1 00:00:00,000 --> 00:00:05,020 [Music throughout] [XMM-Newton] 2 00:00:05,040 --> 00:00:08,980 [Launched on December 10, 1999,] 3 00:00:09,000 --> 00:00:13,020 [XMM-Newton is an ESA (European Space Agency) X-ray telescope supported by NASA.] 4 00:00:13,040 --> 00:00:17,020 [It has revolutionized the study of high-energy phenomena in the universe.] 5 00:00:17,040 --> 00:00:20,980 6 00:00:21,000 --> 00:00:24,980 France Cordova: The longevity of XMM was not foreseen, it just kept 7 00:00:25,000 --> 00:00:29,020 right on going. Stephanie LaMassa: Something about looking at the night sky that just 8 00:00:29,040 --> 00:00:32,980 fills you with a sense of wonder and I just never grew up from that. 9 00:00:33,000 --> 00:00:37,020 Lisa Winter: XMM has been a part of my career from 10 00:00:37,040 --> 00:00:40,980 the earliest stages even until now. 11 00:00:41,000 --> 00:00:45,020 LaMassa: XMM is a space-based observatory that studies X-ray 12 00:00:45,040 --> 00:00:48,980 light from the most energetic phenomena in the universe. It spans 13 00:00:49,000 --> 00:00:53,020 [Stephanie LaMassa, Astronomer, Space Telescope Science Institute. Ph.D. thesis based on XMM-Newton data] the range of everything from studying energetic 14 00:00:53,040 --> 00:00:56,980 stars and exoplanets around those stars to the most distant universe. 15 00:00:57,000 --> 00:01:00,980 [Norbert Schartel, XMM-Newton Project Scientist, ESA] We can start with comets, which are very cold objects. 16 00:01:01,000 --> 00:01:04,980 We go then to compact objects where we observe 17 00:01:05,000 --> 00:01:08,980 very hot plasma near to the event horizon from a black hole. 18 00:01:09,000 --> 00:01:13,020 And then, completely different then we look in 19 00:01:13,040 --> 00:01:17,020 XMM-Newton data for signature of dark matter, and this 20 00:01:17,040 --> 00:01:20,980 I think makes this mission so great, that it allows such a 21 00:01:21,000 --> 00:01:25,020 broad science to be addressed. Cordova: I had a sabbatical 22 00:01:25,040 --> 00:01:28,980 in 1982 in the United Kingdom, 23 00:01:29,000 --> 00:01:32,980 and my officemate at the time was Steve Kahn. We had a 24 00:01:33,000 --> 00:01:37,020 third office mate it was Keith Mason. We came up with the 25 00:01:37,040 --> 00:01:41,020 [France Cordova, Director, National Science Foundation (NSF) Was co-PI of XMM-Newton Optical/UV Monitor Telescope] idea that it would be great to do multiwavelength 26 00:01:41,040 --> 00:01:45,020 observations from space. To do deep X-ray 27 00:01:45,040 --> 00:01:49,020 imaging and spectroscopy and simultaneously 28 00:01:49,040 --> 00:01:53,020 be able to observe cosmic sources in the ultraviolet 29 00:01:53,040 --> 00:01:57,020 and optical bands. If we could do all this from 30 00:01:57,040 --> 00:02:01,020 one platform in space, namely XMM, we 31 00:02:01,040 --> 00:02:05,020 it would be much more efficient. Then, when the X-rays saw something 32 00:02:05,040 --> 00:02:08,980 pop off, the ultraviolet/optical telescope would be right there 33 00:02:09,000 --> 00:02:13,020 seeing it right away. [Lisa Winter, Astronomer, NSF. Ph.D. thesis based on XMM-Newton data] XMM-Newton is 34 00:02:13,040 --> 00:02:17,020 a really fantastic telescope. It’s more than just one telescope 35 00:02:17,040 --> 00:02:20,980 actually. You can study the same object across a range 36 00:02:21,000 --> 00:02:25,020 of energies from the optical, where we can observe from 37 00:02:25,040 --> 00:02:28,980 the Earth, up into the UV and X-rays where you really have to go 38 00:02:29,000 --> 00:02:33,020 above into space. Cordova: It was great to be at the beginning 39 00:02:33,040 --> 00:02:37,020 of multiwavelength astronomy. There’s 40 00:02:37,040 --> 00:02:41,020 virtually no cosmic sources that just radiate at 41 00:02:41,040 --> 00:02:45,020 one frequency, and when you look at the universe with X-ray 42 00:02:45,040 --> 00:02:48,980 eyes you see something much different than when you look at the same universe in 43 00:02:49,000 --> 00:02:52,980 ultraviolet eyes. Steve Kahn: I led the US piece of one 44 00:02:53,000 --> 00:02:57,020 [Steve Kahn, Professor, SLAC National Accelerator Lab. Was co-PI of XMM-Newton Reflection Grating Spectrometer (RGS)] of the three major instruments on XMM-Newton, which was called the Reflection 45 00:02:57,040 --> 00:03:01,020 Grating Spectrometer. I developed the initial 46 00:03:01,040 --> 00:03:05,020 concept for that in the early 1980s when I was quite young. 47 00:03:05,040 --> 00:03:09,020 We knew that many systems in the universe emitted X-rays copiously, but 48 00:03:09,040 --> 00:03:13,020 we didn’t have very detailed models for how that X-ray emission 49 00:03:13,040 --> 00:03:17,020 arises and what it was actually telling us about the systems. 50 00:03:17,040 --> 00:03:21,020 [Maurice Leutenegger, Astronomer, NASA’s Goddard Space Flight Center. Was XMM-Newton RGS team member] Spectroscopy is the study of light emitted by atoms, 51 00:03:21,040 --> 00:03:25,020 but it’s 52 00:03:25,040 --> 00:03:29,020 more than that because atoms are peculiar. When they shine they don't 53 00:03:29,040 --> 00:03:32,980 just give you all the colors of the rainbow, it looks more like 54 00:03:33,000 --> 00:03:37,020 a barcode. Kahn: You get very sharp peaks at very particular 55 00:03:37,040 --> 00:03:40,980 wavelengths and frequencies and those are associated with particular 56 00:03:41,000 --> 00:03:45,020 quantum states. Leutenegger: It’s extremely powerful, it’s just like a barcode, it 57 00:03:45,040 --> 00:03:49,020 looks like a bunch of garbage to human eyes but it can tell you 58 00:03:49,040 --> 00:03:52,980 you know, what’s in a product, and how much it costs, and what country it came from, and all that stuff. 59 00:03:53,000 --> 00:03:57,020 Kahn: By measuring that detailed pattern we can learn about the 60 00:03:57,040 --> 00:04:01,020 fundamental physics of what’s happening in these very exotic environments. What the 61 00:04:01,040 --> 00:04:05,020 temperatures are, the densities, the pressures. The spectroscopy that 62 00:04:05,040 --> 00:04:08,980 XMM-Newton did really answered a huge number of questions. 63 00:04:09,000 --> 00:04:12,980 Dheeraj Pasham: With the most recent result with XMM we were 64 00:04:13,000 --> 00:04:16,980 [Dheeraj Pasham, Einstein fellow, MIT. Ph.D. thesis based on XMM-Newton data] able to measure the spin of the black hole, and I liked the signal so much 65 00:04:17,000 --> 00:04:20,980 so that I put it on a cup and I drink from it every day, so. (laughs) 66 00:04:21,000 --> 00:04:24,980 Schartel: My son was shocked that other people 67 00:04:25,000 --> 00:04:29,020 in the school were knowing XMM-Newton. 68 00:04:29,040 --> 00:04:32,980 Small children from 10 years, that they know that XMM-Newton 69 00:04:33,000 --> 00:04:37,020 is X-ray satellite. Cordova: Ah, you know, it’s amazing. It’s like 70 00:04:37,040 --> 00:04:40,980 the Cal Ripkin of satellites, of space satellites, this 71 00:04:41,000 --> 00:04:44,980 thing that just keeps going and going and going and producing great data. 72 00:04:45,000 --> 00:04:48,980 Kahn: I’m delighted to see that number one the mission 73 00:04:49,000 --> 00:04:53,020 is still working and the instrument is stilling working and that there are 74 00:04:53,040 --> 00:04:56,980 all these young scientists that have been inspired to figure out great things to do with it. 75 00:04:57,000 --> 00:05:01,020 Cordova: And they’re using it for, in all sorts of ways, which is 76 00:05:01,040 --> 00:05:04,980 really amazing to see a telescope used in ways and for 77 00:05:05,000 --> 00:05:08,980 discoveries that you could never have predicted when you first were 78 00:05:09,000 --> 00:05:13,020 designing it and launching it. LaMassa: There’s certain science that 79 00:05:13,040 --> 00:05:17,020 XMM can do that other X-ray observatories 80 00:05:17,040 --> 00:05:21,020 can’t. Recently XMM has invested lots of 81 00:05:21,040 --> 00:05:24,980 time in these large-area multiwavelength survey 82 00:05:25,000 --> 00:05:29,020 fields including work that I’ve been leading, in a region 83 00:05:29,040 --> 00:05:33,020 of the sky that has lots of existing data. 84 00:05:33,040 --> 00:05:36,980 And that multiwavelength data is really important to harness the best scientific 85 00:05:37,000 --> 00:05:41,020 results out of XMM. Pasham: Astronomy is going through a revolution. 86 00:05:41,040 --> 00:05:45,020 There’s gravitational waves detected, there’s several kinds of weird 87 00:05:45,040 --> 00:05:49,020 supernovae detected, and having an X-ray instrument to 88 00:05:49,040 --> 00:05:52,980 simultaneously operate while these optical instruments are operating 89 00:05:53,000 --> 00:05:56,980 will be extremely beneficial. Winter: Many objects change — they have 90 00:05:57,000 --> 00:06:01,020 flares and outbursts — so it’s really a key 91 00:06:01,040 --> 00:06:05,020 observation to have everything from the X-ray, the optical, 92 00:06:05,040 --> 00:06:08,980 and the UV all precisely at the same time. 93 00:06:09,000 --> 00:06:13,020 Cordova: I’m so glad that XMM is a part of that, that it was 94 00:06:13,040 --> 00:06:16,980 taking people originally into the directions 95 00:06:17,000 --> 00:06:21,020 of the time, and today is taking people into entirely new directions. 96 00:06:21,040 --> 00:06:24,980 97 00:06:25,000 --> 00:06:29,020 [XMM-Newton 20 years] 98 00:06:29,040 --> 00:06:33,020 [and looking forward] 99 00:06:33,040 --> 00:06:36,980 100 00:06:37,000 --> 00:06:42,800 [Explore: Solar system & Beyond] 101 00:06:42,820 --> 00:06:42,796 [NASA]