WEBVTT FILE 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]