1 00:00:01,163 --> 00:00:03,429 Once there was a star. 2 00:00:04,082 --> 00:00:06,804 Like everything else, she was born; 3 00:00:06,828 --> 00:00:10,609 grew to be around 30 times the mass of our sun 4 00:00:10,633 --> 00:00:12,926 and lived for a very long time. 5 00:00:13,475 --> 00:00:14,843 Exactly how long, 6 00:00:14,867 --> 00:00:16,606 people cannot really tell. 7 00:00:17,162 --> 00:00:18,941 Just like everything in life, 8 00:00:18,965 --> 00:00:22,414 she reached the end of her regular star days 9 00:00:22,438 --> 00:00:25,015 when her heart, the core of her life, 10 00:00:25,039 --> 00:00:26,505 exhausted its fuel. 11 00:00:26,905 --> 00:00:28,212 But that was no end. 12 00:00:28,236 --> 00:00:31,762 She transformed into a supernova, and in the process 13 00:00:31,786 --> 00:00:34,440 releasing a tremendous amount of energy, 14 00:00:34,464 --> 00:00:37,172 outshining the rest of the galaxy 15 00:00:37,196 --> 00:00:39,530 and emitting, in one second, 16 00:00:39,554 --> 00:00:43,627 the same amount of energy our sun will release in 10 days. 17 00:00:43,651 --> 00:00:46,922 And she evolved into another role in our galaxy. 18 00:00:47,783 --> 00:00:50,257 Supernova explosions are very extreme. 19 00:00:50,638 --> 00:00:54,858 But the ones that emit gamma rays are even more extreme. 20 00:00:55,417 --> 00:00:57,706 In the process of becoming a supernova, 21 00:00:57,730 --> 00:01:01,153 the interior of the star collapses under its own weight 22 00:01:01,177 --> 00:01:04,065 and it starts rotating ever faster, 23 00:01:04,089 --> 00:01:07,954 like an ice skater when pulling their arms in close to their body. 24 00:01:08,592 --> 00:01:13,050 In that way, it starts rotating very fast and it increases, powerfully, 25 00:01:13,074 --> 00:01:14,634 its magnetic field. 26 00:01:15,011 --> 00:01:18,100 The matter around the star is dragged around, 27 00:01:18,124 --> 00:01:21,442 and some energy from that rotation is transferred to that matter 28 00:01:21,466 --> 00:01:24,874 and the magnetic field is increased even further. 29 00:01:25,477 --> 00:01:31,239 In that way, our star had extra energy to outshine the rest of the galaxy 30 00:01:31,263 --> 00:01:33,566 in brightness and gamma ray emission. 31 00:01:34,119 --> 00:01:36,608 My star, the one in my story, 32 00:01:36,632 --> 00:01:39,280 became what is known as a magnetar. 33 00:01:39,304 --> 00:01:40,985 And just for your information, 34 00:01:41,009 --> 00:01:44,890 the magnetic field of a magnetar is 1,000 trillion times 35 00:01:44,914 --> 00:01:46,683 the magnetic field of Earth. 36 00:01:47,953 --> 00:01:50,609 The most energetic events ever measured by astronomers 37 00:01:50,633 --> 00:01:52,888 carry the name gamma-ray bursts 38 00:01:52,912 --> 00:01:56,519 because we observe them as bursts most or explosions, 39 00:01:56,543 --> 00:01:59,076 most strongly measured as gamma-ray light. 40 00:01:59,886 --> 00:02:04,091 Our star, like the one in our story that became a magnetar, 41 00:02:04,115 --> 00:02:06,186 is detected as a gamma-ray burst 42 00:02:06,210 --> 00:02:08,770 during the most energetic portion of the explosion. 43 00:02:10,167 --> 00:02:15,468 Yet, even though gamma-ray bursts are the strongest events 44 00:02:15,492 --> 00:02:17,581 ever measured by astronomers, 45 00:02:17,605 --> 00:02:20,242 we cannot see them with our naked eye. 46 00:02:20,266 --> 00:02:22,594 We depend, we rely on other methods 47 00:02:22,618 --> 00:02:25,407 in order to study this gamma-ray light. 48 00:02:25,431 --> 00:02:27,278 We cannot see them with our naked eye. 49 00:02:27,302 --> 00:02:30,372 We can only see an itty bitty, tiny portion 50 00:02:30,396 --> 00:02:34,122 of the electromagnetic spectrum that we call visible light. 51 00:02:34,146 --> 00:02:36,418 And beyond that, we rely on other methods. 52 00:02:36,442 --> 00:02:41,702 Yet as astronomers, we study a wider range of light 53 00:02:41,726 --> 00:02:44,490 and we depend on other methods to do that. 54 00:02:44,514 --> 00:02:47,090 On the screen, it may look like this. 55 00:02:47,812 --> 00:02:49,544 You're seeing a plot. 56 00:02:49,568 --> 00:02:51,493 That is a light curve. 57 00:02:51,517 --> 00:02:55,066 It's a plot of intensity of light over time. 58 00:02:55,090 --> 00:02:57,554 It is a gamma-ray light curve. 59 00:02:58,013 --> 00:03:01,705 Sighted astronomers depend on this kind of plot 60 00:03:01,729 --> 00:03:06,401 in order to interpret how this light intensity changes over time. 61 00:03:06,933 --> 00:03:12,449 On the left, you will be seeing the light intensity without a burst, 62 00:03:12,473 --> 00:03:16,628 and on the right, you will be seeing the light intensity with the burst. 63 00:03:18,381 --> 00:03:22,082 Early during my career, I could also see this kind of plot. 64 00:03:22,562 --> 00:03:25,290 But then, I lost my sight. 65 00:03:25,314 --> 00:03:28,466 I completely lost my sight because of extended illness, 66 00:03:28,490 --> 00:03:32,175 and with it, I lost the opportunity to see this plot 67 00:03:33,208 --> 00:03:35,965 and the opportunity to do my physics. 68 00:03:37,672 --> 00:03:40,127 It was a very strong transition for me in many ways. 69 00:03:41,295 --> 00:03:45,540 And professionally, it left me without a way to do my science. 70 00:03:45,564 --> 00:03:50,179 I longed to access and scrutinize this energetic light 71 00:03:50,203 --> 00:03:52,889 and figure out the astrophysical cause. 72 00:03:52,913 --> 00:03:56,375 I wanted to experience the spacious wonder, the excitement, 73 00:03:56,399 --> 00:04:00,848 the joy produced by the detection of such a titanic celestial event. 74 00:04:01,352 --> 00:04:04,652 I thought long and hard about it, 75 00:04:04,676 --> 00:04:08,361 when I suddenly realized that all a light curve is, 76 00:04:08,385 --> 00:04:12,226 is a table of numbers converted into a visual plot. 77 00:04:12,861 --> 00:04:14,762 So along with my collaborators, 78 00:04:14,786 --> 00:04:18,994 we worked really hard and we translated the numbers into sound. 79 00:04:19,765 --> 00:04:21,769 I achieved access to the data, 80 00:04:21,793 --> 00:04:26,806 and today I'm able to do physics at the level of the best astronomer, 81 00:04:26,830 --> 00:04:27,981 using sound. 82 00:04:28,005 --> 00:04:30,633 And what people have been able to do, 83 00:04:30,657 --> 00:04:31,810 mainly visually, 84 00:04:31,834 --> 00:04:33,178 for hundreds of years, 85 00:04:33,202 --> 00:04:35,544 now I do it using sound. 86 00:04:35,892 --> 00:04:36,929 (Applause) 87 00:04:36,953 --> 00:04:38,655 Listening to this gamma-ray burst 88 00:04:38,679 --> 00:04:40,999 that you're seeing on the -- (Applause continues) 89 00:04:41,023 --> 00:04:42,174 Thank you. 90 00:04:42,198 --> 00:04:44,906 Listening to this burst that you're seeing on the screen 91 00:04:44,930 --> 00:04:47,525 brought something to the ear beyond the obvious burst. 92 00:04:47,973 --> 00:04:49,908 Now I'm going to play the burst for you. 93 00:04:49,932 --> 00:04:51,986 It's not music, it's sound. 94 00:04:53,264 --> 00:04:56,515 (Digital beeping sounds) 95 00:04:56,539 --> 00:04:59,830 This is scientific data converted into sound, 96 00:04:59,854 --> 00:05:01,088 and it's mapped in pitch. 97 00:05:01,112 --> 00:05:03,531 The process is called sonification. 98 00:05:06,958 --> 00:05:09,268 So listening to this brought something to the ear 99 00:05:09,292 --> 00:05:10,641 besides the obvious burst. 100 00:05:10,665 --> 00:05:15,186 When I examine the very strong low-frequency regions, 101 00:05:15,210 --> 00:05:20,082 or bass line -- I'm zooming into the bass line now. 102 00:05:21,500 --> 00:05:27,019 We noted resonances characteristic of electrically charged gasses 103 00:05:27,043 --> 00:05:28,645 like the solar wind. 104 00:05:28,669 --> 00:05:31,172 And I want you to hear what I heard. 105 00:05:31,196 --> 00:05:34,977 You will hear it as a very fast decrease in volume. 106 00:05:35,001 --> 00:05:37,764 And because you're sighted, I'm giving you a red line 107 00:05:37,788 --> 00:05:41,727 indicating what intensity of light is being converted into sound. 108 00:05:43,672 --> 00:05:46,086 (Digital hum and whistling sound) 109 00:05:46,110 --> 00:05:49,404 The (Whistles) is frogs at home, don't pay attention to that. 110 00:05:49,428 --> 00:05:51,274 (Laughter) 111 00:05:51,298 --> 00:05:56,525 (Digital hum and whistling sound) 112 00:05:56,549 --> 00:05:58,421 I think you heard it, right? 113 00:05:59,503 --> 00:06:00,780 So what we found 114 00:06:00,804 --> 00:06:05,718 is that the bursts last long enough in order to support wave resonances, 115 00:06:05,742 --> 00:06:09,959 which are things caused by exchanges of energy between particles 116 00:06:09,983 --> 00:06:11,301 that may have been excited, 117 00:06:11,325 --> 00:06:12,706 that depend on the volume. 118 00:06:13,151 --> 00:06:16,241 You may remember that I said that the matter around the star 119 00:06:16,265 --> 00:06:17,921 is dragged around? 120 00:06:17,945 --> 00:06:21,759 It transmits power with frequency and field distribution 121 00:06:21,783 --> 00:06:23,505 determined by the dimensions. 122 00:06:24,434 --> 00:06:28,384 You may remember that we were talking about a super-massive star 123 00:06:28,408 --> 00:06:31,576 that became a very strong magnetic field magnetar. 124 00:06:32,264 --> 00:06:36,637 If this is the case, then outflows from the exploding star 125 00:06:36,661 --> 00:06:39,144 may be associated with this gamma-ray burst. 126 00:06:39,168 --> 00:06:40,736 What does that mean? 127 00:06:40,760 --> 00:06:43,727 That star formation may be a very important part 128 00:06:43,751 --> 00:06:45,265 of these supernova explosions. 129 00:06:46,047 --> 00:06:50,434 Listening to this very gamma-ray burst brought us to the notion 130 00:06:50,458 --> 00:06:53,257 that the use of sound as an adjunctive visual display 131 00:06:53,281 --> 00:06:55,506 may also support sighted astronomers 132 00:06:55,530 --> 00:06:57,980 in the search for more information in the data. 133 00:06:58,562 --> 00:07:03,880 Simultaneously, I worked on analyzing measurements from other telescopes, 134 00:07:03,904 --> 00:07:06,107 and my experiments demonstrated 135 00:07:06,131 --> 00:07:10,345 that when you use sound as an adjunctive visual display, 136 00:07:10,369 --> 00:07:13,285 astronomers can find more information 137 00:07:13,309 --> 00:07:16,176 in this now more accessible data set. 138 00:07:17,086 --> 00:07:20,830 This ability to transform data into sound 139 00:07:20,854 --> 00:07:23,931 gives astronomy a tremendous power of transformation. 140 00:07:24,381 --> 00:07:28,322 And the fact that a field that is so visual may be improved 141 00:07:28,346 --> 00:07:33,019 in order to include anyone with interest in understanding what lies in the heavens 142 00:07:33,043 --> 00:07:34,552 is a spirit-lifter. 143 00:07:35,390 --> 00:07:37,279 When I lost my sight, 144 00:07:37,303 --> 00:07:39,379 I noticed that I didn't have access 145 00:07:39,403 --> 00:07:42,029 to the same amount and quality of information 146 00:07:42,053 --> 00:07:43,449 a sighted astronomer had. 147 00:07:44,220 --> 00:07:47,700 It was not until we innovated with the sonification process 148 00:07:47,724 --> 00:07:51,676 that I regained the hope to be a productive member of the field 149 00:07:51,700 --> 00:07:54,310 that I had worked so hard to be part of. 150 00:07:55,429 --> 00:07:59,880 Yet, information access is not the only area in astronomy 151 00:07:59,904 --> 00:08:02,088 where this is important. 152 00:08:02,602 --> 00:08:05,126 The situation is systemic 153 00:08:05,150 --> 00:08:08,119 and scientific fields are not keeping up. 154 00:08:08,825 --> 00:08:11,477 The body is something changeable -- 155 00:08:11,501 --> 00:08:14,866 anyone may develop a disability at any point. 156 00:08:14,890 --> 00:08:17,128 Let's think about, for example, 157 00:08:17,152 --> 00:08:19,939 scientists that are already at the top of their careers. 158 00:08:19,963 --> 00:08:22,803 What happens to them if they develop a disability? 159 00:08:22,827 --> 00:08:25,244 Will they feel excommunicated as I did? 160 00:08:25,839 --> 00:08:29,029 Information access empowers us to flourish. 161 00:08:29,499 --> 00:08:33,099 It gives us equal opportunities to display our talents 162 00:08:33,123 --> 00:08:35,986 and choose what we want to do with our lives, 163 00:08:36,010 --> 00:08:39,318 based on interest and not based on potential barriers. 164 00:08:40,294 --> 00:08:44,661 When we give people the opportunity to succeed without limits, 165 00:08:44,685 --> 00:08:49,243 that will lead to personal fulfillment and prospering life. 166 00:08:49,267 --> 00:08:51,700 And I think that the use of sound in astronomy 167 00:08:51,724 --> 00:08:55,201 is helping us to achieve that and to contribute to science. 168 00:08:56,119 --> 00:09:00,651 While other countries told me that the study of perception techniques 169 00:09:00,675 --> 00:09:04,252 in order to study astronomy data is not relevant to astronomy 170 00:09:04,276 --> 00:09:07,476 because there are no blind astronomers in the field, 171 00:09:07,500 --> 00:09:10,904 South Africa said, "We want people with disabilities 172 00:09:10,928 --> 00:09:12,904 to contribute to the field." 173 00:09:12,928 --> 00:09:14,254 Right now, I'm working 174 00:09:14,278 --> 00:09:17,010 at the South African Astronomical Observatory, 175 00:09:17,034 --> 00:09:20,119 at the Office of Astronomy for Development. 176 00:09:20,436 --> 00:09:25,177 There, we are working on sonification techniques and analysis methods 177 00:09:25,201 --> 00:09:28,647 to impact the students of the Athlone School for the Blind. 178 00:09:29,603 --> 00:09:32,089 These students will be learning radio astronomy, 179 00:09:32,113 --> 00:09:35,351 and they will be learning the sonification methods 180 00:09:35,375 --> 00:09:39,846 in order to study astronomical events like huge ejections of energy 181 00:09:39,870 --> 00:09:42,306 from the sun, known as coronal mass ejections. 182 00:09:43,194 --> 00:09:44,953 What we learn with these students -- 183 00:09:44,977 --> 00:09:48,774 these students have multiple disabilities and coping strategies 184 00:09:48,798 --> 00:09:50,674 that will be accommodated -- 185 00:09:50,698 --> 00:09:53,537 what we learn with these students will directly impact 186 00:09:53,561 --> 00:09:56,718 the way things are being done at the professional level. 187 00:09:56,742 --> 00:09:58,801 I humbly call this development. 188 00:09:58,825 --> 00:10:01,081 And this is happening right now. 189 00:10:02,350 --> 00:10:05,728 I think that science is for everyone. 190 00:10:06,275 --> 00:10:07,723 It belongs to the people, 191 00:10:07,747 --> 00:10:09,998 and it has to be available to everyone, 192 00:10:10,022 --> 00:10:12,235 because we are all natural explorers. 193 00:10:12,956 --> 00:10:18,136 I think that if we limit people with disabilities 194 00:10:18,171 --> 00:10:20,000 from participating in science, 195 00:10:20,024 --> 00:10:23,672 we'll sever our links with history and with society. 196 00:10:23,696 --> 00:10:27,142 I dream of a level scientific playing field, 197 00:10:27,166 --> 00:10:32,154 where people encourage respect and respect each other, 198 00:10:32,178 --> 00:10:35,266 where people exchange strategies and discover together. 199 00:10:35,810 --> 00:10:40,107 If people with disabilities are allowed into the scientific field, 200 00:10:40,131 --> 00:10:44,840 an explosion, a huge titanic burst of knowledge will take place, 201 00:10:44,864 --> 00:10:46,341 I am sure. 202 00:10:49,251 --> 00:10:51,100 (Digital beeping sounds) 203 00:10:51,124 --> 00:10:52,988 That is the titanic burst. 204 00:10:54,420 --> 00:10:55,571 Thank you. 205 00:10:55,595 --> 00:10:56,746 Thank you. 206 00:10:56,770 --> 00:11:02,442 (Applause)