WEBVTT 00:02.170 --> 00:05.180 Years ago, magnetic field provided a 00:05.180 --> 00:08.040 reference for navigation on earth. 00:08.040 --> 00:10.170 So for four or five hundred years, 00:10.170 --> 00:12.130 whenever ships crossed the ocean, 00:12.130 --> 00:15.100 they carried compasses so they could find their way 00:15.100 --> 00:18.090 when you can't see stars or land mass. 00:18.090 --> 00:20.170 A magnetometer is like a fancy compass. 00:20.170 --> 00:22.170 It measures both the direction 00:22.170 --> 00:24.070 and the magnitude of the magnetic field. 00:24.070 --> 00:26.210 So in this case we fly a magnetic sensor 00:26.210 --> 00:29.080 at the very outer extremity of the spacecraft. 00:29.080 --> 00:31.180 We're on what's called magnetometer boom, 00:31.180 --> 00:34.020 which is about 12 feet in length 00:34.020 --> 00:36.090 that's about twice as long as I am tall. 00:36.090 --> 00:39.120 The primary purpose for our investigation 00:39.120 --> 00:41.120 is to map the magnetic field of Jupiter 00:41.120 --> 00:45.130 very accurately, and try to understand how it's generated, 00:45.130 --> 00:47.070 deep down inside Jupiter, 00:47.070 --> 00:50.050 in Jupiter's electrically conducting core. 00:50.050 --> 00:55.010 What we're going to do is make very, very accurate measurements 00:55.010 --> 00:56.200 in orbit about Jupiter, 00:56.200 --> 01:02.150 and basically envelope Jupiter in a net, a dense net, of observations. 01:02.150 --> 01:05.140 And that will give us the ability to image 01:05.140 --> 01:10.070 what the magnetic field looks like down in Jupiter's core where it's generated.