WEBVTT FILE 1 00:00:00.800 --> 00:00:03.603 [Music throughout] 2 00:00:03.837 --> 00:00:04.804 XRISM is 3 00:00:04.804 --> 00:00:07.807 our newest X-ray telescope in space. 4 00:00:07.974 --> 00:00:11.978 It's a JAXA/NASA collaborative mission with ESA participation 5 00:00:12.078 --> 00:00:17.584 and will revolutionize X-ray observations of the universe. 6 00:00:17.684 --> 00:00:20.053 It does this with a one-of-a-kind sensor 7 00:00:20.053 --> 00:00:24.824 that captures data with 36 supercooled pixels. 8 00:00:24.891 --> 00:00:27.527 Yes, you heard that right, 9 00:00:27.527 --> 00:00:31.197 this groundbreaking detector isn't measured in megapixels. 10 00:00:31.297 --> 00:00:35.301 It's a six-by-six grid of 36 pixels, 11 00:00:35.402 --> 00:00:39.005 but they're unlike any others. 12 00:00:39.005 --> 00:00:41.307 Although this detector, called Resolve, 13 00:00:41.307 --> 00:00:43.877 can create low-resolution X-ray images, 14 00:00:43.877 --> 00:00:46.446 that is not what makes it unique. 15 00:00:47.280 --> 00:00:50.183 Each pixel in Resolve is a microcalorimeter 16 00:00:50.183 --> 00:00:52.752 so it can measure tiny amounts of heat. 17 00:00:52.752 --> 00:00:54.621 A six-stage system 18 00:00:54.621 --> 00:00:57.190 cools it to 50 millikelvins, 19 00:00:57.424 --> 00:01:00.093 or a fraction of a degree above absolute zero. 20 00:01:00.460 --> 00:01:02.495 This extreme low temperature 21 00:01:02.662 --> 00:01:05.632 allows Resolve to measure how much a pixel warms 22 00:01:05.632 --> 00:01:07.801 when it absorbs a single X-ray, 23 00:01:08.234 --> 00:01:10.737 and therefore measure the energy 24 00:01:10.737 --> 00:01:12.806 of that one particle of light. 25 00:01:12.872 --> 00:01:14.240 It’s basically 26 00:01:14.240 --> 00:01:15.875 a precise way of measuring 27 00:01:15.875 --> 00:01:17.744 the X-ray’s color. 28 00:01:18.445 --> 00:01:19.446 As a result, 29 00:01:19.446 --> 00:01:22.715 XRISM can create the most detailed X-ray spectrum ever 30 00:01:22.715 --> 00:01:24.250 for distant objects. 31 00:01:24.384 --> 00:01:28.221 This spectrum can give a great deal of useful information, 32 00:01:28.221 --> 00:01:29.923 like temperature, 33 00:01:29.923 --> 00:01:32.058 what elements are present and in what quantities, 34 00:01:32.058 --> 00:01:34.327 and how fast an object is moving 35 00:01:34.327 --> 00:01:36.162 toward or away from us, 36 00:01:36.162 --> 00:01:38.932 even if we can only see it as a dot in the sky, 37 00:01:38.932 --> 00:01:41.201 too distant to resolve details. 38 00:01:41.968 --> 00:01:44.170 This would be a revolutionary achievement 39 00:01:44.170 --> 00:01:46.439 for a detector with a single pixel. 40 00:01:46.673 --> 00:01:48.741 But Resolve has 36. 41 00:01:49.075 --> 00:01:50.543 This allows XRISM to observe 42 00:01:50.543 --> 00:01:52.011 “extended objects” 43 00:01:52.011 --> 00:01:53.680 that aren’t point-source dots 44 00:01:54.013 --> 00:01:56.749 and create spectrum maps of their different regions. 45 00:01:56.749 --> 00:01:58.651 That can reveal speed 46 00:01:58.651 --> 00:01:59.886 and temperature differences 47 00:01:59.886 --> 00:02:01.921 in extremely hot gases. 48 00:02:02.522 --> 00:02:03.823 Using that information, 49 00:02:03.823 --> 00:02:05.024 scientists can determine 50 00:02:05.024 --> 00:02:08.428 how nebulae and galaxy clusters have evolved 51 00:02:08.428 --> 00:02:10.630 and interacted over time. 52 00:02:11.097 --> 00:02:13.299 The Resolve detector was invented 53 00:02:13.299 --> 00:02:15.935 and built at NASA’s Goddard Space Flight Center. 54 00:02:16.569 --> 00:02:18.505 The detector’s success in XRISM 55 00:02:18.738 --> 00:02:21.074 will enable Goddard to further the design 56 00:02:21.074 --> 00:02:24.010 an follow up with X-ray microcalorimeters 57 00:02:24.077 --> 00:02:27.013 with hundreds or even thousands of pixels. 58 00:02:27.814 --> 00:02:31.351 So, while it may not sound as impressive as 4k 59 00:02:31.351 --> 00:02:33.286 or 50 megapixels, 60 00:02:33.286 --> 00:02:35.121 the Resolve detector on XRISM 61 00:02:35.121 --> 00:02:36.956 will be revolutionizing our understanding 62 00:02:36.956 --> 00:02:38.558 of the large-scale 63 00:02:38.558 --> 00:02:39.859 high-energy universe. 64 00:02:40.293 --> 00:02:41.661 And that’s pretty amazing 65 00:02:41.661 --> 00:02:44.330 for a “mere” three-dozen pixels. 66 00:02:45.532 --> 00:02:50.403 [NASA]