WEBVTT 00:00:00.591 --> 00:00:03.096 Five years ago, I was a Ph.D student 00:00:03.096 --> 00:00:04.880 living two lives. 00:00:04.880 --> 00:00:07.396 In one, I used NASA supercomputers 00:00:07.396 --> 00:00:09.985 to design next generation spacecraft, 00:00:09.985 --> 00:00:12.381 and in the other I was a data scientist 00:00:12.381 --> 00:00:14.937 looking for potential smugglers 00:00:14.937 --> 00:00:17.977 of sensitive nuclear technologies. 00:00:17.977 --> 00:00:21.191 As a data scientist, I did a lot of analyses, 00:00:21.191 --> 00:00:22.688 mostly of facilities, 00:00:22.688 --> 00:00:24.696 industrial facilities around the world. 00:00:24.696 --> 00:00:27.571 And I was always looking for a better canvas 00:00:27.571 --> 00:00:29.512 to tie these all together. 00:00:29.512 --> 00:00:31.501 And one day, I was thinking about how 00:00:31.501 --> 00:00:33.563 all data has a location, 00:00:33.563 --> 00:00:35.128 and I realized that the answer 00:00:35.128 --> 00:00:37.108 had been staring me in the face. 00:00:37.108 --> 00:00:39.776 Although I was a satellite engineer, 00:00:39.776 --> 00:00:42.824 I hadn't thought about using satellite imagery 00:00:42.824 --> 00:00:44.513 in my work. NOTE Paragraph 00:00:44.513 --> 00:00:46.399 Now like most of us, I'd been online, 00:00:46.399 --> 00:00:48.273 I'd see my house, so I thought, 00:00:48.273 --> 00:00:50.296 I'll hop in there and I'll start looking up 00:00:50.296 --> 00:00:51.958 some of these facilities. 00:00:51.958 --> 00:00:53.880 And what I found really surprised me. 00:00:53.880 --> 00:00:55.616 The pictures that I was finding 00:00:55.616 --> 00:00:57.501 were years out of date, 00:00:57.501 --> 00:00:58.585 and because of that, 00:00:58.585 --> 00:01:00.194 it had relatively little relevance 00:01:00.194 --> 00:01:02.731 to the work that I was doing today. 00:01:02.731 --> 00:01:04.192 But I was intrigued. 00:01:04.192 --> 00:01:07.428 I mean, satellite imagery is pretty amazing stuff. 00:01:07.428 --> 00:01:09.731 There are millions and millions of sensors 00:01:09.731 --> 00:01:11.129 surrounding us today, 00:01:11.129 --> 00:01:14.320 but there's still so much we don't know on a daily basis. 00:01:14.320 --> 00:01:17.689 How much oil is stored in all of China? 00:01:17.689 --> 00:01:20.529 How much corn is being produced? 00:01:20.529 --> 00:01:24.815 How many ships are in all of our world's ports? 00:01:24.815 --> 00:01:27.390 Now, in theory, all of these questions 00:01:27.390 --> 00:01:29.311 could be answered by imagery, 00:01:29.311 --> 00:01:31.391 but not if it's old. 00:01:31.391 --> 00:01:33.895 And if this data was so valuable, 00:01:33.895 --> 00:01:35.751 then how come I couldn't get my hands 00:01:35.751 --> 00:01:38.377 on more recent pictures? NOTE Paragraph 00:01:38.377 --> 00:01:41.543 So the story begins over 50 years ago 00:01:41.543 --> 00:01:43.399 with the launch of the first generation 00:01:43.399 --> 00:01:46.783 of U.S. government photo reconnaissance satellites. 00:01:46.783 --> 00:01:48.495 And today, there's a handful 00:01:48.495 --> 00:01:50.567 of the great, great grandchildren 00:01:50.567 --> 00:01:52.416 of these early cold war machines 00:01:52.416 --> 00:01:54.472 which are now operated by private companies 00:01:54.472 --> 00:01:57.119 and from which the vast majority of satellite imagery 00:01:57.119 --> 00:01:59.975 that you and I see on a daily basis comes. 00:01:59.975 --> 00:02:03.072 During this period, launching things into space, 00:02:03.072 --> 00:02:05.736 just the rocket to get the satellite up there, 00:02:05.736 --> 00:02:10.029 has cost hundreds of millions of dollars each, 00:02:10.029 --> 00:02:11.889 and that's created tremendous pressure 00:02:11.889 --> 00:02:14.377 to launch things infrequently 00:02:14.377 --> 00:02:15.706 and to make sure that when you do, 00:02:15.706 --> 00:02:19.036 you cram as much functionality in there as possible. 00:02:19.036 --> 00:02:20.802 All of this has only made satellites 00:02:20.802 --> 00:02:23.028 bigger and bigger and bigger 00:02:23.028 --> 00:02:24.786 and more expensive, 00:02:24.786 --> 00:02:30.050 now nearly a billion, with a b, dollars per copy. 00:02:30.050 --> 00:02:31.722 Because they are so expensive, 00:02:31.722 --> 00:02:33.042 there aren't very many of them. 00:02:33.042 --> 00:02:34.426 Because there aren't very many of them, 00:02:34.426 --> 00:02:36.775 the pictures that we see on a daily basis 00:02:36.775 --> 00:02:38.386 tend to be old. NOTE Paragraph 00:02:38.386 --> 00:02:41.514 I think a lot of people actually understand this anecdotally, 00:02:41.514 --> 00:02:43.961 but in order to visualize just how sparsely 00:02:43.961 --> 00:02:45.738 our planet is collected, 00:02:45.738 --> 00:02:48.250 some friends and I put together a data set 00:02:48.250 --> 00:02:50.530 of the 30 million pictures that have been gathered 00:02:50.530 --> 00:02:54.259 by these satellites between 2000 and 2010. 00:02:54.259 --> 00:02:56.829 As you can see in blue, huge areas of our world 00:02:56.829 --> 00:02:59.619 are barely seen, less than once a year, 00:02:59.619 --> 00:03:01.968 and even the areas that are seen most frequently, 00:03:01.968 --> 00:03:05.639 those in red, are seen at best once a quarter. 00:03:05.639 --> 00:03:08.679 Now as aerospace engineering grad students, 00:03:08.679 --> 00:03:12.214 this chart cried out to us as a challenge. 00:03:12.214 --> 00:03:15.715 Why do these things have to be so expensive? 00:03:15.715 --> 00:03:18.297 Does a single satellite really have to cost 00:03:18.297 --> 00:03:22.936 the equivalent of three 747 jumbo jets? 00:03:22.936 --> 00:03:25.238 Wasn't there a way to build a smaller, 00:03:25.238 --> 00:03:28.271 simpler, new satellite design that could enable 00:03:28.271 --> 00:03:30.382 more timely imaging? NOTE Paragraph 00:03:30.382 --> 00:03:34.031 Now I realize that it does sound a little bit crazy 00:03:34.031 --> 00:03:35.514 that we were going to go out and just 00:03:35.514 --> 00:03:37.191 begin designing satellites, 00:03:37.191 --> 00:03:39.200 but fortunately we had help. 00:03:39.200 --> 00:03:42.104 In the late 1990s, a couple of professors 00:03:42.104 --> 00:03:45.616 proposed a concept for radically reducing the price 00:03:45.616 --> 00:03:47.311 of putting things in space. 00:03:47.311 --> 00:03:49.423 This was hitchhiking small satellites 00:03:49.423 --> 00:03:52.392 alongside much larger satellite. 00:03:52.392 --> 00:03:55.563 This dropped the cost of putting objects up there 00:03:55.563 --> 00:03:57.407 by over a factor of 100, 00:03:57.407 --> 00:04:00.585 and suddenly we could afford to experiment, 00:04:00.585 --> 00:04:01.991 to take a little bit of risk, 00:04:01.991 --> 00:04:04.303 and to realize a lot of innovation. 00:04:04.303 --> 00:04:07.423 And a new generation of engineers and scientists, 00:04:07.423 --> 00:04:08.991 mostly out of universities, 00:04:08.991 --> 00:04:11.320 began launching these very small, 00:04:11.320 --> 00:04:13.881 breadbox-sized satellites called CubeSats. 00:04:13.881 --> 00:04:16.056 And these were built with electronics obtained 00:04:16.056 --> 00:04:20.119 from RadioShack instead of Lockheed Martin. NOTE Paragraph 00:04:20.119 --> 00:04:22.836 Now it was using the lessons learned from these early missions 00:04:22.836 --> 00:04:25.516 that my friends and I began a series of sketches 00:04:25.516 --> 00:04:27.420 of our own satellite design. 00:04:27.420 --> 00:04:30.062 And, you know, I can't remember a specific day 00:04:30.062 --> 00:04:31.972 where we made, like, a conscious decision 00:04:31.972 --> 00:04:34.653 that we were actually going to go out and build these things, 00:04:34.653 --> 00:04:37.099 but it was just, once we got that idea in our minds 00:04:37.099 --> 00:04:39.012 of the world as a data set, 00:04:39.012 --> 00:04:41.610 of being able to capture millions of data points 00:04:41.610 --> 00:04:44.387 on a daily basis, describing the global economy, 00:04:44.387 --> 00:04:46.892 of being able to unearth billions of connections 00:04:46.892 --> 00:04:50.196 between them that had never before been found, 00:04:50.196 --> 00:04:52.196 it just seemed boring 00:04:52.196 --> 00:04:54.612 to go work on anything else. NOTE Paragraph 00:04:54.612 --> 00:04:57.892 And so we moved into a cramped, 00:04:57.892 --> 00:05:01.061 windowless office in Palo Alto, 00:05:01.061 --> 00:05:02.780 and began working to take our design 00:05:02.780 --> 00:05:05.976 from the drawing board into the lab. 00:05:05.976 --> 00:05:08.572 Now the first major question we had to tackle 00:05:08.572 --> 00:05:10.860 was just how big to build this thing. 00:05:10.860 --> 00:05:14.012 In space, size drives cost, 00:05:14.012 --> 00:05:16.078 and we had worked with these very small, 00:05:16.078 --> 00:05:18.228 breadbox-sized satellites in school, 00:05:18.228 --> 00:05:20.732 but as we began to better understand the laws of physics, 00:05:20.732 --> 00:05:22.715 we found that the quality of pictures 00:05:22.715 --> 00:05:25.707 those satellites could take was very limited, 00:05:25.707 --> 00:05:27.596 because the laws of physics dictate 00:05:27.596 --> 00:05:30.748 that the best picture you can take through a telescope 00:05:30.748 --> 00:05:33.068 is a function of the diameter of that telescope, 00:05:33.068 --> 00:05:34.572 and these satellites had a very small, 00:05:34.572 --> 00:05:36.601 very constrained volume. 00:05:36.601 --> 00:05:38.227 And we found that the best picture we would 00:05:38.227 --> 00:05:40.438 have been able to get looked something like this. 00:05:40.438 --> 00:05:42.557 And although this was the low-cost option, 00:05:42.557 --> 00:05:44.461 quite frankly it was just too blurry 00:05:44.461 --> 00:05:48.277 to see the things that make satellite imagery valuable. 00:05:48.277 --> 00:05:50.253 So about three or four weeks later, 00:05:50.253 --> 00:05:53.101 we met a group of engineers randomly 00:05:53.101 --> 00:05:54.757 who had worked on the first 00:05:54.757 --> 00:05:57.136 private imaging satellite ever developed, 00:05:57.136 --> 00:05:59.301 and they told us that back in the 1970s, 00:05:59.301 --> 00:06:01.099 the U.S. government had found a powerful 00:06:01.099 --> 00:06:03.125 optimal tradeoff, 00:06:03.125 --> 00:06:06.229 that in taking pictures at right about one meter resolution, 00:06:06.229 --> 00:06:08.944 being able to see objects one meter in size, 00:06:08.944 --> 00:06:11.773 they found that they could not just get very high quality images, 00:06:11.773 --> 00:06:14.681 but get a lot of them at an affordable price. 00:06:14.681 --> 00:06:16.473 From our own computer simulations, 00:06:16.473 --> 00:06:18.693 we quickly found that one meter really was 00:06:18.693 --> 00:06:20.365 the minimum viable product 00:06:20.365 --> 00:06:23.428 to be able to see the drivers of our global economy, 00:06:23.428 --> 00:06:24.974 for the first time, being able to count 00:06:24.974 --> 00:06:27.557 the ships and cars and shipping containers and trucks 00:06:27.557 --> 00:06:30.550 that move around our world on a daily basis, 00:06:30.550 --> 00:06:34.477 while conveniently still not being able to see individuals. 00:06:34.477 --> 00:06:36.221 We had found our compromise. 00:06:36.221 --> 00:06:37.518 We would have to build something larger 00:06:37.518 --> 00:06:39.189 than the original breadbox, 00:06:39.189 --> 00:06:40.809 now more like a mini-fridge, 00:06:40.809 --> 00:06:43.554 but we still wouldn't have to build a pickup truck. 00:06:43.554 --> 00:06:45.642 So now we had our constraint. 00:06:45.642 --> 00:06:47.566 The laws of physics dictated 00:06:47.566 --> 00:06:51.069 the absolute minimum-sized telescope that we could build. NOTE Paragraph 00:06:51.069 --> 00:06:54.009 What came next was making the rest of the satellite 00:06:54.009 --> 00:06:56.101 as small and as simple as possible, 00:06:56.101 --> 00:06:58.613 basically a flying telescope with four walls 00:06:58.613 --> 00:07:01.693 and a set of electronics smaller than a phone book 00:07:01.693 --> 00:07:04.992 that used less power than a 100 watt light bulb. 00:07:04.992 --> 00:07:06.646 The big challenge became actually taking 00:07:06.646 --> 00:07:09.214 the pictures through that telescope. 00:07:09.214 --> 00:07:12.134 Traditional imaging satellites use a line scanner, 00:07:12.134 --> 00:07:13.895 similar to a Xerox machine, 00:07:13.895 --> 00:07:16.295 and as they traverse the earth, they take pictures, 00:07:16.295 --> 00:07:18.615 scanning row by row by row 00:07:18.615 --> 00:07:20.398 to build the complete image. 00:07:20.398 --> 00:07:23.447 Now people use these because they get a lot of light, 00:07:23.447 --> 00:07:25.217 which means less of the noise you see 00:07:25.217 --> 00:07:27.814 in a low-cost cell phone image. 00:07:27.814 --> 00:07:29.575 The problem with them is they require 00:07:29.575 --> 00:07:32.446 very sophisticated pointing. 00:07:32.446 --> 00:07:34.899 You have to stay focused on a 50-centimeter target 00:07:34.899 --> 00:07:36.683 from over 600 miles away 00:07:36.683 --> 00:07:39.030 while moving at more than seven kilometers a second, 00:07:39.030 --> 00:07:41.510 which requires an awesome degree of complexity. 00:07:41.510 --> 00:07:45.193 So instead, we turned to a new generation of video sensors, 00:07:45.193 --> 00:07:48.160 originally created for use in night vision goggles. 00:07:48.160 --> 00:07:51.029 Instead of taking a single, high quality image, 00:07:51.029 --> 00:07:52.446 we could take a videostream 00:07:52.446 --> 00:07:55.631 of individually noisier frames, 00:07:55.631 --> 00:07:57.267 but then we could recombine 00:07:57.267 --> 00:07:58.795 all of those frames together 00:07:58.795 --> 00:08:00.699 into very high quality images 00:08:00.699 --> 00:08:03.476 using sophisticated pixel processing techniques 00:08:03.476 --> 00:08:04.843 here on the ground, 00:08:04.843 --> 00:08:08.119 at a cost of one one-hundredth a traditional system. 00:08:08.119 --> 00:08:09.287 And we applied this technique 00:08:09.287 --> 00:08:12.080 to many of the other systems on the satellite as well, 00:08:12.080 --> 00:08:15.132 and day by day, our design evolved 00:08:15.132 --> 00:08:18.282 from cad to prototypes 00:08:18.282 --> 00:08:21.140 to production units. NOTE Paragraph 00:08:21.140 --> 00:08:22.827 A few short weeks ago, 00:08:22.827 --> 00:08:25.155 we packed up SkySat 1, 00:08:25.155 --> 00:08:26.651 put our signatures on it, 00:08:26.651 --> 00:08:28.859 and waved goodbye for the last time on earth. 00:08:28.859 --> 00:08:32.155 Today, it's sitting in its final launch configuration 00:08:32.155 --> 00:08:35.509 ready to blast off in a few short weeks. 00:08:35.509 --> 00:08:37.682 And soon, we'll turn our attention to launching 00:08:37.682 --> 00:08:40.851 a constellation of 24 or more of these satellites 00:08:40.851 --> 00:08:43.139 and beginning to build the scalable analytics 00:08:43.139 --> 00:08:45.509 that will allow us to unearth the insights 00:08:45.509 --> 00:08:48.667 in the pedabytes of data we will collect. NOTE Paragraph 00:08:48.667 --> 00:08:52.779 So why do all of this? Why build these satellites? 00:08:52.779 --> 00:08:55.251 Well, it turns out imaging satellites 00:08:55.251 --> 00:08:59.100 have a unique ability to provide global transparency, 00:08:59.100 --> 00:09:01.634 and providing that transparency on a timely basis 00:09:01.634 --> 00:09:04.922 is simply an idea whose time has come. 00:09:04.922 --> 00:09:08.338 We see ourselves as pioneers of a new frontier, 00:09:08.338 --> 00:09:10.547 and beyond economic data, 00:09:10.547 --> 00:09:14.365 unlocking the human story, moment by moment. 00:09:14.365 --> 00:09:15.619 For a data scientist 00:09:15.619 --> 00:09:18.230 that just happened to go to space camp as a kid, 00:09:18.230 --> 00:09:21.130 it just doesn't get much better than that. NOTE Paragraph 00:09:21.130 --> 00:09:23.283 Thank you. NOTE Paragraph 00:09:23.283 --> 00:09:27.263 (Applause)