1 00:00:00,010 --> 00:00:04,010 [XMM-Newton] (Music throughout) 2 00:00:04,030 --> 00:00:08,050 [Launched on December 10, 1999] 3 00:00:08,070 --> 00:00:12,080 [XMM is a joint ESA and NASA X-ray telescope] 4 00:00:12,100 --> 00:00:16,120 [It has revolutionized the study of high-energy phenomena in the universe] 5 00:00:16,140 --> 00:00:20,170 Norbert Schartel: When XMM-Newton 6 00:00:20,190 --> 00:00:24,250 was launched, we never were expecting it would last 20 years or more. 7 00:00:24,270 --> 00:00:28,340 Dheeraj Pasham: XMM is an awesome mission. It’s one of my 8 00:00:28,360 --> 00:00:32,410 top favorite missions of all time. Lisa Winter: XMM has been a 9 00:00:32,430 --> 00:00:36,500 part of my career from the earliest stages even until now. 10 00:00:36,520 --> 00:00:40,590 Laura Brenneman: My work simply wouldn’t have been possible without XMM. 11 00:00:40,610 --> 00:00:44,780 Ed Cackett: XMM is an X-ray astronomy satellite. It allows us to look at X-ray 12 00:00:44,800 --> 00:00:48,910 light coming from some of the most extreme objects in the universe; all the way 13 00:00:48,930 --> 00:00:52,940 from stars to black holes and distant galaxies. 14 00:00:52,960 --> 00:00:56,990 Stephanie LaMassa, Space Telescope Science Institute: XMM has influenced modern astrophysics by having 15 00:00:57,010 --> 00:01:01,040 great sensitivity and large collecting area in X-rays, 16 00:01:01,060 --> 00:01:05,090 which has addressed science questions which we wouldn’t have been able to address otherwise. 17 00:01:05,110 --> 00:01:09,200 Dheeraj Pasham, MIT: If you want to study extragalactic point sources, 18 00:01:09,220 --> 00:01:13,320 then XMM-Newton is essentially the only 19 00:01:13,340 --> 00:01:17,370 instrument out there if you want really good signal-to-noise in the data. 20 00:01:17,390 --> 00:01:21,420 Ed Cackett, Wayne State University: Most recently I’ve been using XMM data to look at the variability of X-ray light 21 00:01:21,440 --> 00:01:25,470 from material that falls into supermassive black holes. 22 00:01:25,490 --> 00:01:29,640 We’ve developed a technique called reverberation mapping that looks at echoes 23 00:01:29,660 --> 00:01:33,800 of light to figure out the size scale of material as it falls into a black hole. 24 00:01:33,820 --> 00:01:37,830 Stephanie: In 2006 I started working with XMM data 25 00:01:37,850 --> 00:01:41,950 and a couple years later I started my Ph.D. work on 26 00:01:41,970 --> 00:01:46,080 active galactic nuclei, where XMM-Newton data formed the basis 27 00:01:46,100 --> 00:01:50,110 of a lot of that work, especially for my first paper on that. 28 00:01:50,130 --> 00:01:54,160 Maurice Leutenegger, NASA’s Goddard Space Flight Center: I started working with XMM data in the summer of 2000. 29 00:01:54,180 --> 00:01:58,210 That was when I started doing my Ph.D. research. 30 00:01:58,230 --> 00:02:02,270 Lisa Winter, NSF: I thought it was very cool to have been reading in high school 31 00:02:02,290 --> 00:02:06,340 about it being launched and then be able to 32 00:02:06,360 --> 00:02:10,420 really use the data from that same telescope in my 33 00:02:10,440 --> 00:02:14,540 graduate career to get my Ph.D. from. Daniel Wik, University of Utah: My Ph.D., 34 00:02:14,560 --> 00:02:18,710 the majority of it was around searching for a certain type of 35 00:02:18,730 --> 00:02:22,760 radiation from galaxy clusters, and so we needed to characterize that really well, 36 00:02:22,780 --> 00:02:26,810 and the only telescope that could do it efficiently 37 00:02:26,830 --> 00:02:30,900 was the XMM-Newton Observatory. Laura Brenneman, Smithsonian Astrophysical Observatory: Actually all 38 00:02:30,920 --> 00:02:34,990 of my thesis, except for the theoretical work, required XMM data. All of the 39 00:02:35,010 --> 00:02:39,090 active galaxies that I studied were data taken from the XMM 40 00:02:39,110 --> 00:02:43,200 archive. Daniel: XMM has been around for 20 years, 41 00:02:43,220 --> 00:02:47,220 and has this just phenomenal archive of data, 42 00:02:47,240 --> 00:02:51,250 and so a lot of this archival data can be searched 43 00:02:51,270 --> 00:02:55,290 and and new science results can come out. Stephanie: Without XMM, 44 00:02:55,310 --> 00:02:59,350 strophysics would not be as far as it is today. 45 00:02:59,370 --> 00:03:03,400 There is certain science that XMM can do that other 46 00:03:03,420 --> 00:03:07,550 X-ray observatories can’t. Dheeraj: Time domain astronomy is going through 47 00:03:07,570 --> 00:03:11,590 a revolution. There’s gravitational waves detected, there’s several kinds 48 00:03:11,610 --> 00:03:15,630 of weird supernovae detected and having an X-ray instrument 49 00:03:15,650 --> 00:03:19,710 to simultaneously operate while these optical instruments are operating 50 00:03:19,730 --> 00:03:23,750 will be extremely beneficial. Lisa: Many objects change, 51 00:03:23,770 --> 00:03:27,940 they have flares and outbursts, so it’s really 52 00:03:27,960 --> 00:03:32,050 a key observation to have everything from the X-ray, the 53 00:03:32,070 --> 00:03:36,080 optical, and the UV, all precisely at the same time. 54 00:03:36,100 --> 00:03:40,100 Stephanie: XMM can contribute to the future by serving 55 00:03:40,120 --> 00:03:44,210 as a pathfinder to find really interesting sources 56 00:03:44,230 --> 00:03:48,330 that can then be followed up with the next generation of telescopes. 57 00:03:48,350 --> 00:03:52,380 Maurice: the continued opportunities for 58 00:03:52,400 --> 00:03:56,470 time domain studies, which are both 59 00:03:56,490 --> 00:04:00,570 photon hungry and just overall time hungry, is 60 00:04:00,590 --> 00:04:04,690 an argument for keeping XMM going for as long as it’s technically feasible. 61 00:04:04,710 --> 00:04:08,740 Daniel: We really need to support the observatories that we have and 62 00:04:08,760 --> 00:04:12,800 keeping those aloft, because those are the things that excite everyone about science, 63 00:04:12,820 --> 00:04:16,860 and especially that excite students to go into it. 64 00:04:16,880 --> 00:04:20,990 Lisa: I would say that my career has really been inspired 65 00:04:21,010 --> 00:04:25,160 by XMM-Newton and has followed along it in a lot of different ways 66 00:04:25,180 --> 00:04:29,240 that I didn’t expect. Laura: It’s remarkable to me that XMM is still performing at the level 67 00:04:29,260 --> 00:04:33,290 it is 20 years after the mission originated. And really, that’s the best possible 68 00:04:33,310 --> 00:04:37,320 PR for the mission. (Music) 69 00:04:37,340 --> 00:04:41,350 [XMM-Newton] 70 00:04:41,370 --> 00:04:45,370 [20 Years, and looking forward] 71 00:04:45,390 --> 00:04:54,460 [Additional interviews and footage courtesy of: ESA/Norbert Schartel, Wayne State University, University of Utah, Smithsonian Astrophysical Observatory] 72 00:04:54,480 --> 00:05:00,680 [Explore, Solar System & Beyond. NASA]