1 00:00:00,208 --> 00:00:05,422 ♪♪ 2 00:00:05,422 --> 00:00:08,591 We've never detected a magnetic field around 3 00:00:08,591 --> 00:00:12,762 an asteroid, but we've measured magnetization 4 00:00:12,762 --> 00:00:15,932 in meteorite samples. 5 00:00:15,932 --> 00:00:19,602 I can remember so clearly the day that we talked about 6 00:00:19,602 --> 00:00:22,605 the concept that actually led to the mission. I had 7 00:00:22,605 --> 00:00:24,941 just finished teaching a course and I came out of 8 00:00:24,941 --> 00:00:27,110 the classroom and Ben was standing there. His office 9 00:00:27,110 --> 00:00:29,237 is right there, and he said, “Lindy, we just made a 10 00:00:29,237 --> 00:00:32,282 measurement from this meteorite that shows that 11 00:00:32,282 --> 00:00:34,951 it has a magnetic field that it recorded from 12 00:00:34,951 --> 00:00:37,537 back at the time of its formation. 13 00:00:37,537 --> 00:00:39,622 We don't understand how this could happen. Can we 14 00:00:39,622 --> 00:00:42,250 talk about it for a minute? Maybe you have some ideas. 15 00:00:42,250 --> 00:00:44,878 I was like, “I totally have an idea. It's based on what 16 00:00:44,878 --> 00:00:47,088 I was just teaching.” And we sat down in his office 17 00:00:47,088 --> 00:00:49,090 and we drew things on the whiteboard and suddenly we 18 00:00:49,090 --> 00:00:52,218 had this idea about how planetesimals could form. 19 00:00:52,218 --> 00:00:56,556 We wrote a paper about this idea. That paper was read 20 00:00:56,556 --> 00:01:00,602 by Daniel Lankerd and Bruce Bills at JPL, who 21 00:01:00,602 --> 00:01:03,605 actually ended up contacting us and proposing 22 00:01:03,605 --> 00:01:06,441 to build a mission around it. 23 00:01:06,441 --> 00:01:09,736 Psyche represents one of the best opportunities we'll 24 00:01:09,736 --> 00:01:13,198 have to search for the first evidence of asteroid 25 00:01:13,198 --> 00:01:16,993 magnetism. It's now long frozen, billions of years 26 00:01:16,993 --> 00:01:19,746 ago, but that ancient magnetic field that it 27 00:01:19,746 --> 00:01:23,708 could have generated could be imprinted in the surface 28 00:01:23,708 --> 00:01:26,711 layers of Psyche which cooled in the presence of 29 00:01:26,711 --> 00:01:28,922 this field. And so, they would have what we call 30 00:01:28,922 --> 00:01:32,801 magnetization, which is like a fossil or an echo of 31 00:01:32,801 --> 00:01:37,013 the ancient magnetic field that it generated. 32 00:01:37,013 --> 00:01:39,390 And the way you sense magnetic fields is you use 33 00:01:39,390 --> 00:01:41,434 an instrument called a magnetometer and that's 34 00:01:41,434 --> 00:01:44,062 what we have on Psyche. 35 00:01:44,062 --> 00:01:51,694 ♪ 36 00:01:51,694 --> 00:01:54,656 The Psyche team contacted us because they know we 37 00:01:54,656 --> 00:01:58,660 have very high-quality magnetometer based on 38 00:01:58,660 --> 00:02:02,122 the magnetic materials that, that we are producing. 39 00:02:02,122 --> 00:02:05,792 So, we have a huge experience in how to do 40 00:02:05,792 --> 00:02:08,628 this and how to drive space magnetometers on 41 00:02:08,628 --> 00:02:11,131 very long timescales. Here, we're talking many, 42 00:02:11,131 --> 00:02:11,881 many years. 43 00:02:11,881 --> 00:02:13,174 We build the hardware. 44 00:02:13,174 --> 00:02:16,719 We qualify hardware here on ground. We calibrate the 45 00:02:16,719 --> 00:02:20,306 hardware and then we deliver it to Psyche, and 46 00:02:20,306 --> 00:02:23,935 MIT is responsible for the science operations and 47 00:02:23,935 --> 00:02:29,023 data processing of the magnetometer from Psyche. 48 00:02:29,023 --> 00:02:31,568 The magnetometer is on the whole time. It turns on 49 00:02:31,568 --> 00:02:34,445 after launch. It's on for the whole mission. And so, 50 00:02:34,445 --> 00:02:38,366 we'll have a lot of time to observe the signals 51 00:02:38,366 --> 00:02:42,370 from the spacecraft and to calibrate for those. So, by 52 00:02:42,370 --> 00:02:45,498 the time we actually get to Psyche we'll be able to get 53 00:02:45,498 --> 00:02:48,835 a good, clean measurement of the 54 00:02:48,835 --> 00:02:52,547 asteroid's magnetic field. 55 00:02:52,547 --> 00:02:56,009 So, my role was to model the interaction of 56 00:02:56,009 --> 00:02:59,095 the asteroid with the solar wind and then kind of fly a 57 00:02:59,095 --> 00:03:03,057 simulated Psyche to fly through the simulated 58 00:03:03,057 --> 00:03:08,229 asteroid. This is a 3-D print of Psyche. So, if 59 00:03:08,229 --> 00:03:10,690 this asteroid is magnetized you can imagine a magnetic 60 00:03:10,690 --> 00:03:12,567 field around it, kind of like the earth magnetic 61 00:03:12,567 --> 00:03:15,987 field, like a big bubble but like smaller, and then 62 00:03:15,987 --> 00:03:17,906 you're going to have the solar wind flying around it, 63 00:03:17,906 --> 00:03:20,366 a bunch of electrons and protons coming in from the 64 00:03:20,366 --> 00:03:23,244 sun interacting with this magnetic field and changing 65 00:03:23,244 --> 00:03:26,372 it constantly. And then, we're kind of flying in a 66 00:03:26,372 --> 00:03:30,043 small computer-generated spacecraft that is going to 67 00:03:30,043 --> 00:03:32,337 measure this magnetic field while everything is 68 00:03:32,337 --> 00:03:35,632 changing and analyze it and say, “Are we going to be 69 00:03:35,632 --> 00:03:38,009 able to tell if there's a magnetic field coming in 70 00:03:38,009 --> 00:03:41,179 from this body, or are we just seeing all this space 71 00:03:41,179 --> 00:03:42,722 magnetic field around it?” 72 00:03:42,722 --> 00:03:45,683 The real precise mapping that we expect to do when 73 00:03:45,683 --> 00:03:48,186 we are closest in on the asteroid, when we are 74 00:03:48,186 --> 00:03:51,022 really orbiting close in the final science orbit. 75 00:03:51,022 --> 00:03:55,526 But, it's possible that Psyche is so magnetic that 76 00:03:55,526 --> 00:03:57,820 we could even detect its field before we go into 77 00:03:57,820 --> 00:04:02,492 orbit. That's conceivable. 78 00:04:02,492 --> 00:04:04,827 This is my first opportunity to actually be 79 00:04:04,827 --> 00:04:07,830 involved with that process of designing the 80 00:04:07,830 --> 00:04:11,793 investigation and figuring out how to clean up that 81 00:04:11,793 --> 00:04:14,879 data so it will be usable by the science community 82 00:04:14,879 --> 00:04:16,005 at large. 83 00:04:16,005 --> 00:04:18,925 An important part of building a space mission 84 00:04:18,925 --> 00:04:22,387 is to imagine the whole range of possibilities and 85 00:04:22,387 --> 00:04:23,888 to build for all of them. 86 00:04:23,888 --> 00:04:28,059 A big part of the spirit of the team is to talk across 87 00:04:28,059 --> 00:04:31,771 disciplines. I get a chance to share my science with 88 00:04:31,771 --> 00:04:34,482 this very broad group of people. 89 00:04:34,482 --> 00:04:37,986 Everybody on this mission is dedicated in a way you 90 00:04:37,986 --> 00:04:40,947 rarely ever see anywhere else and that actually 91 00:04:40,947 --> 00:04:43,074 makes a huge difference when you are trying to 92 00:04:43,074 --> 00:04:44,659 achieve a goal this difficult. 93 00:04:44,659 --> 00:04:48,663 Never did I ever imagine that I would actually be 94 00:04:48,663 --> 00:04:52,000 involved in a project to actually send a spacecraft 95 00:04:52,000 --> 00:04:55,712 up to an asteroid. Being able to basically be part 96 00:04:55,712 --> 00:04:57,964 what feels like live science fiction is 97 00:04:57,964 --> 00:05:00,967 something that for me that I really enjoy about this. 98 00:05:00,967 --> 00:05:04,512 If we can do things like send this robotic orbiter 99 00:05:04,512 --> 00:05:07,598 out to this asteroid so far away to learn things 100 00:05:07,598 --> 00:05:10,268 that we cannot learn in person, then surely, we can 101 00:05:10,268 --> 00:05:12,186 solve these problems that are in front of us here on