1 00:00:00,200 --> 00:00:04,938 [Music] 2 00:00:04,938 --> 00:00:07,841 There are many important reasons for studying asteroids 3 00:00:07,841 --> 00:00:10,744 like the target of OSIRIS-REx, asteroid Bennu. 4 00:00:10,744 --> 00:00:13,814 First and foremost, for me especially, they're geologic 5 00:00:13,814 --> 00:00:16,116 remnants from the dawn of our solar system. 6 00:00:16,116 --> 00:00:19,052 They're literally the first material that formed around our 7 00:00:19,052 --> 00:00:22,890 star, and they represent the building blocks of planets, and 8 00:00:22,890 --> 00:00:26,326 we hope, in the case of Bennu of life, and the reason that Earth 9 00:00:26,326 --> 00:00:28,996 may be a habitable planet in the form of delivering water and 10 00:00:28,996 --> 00:00:31,198 other important volatile material. 11 00:00:31,198 --> 00:00:33,934 When we look at asteroids which are these primitive objects, 12 00:00:33,934 --> 00:00:37,704 these little leftover pieces from solar system formation, and 13 00:00:37,704 --> 00:00:40,707 we find they may have organics, then that tells us perhaps the 14 00:00:40,707 --> 00:00:43,110 conditions for life could have erupted anywhere in the solar 15 00:00:43,110 --> 00:00:45,312 system, and Earth was just right. 16 00:00:45,312 --> 00:00:48,682 When we study meteorites, we think they represent these 17 00:00:48,682 --> 00:00:51,385 asteroids and their different histories, but they've all 18 00:00:51,385 --> 00:00:55,088 interacted with the Earth's atmosphere, its biosphere, its 19 00:00:55,088 --> 00:00:57,758 hydrosphere, and so we don't know what effect just 20 00:00:57,758 --> 00:01:01,061 interacting with the Earth has had on these meteorites. 21 00:01:01,061 --> 00:01:05,032 We really want to get samples that are pristine, and so we can 22 00:01:05,032 --> 00:01:07,601 do all of those things through this mission. 23 00:01:07,601 --> 00:01:11,805 OSIRIS-REx is a mission in the NASA New Frontiers Program. 24 00:01:11,805 --> 00:01:15,342 Our objective is to travel out to a near-Earth asteroid named 25 00:01:15,342 --> 00:01:19,346 Bennu, survey that object in great detail to understand its 26 00:01:19,346 --> 00:01:23,650 geology, its mineralogy and composition, ultimately select a 27 00:01:23,650 --> 00:01:26,286 single location on the asteroid's surface to acquire a 28 00:01:26,286 --> 00:01:29,423 sample, and return that material back to the Earth for scientific 29 00:01:29,423 --> 00:01:30,857 analysis. 30 00:01:30,857 --> 00:01:33,961 Asteroid Bennu is a fragment of the early solar system, an 31 00:01:33,961 --> 00:01:37,998 un-melted, unaltered piece of the origin of the solar system. 32 00:01:37,998 --> 00:01:41,268 It preserves the ingredients, the raw materials that went into 33 00:01:41,268 --> 00:01:44,237 the formation of planets, the formation of life. 34 00:01:44,237 --> 00:01:47,441 By bringing a sample back to the Earth, such as OSIRIS-REx will 35 00:01:47,441 --> 00:01:51,545 do with samples of Bennu in 2023, we'll be able to look at 36 00:01:51,545 --> 00:01:54,948 the samples in laboratories around the world, to understand 37 00:01:54,948 --> 00:02:00,087 in great detail the nature of the sample and its place in the 38 00:02:00,087 --> 00:02:01,922 origin of the solar system. 39 00:02:01,922 --> 00:02:04,891 The OSIRIS-REx spacecraft launched in 2016, and it's 40 00:02:04,891 --> 00:02:08,762 actually taken us two years to get to the asteroid Bennu, and 41 00:02:08,762 --> 00:02:10,497 in that time we had an Earth flyby. 42 00:02:10,497 --> 00:02:14,334 So, we used an Earth flyby in 2017 to change the plane of our 43 00:02:14,334 --> 00:02:17,604 orbit to match Bennu's orbit plane, and it's also provided a 44 00:02:17,604 --> 00:02:21,208 great opportunity from a flight dynamics perspective to really 45 00:02:21,208 --> 00:02:24,411 calibrate our models and learn how to fly the spacecraft which 46 00:02:24,411 --> 00:02:26,980 will help us in the really challenging part of the mission, 47 00:02:26,980 --> 00:02:29,516 which is orbiting in the low-gravity environment of the 48 00:02:29,516 --> 00:02:30,751 asteroid. 49 00:02:30,751 --> 00:02:32,919 Over the past few months, the flight dynamics team has been 50 00:02:32,919 --> 00:02:35,689 getting images of the asteroid Bennu, and it started out as 51 00:02:35,689 --> 00:02:38,892 just a very small point source in the camera, and it's been 52 00:02:38,892 --> 00:02:41,561 getting bigger and bigger and bigger in the field of view. 53 00:02:41,561 --> 00:02:45,232 And that's allowed us to perform optical navigation, to refine 54 00:02:45,232 --> 00:02:49,236 our prediction of the asteroid's orbit, and allow us to more 55 00:02:49,236 --> 00:02:53,040 precisely navigate and target our approach to the asteroid. 56 00:02:53,040 --> 00:02:56,043 As OSIRIS-REx approaches the asteroid, we've done a series of 57 00:02:56,043 --> 00:02:58,412 braking maneuvers called Asteroid Approach Maneuvers to 58 00:02:58,412 --> 00:03:01,615 slow down the spacecraft, so that we can get into orbit 59 00:03:01,615 --> 00:03:03,550 around the asteroid later this year. 60 00:03:03,550 --> 00:03:06,887 We're also taking lots of images of Bennu to understand its 61 00:03:06,887 --> 00:03:09,856 rotation, look for natural satellites, and potential dust 62 00:03:09,856 --> 00:03:11,058 plumes. 63 00:03:11,058 --> 00:03:14,127 This is an extremely exciting time on OSIRIS-REx as we're just 64 00:03:14,127 --> 00:03:16,029 poised at arrival at Bennu. 65 00:03:16,029 --> 00:03:18,799 And one of the most exciting things to us, and relieving too 66 00:03:18,799 --> 00:03:22,269 to the engineers, is how closely the asteroid has resembled what 67 00:03:22,269 --> 00:03:23,270 we had predicted. 68 00:03:23,270 --> 00:03:26,273 Early on our science team, prior to launch, had come up with of a 69 00:03:26,273 --> 00:03:29,142 model of what they thought the asteroid would look like, based 70 00:03:29,142 --> 00:03:32,712 purely on ground-based radar observations from Arecibo, and 71 00:03:32,712 --> 00:03:36,349 from that they created a reference asteroid that we used 72 00:03:36,349 --> 00:03:38,752 as the requirements to design the mission against. 73 00:03:38,752 --> 00:03:41,054 But no one could be sure that the asteroid would really look 74 00:03:41,054 --> 00:03:43,256 like the scientists had predicted, so it's been a 75 00:03:43,256 --> 00:03:47,060 tremendous relief to us to find that the actual Bennu is very 76 00:03:47,060 --> 00:03:49,563 similar to what the scientists had predicted. 77 00:03:49,563 --> 00:03:51,264 So, the science team really nailed it. 78 00:03:51,264 --> 00:03:54,367 Well right now as we're approaching asteroid Bennu, 79 00:03:54,367 --> 00:03:57,771 we're looking for debris or other objects that are orbiting 80 00:03:57,771 --> 00:04:00,373 the asteroid just in case we need to avoid those. 81 00:04:00,373 --> 00:04:03,176 And then once we arrive on December 3 we'll perform 82 00:04:03,176 --> 00:04:06,046 Preliminary Survey, and in Preliminary Survey we fly over 83 00:04:06,046 --> 00:04:08,982 the north pole, south pole, and the middle of the asteroid. 84 00:04:08,982 --> 00:04:11,985 This helps us to map the gravity of the asteroid and understand 85 00:04:11,985 --> 00:04:14,421 how to operate near such a small body. 86 00:04:14,421 --> 00:04:16,656 Additionally, this will be the first time that we get close-up 87 00:04:16,656 --> 00:04:19,292 pictures of the surface, and we'll know how smooth or rocky 88 00:04:19,292 --> 00:04:21,161 the surface that we're going to study is. 89 00:04:21,161 --> 00:04:25,098 As we get closer to asteroid Bennu, we'll begin to map its 90 00:04:25,098 --> 00:04:27,968 surface in higher detail. 91 00:04:27,968 --> 00:04:31,872 What we'll be able to do is first identify the distribution 92 00:04:31,872 --> 00:04:36,176 of rocks and particles that might pose a hazard to the 93 00:04:36,176 --> 00:04:39,479 sampling mechanism on the spacecraft, and we'll also get a 94 00:04:39,479 --> 00:04:42,849 better sense of what the shape of Bennu is like at smaller 95 00:04:42,849 --> 00:04:43,517 scales. 96 00:04:43,517 --> 00:04:46,820 Looking at Bennu in more and more detail is going to help us 97 00:04:46,820 --> 00:04:50,524 identify all the areas that we shouldn't go to grab a sample 98 00:04:50,524 --> 00:04:51,191 from. 99 00:04:51,191 --> 00:04:54,261 Throughout 2019 we'll be doing global characterization of the 100 00:04:54,261 --> 00:04:57,797 asteroid, basically making maps of the entire surface. 101 00:04:57,797 --> 00:05:00,100 We're interested in its topography. 102 00:05:00,100 --> 00:05:01,034 Are there craters? 103 00:05:01,034 --> 00:05:03,703 Where are the boulders, the valleys, the mountains of the 104 00:05:03,703 --> 00:05:04,371 asteroid? 105 00:05:04,371 --> 00:05:07,240 And then we want to understand the distribution of geologic 106 00:05:07,240 --> 00:05:10,177 materials: are we finding different patches of minerals in 107 00:05:10,177 --> 00:05:13,680 one location versus another, and why are certain areas that have 108 00:05:13,680 --> 00:05:15,682 a composition and others maybe different? 109 00:05:15,682 --> 00:05:19,085 We're going to be looking most importantly for areas where we 110 00:05:19,085 --> 00:05:21,021 can collect a sample. 111 00:05:21,021 --> 00:05:24,424 OSIRIS-REx will collect a sample from Bennu using our TAGSAM, 112 00:05:24,424 --> 00:05:27,594 which is the Touch And Go Sample Acquisition Mechanism. 113 00:05:27,594 --> 00:05:30,697 What that is, is an arm connected to this sampler head 114 00:05:30,697 --> 00:05:31,464 that you see here. 115 00:05:31,464 --> 00:05:34,968 This is similar in size to an air filter from a car. 116 00:05:34,968 --> 00:05:38,238 How this mechanism works is there's compressed gas that is 117 00:05:38,238 --> 00:05:41,174 released that will stir up the regolith from Bennu, store it 118 00:05:41,174 --> 00:05:44,611 into this canister, which we will then put inside of our 119 00:05:44,611 --> 00:05:47,080 sample release capsule and bring back to Earth. 120 00:05:47,080 --> 00:05:50,617 We will collect the sample of Bennu in 2020 and return it to 121 00:05:50,617 --> 00:05:51,751 Earth in 2023. 122 00:05:51,751 --> 00:05:55,889 Once we're in the vicinity of our home world, about 123 00:05:55,889 --> 00:05:59,226 four-and-a-half hours before impacting the top of the 124 00:05:59,226 --> 00:06:02,162 atmosphere, the spacecraft spins up and releases that sample 125 00:06:02,162 --> 00:06:02,963 return capsule. 126 00:06:02,963 --> 00:06:06,867 The spacecraft fires its engines to perform a deflection burn, 127 00:06:06,867 --> 00:06:09,936 going off into orbit around the sun, and the return capsule 128 00:06:09,936 --> 00:06:13,173 enters the Earth's atmosphere, targeting a landing in the Utah 129 00:06:13,173 --> 00:06:14,074 desert. 130 00:06:14,074 --> 00:06:17,344 I'll be there on site when we open that capsule up and we see 131 00:06:17,344 --> 00:06:21,014 those samples for the first time, and science begins at that 132 00:06:21,014 --> 00:06:23,984 point on the next phase of the mission, the sample analysis 133 00:06:23,984 --> 00:06:24,985 period. 134 00:06:24,985 --> 00:06:27,520 [Music] 135 00:06:27,520 --> 00:06:39,266 [Satellite beeping]