WEBVTT FILE 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]