1 00:00:00,200 --> 00:00:02,035 ♪ 2 00:00:02,068 --> 00:00:04,737 >> Tim Pyle: Our artist concepts are going to be the public face 3 00:00:04,770 --> 00:00:07,306 for some of these objects, and there's a lot of responsibility 4 00:00:07,339 --> 00:00:09,709 that comes with that. 5 00:00:09,742 --> 00:00:12,311 I'm Robert Hurt, I'm the visualization scientist 6 00:00:12,344 --> 00:00:14,580 at IPAC, which is a science and data center 7 00:00:14,613 --> 00:00:17,717 for astrophysics and planetary science at Caltech. 8 00:00:17,750 --> 00:00:18,651 My name is Tim Pyle, 9 00:00:18,684 --> 00:00:20,653 I'm a multimedia producer at IPAC. 10 00:00:20,686 --> 00:00:22,322 I work with Robert. 11 00:00:23,422 --> 00:00:26,659 >> Hurt:We've done illustrations of regions where stars form 12 00:00:26,692 --> 00:00:29,162 and cores, the stellar remnants after a star 13 00:00:29,195 --> 00:00:31,664 like our sun dies leaving a white dwarf. 14 00:00:31,697 --> 00:00:33,399 A neutron star that's left at the core 15 00:00:33,432 --> 00:00:34,667 of a supernova explosion. 16 00:00:34,700 --> 00:00:37,904 Super massive black holes that sit in the cores of galaxies. 17 00:00:37,937 --> 00:00:39,705 >> Pyle: Show the rocky planets, gas giants, 18 00:00:39,738 --> 00:00:41,908 brown dwarfs, cool stars. 19 00:00:41,941 --> 00:00:43,876 >> Hurt: With TRAPPIST-1, I was immediately thinking, 20 00:00:43,909 --> 00:00:46,079 "This is going to be the most significant thing 21 00:00:46,112 --> 00:00:47,647 that has come out of the Spitzer mission." 22 00:00:47,680 --> 00:00:49,348 It's going to be the result that I think 23 00:00:49,381 --> 00:00:52,351 Spitzer will really be remembered for. 24 00:00:52,384 --> 00:00:53,853 The properties that we come away with, 25 00:00:53,886 --> 00:00:55,788 from this kind of observation 26 00:00:55,821 --> 00:00:58,524 include the diameter of the planet, its orbital period, 27 00:00:58,557 --> 00:01:00,059 >> Pyle: whether it's likely to be tidally locked 28 00:01:00,092 --> 00:01:01,727 which will say something about 29 00:01:01,760 --> 00:01:03,496 what the planet probably looks like. 30 00:01:03,529 --> 00:01:05,164 >> Hurt: If it's less dense than the Earth, 31 00:01:05,197 --> 00:01:07,433 it might have more volatiles like water on it, 32 00:01:07,466 --> 00:01:09,602 which is why a two of the TRAPPIST planets 33 00:01:09,635 --> 00:01:10,670 were shown as water worlds. 34 00:01:10,703 --> 00:01:12,071 If it has a higher density than Earth, 35 00:01:12,104 --> 00:01:14,040 then it's probably a little more rocky. 36 00:01:14,073 --> 00:01:15,475 >> Pyle: By doing these artist concepts 37 00:01:15,508 --> 00:01:17,110 we are actually getting across the point that 38 00:01:17,143 --> 00:01:19,946 no, these aren't just “we know there's a planet ther”" 39 00:01:19,979 --> 00:01:22,615 and that's the extent of our information about it. 40 00:01:22,648 --> 00:01:23,950 All of these decisions are made 41 00:01:23,983 --> 00:01:25,852 in conjunction with the scientists. 42 00:01:26,852 --> 00:01:30,056 >> Hurt: I got my PhD in astrophysics from UCLA. 43 00:01:30,089 --> 00:01:33,326 >> Pyle: I'm an artist with a Hollywood background. 44 00:01:33,359 --> 00:01:35,862 >> Hurt: A lot of times I'm very focused on you know 45 00:01:35,895 --> 00:01:38,364 the science bullet points that I'm trying to get across. 46 00:01:38,397 --> 00:01:41,767 We, we kind of cover each other's blind spots a bit. 47 00:01:41,800 --> 00:01:44,070 If you go back and you look at the whole history of space art, 48 00:01:44,103 --> 00:01:46,672 and science-based illustration, for ya know 49 00:01:46,705 --> 00:01:48,541 reaching back many, many decades 50 00:01:48,574 --> 00:01:50,676 you have a visual history, 51 00:01:50,709 --> 00:01:53,813 a visual record of our evolving understanding. 52 00:01:53,846 --> 00:01:55,948 The art is as much historical record of 53 00:01:55,981 --> 00:01:57,917 our changing understanding of the universe