WEBVTT FILE 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]