WEBVTT 00:00:00.498 --> 00:00:03.097 Five years ago, I was a Ph.D. student 00:00:03.097 --> 00:00:04.741 living two lives. 00:00:04.741 --> 00:00:07.057 In one, I used NASA supercomputers 00:00:07.057 --> 00:00:09.785 to design next-generation spacecraft, 00:00:09.785 --> 00:00:12.364 and in the other I was a data scientist 00:00:12.364 --> 00:00:14.783 looking for potential smugglers 00:00:14.783 --> 00:00:18.022 of sensitive nuclear technologies. 00:00:18.022 --> 00:00:20.881 As a data scientist, I did a lot of analyses, 00:00:20.881 --> 00:00:22.348 mostly of facilities, 00:00:22.348 --> 00:00:24.619 industrial facilities around the world. 00:00:24.619 --> 00:00:27.307 And I was always looking for a better canvas 00:00:27.307 --> 00:00:29.373 to tie these all together. 00:00:29.373 --> 00:00:31.239 And one day, I was thinking about how 00:00:31.239 --> 00:00:33.363 all data has a location, 00:00:33.363 --> 00:00:35.096 and I realized that the answer 00:00:35.096 --> 00:00:36.984 had been staring me in the face. 00:00:36.984 --> 00:00:39.622 Although I was a satellite engineer, 00:00:39.622 --> 00:00:42.793 I hadn't thought about using satellite imagery 00:00:42.793 --> 00:00:44.359 in my work. NOTE Paragraph 00:00:44.359 --> 00:00:46.306 Now, like most of us, I'd been online, 00:00:46.306 --> 00:00:48.088 I'd see my house, so I thought, 00:00:48.088 --> 00:00:50.386 I'll hop in there and I'll start looking up 00:00:50.386 --> 00:00:51.803 some of these facilities. 00:00:51.803 --> 00:00:53.772 And what I found really surprised me. 00:00:53.772 --> 00:00:55.446 The pictures that I was finding 00:00:55.446 --> 00:00:57.347 were years out of date, 00:00:57.347 --> 00:00:58.415 and because of that, 00:00:58.415 --> 00:01:00.086 it had relatively little relevance 00:01:00.086 --> 00:01:02.546 to the work that I was doing today. 00:01:02.546 --> 00:01:04.007 But I was intrigued. 00:01:04.007 --> 00:01:07.243 I mean, satellite imagery is pretty amazing stuff. 00:01:07.243 --> 00:01:09.546 There are millions and millions of sensors 00:01:09.546 --> 00:01:10.990 surrounding us today, 00:01:10.990 --> 00:01:13.950 but there's still so much we don't know on a daily basis. 00:01:13.950 --> 00:01:17.703 How much oil is stored in all of China? 00:01:17.703 --> 00:01:20.636 How much corn is being produced? 00:01:20.636 --> 00:01:24.707 How many ships are in all of our world's ports? 00:01:24.707 --> 00:01:27.266 Now, in theory, all of these questions 00:01:27.266 --> 00:01:29.510 could be answered by imagery, 00:01:29.510 --> 00:01:31.237 but not if it's old. 00:01:31.237 --> 00:01:33.695 And if this data was so valuable, 00:01:33.695 --> 00:01:35.627 then how come I couldn't get my hands 00:01:35.627 --> 00:01:38.177 on more recent pictures? NOTE Paragraph 00:01:38.177 --> 00:01:41.312 So the story begins over 50 years ago 00:01:41.312 --> 00:01:43.183 with the launch of the first generation 00:01:43.183 --> 00:01:46.783 of U.S. government photo reconnaissance satellites. 00:01:46.783 --> 00:01:48.479 And today, there's a handful 00:01:48.479 --> 00:01:50.674 of the great, great grandchildren 00:01:50.674 --> 00:01:52.339 of these early Cold War machines 00:01:52.339 --> 00:01:54.348 which are now operated by private companies 00:01:54.348 --> 00:01:57.057 and from which the vast majority of satellite imagery 00:01:57.057 --> 00:01:59.882 that you and I see on a daily basis comes. 00:01:59.882 --> 00:02:02.796 During this period, launching things into space, 00:02:02.796 --> 00:02:05.473 just the rocket to get the satellite up there, 00:02:05.473 --> 00:02:10.074 has cost hundreds of millions of dollars each, 00:02:10.074 --> 00:02:11.826 and that's created tremendous pressure 00:02:11.826 --> 00:02:14.115 to launch things infrequently 00:02:14.115 --> 00:02:15.459 and to make sure that when you do, 00:02:15.459 --> 00:02:19.098 you cram as much functionality in there as possible. 00:02:19.098 --> 00:02:20.709 All of this has only made satellites 00:02:20.709 --> 00:02:23.126 bigger and bigger and bigger 00:02:23.126 --> 00:02:24.724 and more expensive, 00:02:24.724 --> 00:02:29.761 now nearly a billion, with a b, dollars per copy. 00:02:29.761 --> 00:02:31.460 Because they are so expensive, 00:02:31.460 --> 00:02:32.927 there aren't very many of them. 00:02:32.927 --> 00:02:34.272 Because there aren't very many of them, 00:02:34.272 --> 00:02:36.728 the pictures that we see on a daily basis 00:02:36.728 --> 00:02:38.232 tend to be old. NOTE Paragraph 00:02:38.232 --> 00:02:41.514 I think a lot of people actually understand this anecdotally, 00:02:41.514 --> 00:02:44.053 but in order to visualize just how sparsely 00:02:44.053 --> 00:02:45.937 our planet is collected, 00:02:45.937 --> 00:02:48.003 some friends and I put together a dataset 00:02:48.003 --> 00:02:50.590 of the 30 million pictures that have been gathered 00:02:50.590 --> 00:02:54.074 by these satellites between 2000 and 2010. 00:02:54.074 --> 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 --> 00:03:01.891 and even the areas that are seen most frequently, 00:03:01.891 --> 00:03:05.639 those in red, are seen at best once a quarter. 00:03:05.639 --> 00:03:08.555 Now as aerospace engineering grad students, 00:03:08.555 --> 00:03:11.983 this chart cried out to us as a challenge. 00:03:11.983 --> 00:03:15.438 Why do these things have to be so expensive? 00:03:15.438 --> 00:03:18.173 Does a single satellite really have to cost 00:03:18.173 --> 00:03:22.936 the equivalent of three 747 jumbo jets? 00:03:22.936 --> 00:03:25.099 Wasn't there a way to build a smaller, 00:03:25.099 --> 00:03:28.271 simpler, new satellite design that could enable 00:03:28.271 --> 00:03:30.289 more timely imaging? NOTE Paragraph 00:03:30.289 --> 00:03:33.740 I realize that it does sound a little bit crazy 00:03:33.740 --> 00:03:35.251 that we were going to go out and just 00:03:35.251 --> 00:03:37.098 begin designing satellites, 00:03:37.098 --> 00:03:39.061 but fortunately we had help. 00:03:39.061 --> 00:03:41.996 In the late 1990s, a couple of professors 00:03:41.996 --> 00:03:45.477 proposed a concept for radically reducing the price 00:03:45.477 --> 00:03:47.249 of putting things in space. 00:03:47.249 --> 00:03:49.360 This was hitchhiking small satellites 00:03:49.360 --> 00:03:52.376 alongside much larger satellites. 00:03:52.376 --> 00:03:55.285 This dropped the cost of putting objects up there 00:03:55.285 --> 00:03:57.283 by over a factor of 100, 00:03:57.283 --> 00:04:00.369 and suddenly we could afford to experiment, 00:04:00.369 --> 00:04:01.837 to take a little bit of risk, 00:04:01.837 --> 00:04:04.103 and to realize a lot of innovation. 00:04:04.103 --> 00:04:07.192 And a new generation of engineers and scientists, 00:04:07.192 --> 00:04:08.791 mostly out of universities, 00:04:08.791 --> 00:04:11.134 began launching these very small, 00:04:11.134 --> 00:04:13.725 breadbox-sized satellites called CubeSats. 00:04:13.725 --> 00:04:16.128 And these were built with electronics obtained 00:04:16.128 --> 00:04:20.026 from RadioShack instead of Lockheed Martin. NOTE Paragraph 00:04:20.026 --> 00:04:22.866 Now it was using the lessons learned from these early missions 00:04:22.866 --> 00:04:25.561 that my friends and I began a series of sketches 00:04:25.561 --> 00:04:27.250 of our own satellite design. 00:04:27.250 --> 00:04:30.034 And I can't remember a specific day 00:04:30.034 --> 00:04:31.894 where we made a conscious decision 00:04:31.894 --> 00:04:34.529 that we were actually going to go out and build these things, 00:04:34.529 --> 00:04:36.959 but once we got that idea in our minds 00:04:36.959 --> 00:04:39.120 of the world as a dataset, 00:04:39.120 --> 00:04:41.610 of being able to capture millions of data points 00:04:41.610 --> 00:04:44.663 on a daily basis describing the global economy, 00:04:44.663 --> 00:04:47.183 of being able to unearth billions of connections 00:04:47.183 --> 00:04:50.348 between them that had never before been found, 00:04:50.348 --> 00:04:51.996 it just seemed boring 00:04:51.996 --> 00:04:54.903 to go work on anything else. NOTE Paragraph 00:04:54.903 --> 00:04:57.876 And so we moved into a cramped, 00:04:57.876 --> 00:05:00.855 windowless office in Palo Alto, 00:05:00.855 --> 00:05:02.822 and began working to take our design 00:05:02.822 --> 00:05:05.760 from the drawing board into the lab. 00:05:05.760 --> 00:05:08.418 The first major question we had to tackle 00:05:08.418 --> 00:05:10.752 was just how big to build this thing. 00:05:10.752 --> 00:05:13.935 In space, size drives cost, 00:05:13.935 --> 00:05:15.948 and we had worked with these very small, 00:05:15.948 --> 00:05:18.042 breadbox-sized satellites in school, 00:05:18.042 --> 00:05:20.593 but as we began to better understand the laws of physics, 00:05:20.593 --> 00:05:22.715 we found that the quality of pictures 00:05:22.715 --> 00:05:25.799 those satellites could take was very limited, 00:05:25.799 --> 00:05:27.503 because the laws of physics dictate 00:05:27.503 --> 00:05:30.609 that the best picture you can take through a telescope 00:05:30.609 --> 00:05:32.848 is a function of the diameter of that telescope, 00:05:32.848 --> 00:05:34.510 and these satellites had a very small, 00:05:34.510 --> 00:05:36.216 very constrained volume. 00:05:36.216 --> 00:05:38.011 And we found that the best picture we would 00:05:38.011 --> 00:05:40.496 have been able to get looked something like this. 00:05:40.496 --> 00:05:42.741 Although this was the low-cost option, 00:05:42.741 --> 00:05:44.414 quite frankly it was just too blurry 00:05:44.414 --> 00:05:47.983 to see the things that make satellite imagery valuable. 00:05:47.983 --> 00:05:50.129 So about three or four weeks later, 00:05:50.129 --> 00:05:52.946 we met a group of engineers randomly 00:05:52.946 --> 00:05:54.587 who had worked on the first 00:05:54.587 --> 00:05:57.028 private imaging satellite ever developed, 00:05:57.028 --> 00:05:59.146 and they told us that back in the 1970s, 00:05:59.146 --> 00:06:01.328 the U.S. government had found a powerful 00:06:01.328 --> 00:06:02.971 optimal tradeoff -- 00:06:02.971 --> 00:06:06.059 that in taking pictures at right about one meter resolution, 00:06:06.059 --> 00:06:08.943 being able to see objects one meter in size, 00:06:08.943 --> 00:06:11.634 they had found that they could not just get very high-quality images, 00:06:11.634 --> 00:06:14.527 but get a lot of them at an affordable price. 00:06:14.527 --> 00:06:16.503 From our own computer simulations, 00:06:16.503 --> 00:06:18.508 we quickly found that one meter really was 00:06:18.508 --> 00:06:20.272 the minimum viable product 00:06:20.272 --> 00:06:23.351 to be able to see the drivers of our global economy, 00:06:23.351 --> 00:06:24.912 for the first time, being able to count 00:06:24.912 --> 00:06:27.633 the ships and cars and shipping containers and trucks 00:06:27.633 --> 00:06:30.457 that move around our world on a daily basis, 00:06:30.457 --> 00:06:34.261 while conveniently still not being able to see individuals. 00:06:34.261 --> 00:06:35.882 We had found our compromise. 00:06:35.882 --> 00:06:37.486 We would have to build something larger 00:06:37.486 --> 00:06:39.049 than the original breadbox, 00:06:39.049 --> 00:06:40.700 now more like a mini-fridge, 00:06:40.700 --> 00:06:43.461 but we still wouldn't have to build a pickup truck. 00:06:43.461 --> 00:06:46.085 So now we had our constraint. 00:06:46.085 --> 00:06:47.842 The laws of physics dictated 00:06:47.842 --> 00:06:51.166 the absolute minimum-sized telescope that we could build. NOTE Paragraph 00:06:51.166 --> 00:06:54.220 What came next was making the rest of the satellite 00:06:54.220 --> 00:06:55.961 as small and as simple as possible, 00:06:55.961 --> 00:06:58.613 basically a flying telescope with four walls 00:06:58.613 --> 00:07:01.554 and a set of electronics smaller than a phone book 00:07:01.554 --> 00:07:04.992 that used less power than a 100 watt lightbulb. 00:07:04.992 --> 00:07:06.892 The big challenge became actually taking 00:07:06.892 --> 00:07:09.090 the pictures through that telescope. 00:07:09.090 --> 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 --> 00:07:18.491 scanning row by row by row 00:07:18.491 --> 00:07:20.166 to build the complete image. 00:07:20.166 --> 00:07:23.170 Now people use these because they get a lot of light, 00:07:23.170 --> 00:07:25.001 which means less of the noise you see 00:07:25.016 --> 00:07:27.752 in a low-cost cell phone image. 00:07:27.752 --> 00:07:30.113 The problem with them is they require 00:07:30.113 --> 00:07:32.353 very sophisticated pointing. 00:07:32.353 --> 00:07:34.899 You have to stay focused on a 50-centimeter target 00:07:34.899 --> 00:07:36.651 from over 600 miles away 00:07:36.651 --> 00:07:38.883 while moving at more than seven kilometers a second, 00:07:38.883 --> 00:07:41.632 which requires an awesome degree of complexity. 00:07:41.632 --> 00:07:45.069 So instead, we turned to a new generation of video sensors, 00:07:45.069 --> 00:07:48.160 originally created for use in night vision goggles. 00:07:48.160 --> 00:07:51.059 Instead of taking a single, high quality image, 00:07:51.059 --> 00:07:52.446 we could take a videostream 00:07:52.446 --> 00:07:55.369 of individually noisier frames, 00:07:55.369 --> 00:07:57.113 but then we could recombine 00:07:57.113 --> 00:07:58.579 all of those frames together 00:07:58.579 --> 00:08:00.575 into very high-quality images 00:08:00.575 --> 00:08:03.168 using sophisticated pixel processing techniques 00:08:03.168 --> 00:08:04.689 here on the ground, 00:08:04.689 --> 00:08:07.826 at a cost of one one hundredth a traditional system. 00:08:07.826 --> 00:08:08.979 And we applied this technique 00:08:08.979 --> 00:08:11.953 to many of the other systems on the satellite as well, 00:08:11.953 --> 00:08:14.793 and day by day, our design evolved 00:08:14.793 --> 00:08:18.282 from CAD to prototypes 00:08:18.282 --> 00:08:21.170 to production units. NOTE Paragraph 00:08:21.170 --> 00:08:22.827 A few short weeks ago, 00:08:22.827 --> 00:08:24.678 we packed up SkySat 1, 00:08:24.678 --> 00:08:26.451 put our signatures on it, 00:08:26.451 --> 00:08:28.674 and waved goodbye for the last time on Earth. 00:08:28.674 --> 00:08:32.155 Today, it's sitting in its final launch configuration 00:08:32.155 --> 00:08:35.216 ready to blast off in a few short weeks. 00:08:35.216 --> 00:08:37.558 And soon, we'll turn our attention to launching 00:08:37.558 --> 00:08:40.589 a constellation of 24 or more of these satellites 00:08:40.589 --> 00:08:43.139 and beginning to build the scalable analytics 00:08:43.139 --> 00:08:45.478 that will allow us to unearth the insights 00:08:45.478 --> 00:08:48.667 in the petabytes of data we will collect. NOTE Paragraph 00:08:48.667 --> 00:08:52.640 So why do all of this? Why build these satellites? 00:08:52.640 --> 00:08:55.251 Well, it turns out imaging satellites 00:08:55.251 --> 00:08:58.961 have a unique ability to provide global transparency, 00:08:58.961 --> 00:09:01.587 and providing that transparency on a timely basis 00:09:01.587 --> 00:09:04.998 is simply an idea whose time has come. 00:09:04.998 --> 00:09:08.521 We see ourselves as pioneers of a new frontier, 00:09:08.521 --> 00:09:10.285 and beyond economic data, 00:09:10.285 --> 00:09:13.886 unlocking the human story, moment by moment. 00:09:13.886 --> 00:09:15.449 For a data scientist 00:09:15.449 --> 00:09:18.199 that just happened to go to space camp as a kid, 00:09:18.199 --> 00:09:20.914 it just doesn't get much better than that. NOTE Paragraph 00:09:20.914 --> 00:09:23.129 Thank you. NOTE Paragraph 00:09:23.129 --> 00:09:27.263 (Applause)