1 00:00:00,000 --> 00:00:07,000 How do engineers take care of the Hubble Space Telescope while it's in space? 2 00:00:07,000 --> 00:00:12,000 Hey guys, meet Patti Hanson. She works on the Hubble Space Telescope project. 3 00:00:12,000 --> 00:00:16,000 Today, we're at NASA Goddard Space Flight Center in Greenbelt, Maryland. 4 00:00:16,000 --> 00:00:23,000 Okay, Patti, so far we've learned about algebra, optics, telescopes, and a little about the Hubble Space Telescope. 5 00:00:23,000 --> 00:00:28,000 Now, what is NASA Goddard doing to protect the Hubble while it's orbiting around the Earth? 6 00:00:28,000 --> 00:00:31,000 Yeah, and how do engineers like you use algebra in your jobs? 7 00:00:31,000 --> 00:00:33,000 Whoa, those are a lot of questions. 8 00:00:33,000 --> 00:00:37,000 Here at Goddard, we're actually the servicing part of the Hubble Space Telescope project. 9 00:00:37,000 --> 00:00:46,000 We actually prepare scientific instruments, computers, tape recorders to go up on the shuttle, rendezvous with Hubble, 10 00:00:46,000 --> 00:00:49,000 and perform servicing of the telescope. 11 00:00:49,000 --> 00:00:54,000 Astronauts go out into the payload bay, get the new equipment out of carriers, 12 00:00:54,000 --> 00:00:58,000 and install it on the telescope, and we bring the old hardware home. 13 00:00:58,000 --> 00:01:03,000 Now, when we're getting ready for a servicing mission, we have our instruments in our clean room. 14 00:01:03,000 --> 00:01:09,000 And in the clean room, we want to make sure we control contamination by having everyone get dressed in what we call bunny suits. 15 00:01:09,000 --> 00:01:14,000 And you'll see that everybody in the clean room is dressed head to toe in white. 16 00:01:14,000 --> 00:01:20,000 What this does is it controls all the contamination from your clothing, which is lint, your hair. 17 00:01:20,000 --> 00:01:23,000 We don't want any dropped hairs on our science instruments. 18 00:01:23,000 --> 00:01:25,000 And our skin flakes. 19 00:01:25,000 --> 00:01:32,000 Here on Hubble, we're really worried about both particulate and molecular contamination accumulating on the primary and secondary mirrors. 20 00:01:32,000 --> 00:01:37,000 Particulate contamination is like a fine layer of dust that scatters the light 21 00:01:37,000 --> 00:01:42,000 and doesn't allow it to transmit through the optic and gather into the detector very well. 22 00:01:42,000 --> 00:01:50,000 Molecular contamination is a thin film similar to the condensation that you see on this mirror when I squirt it with the nitrogen cleaner. 23 00:01:51,000 --> 00:01:55,000 This doesn't allow the light to be transmitted very well through the optic. 24 00:01:55,000 --> 00:01:59,000 Okay, Van, to get back to your question about how I use algebra in my job, 25 00:01:59,000 --> 00:02:04,000 is that I have an end-of-life requirement for the amount of contamination I can accumulate on flight optics. 26 00:02:04,000 --> 00:02:07,000 Now, for Hubble, that's the primary and secondary mirrors. 27 00:02:07,000 --> 00:02:12,000 End-of-life is the amount of contamination that we can accumulate from the time it was launched 28 00:02:12,000 --> 00:02:15,000 until the time that we no longer expect to take science. 29 00:02:15,000 --> 00:02:17,000 And for Hubble, that's 20 years. 30 00:02:17,000 --> 00:02:22,000 So you're saying that in 20 years, you will accumulate some type of contamination on Hubble's mirrors? 31 00:02:22,000 --> 00:02:23,000 That is correct. 32 00:02:23,000 --> 00:02:24,000 Okay. 33 00:02:24,000 --> 00:02:29,000 And what we do is we take periodic measurements and we compare that to our end-of-life requirement. 34 00:02:29,000 --> 00:02:32,000 Okay, let's look at the algebra Patty is talking about. 35 00:02:32,000 --> 00:02:38,000 NASA engineers know the total amount of contamination on the Hubble has to be less than 5 percent 36 00:02:38,000 --> 00:02:40,000 or the telescope won't work the way it should. 37 00:02:40,000 --> 00:02:44,000 Before Hubble was launched, three measurements for contamination were taken. 38 00:02:44,000 --> 00:02:46,000 The first was 8 tenths of a percent. 39 00:02:46,000 --> 00:02:48,000 The second was 6 tenths of a percent. 40 00:02:48,000 --> 00:02:50,000 And the third was 1 tenth of a percent. 41 00:02:50,000 --> 00:02:56,000 The total amount of contamination on the Hubble consists of the amount of contamination measured on Earth 42 00:02:56,000 --> 00:03:00,000 plus the amount of contamination that it collects on orbit. 43 00:03:00,000 --> 00:03:04,000 If we substitute the values we know into the inequality, 44 00:03:04,000 --> 00:03:11,000 we find that the amount of contamination the Hubble can collect on orbit has to be less than 3.5 percent. 45 00:03:11,000 --> 00:03:14,000 Using algebra, you can see that we have plenty of on-orbit margin left 46 00:03:14,000 --> 00:03:18,000 to accumulate contamination on both the primary and secondary optics. 47 00:03:18,000 --> 00:03:19,000 Hey, check it. 48 00:03:19,000 --> 00:03:24,000 Did you know that the Hubble Space Telescope is about the same size as this school bus? 49 00:03:24,000 --> 00:03:30,000 This is where all of the data from the Hubble Space Telescope is continuously being collected. 50 00:03:30,000 --> 00:03:35,000 Back in 1995, NASA Goddard collected images from the Hubble Deep Field. 51 00:03:35,000 --> 00:03:41,000 A few thousand never-before-seen galaxies are visible in this deepest-ever view of the universe.