1 00:00:18,070 --> 00:00:15,070 we're here at the Marshall Space Flight 2 00:00:20,200 --> 00:00:18,080 Center in Huntsville Alabama known for 3 00:00:22,900 --> 00:00:20,210 its long history in propulsion research 4 00:00:25,120 --> 00:00:22,910 but this NASA site is still a big player 5 00:00:27,909 --> 00:00:25,130 this time for the James Webb Space 6 00:00:29,530 --> 00:00:27,919 Telescope we're right outside the vacuum 7 00:00:32,230 --> 00:00:29,540 chamber where the mirrors for the Webb 8 00:00:34,210 --> 00:00:32,240 Space Telescope are being tested back in 9 00:00:35,880 --> 00:00:34,220 the 90s this facility was used to test 10 00:00:39,550 --> 00:00:35,890 out one of NASA's Great observatories 11 00:00:41,500 --> 00:00:39,560 the Chandra x-ray Observatory we have 12 00:00:43,599 --> 00:00:41,510 here the project scientist for Chandra 13 00:00:45,610 --> 00:00:43,609 Martin Weiskopf can you tell us a little 14 00:00:48,099 --> 00:00:45,620 bit about the differences between Hubble 15 00:00:50,200 --> 00:00:48,109 and Chandra and James Webb these are 16 00:00:51,520 --> 00:00:50,210 observatories that look at different 17 00:00:53,830 --> 00:00:51,530 parts of what we call the 18 00:00:56,500 --> 00:00:53,840 electromagnetic spectrum that is light 19 00:00:59,080 --> 00:00:56,510 at various different energies from 20 00:01:01,419 --> 00:00:59,090 x-rays where it takes a lot of energy to 21 00:01:03,819 --> 00:01:01,429 produce them to visible light where the 22 00:01:06,130 --> 00:01:03,829 Hubble Space Telescope operates and the 23 00:01:09,010 --> 00:01:06,140 near-infrared where the James Webb 24 00:01:10,990 --> 00:01:09,020 telescope will operate in this way by 25 00:01:13,510 --> 00:01:11,000 studying objects in the universe we can 26 00:01:15,340 --> 00:01:13,520 learn a lot about them that we can't 27 00:01:17,440 --> 00:01:15,350 learn by just simply looking at one 28 00:01:21,100 --> 00:01:17,450 wavelength what kind of information can 29 00:01:23,740 --> 00:01:21,110 be gleaned from x-rays x-ray astronomy 30 00:01:25,480 --> 00:01:23,750 is a system that brought the first 31 00:01:28,480 --> 00:01:25,490 discoveries of black holes in the 32 00:01:30,670 --> 00:01:28,490 universe so we look at very interesting 33 00:01:33,789 --> 00:01:30,680 astronomical objects at very great 34 00:01:36,550 --> 00:01:33,799 distances and conjunction with Hubble 35 00:01:38,740 --> 00:01:36,560 Webb will be looking to identify many 36 00:01:41,230 --> 00:01:38,750 Chandra sources that are not seen with 37 00:01:43,030 --> 00:01:41,240 Hubble now we're outside the facility 38 00:01:45,069 --> 00:01:43,040 where the mirror testing is being done 39 00:01:47,260 --> 00:01:45,079 and you can't help but see this long 40 00:01:50,350 --> 00:01:47,270 tube that is connected to the building 41 00:01:52,959 --> 00:01:50,360 itself I'm told it's almost six football 42 00:01:56,459 --> 00:01:52,969 fields long Martin what was this tube 43 00:01:59,469 --> 00:01:56,469 used for this tube is very important for 44 00:02:02,440 --> 00:01:59,479 separating the telescope that was on the 45 00:02:04,749 --> 00:02:02,450 Chandra x-ray Observatory from x-ray 46 00:02:07,749 --> 00:02:04,759 sources located at the other end of the 47 00:02:10,480 --> 00:02:07,759 building it has to be this length in 48 00:02:13,360 --> 00:02:10,490 order to make those x-ray sources appear 49 00:02:15,760 --> 00:02:13,370 like tiny stars so that we could 50 00:02:18,310 --> 00:02:15,770 determine whether our x-ray telescope 51 00:02:20,350 --> 00:02:18,320 could distinguish small objects in the 52 00:02:22,080 --> 00:02:20,360 sky why is it still here Chandra was 53 00:02:25,240 --> 00:02:22,090 tested in the mid night 54 00:02:27,699 --> 00:02:25,250 it's still here because it's very very 55 00:02:29,949 --> 00:02:27,709 useful for many programs the vacuum 56 00:02:33,130 --> 00:02:29,959 chamber is being used to test the web 57 00:02:36,040 --> 00:02:33,140 optics and we hope to be testing x-ray 58 00:02:37,720 --> 00:02:36,050 telescopes in future programs well 59 00:02:40,420 --> 00:02:37,730 thanks for your time Martin quite 60 00:02:42,490 --> 00:02:40,430 welcome the testing here for the Chandra 61 00:02:46,059 --> 00:02:42,500 Observatory ran about six months from 62 00:02:48,039 --> 00:02:46,069 1996 to 1997 then to telescope was sent 63 00:02:50,620 --> 00:02:48,049 off to be integrated with the rest of 64 00:02:54,339 --> 00:02:50,630 the observatory Chandra was launched on