WEBVTT 00:04.000 --> 00:08.230 The interior of Jupiter is a tough problem for us. 00:08.230 --> 00:13.460 To get deep inside, we have to use indirect methods. We can't go there. 00:13.460 --> 00:17.000 We think that Jupiter has a core but we don't know for sure. 00:17.000 --> 00:21.800 It is nonetheless likely to be perhaps ten times the mass of the earth. 00:21.800 --> 00:24.120 It may not be solid, it's very hot. 00:24.120 --> 00:30.640 The pressure is too great, the temperature is too high, it's just too far in. We can't get there. 00:30.640 --> 00:39.150 So what we have to do is to use radiation that's coming to us from those lower depths to tell us what's going on down there. 00:39.150 --> 00:41.000 And this is where Juno comes in. 00:41.000 --> 00:45.590 Juno is exciting because we will learn such a wide range of things. 00:45.590 --> 00:50.000 For indeed Jupiter is the most massive planet in the solar system. 00:50.000 --> 00:58.000 It is the body you want to understand in order to understand the architecture of everything else, including Earth. 00:58.000 --> 01:03.400 What is the proportion of water on Jupiter compared to the amount of hydrogen on Jupiter? 01:03.400 --> 01:10.300 And how does that compare with the proportion of hydrogen to water in interstellar space and in the sun? 01:10.300 --> 01:15.800 That's a very important question and that's one of the things that Juno is going to address directly. 01:15.800 --> 01:21.700 I would expect Juno to tell us more about how planets work. 01:21.700 --> 01:27.660 Meaning how the heat gets out, what kinds of flows exist inside the body, 01:27.660 --> 01:29.740 how magnetic fields get generated. 01:29.740 --> 01:35.120 Learning what Jupiter is made of and learning about how it works 01:35.120 --> 01:39.210 Those to me are what make the Juno mission exciting.