1 00:00:00,033 --> 00:00:05,038 [Music] 2 00:00:05,038 --> 00:00:10,811 NASA is sending the OSIRIS-REx spacecraft to explore near-Earth asteroid Bennu. 3 00:00:10,811 --> 00:00:13,747 To carry out its mission, OSIRIS-REx is equipped with a 4 00:00:13,747 --> 00:00:15,983 suite of remote sensing instruments, 5 00:00:15,983 --> 00:00:19,887 including a spectrometer called OVIRS. 6 00:00:19,887 --> 00:00:24,224 OSIRIS-REx is a mission to bring a sample back from an asteroid. 7 00:00:24,224 --> 00:00:27,761 That's not something that we've done before and that's very exciting. 8 00:00:27,761 --> 00:00:31,899 The idea behind OSIRIS-REx is to go to a pristine building block 9 00:00:31,899 --> 00:00:34,468 of the solar system to try to find out more about how they 10 00:00:34,468 --> 00:00:37,537 formed, and to bring a sample back here to Earth. 11 00:00:37,537 --> 00:00:40,540 OSIRIS-REx's primary science goal is to grab a sample 12 00:00:40,540 --> 00:00:44,378 of asteroid Bennu and return it to Earth for analysis. 13 00:00:44,378 --> 00:00:47,614 Planetary scientists are interested in asteroids because they're 14 00:00:47,614 --> 00:00:51,251 chemistry sets representing the formation of the solar system. 15 00:00:51,251 --> 00:00:54,788 We can't learn that on Earth, because the Earth has erosion 16 00:00:54,788 --> 00:00:58,592 and other processes that have changed its pristine condition. 17 00:00:58,592 --> 00:01:01,128 Asteroid Bennu is interesting because it's one of the blackest 18 00:01:01,128 --> 00:01:03,830 objects in the solar system, so we think it's covered with 19 00:01:03,830 --> 00:01:07,267 carbon material, organics, the building blocks of life. 20 00:01:08,302 --> 00:01:12,506 To search for organics on Bennu, a team at NASA's Goddard Space Flight Center 21 00:01:12,506 --> 00:01:17,411 built the OSIRIS-REx Visible and Infrared Spectrometer, or OVIRS. 22 00:01:17,411 --> 00:01:20,747 OVIRS is a spectrometer, and what that means is it breaks 23 00:01:20,747 --> 00:01:24,384 down light into a lot of little individual wavelength packets. 24 00:01:24,384 --> 00:01:28,088 When you look at very fine detail from spectra, you can 25 00:01:28,088 --> 00:01:30,824 tell what the material is that you're looking at, and that's 26 00:01:30,824 --> 00:01:33,961 what we're excited about – the idea of going out and looking at 27 00:01:33,961 --> 00:01:36,463 something and saying, "Oh, I know what that's made of, and 28 00:01:36,463 --> 00:01:38,899 that would be a good place to take a sample." 29 00:01:38,899 --> 00:01:41,702 Before arriving at asteroid Bennu, OVIRS will have to 30 00:01:41,702 --> 00:01:45,739 survive two years in the unforgiving conditions of space. 31 00:01:45,739 --> 00:01:48,842 Fixing a broken part after launch is not an option, 32 00:01:48,842 --> 00:01:51,812 so OVIRS has a uniquely durable design. 33 00:01:51,812 --> 00:01:55,816 OVIRS is a very simple instrument: it has two mirrors and no moving parts. 34 00:01:55,816 --> 00:01:59,119 And the reason we like that kind of design is because moving 35 00:01:59,119 --> 00:02:01,688 parts are one of the things we worry about breaking in space, 36 00:02:01,688 --> 00:02:03,824 and once it breaks your instrument is lost. 37 00:02:03,824 --> 00:02:07,194 The instrument has to operate in a very harsh environment, 38 00:02:07,194 --> 00:02:10,597 there's no air in space, there's a high vacuum, things can heat up. 39 00:02:10,597 --> 00:02:14,534 Well if you can eliminate moving parts, that's just one more risk 40 00:02:14,534 --> 00:02:16,036 that you don't have to worry about. 41 00:02:16,036 --> 00:02:18,739 I don't have to worry about, "Oh is that shutter open or closed?" 42 00:02:18,739 --> 00:02:19,940 or "Is that motor moving?" 43 00:02:19,940 --> 00:02:24,177 So we very specifically tried to get rid of things that can fail, 44 00:02:24,177 --> 00:02:26,680 and fail in a bad way. 45 00:02:27,614 --> 00:02:30,784 Designing instruments to survive in space is critical, 46 00:02:30,784 --> 00:02:33,520 but just getting there can be a bumpy ride. 47 00:02:33,520 --> 00:02:37,591 Rockets shake their payloads during launch, so instruments like OVIRS 48 00:02:37,591 --> 00:02:41,862 must pass a vibration test to prove that they are launch-worthy. 49 00:02:41,862 --> 00:02:44,631 It is the test that I hate the most in the world. 50 00:02:44,631 --> 00:02:48,168 You've spent five years making this nice little beautiful thing 51 00:02:48,168 --> 00:02:50,470 and you hand it to somebody and say, "Try to break it." 52 00:02:50,470 --> 00:02:53,040 So one of the things we do in vibration testing is we'll shake 53 00:02:53,040 --> 00:02:56,643 it as hard as we think it's going to see, plus a little bit more, 54 00:02:56,643 --> 00:02:58,345 in every possible direction just to make sure 55 00:02:58,345 --> 00:03:00,347 nothing is going to break off during launch. 56 00:03:00,347 --> 00:03:04,584 On OVIRS we actually had a case where the glue came a bit apart 57 00:03:04,584 --> 00:03:07,988 during thermal testing, and then when we put it on the vibration chamber 58 00:03:07,988 --> 00:03:11,758 a full assembly gave way and there was a big pulse on the instrument. 59 00:03:11,758 --> 00:03:15,595 We had to stop and go back and make sure that everything was fine, 60 00:03:15,595 --> 00:03:18,498 which it was, and we also had to redesign things a little bit. 61 00:03:18,498 --> 00:03:21,435 And that shows you the value of testing – had that been on the 62 00:03:21,435 --> 00:03:26,039 launch chamber, we wouldn't have been able to do anything about it. 63 00:03:26,039 --> 00:03:28,875 OSIRIS-REx is a cutting-edge mission to explore 64 00:03:28,875 --> 00:03:32,012 asteroid Bennu and the origins of our solar system, 65 00:03:32,012 --> 00:03:35,082 and OVIRS is critical to the mission's success. 66 00:03:35,082 --> 00:03:37,584 OSIRIS-REx is just such an interesting mission, 67 00:03:37,584 --> 00:03:40,554 the concept of going to one of these really primitive bodies 68 00:03:40,554 --> 00:03:43,757 and bringing back a sample that we can then study here in the Earth, 69 00:03:43,757 --> 00:03:46,626 is pretty spectacular when you think about it. 70 00:03:46,626 --> 00:03:48,628 From the OVIRS instrument itself, I'm actually quite 71 00:03:48,628 --> 00:03:52,065 excited to see if we can see organics on the surface and what 72 00:03:52,065 --> 00:03:56,203 interesting minerals we actually do find, because we won't know that until we get there. 73 00:03:56,203 --> 00:04:00,907 We've got a very good instrument compliment on top of a mission that's taking a sample. 74 00:04:00,907 --> 00:04:04,578 So we can tell what we're taking samples of, we understand the 75 00:04:04,578 --> 00:04:07,747 context of the sample that's returned, and the sample when it 76 00:04:07,747 --> 00:04:12,786 comes back will be analyzed by people all over the world for the next forty years. 77 00:04:12,786 --> 00:04:16,990 So it's just this very nice complete package. 78 00:04:21,428 --> 00:04:33,173 [Satellite beeping]