WEBVTT 00:03.000 --> 00:08.080 So in a lot of ways, the most innovative or dramatic thing about Juno is the orbit. 00:08.080 --> 00:16.590 We're going to orbit Jupiter in a way where we get to go very close to the planet, inside the radiation belts instead of outside the radiation belts. 00:16.590 --> 00:26.200 We're in a polar orbit, so by small adjustments of the timing, we can map the entire planet. We can get repeated stripes at different longitudes as Jupiter spins underneath us. 00:26.200 --> 00:41.020 It does mean that Juno is going to see the polar regions to a greater extent than with other spacecraft, but I think the most important thing is that it gets in very close to the planet as part of that ellipse 00:41.020 --> 00:46.300 brings it in a few thousand miles above those cloud tops very close near the equator. 00:46.300 --> 00:55.100 We're going to go over the poles of Jupiter - that means we can study the magnetosphere in a different way, where all the magnetic field lines come together, we get to see from Juno. 00:55.100 --> 01:07.000 This is the first time we're really using passive microwave radiometry in multiple channels to try to study the composition of an atmosphere, especially a giant planet like Jupiter, and that's new and unique. 01:07.000 --> 01:14.100 But in some ways, the moment unique part of the Juno mission, the thing that really makes it stand out, is just the orbit.