1 00:00:08,950 --> 00:00:06,789 using nasa's spitzer space telescope 2 00:00:10,470 --> 00:00:08,960 we've looked at many nearby stars to 3 00:00:13,589 --> 00:00:10,480 look for orbiting 4 00:00:15,509 --> 00:00:13,599 dust and asteroids and comets orbiting 5 00:00:17,430 --> 00:00:15,519 debris left over from the process of 6 00:00:19,189 --> 00:00:17,440 planet formation 7 00:00:21,349 --> 00:00:19,199 we saw something very unusual that we 8 00:00:25,509 --> 00:00:21,359 hadn't seen around any other star 9 00:00:27,429 --> 00:00:25,519 we saw evidence for a massive collision 10 00:00:30,630 --> 00:00:27,439 when the two objects collide 11 00:00:32,790 --> 00:00:30,640 everything happens very quickly in the 12 00:00:34,389 --> 00:00:32,800 animation things have been slowed down 13 00:00:36,790 --> 00:00:34,399 to allow you to see 14 00:00:39,270 --> 00:00:36,800 the impacting shock wave propagate 15 00:00:41,990 --> 00:00:39,280 across the surface of this devastated 16 00:00:45,670 --> 00:00:43,670 starting from the point of impact and 17 00:00:48,150 --> 00:00:45,680 circulating to the backside 18 00:00:50,709 --> 00:00:48,160 causing waves on the surface 19 00:00:52,470 --> 00:00:50,719 the entire planet becomes molten 20 00:00:54,790 --> 00:00:52,480 meanwhile tremendous amounts of material 21 00:00:56,869 --> 00:00:54,800 are ejected from the planet both outside 22 00:00:58,709 --> 00:00:56,879 of the system and some falls back onto 23 00:01:00,869 --> 00:00:58,719 the system itself depending on the 24 00:01:02,950 --> 00:01:00,879 details of the collision whether it's a 25 00:01:05,509 --> 00:01:02,960 high impact or depending on the angle 26 00:01:07,510 --> 00:01:05,519 that the objects hit each other at 27 00:01:10,149 --> 00:01:07,520 the there may be a growth or there may 28 00:01:11,590 --> 00:01:10,159 be a grinding away so sometimes the 29 00:01:13,750 --> 00:01:11,600 planet actually ends up smaller after 30 00:01:16,149 --> 00:01:13,760 the collision but generally the planet 31 00:01:17,910 --> 00:01:16,159 grows to larger and larger until there's 32 00:01:21,030 --> 00:01:17,920 no more material left in the system for 33 00:01:26,149 --> 00:01:23,830 while collisions like this are rare we 34 00:01:27,910 --> 00:01:26,159 don't see this large event in any other 35 00:01:29,590 --> 00:01:27,920 systems we've looked at with the spitzer 36 00:01:31,670 --> 00:01:29,600 space telescope 37 00:01:33,670 --> 00:01:31,680 collisions like this have happened in 38 00:01:35,590 --> 00:01:33,680 our own solar system so there was a 39 00:01:38,230 --> 00:01:35,600 large collision that formed our own moon 40 00:01:53,190 --> 00:01:38,240 early on as our planets formed similarly