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]