WEBVTT 00:03.000 --> 00:06.050 JADE, the Jovian Auroral Dynamics Experiment, 00:06.050 --> 00:09.150 is a set of instruments that measures the electrons and ions 00:09.150 --> 00:12.140 those are particles, very tiny charged particles, 00:12.140 --> 00:13.220 that are parts of an atom. 00:13.220 --> 00:17.000 And those particles actually produce the aurora. 00:17.000 --> 00:19.070 They follow along the magnetic field lines 00:19.070 --> 00:21.150 and they come down into the atmosphere of Jupiter 00:21.150 --> 00:24.050 and they excite different sorts of interactions that 00:24.050 --> 00:26.130 that emit light, different wavelengths of light. 00:26.130 --> 00:28.060 Those we observe as the aurora. 00:28.060 --> 00:31.050 But the aurora's really caused by these tiny, tiny particles 00:31.050 --> 00:32.160 coming down into the atmosphere. 00:32.160 --> 00:35.180 And JADE actually measures those individual particles. 00:35.158 --> 00:38.150 There are three identical electron sensors, 00:38.150 --> 00:41.020 and they look off in three different directions 00:41.020 --> 00:43.170 around the belly-band of the spacecraft 00:43.170 --> 00:46.020 so that they've got a broad field of view 00:46.020 --> 00:47.090 120 degrees wide 00:47.090 --> 00:51.100 so the three of them actually can see all the way around the spacecraft all of the time. 00:51.100 --> 00:54.010 The JADE Ion instrument is different. 00:54.010 --> 00:57.160 It actually has a thing that looks a little bit more like a hamster wheel 00:57.160 --> 00:58.160 in a hamster cage. 00:58.160 --> 01:02.080 And that's to allow particles to come in over 270 degrees 01:02.080 --> 01:04.060 of observing angle 01:04.060 --> 01:07.080 and twice per minute the Juno spacecraft spins around 01:07.080 --> 01:10.060 and that allows that field of view to observe all of space. 01:10.060 --> 01:14.130 And so we're trying to understand what's the same and different between our own aurora 01:14.130 --> 01:19.020 and the aurora of Jupiter, so that we can understand the processes really in detail for the first time. 01:19.020 --> 01:23.080 We'll be fully successful, and we can come back and tell the world 01:23.080 --> 01:26.110 how it really works, what particles are involved, and why.