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These are the user uploaded subtitles that are being translated: 1 00:00:06,700 --> 00:00:09,200 In July 2022, the first images 2 00:00:09,200 --> 00:00:12,320 from the James Webb Space Telescope were released, 3 00:00:12,320 --> 00:00:15,560 to the joy of myself and millions of astronomy fans 4 00:00:15,560 --> 00:00:17,040 all around the world. 5 00:00:20,480 --> 00:00:22,040 Oh, my gosh! 6 00:00:23,200 --> 00:00:25,400 CROWD EXCLAIMS 7 00:00:25,400 --> 00:00:27,160 Wow, look at that. 8 00:00:27,160 --> 00:00:29,120 At the time, we were all blown away 9 00:00:29,120 --> 00:00:31,200 by the stunning new images. 10 00:00:31,200 --> 00:00:34,880 Their exquisite detail reminded us of the beauty of the universe 11 00:00:34,880 --> 00:00:36,640 in which we live. 12 00:00:36,640 --> 00:00:38,520 But as well as the pretty pictures, 13 00:00:38,520 --> 00:00:40,960 we've also been getting data from the telescope's 14 00:00:40,960 --> 00:00:44,040 various instruments, which have continued working throughout, 15 00:00:44,040 --> 00:00:47,640 flooding scientists with information about planets, galaxies, 16 00:00:47,640 --> 00:00:49,320 and so much more besides. 17 00:00:50,440 --> 00:00:53,040 Now we're two years on - and in that time, 18 00:00:53,040 --> 00:00:56,920 scientists have been busy analysing the data and putting out papers. 19 00:00:56,920 --> 00:01:01,240 But has JWST been as exciting and ground-breaking as we'd hoped? 20 00:01:01,240 --> 00:01:04,280 And has it been plain sailing for the telescope itself? 21 00:01:04,280 --> 00:01:07,120 Well, tonight, we're looking at the story so far of 22 00:01:07,120 --> 00:01:09,360 the James Webb Space Telescope. 23 00:01:09,360 --> 00:01:11,680 Welcome to The Sky At Night. 24 00:01:41,440 --> 00:01:45,200 So today, I'm on the road, retracing the steps of 25 00:01:45,200 --> 00:01:48,480 a journey that Chris made in the summer of 2022, 26 00:01:48,480 --> 00:01:50,840 when we got the first release 27 00:01:50,840 --> 00:01:54,120 of the data from the James Webb Space Telescope. 28 00:01:54,120 --> 00:01:57,440 Chris had hit the road to meet up with researchers 29 00:01:57,440 --> 00:02:01,040 around the country to find out what they were hoping 30 00:02:01,040 --> 00:02:03,520 this new space telescope could reveal. 31 00:02:05,840 --> 00:02:09,880 Since then, these scientists and others have been working hard 32 00:02:09,880 --> 00:02:13,960 to understand the information that the JWST sent back. 33 00:02:13,960 --> 00:02:16,880 And we're off to find out what they've discovered. 34 00:02:18,920 --> 00:02:23,680 But first, what has the JWST story been so far? 35 00:02:24,720 --> 00:02:27,520 Billions of years ago, when the universe was young, 36 00:02:27,520 --> 00:02:30,480 the first galaxies began to shine brightly, 37 00:02:30,480 --> 00:02:33,560 illuminated by some of the earliest stars. 38 00:02:33,560 --> 00:02:36,440 Their light has been travelling through the cosmos ever since, 39 00:02:36,440 --> 00:02:40,240 streaming unnoticed past the Earth for all of human history. 40 00:02:40,240 --> 00:02:43,600 Unnoticed, that is, until two years ago, 41 00:02:43,600 --> 00:02:47,160 when that ancient light encountered a fragile golden mirror floating 42 00:02:47,160 --> 00:02:49,840 in space a million miles from here, 43 00:02:49,840 --> 00:02:52,360 It was brought to a focus in some of the most delicate 44 00:02:52,360 --> 00:02:54,800 and sophisticated instruments ever launched - 45 00:02:54,800 --> 00:02:57,800 and we can read its story for the first time. 46 00:02:57,800 --> 00:03:00,200 This is the miracle of JWST - 47 00:03:00,200 --> 00:03:04,080 a telescope built to show us the hidden places of the universe 48 00:03:04,080 --> 00:03:06,760 and reveal unimagined wonders. 49 00:03:06,760 --> 00:03:08,960 In the more than two years since it launched, 50 00:03:08,960 --> 00:03:11,440 the telescope has had its problems, sure. 51 00:03:11,440 --> 00:03:14,720 It's been hit more than 20 times by micrometeorites - 52 00:03:14,720 --> 00:03:17,720 tiny particles of dust zipping about the solar system. 53 00:03:17,720 --> 00:03:21,520 And one of them's left a permanent dent on one of those mirrors. 54 00:03:21,520 --> 00:03:25,440 JWST's controllers now avoid pointing in directions where 55 00:03:25,440 --> 00:03:27,400 there are plenty of micrometeorites, 56 00:03:27,400 --> 00:03:28,880 keeping the telescope safe. 57 00:03:28,880 --> 00:03:32,120 Actually, we've learned about the distribution of dust 58 00:03:32,120 --> 00:03:34,880 in the solar system - a scientific reward for placing 59 00:03:34,880 --> 00:03:37,280 our telescope in such peril. 60 00:03:37,280 --> 00:03:39,920 Otherwise, despite occasional problems getting used 61 00:03:39,920 --> 00:03:42,240 to using JWST's instruments, 62 00:03:42,240 --> 00:03:45,600 our biggest problem has been deciding where to point. 63 00:03:45,600 --> 00:03:49,040 Astronomers around the world have produced enough ideas 64 00:03:49,040 --> 00:03:51,720 to keep seven or eight versions of JWST busy. 65 00:03:51,720 --> 00:03:55,120 And though it's easy to get lost in the iconic images... 66 00:03:55,120 --> 00:03:56,560 Oh, look, the Horsehead! 67 00:03:56,560 --> 00:03:59,120 Orion! Merging galaxies! 68 00:03:59,120 --> 00:04:02,360 ..the telescope actually spends about three quarters of its time 69 00:04:02,360 --> 00:04:04,120 doing spectroscopy, 70 00:04:04,120 --> 00:04:07,480 splitting up the light it receives into its constituent wavelengths, 71 00:04:07,480 --> 00:04:10,200 revealing what planetary atmospheres are made of, 72 00:04:10,200 --> 00:04:13,440 what's happening deep in the heart of star-forming regions, 73 00:04:13,440 --> 00:04:17,720 and finding out quite how far away those oh-so-distant galaxies are. 74 00:04:17,720 --> 00:04:20,200 Answer - very. 75 00:04:20,200 --> 00:04:23,400 Together, JWST's three instruments have shown us 76 00:04:23,400 --> 00:04:25,520 a completely new view of Mars. 77 00:04:25,520 --> 00:04:28,240 They've revealed rings around a centaur asteroid in 78 00:04:28,240 --> 00:04:30,360 the frozen outer solar system, 79 00:04:30,360 --> 00:04:34,400 have given us a new view of old clusters of stars in our galaxy, 80 00:04:34,400 --> 00:04:38,400 and shown a spectacular star formation in more distant systems. 81 00:04:38,400 --> 00:04:42,080 Best of all, it gives us new views of very familiar objects, 82 00:04:42,080 --> 00:04:43,920 like this one of the Ring Nebula, 83 00:04:43,920 --> 00:04:47,200 which shows mysterious spikes pointing away from the centre, 84 00:04:47,200 --> 00:04:51,080 a ring that's comprised of 20,000 separate clumps of gas, 85 00:04:51,080 --> 00:04:53,200 each the mass of the Earth. 86 00:04:53,200 --> 00:04:57,760 And the telescope has also revealed a complex soup of carbon molecules - 87 00:04:57,760 --> 00:04:59,720 unusual for a planetary nebula. 88 00:04:59,720 --> 00:05:01,960 And this is just one object. 89 00:05:01,960 --> 00:05:04,400 Imagine how much more there is to see. 90 00:05:04,400 --> 00:05:08,200 The truth is, we could fill every episode of The Sky At Night 91 00:05:08,200 --> 00:05:10,280 for the next 20 years with new data 92 00:05:10,280 --> 00:05:13,560 and new images from this most marvellous of observatories. 93 00:05:13,560 --> 00:05:15,920 And, you know, we probably will. 94 00:05:23,440 --> 00:05:26,240 So, that's what the JWST has achieved. 95 00:05:26,240 --> 00:05:29,160 But science can be more complicated than that. 96 00:05:29,160 --> 00:05:33,080 For every answer, it reveals another exciting question. 97 00:05:35,920 --> 00:05:38,760 I'm off to the University of Bristol 98 00:05:38,760 --> 00:05:42,360 to find out what Dr Hannah Wakeford has discovered since 99 00:05:42,360 --> 00:05:44,880 she met Chris two years ago. 100 00:05:44,880 --> 00:05:46,600 Hannah, good to see you again. 101 00:05:46,600 --> 00:05:47,720 Good to see you. 102 00:05:47,720 --> 00:05:51,680 So, can you believe it was two years since you last met up with Chris? 103 00:05:51,680 --> 00:05:53,440 Not really, to be honest. THEY CHUCKLE 104 00:05:53,440 --> 00:05:56,000 It seems like yesterday we were just getting data down 105 00:05:56,000 --> 00:05:57,440 from the telescope. 106 00:05:57,440 --> 00:06:00,680 Well, I wanted to play you the clip just to remind you what happened. 107 00:06:00,680 --> 00:06:03,800 So, you've been planning these observations with colleagues 108 00:06:03,800 --> 00:06:05,280 for a long while, I know. 109 00:06:05,280 --> 00:06:08,400 How does it feel to finally have data sitting on this computer? 110 00:06:08,400 --> 00:06:09,560 Overwhelming. 111 00:06:09,560 --> 00:06:11,800 I'm getting all teary - every time I think about it, 112 00:06:11,800 --> 00:06:14,920 I'm just like, "This is so amazing!" 113 00:06:14,920 --> 00:06:17,560 You were truly so excited to get the data. 114 00:06:17,560 --> 00:06:19,360 I'm still so excited to get the data! 115 00:06:19,360 --> 00:06:21,720 Whenever I can get data, I'm happy to get data. 116 00:06:21,720 --> 00:06:24,520 I think that's the beauty of being an observer - is just 117 00:06:24,520 --> 00:06:26,320 we're always excited to learn new things. 118 00:06:27,840 --> 00:06:31,000 One planet that Hannah and her team were excited to observe 119 00:06:31,000 --> 00:06:34,600 with JWST was WASP-17b. 120 00:06:36,280 --> 00:06:38,480 And what's interesting about this exoplanet? 121 00:06:38,480 --> 00:06:40,480 So, it is a giant planet. 122 00:06:40,480 --> 00:06:42,800 It is about twice the radius of Jupiter, 123 00:06:42,800 --> 00:06:44,520 but only half of its mass. 124 00:06:44,520 --> 00:06:46,480 So, it's very low density. 125 00:06:46,480 --> 00:06:49,160 So, this is an artist's impression that is now based on 126 00:06:49,160 --> 00:06:51,320 the observations we got with JWST. 127 00:06:51,320 --> 00:06:52,840 Oh, wow. So... 128 00:06:52,840 --> 00:06:54,240 So, people take that data, 129 00:06:54,240 --> 00:06:56,640 and then create what they think it might look like? 130 00:06:56,640 --> 00:06:59,520 So, we talk with the artists, and we work with them to try 131 00:06:59,520 --> 00:07:01,800 and describe what we're seeing. 132 00:07:01,800 --> 00:07:04,240 Now, the data itself looks something like this. 133 00:07:04,240 --> 00:07:06,200 Ah, yeah - less artistic. 134 00:07:06,200 --> 00:07:08,960 It's a little bit harder to sell, let's say. 135 00:07:08,960 --> 00:07:12,600 Data from the Hubble Space Telescope had already revealed 136 00:07:12,600 --> 00:07:16,560 tiny particles in the planet's atmosphere. 137 00:07:16,560 --> 00:07:21,200 But Hannah had hoped data from JWST's mid-infrared instrument 138 00:07:21,200 --> 00:07:24,480 could finally tell them what these particles were made of. 139 00:07:25,680 --> 00:07:29,440 With JWST, it's our only opportunity to get these features 140 00:07:29,440 --> 00:07:31,560 way out in the infrared 141 00:07:31,560 --> 00:07:35,000 which tell us what that cloud is actually composed of... 142 00:07:35,000 --> 00:07:37,720 Yes. ..and in this case, are silicon dioxide. 143 00:07:37,720 --> 00:07:41,920 OK. So, if there were not these clouds made of silicon dioxide 144 00:07:41,920 --> 00:07:45,480 in the atmosphere, we would have measured this yellow line. 145 00:07:45,480 --> 00:07:47,080 OK. 146 00:07:47,080 --> 00:07:49,040 The peak on the grey and pink lines, 147 00:07:49,040 --> 00:07:50,800 compared to the yellow one, 148 00:07:50,800 --> 00:07:55,440 show that light from WASP-17b's local star had been absorbed 149 00:07:55,440 --> 00:07:58,280 by a specific molecule in the atmosphere. 150 00:07:58,280 --> 00:08:02,920 Hannah was expecting it to be magnesium silicate - 151 00:08:02,920 --> 00:08:05,360 particles which make up rocks and sand - 152 00:08:05,360 --> 00:08:07,600 as seen on other exoplanets. 153 00:08:07,600 --> 00:08:09,560 But that's not what they found. 154 00:08:10,920 --> 00:08:12,520 So, what we actually found 155 00:08:12,520 --> 00:08:14,600 was more of that kind of pure quartz form. 156 00:08:14,600 --> 00:08:16,760 And this is what quartz looks like here on the Earth. 157 00:08:16,760 --> 00:08:20,920 So, it's a solid, it's kind of nice and glittery, and it's clear. 158 00:08:20,920 --> 00:08:22,880 When you've got magnesium silicates - 159 00:08:22,880 --> 00:08:24,320 or iron silicates, in this case - 160 00:08:24,320 --> 00:08:25,960 you get more of that amethyst colour. 161 00:08:25,960 --> 00:08:28,520 Yeah, so it's, like, that's a contamination... Exactly. 162 00:08:28,520 --> 00:08:29,800 ..but it leads to that beautiful colour. 163 00:08:29,800 --> 00:08:31,240 What we actually think is happening 164 00:08:31,240 --> 00:08:33,160 is we've got these beautiful quartz crystals 165 00:08:33,160 --> 00:08:35,080 that are being formed high in the atmosphere. 166 00:08:35,080 --> 00:08:38,560 And then, what we found was that these are nanocrystals. 167 00:08:38,560 --> 00:08:40,560 So, they're very, very tiny particles, 168 00:08:40,560 --> 00:08:43,320 about 100 times smaller than the width of a human hair. 169 00:08:43,320 --> 00:08:46,360 And that's what's really interesting, is that tells us 170 00:08:46,360 --> 00:08:48,960 that these are likely the precursors, the first things 171 00:08:48,960 --> 00:08:50,520 that are forming in the atmosphere. 172 00:08:51,840 --> 00:08:56,040 This discovery, along with data from hundreds of other exoplanets 173 00:08:56,040 --> 00:08:58,400 that JWST has now studied, 174 00:08:58,400 --> 00:09:02,080 is revealing some of the very fundamentals of our universe. 175 00:09:03,440 --> 00:09:06,200 These planets operate as these individual little 176 00:09:06,200 --> 00:09:08,120 laboratories for us. Oh, yes. 177 00:09:08,120 --> 00:09:11,000 Because we can't create these conditions on Earth. 178 00:09:11,000 --> 00:09:15,040 This is a high-temperature, low-pressure, 179 00:09:15,040 --> 00:09:17,280 hydrogen-dominated environment. 180 00:09:17,280 --> 00:09:18,880 Ooh - sounds flammable. 181 00:09:18,880 --> 00:09:21,880 It's not fundable, for certain. Yes! 182 00:09:21,880 --> 00:09:25,960 It allows us to really take these, you know, natural test tubes 183 00:09:25,960 --> 00:09:28,400 to try and understand what's going on. 184 00:09:28,400 --> 00:09:32,040 How would this kind of material change under different conditions? 185 00:09:32,040 --> 00:09:35,200 And we've got hundreds of exoplanets to look at, 186 00:09:35,200 --> 00:09:38,200 to be able to see, if we change those conditions, 187 00:09:38,200 --> 00:09:40,680 what happens to our clouds? I see - wow. 188 00:09:40,680 --> 00:09:43,720 So, yeah, it's remote laboratories where you can do these experiments, 189 00:09:43,720 --> 00:09:46,520 and you get the data and can compare. That's powerful. 190 00:09:46,520 --> 00:09:50,080 And that is the beauty of the thousands of exoplanets, 191 00:09:50,080 --> 00:09:52,640 is that we've got enough of them to start to really understand 192 00:09:52,640 --> 00:09:55,920 the nature of chemistry and physics that we think we understand here. 193 00:09:55,920 --> 00:09:57,280 Hannah, thank you so much. 194 00:09:57,280 --> 00:09:59,240 It's been fantastic, as always, 195 00:09:59,240 --> 00:10:01,600 and I look forward to coming back soon. Take care. 196 00:10:03,800 --> 00:10:07,600 I would never have envisaged that these other-worldly atmospheres 197 00:10:07,600 --> 00:10:10,960 would reveal so much, when I worked on the James Webb Space Telescope 198 00:10:10,960 --> 00:10:12,760 over ten years ago. 199 00:10:12,760 --> 00:10:16,760 And these atmospheres are revealing detail that is unexpected - 200 00:10:16,760 --> 00:10:18,600 crystalline structures. 201 00:10:18,600 --> 00:10:21,400 But we're detecting this from an atmosphere that is over 202 00:10:21,400 --> 00:10:23,680 1,000 light years away from us. 203 00:10:23,680 --> 00:10:26,400 This is the stuff that is truly mind-boggling. 204 00:10:28,120 --> 00:10:32,320 While Hannah has been looking at the planets around distant stars, 205 00:10:32,320 --> 00:10:35,000 it's the planets around our own star 206 00:10:35,000 --> 00:10:38,800 that, two years ago, led me to the University of Leicester, 207 00:10:38,800 --> 00:10:42,240 just after some astonishing pictures were hot off the press. 208 00:10:43,880 --> 00:10:45,440 Just a few days ago, 209 00:10:45,440 --> 00:10:47,640 this image of Jupiter was released. 210 00:10:47,640 --> 00:10:49,320 And what I love about this image 211 00:10:49,320 --> 00:10:51,960 is that it shows an old friend in a new light, 212 00:10:51,960 --> 00:10:54,200 with Jupiter's belts and the Great Red Spot 213 00:10:54,200 --> 00:10:56,120 glowing in infrared light. 214 00:10:56,120 --> 00:11:00,360 Since then, JWST has taken a closer look 215 00:11:00,360 --> 00:11:03,200 at all four outer planets in our solar system. 216 00:11:03,200 --> 00:11:04,960 And George is off to find out 217 00:11:04,960 --> 00:11:07,520 what they've revealed. 218 00:11:07,520 --> 00:11:09,000 As an exoplaneteer, 219 00:11:09,000 --> 00:11:13,000 I usually spend my time studying planets orbiting distant stars. 220 00:11:13,000 --> 00:11:15,360 So, it's kind of nice for a change of pace to learn about 221 00:11:15,360 --> 00:11:18,400 what's going on with the planets in our own solar system. 222 00:11:22,600 --> 00:11:25,040 I'm meeting Professor Leigh Fletcher 223 00:11:25,040 --> 00:11:27,480 to find out how the last two years have been for him. 224 00:11:29,160 --> 00:11:30,560 Welcome to Leicester. 225 00:11:30,560 --> 00:11:32,400 Thank you so much. It's so good to be here! 226 00:11:32,400 --> 00:11:34,800 So, first of all, I just want to remind you of what you said 227 00:11:34,800 --> 00:11:36,600 last time we were here. OK, all right. 228 00:11:38,120 --> 00:11:40,160 So, tell us about the other planets. What will we see? 229 00:11:40,160 --> 00:11:43,240 Uranus is coming up in August and September. 230 00:11:43,240 --> 00:11:45,920 Saturn is coming up in October. 231 00:11:45,920 --> 00:11:48,440 And Neptune, we're going to have an opportunity to do that 232 00:11:48,440 --> 00:11:50,640 in 2023 - so about 12 months. 233 00:11:50,640 --> 00:11:53,560 It is a tremendously exciting time. 234 00:11:53,560 --> 00:11:57,120 And it's going to keep us with sleepless nights 235 00:11:57,120 --> 00:12:01,240 and heavy workloads, I think, for at least five or six years. 236 00:12:02,680 --> 00:12:05,720 You said "sleepless nights and heavy workloads" - 237 00:12:05,720 --> 00:12:07,640 has that become a reality? 238 00:12:07,640 --> 00:12:09,800 Gosh, that feels like a lifetime ago as well. 239 00:12:09,800 --> 00:12:12,440 It's been a couple of years now since we filmed that, 240 00:12:12,440 --> 00:12:15,080 and, honestly, all of our dreams came true. 241 00:12:15,080 --> 00:12:17,320 We got all of the data sets that we were planning 242 00:12:17,320 --> 00:12:19,120 when Chris and I spoke... Amazing. 243 00:12:19,120 --> 00:12:22,440 ..and the data sets have confounded us, confused us, 244 00:12:22,440 --> 00:12:23,880 got us excited. 245 00:12:23,880 --> 00:12:25,360 We're going to start with Jupiter. 246 00:12:25,360 --> 00:12:27,840 So, I hear you've had a few surprises - 247 00:12:27,840 --> 00:12:29,040 pleasant ones, though. 248 00:12:29,040 --> 00:12:32,000 Yeah, I think, you know, if you think about the Jovian system, 249 00:12:32,000 --> 00:12:33,720 you might ask the question quite reasonably - 250 00:12:33,720 --> 00:12:35,520 we've been there before, we've sent missions there - 251 00:12:35,520 --> 00:12:37,880 what else can JWST really tell you? 252 00:12:37,880 --> 00:12:41,000 And even I was surprised when we got some of these data back. 253 00:12:41,000 --> 00:12:42,640 So, on the screen behind me 254 00:12:42,640 --> 00:12:46,040 is one of JWST's fantastic images of Jupiter. Mm. 255 00:12:46,040 --> 00:12:48,720 And what we can do is, when you look at Jupiter over several hours, 256 00:12:48,720 --> 00:12:51,160 you can see all the cloud features moving around. 257 00:12:51,160 --> 00:12:53,800 We did it at a different wavelength of light, 258 00:12:53,800 --> 00:12:56,920 and one that you can only really access with JWST. 259 00:12:56,920 --> 00:12:59,920 And, lo and behold, out pops a brand-new jet stream 260 00:12:59,920 --> 00:13:01,720 that's gone hidden from Earth view 261 00:13:01,720 --> 00:13:05,520 for the last four decades of observations of this planet. 262 00:13:05,520 --> 00:13:07,960 And it was just there waiting for us in the data. 263 00:13:07,960 --> 00:13:11,120 So, my colleagues published this last year - and what this is, 264 00:13:11,120 --> 00:13:13,040 is a very powerful stream of air 265 00:13:13,040 --> 00:13:14,920 high above the Jovian equator 266 00:13:14,920 --> 00:13:18,000 that is somehow linked to the atmosphere high above. 267 00:13:18,000 --> 00:13:20,480 And this is something that was completely unexpected 268 00:13:20,480 --> 00:13:22,960 when we first started inspecting these data. 269 00:13:22,960 --> 00:13:25,880 Seems we've learned a lot about Jupiter's system. Mm-hm. 270 00:13:25,880 --> 00:13:28,840 Have we learned anything new and exciting about Saturn so far? 271 00:13:28,840 --> 00:13:30,920 On the screen behind you is the first image 272 00:13:30,920 --> 00:13:32,400 we captured of Saturn. 273 00:13:32,400 --> 00:13:35,240 The atmosphere looks fairly bland there, but the rings 274 00:13:35,240 --> 00:13:38,000 are absolutely resplendent in these data. Stunning. 275 00:13:38,000 --> 00:13:39,720 We saw that the rings are 276 00:13:39,720 --> 00:13:42,440 astonishingly pure, crystalline water ice 277 00:13:42,440 --> 00:13:44,920 with just a tiny, tiny fraction 278 00:13:44,920 --> 00:13:46,920 of things like organics peppering the rings 279 00:13:46,920 --> 00:13:48,760 to give them their glorious colours. 280 00:13:48,760 --> 00:13:50,760 We saw that the atmosphere of Saturn, 281 00:13:50,760 --> 00:13:54,240 which is seasonal, and we had a prediction that 282 00:13:54,240 --> 00:13:58,040 the atmospheric flows on Saturn would shift direction, 283 00:13:58,040 --> 00:14:01,160 and those predictions were borne out quite accurately. 284 00:14:02,680 --> 00:14:05,440 While Jupiter and Saturn are building a more detailed 285 00:14:05,440 --> 00:14:07,320 picture of their systems, 286 00:14:07,320 --> 00:14:10,560 it is the two most distant planets that have Leigh and his colleagues 287 00:14:10,560 --> 00:14:13,120 relooking at their models. 288 00:14:13,120 --> 00:14:17,160 So, now what about our two big enigmas, Uranus and Neptune? 289 00:14:17,160 --> 00:14:18,920 So, you have to remember that 290 00:14:18,920 --> 00:14:21,520 Uranus and Neptune have only had a single fly-by mission, 291 00:14:21,520 --> 00:14:24,480 the venerable Voyager 2, back in the late 1980s. 292 00:14:24,480 --> 00:14:27,040 And since then, we've been observing with ground-based telescopes, 293 00:14:27,040 --> 00:14:28,960 with the Hubble Space Telescope. 294 00:14:28,960 --> 00:14:31,800 And we thought we were starting to generate a decent 295 00:14:31,800 --> 00:14:33,640 understanding of these worlds. 296 00:14:33,640 --> 00:14:38,480 And, unfortunately, when we started to apply our models 297 00:14:38,480 --> 00:14:41,960 based on all that prior knowledge to the new JWST data, 298 00:14:41,960 --> 00:14:44,400 we started to realise something wasn't adding up, 299 00:14:44,400 --> 00:14:45,680 something was missing. 300 00:14:45,680 --> 00:14:49,320 It was like making a cake and having all of the ingredients for the cake, 301 00:14:49,320 --> 00:14:51,960 but then, when you actually taste the cake, there's something just 302 00:14:51,960 --> 00:14:53,240 not quite right in the flavour. 303 00:14:53,240 --> 00:14:56,440 And it's that missing ingredient in our spectral models 304 00:14:56,440 --> 00:14:58,440 that we're trying to pin down at the moment. 305 00:14:58,440 --> 00:15:00,000 But that's exciting, right? 306 00:15:00,000 --> 00:15:03,600 Because it means that we are going to learn something fundamentally new 307 00:15:03,600 --> 00:15:06,400 about the chemical composition of these two worlds that 308 00:15:06,400 --> 00:15:08,480 we didn't expect to be even asking about 309 00:15:08,480 --> 00:15:10,280 when we first launched JWST. 310 00:15:11,960 --> 00:15:15,240 Research continues on Uranus and Neptune, 311 00:15:15,240 --> 00:15:17,160 but this was to be expected. 312 00:15:17,160 --> 00:15:20,200 Leigh did say there was about six years' work to be done, 313 00:15:20,200 --> 00:15:22,520 and we've come back after just two. 314 00:15:22,520 --> 00:15:26,200 But it's still amazes me just how much JWST is changing 315 00:15:26,200 --> 00:15:29,120 our understanding of objects around our own sun. 316 00:15:30,720 --> 00:15:33,160 The solar system is our home planetary system, 317 00:15:33,160 --> 00:15:36,840 and we've been studying it with telescopes for a while now and, 318 00:15:36,840 --> 00:15:39,640 you know, staring at it for thousands of years. 319 00:15:39,640 --> 00:15:43,680 Is it surprising that there's still so much more new stuff 320 00:15:43,680 --> 00:15:45,120 to learn about it? 321 00:15:45,120 --> 00:15:48,720 I think, whenever you have a brand-new capability like JWST, 322 00:15:48,720 --> 00:15:51,560 there's always going to be something, some wavelength of light 323 00:15:51,560 --> 00:15:53,720 that's going to deliver something that surprises you. 324 00:15:53,720 --> 00:15:55,280 And you're absolutely right, 325 00:15:55,280 --> 00:15:57,760 the solar system has been fabulously well studied, 326 00:15:57,760 --> 00:16:00,800 but some of the questions that we're trying to answer now, 327 00:16:00,800 --> 00:16:02,880 like little pieces of a jigsaw puzzle, 328 00:16:02,880 --> 00:16:06,960 they add up to a much greater, much more impactful 329 00:16:06,960 --> 00:16:09,800 and deep understanding of this wonderful solar system 330 00:16:09,800 --> 00:16:11,400 that we're a part of. 331 00:16:11,400 --> 00:16:13,600 Well, thank you so much for having me. 332 00:16:13,600 --> 00:16:16,000 It's been so great chatting to you. Always a pleasure to have you. 333 00:16:16,000 --> 00:16:18,840 Well, look forward to next time. OK. Take care. Bye-bye. 334 00:16:21,680 --> 00:16:24,600 While Maggie and George have been catching up with scientists 335 00:16:24,600 --> 00:16:26,600 we met two years ago, 336 00:16:26,600 --> 00:16:28,840 I've headed to the University of Cambridge's 337 00:16:28,840 --> 00:16:31,240 Kavli Institute of Cosmology, 338 00:16:31,240 --> 00:16:36,080 where a fetching set of 1:1 scale replicas of JWST's mirrors 339 00:16:36,080 --> 00:16:37,200 can be found. 340 00:16:38,600 --> 00:16:41,640 Because light can travel through the universe for millions, 341 00:16:41,640 --> 00:16:43,120 or even billions of years, 342 00:16:43,120 --> 00:16:46,800 our telescopes are time machines, showing us the past. 343 00:16:48,040 --> 00:16:50,240 And, with its 6.5-metre mirror, 344 00:16:50,240 --> 00:16:52,920 JWST is allowing us to peer back further 345 00:16:52,920 --> 00:16:54,680 than we ever have before. 346 00:16:58,520 --> 00:17:00,800 I'm meeting Dr Sandro Tacchella, 347 00:17:00,800 --> 00:17:03,280 who studies these very young galaxies 348 00:17:03,280 --> 00:17:05,440 to find out what has been revealed. 349 00:17:05,440 --> 00:17:06,520 Hey, how are you? 350 00:17:06,520 --> 00:17:09,520 Hi, Chris, good to see you. Nice to see you. Thanks for having us. 351 00:17:09,520 --> 00:17:11,960 You're welcome. Well, I'm excited by this. 352 00:17:11,960 --> 00:17:15,240 What did we know about the early universe before JWST? 353 00:17:15,240 --> 00:17:18,320 What have we learned from all of those years of pointing 354 00:17:18,320 --> 00:17:20,200 at these things with the Hubble Space Telescope? 355 00:17:20,200 --> 00:17:22,680 Yes, so Hubble gave us really already a very good overview of 356 00:17:22,680 --> 00:17:24,120 what happened in the universe 357 00:17:24,120 --> 00:17:26,680 through most of cosmic time, which means that we are, you know, 358 00:17:26,680 --> 00:17:29,680 looking at the universe of the age at about two to three billion years. 359 00:17:29,680 --> 00:17:31,680 That's pretty good. That's pretty good indeed. 360 00:17:31,680 --> 00:17:33,800 But the growth at earlier cosmic time - 361 00:17:33,800 --> 00:17:35,440 so that's in the first billion years - 362 00:17:35,440 --> 00:17:37,880 is actually the most active growth and the most interesting growth, 363 00:17:37,880 --> 00:17:40,120 in that sense, because that's where the very first stars, 364 00:17:40,120 --> 00:17:42,880 the very first black holes and the very first galaxies 365 00:17:42,880 --> 00:17:44,520 started to form and to assemble. 366 00:17:46,600 --> 00:17:48,320 And it's this early universe, 367 00:17:48,320 --> 00:17:51,360 when galaxies and stars were first forming, 368 00:17:51,360 --> 00:17:54,400 that JWST is showing us for the first time. 369 00:17:56,360 --> 00:17:59,240 Scientists around the world are working together to build 370 00:17:59,240 --> 00:18:02,120 a detailed map of the deep cosmos 371 00:18:02,120 --> 00:18:04,320 as part of a project called JADES - 372 00:18:04,320 --> 00:18:08,040 the JWST Advanced Deep Extragalactic Survey. 373 00:18:10,600 --> 00:18:13,520 Well, I think what we should do is take a tour of some of the data. 374 00:18:13,520 --> 00:18:15,760 So, you've got an interactive tool? Sure, yes. 375 00:18:15,760 --> 00:18:17,800 What you see here is a mosaic. 376 00:18:17,800 --> 00:18:21,160 So, these are basically over, you know, 400 images that 377 00:18:21,160 --> 00:18:22,600 we have taken over the last two years 378 00:18:22,600 --> 00:18:24,320 with the James Webb Space Telescope. 379 00:18:24,320 --> 00:18:25,720 And we have put them together. 380 00:18:25,720 --> 00:18:27,480 You know, one of the very interesting structures 381 00:18:27,480 --> 00:18:29,080 is what we term the cosmic rose, 382 00:18:29,080 --> 00:18:30,640 OK, and you might see why. 383 00:18:30,640 --> 00:18:33,120 So, when I zoom in here, you can see that this looks like, 384 00:18:33,120 --> 00:18:34,960 you know, a rose-like structure. 385 00:18:34,960 --> 00:18:37,360 And so, this system is actually very distant, 386 00:18:37,360 --> 00:18:40,360 formed about two billion years after the Big Bang. 387 00:18:40,360 --> 00:18:42,760 And what you see here is not just a single galaxy, 388 00:18:42,760 --> 00:18:45,760 but actually a whole group of galaxies. 389 00:18:45,760 --> 00:18:50,760 But JWST has been able to look back at even younger galaxies. 390 00:18:50,760 --> 00:18:53,600 So, are there other places we should visit in this image? 391 00:18:53,600 --> 00:18:56,000 So, this is one of the deeper patches in the image. 392 00:18:56,000 --> 00:18:58,880 And what I'll show you here is a galaxy, 393 00:18:58,880 --> 00:19:01,680 which seems to be kind of this yellowish colour. Yeah. 394 00:19:01,680 --> 00:19:03,920 And this is basically the most distant galaxy 395 00:19:03,920 --> 00:19:06,000 that is known to us. That splodge there? 396 00:19:06,000 --> 00:19:07,480 Yeah, that splodge here. 397 00:19:07,480 --> 00:19:10,200 So, it's really probing, basically, the earliest structures 398 00:19:10,200 --> 00:19:11,760 we know in the universe. 399 00:19:11,760 --> 00:19:15,600 This is the furthest back in time we've ever seen, 400 00:19:15,600 --> 00:19:19,680 showing us the very earliest moments of our universe's story, 401 00:19:19,680 --> 00:19:23,280 fewer than 300 million years after the Big Bang. 402 00:19:23,280 --> 00:19:25,760 So, when you look at this image, 403 00:19:25,760 --> 00:19:28,320 there are lots of splodges all over the place. 404 00:19:28,320 --> 00:19:30,400 What made you look at that one in particular? 405 00:19:30,400 --> 00:19:33,520 We have been seeing this object already in the very early data 406 00:19:33,520 --> 00:19:35,520 we obtained nearly two years ago. 407 00:19:35,520 --> 00:19:38,960 And I think the surprising thing was that it's actually very bright. 408 00:19:38,960 --> 00:19:41,120 And so, our initial reaction was, 409 00:19:41,120 --> 00:19:44,640 "Well, it cannot be that distant because it's too bright." 410 00:19:44,640 --> 00:19:46,120 And so, we took better data - 411 00:19:46,120 --> 00:19:48,320 in particular, we also took spectroscopy. 412 00:19:48,320 --> 00:19:51,040 And we could clearly see that, no, that galaxy, 413 00:19:51,040 --> 00:19:54,600 this yellow blob here, is really this most distant galaxy 414 00:19:54,600 --> 00:19:56,080 that we have ever seen. 415 00:19:56,080 --> 00:19:57,920 So, if this is the record-holder, 416 00:19:57,920 --> 00:20:00,520 how common are galaxies like this? 417 00:20:00,520 --> 00:20:03,320 Yes, so we don't know at the moment. 418 00:20:03,320 --> 00:20:05,320 Er, it's really... 419 00:20:05,320 --> 00:20:08,160 It's basically far off than whatever we have seen before. 420 00:20:08,160 --> 00:20:10,480 And so, in that sense, this galaxy is very peculiar. 421 00:20:10,480 --> 00:20:13,320 It's really bright. It's a very early cosmic times. 422 00:20:13,320 --> 00:20:15,800 And so, it's a really one-off record-holder at the moment. 423 00:20:15,800 --> 00:20:18,520 But it might be that, because we have been biased in 424 00:20:18,520 --> 00:20:21,320 the way of how we thought about these early galaxies - 425 00:20:21,320 --> 00:20:24,160 we were looking mostly for very young systems, 426 00:20:24,160 --> 00:20:25,760 quite small systems - 427 00:20:25,760 --> 00:20:28,800 we might have seen those galaxies, but we said, like, "Ah, no." 428 00:20:28,800 --> 00:20:32,400 So we have to go back and look more carefully at those. 429 00:20:32,400 --> 00:20:34,400 So, maybe they are more common than we thought. 430 00:20:35,760 --> 00:20:38,800 Finding this particular galaxy may have been a surprise, 431 00:20:38,800 --> 00:20:42,080 but it's just one of many that JWST is detecting 432 00:20:42,080 --> 00:20:45,120 from the very early universe. 433 00:20:45,120 --> 00:20:48,760 And the picture the telescope is giving us is of a young universe 434 00:20:48,760 --> 00:20:50,880 full of galaxies growing quicker, 435 00:20:50,880 --> 00:20:54,240 and forming stars faster, than had been expected. 436 00:20:57,600 --> 00:21:00,160 How much has this early universe surprised you, 437 00:21:00,160 --> 00:21:02,360 like, compared to what you thought you were going to get 438 00:21:02,360 --> 00:21:03,720 a couple of years ago? 439 00:21:03,720 --> 00:21:06,840 It was really, erm, surprising in the sense of 440 00:21:06,840 --> 00:21:10,480 how much excitement it triggered also in the general public. 441 00:21:10,480 --> 00:21:13,120 So, I think, you know, it was beyond just like, you know, 442 00:21:13,120 --> 00:21:15,000 me looking at the screen and being astonished by 443 00:21:15,000 --> 00:21:16,320 these beautiful images. 444 00:21:16,320 --> 00:21:21,080 For me personally, I think I was surprised to see of how much - 445 00:21:21,080 --> 00:21:22,520 how good the telescope works. 446 00:21:22,520 --> 00:21:24,600 It's really works amazingly well. 447 00:21:24,600 --> 00:21:27,000 And, you know, like, the images are beautiful, 448 00:21:27,000 --> 00:21:30,360 but we can take spectra and really learn about these, you know, 449 00:21:30,360 --> 00:21:33,960 systems in really great detail that I didn't expect to, you know... 450 00:21:33,960 --> 00:21:35,480 ..only maybe dream about. 451 00:21:35,480 --> 00:21:38,200 Well, thank you very much. It's fascinating stuff. 452 00:21:38,200 --> 00:21:39,800 Thank you very much, Chris. 453 00:21:39,800 --> 00:21:42,360 While the scientists we've been meeting this month 454 00:21:42,360 --> 00:21:46,760 have their heads down working on the data that JWST is supplying, 455 00:21:46,760 --> 00:21:50,040 Pete is in Bedford, looking up to the skies. 456 00:21:52,600 --> 00:21:56,040 The pictures taken by JWST over the last couple of years 457 00:21:56,040 --> 00:21:58,560 have been nothing short of mind-blowing. 458 00:21:58,560 --> 00:22:01,000 And although we can't get the same level of detail 459 00:22:01,000 --> 00:22:03,480 a million miles away here on Earth, 460 00:22:03,480 --> 00:22:08,480 we can find the objects in those iconic JWST images. 461 00:22:10,400 --> 00:22:14,600 While what we can get from our back gardens may not compare, 462 00:22:14,600 --> 00:22:17,920 the planets are slowly moving out of the sun's glare 463 00:22:17,920 --> 00:22:21,680 and will become spectacular at the end of this month. 464 00:22:21,680 --> 00:22:25,040 In particular, an early-morning view 465 00:22:25,040 --> 00:22:27,800 low over the east-northeast horizon 466 00:22:27,800 --> 00:22:29,320 before sunrise 467 00:22:29,320 --> 00:22:31,240 will reveal bright Jupiter, 468 00:22:31,240 --> 00:22:32,960 brightening Mars, 469 00:22:32,960 --> 00:22:34,920 and binocular-dim Uranus 470 00:22:34,920 --> 00:22:36,440 against the wonderful 471 00:22:36,440 --> 00:22:38,520 stars of Taurus. 472 00:22:38,520 --> 00:22:40,040 At the end of July, 473 00:22:40,040 --> 00:22:41,840 the waning crescent moon moves 474 00:22:41,840 --> 00:22:43,440 through this region too, 475 00:22:43,440 --> 00:22:45,160 presenting a lovely scene 476 00:22:45,160 --> 00:22:47,120 just asking to be photographed. 477 00:22:51,080 --> 00:22:54,600 Saturn is further to the west of this group, 478 00:22:54,600 --> 00:22:58,840 with dim Neptune in tow just to the east of it, 479 00:22:58,840 --> 00:23:02,720 Saturn will be reaching its highest position in the sky 480 00:23:02,720 --> 00:23:06,920 due south under relatively dark conditions during August - 481 00:23:06,920 --> 00:23:10,360 this being the best time to get a steady view of the planet. 482 00:23:12,720 --> 00:23:16,240 One of the most popular images taken by the Hubble Space Telescope 483 00:23:16,240 --> 00:23:18,800 was that of the Pillars of Creation. 484 00:23:18,800 --> 00:23:21,960 JWST took that iconic image 485 00:23:21,960 --> 00:23:23,280 to another level. 486 00:23:24,600 --> 00:23:27,320 While you may not be able to see the Pillars themselves 487 00:23:27,320 --> 00:23:29,240 unless you have a large telescope, 488 00:23:29,240 --> 00:23:32,080 you can see the nebula in which they're located - 489 00:23:32,080 --> 00:23:33,920 that's the Eagle Nebula. 490 00:23:33,920 --> 00:23:36,680 Now, this is best seen in the summer months, 491 00:23:36,680 --> 00:23:40,760 when it's at its highest position above the southern horizon, 492 00:23:40,760 --> 00:23:42,360 under dark conditions. 493 00:23:42,360 --> 00:23:44,720 The Eagle Nebula can be found 494 00:23:44,720 --> 00:23:47,160 by first identifying Altair, 495 00:23:47,160 --> 00:23:48,840 the southernmost star 496 00:23:48,840 --> 00:23:51,240 in the Summer Triangle asterism. 497 00:23:51,240 --> 00:23:55,200 This is the brightest star in Aquila - the Eagle. 498 00:23:55,200 --> 00:24:00,040 Locate Delta Aquilae in the centre below and right of Altair. 499 00:24:00,040 --> 00:24:02,120 Extend the line from Altair 500 00:24:02,120 --> 00:24:04,480 through Delta for three times 501 00:24:04,480 --> 00:24:06,400 that distance again, 502 00:24:06,400 --> 00:24:09,880 passing through the diamond-shaped constellation of Scutum - 503 00:24:09,880 --> 00:24:12,120 the Shield - as you go, 504 00:24:12,120 --> 00:24:15,280 after which you will find the Eagle Nebula - 505 00:24:15,280 --> 00:24:16,720 known as M16. 506 00:24:18,080 --> 00:24:21,120 Through small and medium-sized telescopes, 507 00:24:21,120 --> 00:24:24,600 the Eagle Nebula appears as a cluster of stars, 508 00:24:24,600 --> 00:24:28,040 the faint nebula gas being hard to see. 509 00:24:28,040 --> 00:24:30,960 Long-exposure photography or a large scope 510 00:24:30,960 --> 00:24:33,680 are needed to reveal it properly. 511 00:24:33,680 --> 00:24:35,680 While you're in the region, 512 00:24:35,680 --> 00:24:38,440 look slightly south of the Eagle Nebula 513 00:24:38,440 --> 00:24:41,760 to see the Swan Nebula - M17. 514 00:24:41,760 --> 00:24:44,280 This is much easier to see. 515 00:24:44,280 --> 00:24:47,640 It's wonderful to think that with amateur telescopes 516 00:24:47,640 --> 00:24:49,600 or even just your eyes, 517 00:24:49,600 --> 00:24:51,400 you can see the same objects 518 00:24:51,400 --> 00:24:54,520 as the most powerful telescope sent into space. 519 00:24:54,520 --> 00:24:57,880 Sure, we can't see the same level of detail, 520 00:24:57,880 --> 00:25:00,200 but it's nice to be reminded that, 521 00:25:00,200 --> 00:25:03,960 as we send telescopes deeper and deeper into space, 522 00:25:03,960 --> 00:25:06,840 we're all looking at the same universe. 523 00:25:06,840 --> 00:25:08,960 As ever, if you get some images, 524 00:25:08,960 --> 00:25:11,800 do share them on The Sky At Night Flickr, 525 00:25:11,800 --> 00:25:13,560 and we'll pick some of our favourites 526 00:25:13,560 --> 00:25:15,520 and show them next month. 527 00:25:15,520 --> 00:25:17,880 Further details can be found at... 528 00:25:21,280 --> 00:25:24,960 In the meantime, here are some of our favourites from last month. 529 00:25:51,320 --> 00:25:54,560 JWST can do so much with a single image. 530 00:25:54,560 --> 00:25:57,600 It can astound, amaze and surprise us. 531 00:25:57,600 --> 00:25:59,360 And so we thought, before we go, 532 00:25:59,360 --> 00:26:01,840 we'd show you a few of our favourite images. 533 00:26:01,840 --> 00:26:03,600 This is mine. 534 00:26:03,600 --> 00:26:06,200 It's the Cigar Galaxy - M82. 535 00:26:06,200 --> 00:26:10,760 What you can see is a powerful wind sweeping away from the galaxy, 536 00:26:10,760 --> 00:26:12,000 driven by the star formation 537 00:26:12,000 --> 00:26:14,200 that's happening at the galaxy's heart. 538 00:26:14,200 --> 00:26:16,800 This is my favourite JWST image. 539 00:26:16,800 --> 00:26:18,680 It shows you the Goods-North region. 540 00:26:18,680 --> 00:26:22,440 It has been imaged with JWST in nine different filters, 541 00:26:22,440 --> 00:26:26,040 and what you can see here are about 50,000 different galaxies. 542 00:26:26,040 --> 00:26:28,880 But there is one particular galaxy that is highlighted. 543 00:26:28,880 --> 00:26:30,280 This is GN-z11, 544 00:26:30,280 --> 00:26:33,520 this is the most distant galaxy with a known black hole. 545 00:26:33,520 --> 00:26:37,640 So, this is my favourite JWST picture. 546 00:26:37,640 --> 00:26:40,000 It is actually a spectrum 547 00:26:40,000 --> 00:26:43,640 which includes the JWST information 548 00:26:43,640 --> 00:26:47,600 from the clouds in the atmosphere of WASP-17b, 549 00:26:47,600 --> 00:26:50,000 and the information that we had previously from 550 00:26:50,000 --> 00:26:52,440 the Hubble Space Telescope. 551 00:26:52,440 --> 00:26:56,160 So, this is my favourite JWST image. 552 00:26:56,160 --> 00:26:57,600 And it is, believe it or not, 553 00:26:57,600 --> 00:26:59,800 the Horsehead Nebula. 554 00:26:59,800 --> 00:27:03,240 It's looking over the very top of the horse's head, 555 00:27:03,240 --> 00:27:05,920 which has been an object very iconic to me, 556 00:27:05,920 --> 00:27:08,040 as I've been growing up with astronomy. 557 00:27:08,040 --> 00:27:10,800 So, this image is blowing my mind because, 558 00:27:10,800 --> 00:27:14,280 as JWST is looking over the top of the Horsehead into deep space, 559 00:27:14,280 --> 00:27:15,720 what can it see? 560 00:27:15,720 --> 00:27:17,080 Galaxies. 561 00:27:17,080 --> 00:27:19,280 It's an incredible image. 562 00:27:19,280 --> 00:27:20,760 This is my favourite picture. 563 00:27:20,760 --> 00:27:23,920 This is an image of HIP 6546 b. 564 00:27:23,920 --> 00:27:26,960 Now, actual images of exoplanets are a rarity, 565 00:27:26,960 --> 00:27:29,320 because direct imaging is so hard. 566 00:27:29,320 --> 00:27:32,800 But this was JWST's first attempt at direct imaging - 567 00:27:32,800 --> 00:27:35,520 and we got this stunning picture in four different colours, 568 00:27:35,520 --> 00:27:37,360 which is marvellous. 569 00:27:37,360 --> 00:27:41,120 So, I think my favourite image from JWST so far has been 570 00:27:41,120 --> 00:27:42,960 this image of the ice giant Uranus. 571 00:27:42,960 --> 00:27:46,200 I was so looking forward to seeing what Uranus and Neptune would 572 00:27:46,200 --> 00:27:48,360 look like through this fabulous new facility. 573 00:27:48,360 --> 00:27:50,000 So, when these images came out, 574 00:27:50,000 --> 00:27:51,720 I almost had tears in my eyes. 575 00:27:51,720 --> 00:27:54,960 This is a destination that humanity now needs to send 576 00:27:54,960 --> 00:27:57,000 its next robotic explorer to. 577 00:27:57,000 --> 00:28:00,360 And here, James Webb has captured it in all of its glory. 578 00:28:00,360 --> 00:28:03,800 One of my favourite pictures taken by Webb so far is this one, 579 00:28:03,800 --> 00:28:06,240 and it's because of a few different aspects. 580 00:28:06,240 --> 00:28:08,920 Firstly, I love the beautiful images, 581 00:28:08,920 --> 00:28:10,480 but this is raw data. 582 00:28:10,480 --> 00:28:12,320 Secondly, it was taken by NIRSpec, 583 00:28:12,320 --> 00:28:14,400 which is one of the instruments that I worked on. 584 00:28:14,400 --> 00:28:17,560 And thirdly, this is showing one of the earliest galaxies 585 00:28:17,560 --> 00:28:19,760 that ever existed in the universe. 586 00:28:19,760 --> 00:28:22,800 The fact that we can build an instrument that goes up in space 587 00:28:22,800 --> 00:28:24,840 and tells us this level of detail 588 00:28:24,840 --> 00:28:27,400 is still quite mind-boggling to me. 589 00:28:27,400 --> 00:28:30,920 If this is what JWST has achieved in just two years, 590 00:28:30,920 --> 00:28:35,200 its potential over the next 10, or even 20, must be enormous. 591 00:28:35,200 --> 00:28:38,040 I can't wait to find out what it's going to tell us. 592 00:28:38,040 --> 00:28:41,080 In the meantime, we're filming our annual Question Time show 593 00:28:41,080 --> 00:28:42,240 in a few months. 594 00:28:42,240 --> 00:28:45,160 So, if you have a question for this year's expert panel, 595 00:28:45,160 --> 00:28:48,680 go to our website right now to find out how to submit it. 596 00:28:48,680 --> 00:28:51,360 Until next time, goodnight. 47067

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