it's a high impact or 24 00:01:06,580 --> 00:01:03,739 depending on the angle that the objects 25 00:01:09,130 --> 00:01:06,590 at each other at there there may be a 26 00:01:11,020 --> 00:01:09,140 growth or there may be grinding away so 27 00:01:12,760 --> 00:01:11,030 sometimes the planet actually ends up 28 00:01:14,890 --> 00:01:12,770 smaller after the collision but 29 00:01:16,780 --> 00:01:14,900 generally the planet grows to larger and 30 00:01:20,310 --> 00:01:16,790 larger until there's no more material 31 00:01:23,890 --> 00:01:20,320 left in the system for it to grow from 32 00:01:26,140 --> 00:01:23,900 while collisions like this are rare we 33 00:01:27,880 --> 00:01:26,150 don't see this large event in any other 34 00:01:30,550 --> 00:01:27,890 systems we've looked at with the spitzer 35 00:01:33,400 --> 00:01:30,560 space telescope collisions like this 36 00:01:34,900 --> 00:01:33,410 have happened in our own solar system so 37 00:01:36,940 --> 00:01:34,910 there was a large collision that formed 38 00:01:39,190 --> 00:01:36,950 our own moon early on as our planets 39 00:01:40,900 --> 00:01:39,200 formed similarly there are collisions 40 00:01:42,700 --> 00:01:40,910 like this that stripped the mantle off 41 00:01:45,100 --> 00:01:42,710 of the planet Mercury and maybe another 42 00:01:48,580 --> 00:01:45,110 similar large collision Tilted Uranus 43 00:01:50,430 --> 00:01:48,590 onto its side events like this events 44 00:01:52,840 --> 00:01:50,440 that we see around this other star and 45 00:01:55,960 --> 00:01:52,850 events that formed our own moon