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These are the user uploaded subtitles that are being translated: 1 00:00:02,640 --> 00:00:04,640 The Sky At Night is back, 2 00:00:04,640 --> 00:00:07,880 bringing you the latest in all things astronomical. 3 00:00:07,880 --> 00:00:10,800 There's been a lot going on since our last episode, 4 00:00:10,800 --> 00:00:14,160 and one particular object caught our eye. 5 00:00:14,160 --> 00:00:17,480 The biggest story to hit the news since we've been off air 6 00:00:17,480 --> 00:00:21,680 was about an asteroid called 2024 YR4. 7 00:00:21,680 --> 00:00:23,320 The City Killer, 8 00:00:23,320 --> 00:00:27,360 an asteroid that had the potential of hitting Earth in 2032. 9 00:00:27,360 --> 00:00:29,240 The headlines were everywhere. 10 00:00:29,240 --> 00:00:31,760 BBC NEWS THEME 11 00:00:31,760 --> 00:00:36,360 Now, an asteroid spotted late last year is now being carefully tracked. 12 00:00:36,360 --> 00:00:39,080 Scientists are trying to work out whether there's a chance of it 13 00:00:39,080 --> 00:00:40,480 hitting the Earth. 14 00:00:40,480 --> 00:00:43,320 {\an8}Astronomers estimate that the space rock is roughly 15 00:00:43,320 --> 00:00:45,040 {\an8}the size of a football field. 16 00:00:45,040 --> 00:00:49,760 Suddenly, the night sky wasn't a place of comfort. 17 00:00:49,760 --> 00:00:51,240 With that asteroid out there 18 00:00:51,240 --> 00:00:53,360 and its potential to change life as we know it, 19 00:00:53,360 --> 00:00:56,400 looking up at the night sky wasn't a place of quiet contemplation, 20 00:00:56,400 --> 00:00:58,240 but a place to fear. 21 00:00:58,240 --> 00:01:01,080 So the level of damage that an asteroid the same size 22 00:01:01,080 --> 00:01:02,600 as 2024 YR4 could cause, 23 00:01:02,600 --> 00:01:04,480 it really depends on where it hits. 24 00:01:04,480 --> 00:01:06,920 We're probably talking about the destruction of a city, 25 00:01:06,920 --> 00:01:09,080 were it to hit the land. 26 00:01:09,080 --> 00:01:12,040 Something you really don't want landing on top of you. 27 00:01:12,040 --> 00:01:15,960 Not enough to wipe out dinosaurs or cause a global shift in climate, 28 00:01:15,960 --> 00:01:18,720 but big enough that you want to avoid it, for sure. 29 00:01:18,720 --> 00:01:21,120 But what lies behind the headlines? 30 00:01:21,120 --> 00:01:23,760 And are we prepared for an asteroid strike? 31 00:01:23,760 --> 00:01:26,720 Welcome to The Sky At Night. 32 00:01:56,200 --> 00:01:58,200 On a beautiful day like today, 33 00:01:58,200 --> 00:02:00,920 it's easy to forget that beyond that gorgeous sky, 34 00:02:00,920 --> 00:02:03,600 there could be legitimate threats heading our way. 35 00:02:03,600 --> 00:02:05,800 I'm not talking about aliens. 36 00:02:05,800 --> 00:02:07,600 Obviously, I'm talking about asteroids. 37 00:02:07,600 --> 00:02:10,640 Now we actually get hit by asteroids every single day. 38 00:02:10,640 --> 00:02:13,080 In fact, in any given 24-hour period, 39 00:02:13,080 --> 00:02:17,600 we might get hit by roughly 73 Earthling cows' worth of material. 40 00:02:17,600 --> 00:02:20,040 So why aren't we fussed about this? 41 00:02:20,040 --> 00:02:22,320 Well, the scale of this material is such 42 00:02:22,320 --> 00:02:25,120 that it's like a sprinkling of dust, mostly just burning up in 43 00:02:25,120 --> 00:02:27,960 the atmosphere and not even reaching the ground. 44 00:02:27,960 --> 00:02:30,240 Bigger things do hit us too. 45 00:02:30,240 --> 00:02:33,320 The asteroid that wiped out the dinosaurs a while back 46 00:02:33,320 --> 00:02:35,280 was tens of kilometres across, 47 00:02:35,280 --> 00:02:37,800 and something that size is expected to hit us 48 00:02:37,800 --> 00:02:40,960 roughly every 100 million years. 49 00:02:40,960 --> 00:02:43,120 But between these extremes, 50 00:02:43,120 --> 00:02:46,400 mass extinction event, rather nice light show, 51 00:02:46,400 --> 00:02:48,360 you have your midsize asteroids. 52 00:02:48,360 --> 00:02:50,840 Now your midsize asteroid 53 00:02:50,840 --> 00:02:55,120 could cause a heat blast capable of vaporising solid rock. 54 00:02:55,120 --> 00:02:56,880 We're talking wind speeds 55 00:02:56,880 --> 00:02:59,440 five times the strongest hurricanes. 56 00:02:59,440 --> 00:03:01,440 We're talking a shock wave 57 00:03:01,440 --> 00:03:05,040 that could flatten buildings for hundreds of miles. 58 00:03:05,040 --> 00:03:09,280 That would mean a city the size of London and the surrounding areas, 59 00:03:09,280 --> 00:03:12,560 maybe even as far as Kent, gone. 60 00:03:12,560 --> 00:03:14,680 Now, at the start of this year, 61 00:03:14,680 --> 00:03:18,200 we thought there was just such an asteroid coming our way 62 00:03:18,200 --> 00:03:21,280 when Asteroid 2024 YR4 was spotted. 63 00:03:21,280 --> 00:03:25,400 Now, at the time, it was still over 30 million miles away, 64 00:03:25,400 --> 00:03:29,640 but it looked like it was on course to collide with us in 2032. 65 00:03:29,640 --> 00:03:32,200 It has since been downgraded, 66 00:03:32,200 --> 00:03:35,520 and we're now pretty confident it's actually going to be a near miss. 67 00:03:35,520 --> 00:03:39,720 However, what it did provide is a practice run, like a fire drill, 68 00:03:39,720 --> 00:03:42,400 or even an asteroid drill, if you will, 69 00:03:42,400 --> 00:03:46,120 so that when the real threat does come along, we know what to do. 70 00:03:50,880 --> 00:03:52,800 When YR4 was discovered, 71 00:03:52,800 --> 00:03:55,960 it was no more than a dot moving amongst the background stars. 72 00:03:55,960 --> 00:03:57,640 And even once it had been found, 73 00:03:57,640 --> 00:04:00,520 it was just one of a million asteroids in our books. 74 00:04:00,520 --> 00:04:02,400 So what was special about this one? 75 00:04:04,960 --> 00:04:08,000 To explain, I've come to a football pitch, obviously, 76 00:04:08,000 --> 00:04:09,760 where I'm meeting my old friend, 77 00:04:09,760 --> 00:04:12,600 planetary scientist, Dr Meg Schwamb. 78 00:04:12,600 --> 00:04:15,200 - Hey! - Hey! we've talked about football a lot, 79 00:04:15,200 --> 00:04:16,920 so I thought you were the perfect person 80 00:04:16,920 --> 00:04:19,520 to bring here and talk about YR4. 81 00:04:19,520 --> 00:04:22,560 When we were watching the odds of it hitting the Earth go up, 82 00:04:22,560 --> 00:04:24,320 I did think of it like watching 83 00:04:24,320 --> 00:04:26,680 a striker's shot head towards the goal. 84 00:04:26,680 --> 00:04:28,880 Yeah, definitely, exactly that playing out, right? 85 00:04:28,880 --> 00:04:30,440 I think as the world, 86 00:04:30,440 --> 00:04:32,760 {\an8}but also astronomers sitting there watching, right, 87 00:04:32,760 --> 00:04:34,640 {\an8}waiting to see as they got more data, 88 00:04:34,640 --> 00:04:36,480 {\an8}as you get closer to that goal, right, 89 00:04:36,480 --> 00:04:38,760 {\an8}of whether it's going to go in or in this case, 90 00:04:38,760 --> 00:04:40,360 we really want it to miss. 91 00:04:40,360 --> 00:04:41,680 Yes, that's the unusual bit. 92 00:04:41,680 --> 00:04:43,560 But let's go back to the beginning. 93 00:04:43,560 --> 00:04:48,160 2024 YR4's an asteroid. But what are asteroids? 94 00:04:48,160 --> 00:04:50,760 Asteroids are the debris left over after planet formation. 95 00:04:50,760 --> 00:04:52,760 Most are between Mars and Jupiter. 96 00:04:52,760 --> 00:04:55,440 Some get disturbed in their orbits and get sent inward. 97 00:04:55,440 --> 00:04:58,480 That potentially can be an orbit that will cross the Earth. 98 00:05:01,360 --> 00:05:03,640 On the 27th of December 2024, 99 00:05:03,640 --> 00:05:07,520 YR4 was first spotted by a telescope in Chile, 100 00:05:07,520 --> 00:05:10,200 as nothing more than a faint point of light. 101 00:05:10,200 --> 00:05:13,160 It soon gathered a lot of attention, 102 00:05:13,160 --> 00:05:17,120 as calculations showed it had around a 1% chance of hitting Earth. 103 00:05:17,120 --> 00:05:18,720 So in January, 104 00:05:18,720 --> 00:05:21,000 other astronomers jumped on this and started trying to observe it. 105 00:05:21,000 --> 00:05:22,360 Everybody was jumping on it. 106 00:05:22,360 --> 00:05:24,440 Amateur astronomers, anyone with a telescope 107 00:05:24,440 --> 00:05:26,040 that had time was jumping on this 108 00:05:26,040 --> 00:05:28,760 because very few objects have jumped above that 1%. 109 00:05:28,760 --> 00:05:30,320 And when it hits that level for the size 110 00:05:30,320 --> 00:05:31,960 that we thought this object might be, 111 00:05:31,960 --> 00:05:33,800 which is about 30m to 90m, 112 00:05:33,800 --> 00:05:34,920 that's when we start worrying, 113 00:05:34,920 --> 00:05:37,760 because that's where you could do damage on a city scale. 114 00:05:37,760 --> 00:05:40,840 What happened to the odds of YR4 hitting us? 115 00:05:40,840 --> 00:05:43,360 It went up and it went up a lot. 116 00:05:43,360 --> 00:05:45,840 It went from about 1.2% to 2.8 117 00:05:45,840 --> 00:05:47,560 or over 3% roughly. 118 00:05:47,560 --> 00:05:49,480 And so that might feel really scary, right? 119 00:05:49,480 --> 00:05:52,520 So it IS interesting, I think, the fact that we went from 120 00:05:52,520 --> 00:05:54,720 a low probability and then it rose before dropping off. 121 00:05:54,720 --> 00:05:56,840 I think it's easy to get the impression 122 00:05:56,840 --> 00:05:59,320 that somebody made an error, but that's not what happened. 123 00:05:59,320 --> 00:06:03,400 No. It's really trying to understand where right in space 124 00:06:03,400 --> 00:06:05,680 the Earth is compared to where we think 125 00:06:05,680 --> 00:06:08,680 all the possible orbits that this object could have. 126 00:06:08,680 --> 00:06:11,280 Well, I really think we can explain this with football, 127 00:06:11,280 --> 00:06:13,200 but I decided neither you nor I should kick a ball. 128 00:06:13,200 --> 00:06:14,480 Definitely not. 129 00:06:14,480 --> 00:06:15,880 I've got some students here. 130 00:06:15,880 --> 00:06:17,600 Gabe! Gabe! Come here. 131 00:06:18,880 --> 00:06:20,920 I feel like we're bringing on a substitute. 132 00:06:20,920 --> 00:06:23,280 Someone much better skilled! 133 00:06:23,280 --> 00:06:26,240 So if we get Gabe to kick the ball towards the goal. 134 00:06:26,240 --> 00:06:29,960 At first, we don't have much information about where it's going, 135 00:06:29,960 --> 00:06:31,760 whether it's going in or not. 136 00:06:31,760 --> 00:06:34,920 Tracking the asteroid after it was first spotted is like freezing 137 00:06:34,920 --> 00:06:36,640 the ball just after Gabe kicks it. 138 00:06:38,120 --> 00:06:39,840 It might go in the goal, 139 00:06:39,840 --> 00:06:42,440 but the goal makes up just one small part of the area 140 00:06:42,440 --> 00:06:44,840 the ball could end up in. 141 00:06:44,840 --> 00:06:49,160 For YR4, the odds of hitting Earth were 1%. 142 00:06:49,160 --> 00:06:51,480 No, we've got an initial idea of position, right? 143 00:06:51,480 --> 00:06:54,320 Right when it's kicked, we have an idea of the velocity, 144 00:06:54,320 --> 00:06:56,120 but it can go any direction. 145 00:06:56,120 --> 00:06:58,640 But a little bit later on we've got more information 146 00:06:58,640 --> 00:07:00,840 - as the ball heads towards the goal. - Right. 147 00:07:00,840 --> 00:07:03,400 Because if you could just stop the ball for a second in midair, 148 00:07:03,400 --> 00:07:05,880 you now can see more of where it's headed. 149 00:07:05,880 --> 00:07:07,960 You have extra information, another data point, right? 150 00:07:07,960 --> 00:07:10,600 You have another position, another possible velocity. 151 00:07:12,240 --> 00:07:14,800 This additional data narrows the ellipse, 152 00:07:14,800 --> 00:07:17,880 removing much of the area outside the goal. 153 00:07:17,880 --> 00:07:20,920 The goal now takes up more of the remaining ellipse, 154 00:07:20,920 --> 00:07:23,240 and so the odds of a hit go up. 155 00:07:23,240 --> 00:07:25,640 Things are getting exciting. 156 00:07:25,640 --> 00:07:27,960 For YR4, it was over 3%. 157 00:07:29,400 --> 00:07:30,920 And that's what happened here. 158 00:07:30,920 --> 00:07:32,720 We ruled out parts of space 159 00:07:32,720 --> 00:07:36,680 where the Earth wasn't, and so the probability of impact went up. 160 00:07:36,680 --> 00:07:39,320 And then if we let the shot play out... 161 00:07:40,480 --> 00:07:43,560 ..the third freeze frame shows the ellipses reduce down again. 162 00:07:43,560 --> 00:07:46,160 We're now sure the ball will miss the goal... 163 00:07:46,160 --> 00:07:47,360 Bad luck, Gabe! 164 00:07:47,360 --> 00:07:50,680 ..and YR4 will miss the Earth. 165 00:07:50,680 --> 00:07:53,920 And it was observations from one of the most advanced telescopes 166 00:07:53,920 --> 00:07:57,920 on Earth that told us that this asteroid...would not score. 167 00:07:59,040 --> 00:08:01,600 And so we have the additional data 168 00:08:01,600 --> 00:08:03,920 from the Very Large Telescope helped, 169 00:08:03,920 --> 00:08:06,080 because that helped with all the other observations 170 00:08:06,080 --> 00:08:08,000 to give us enough of the trajectory 171 00:08:08,000 --> 00:08:10,080 to show it's going to come close, 172 00:08:10,080 --> 00:08:12,920 but it's just going to eke away and not hit the goal. 173 00:08:12,920 --> 00:08:15,680 But it's still close, it's not like it missed by miles. 174 00:08:15,680 --> 00:08:17,360 No, and there's even a small chance 175 00:08:17,360 --> 00:08:19,200 this object could still hit the moon. 176 00:08:19,200 --> 00:08:21,200 That'd be pretty spectacular, wouldn't it? 177 00:08:21,200 --> 00:08:22,960 Yes, but not threaten the Earth in any way? 178 00:08:22,960 --> 00:08:24,320 - No. - It would just be a good show. 179 00:08:24,320 --> 00:08:26,560 If we even see it, it might be the far side of the moon 180 00:08:26,560 --> 00:08:27,800 and we see nothing. 181 00:08:27,800 --> 00:08:29,080 I promised I'd say, by the way, 182 00:08:29,080 --> 00:08:30,960 that Gabe missed that on purpose for us. 183 00:08:30,960 --> 00:08:32,480 But I think the demo really works, 184 00:08:32,480 --> 00:08:35,400 - and it's good to know that YR4, too, is missing. - Yeah. 185 00:08:35,400 --> 00:08:37,480 But the threat is still there. 186 00:08:37,480 --> 00:08:39,640 There's many other objects of the size 187 00:08:39,640 --> 00:08:42,280 that can do damage to cities that we still don't know about. 188 00:08:42,280 --> 00:08:45,480 But the nice thing is there are telescopes searching 189 00:08:45,480 --> 00:08:47,640 the skies nightly to try to find these objects. 190 00:08:49,000 --> 00:08:51,720 - I enjoyed that. - Good. It's a bit like Ted Lasso. 191 00:08:51,720 --> 00:08:54,080 We brought in an American to explain football to us! 192 00:08:54,080 --> 00:08:55,360 MEG LAUGHS 193 00:08:58,240 --> 00:09:01,120 While multiple observations allowed us to confidently predict 194 00:09:01,120 --> 00:09:03,200 a miss for YR4, 195 00:09:03,200 --> 00:09:05,640 one day, there WILL be a direct hit. 196 00:09:07,680 --> 00:09:11,920 So what can we do if we know an asteroid strike is imminent? 197 00:09:11,920 --> 00:09:14,640 Maggie's taking a tea break to explain. 198 00:09:14,640 --> 00:09:17,760 Hollywood movies are full of ideas 199 00:09:17,760 --> 00:09:20,320 of how we might handle an asteroid strike. 200 00:09:20,320 --> 00:09:22,160 But in the world of reality, 201 00:09:22,160 --> 00:09:24,520 what tools do we have in our toolkit? 202 00:09:24,520 --> 00:09:27,640 Well, to understand this, I'm going to use this 203 00:09:27,640 --> 00:09:30,440 as the asteroid and this as planet Earth. 204 00:09:30,440 --> 00:09:32,240 Now the challenge is the asteroid 205 00:09:32,240 --> 00:09:34,000 is heading straight towards the Earth. 206 00:09:34,000 --> 00:09:35,920 So what can we do to deflect it? 207 00:09:35,920 --> 00:09:38,480 Well, there's a number of different techniques out there. 208 00:09:38,480 --> 00:09:41,160 And the first one is the nudge method. 209 00:09:41,160 --> 00:09:43,280 So... Oh, sorry, they're good. 210 00:09:43,280 --> 00:09:45,560 The first one is where you want to use 211 00:09:45,560 --> 00:09:47,600 a projectile to hit the asteroid. 212 00:09:47,600 --> 00:09:50,800 When this happens, we'll transfer some momentum to the asteroid. 213 00:09:50,800 --> 00:09:52,560 And it will be deflected 214 00:09:52,560 --> 00:09:54,600 and hopefully, won't hit planet Earth. 215 00:09:57,080 --> 00:09:59,120 And the great thing about this method 216 00:09:59,120 --> 00:10:01,720 is that it's already been tested. 217 00:10:01,720 --> 00:10:06,440 In 2022, the DART mission flew into an asteroid, Dimorphos, 218 00:10:06,440 --> 00:10:10,080 changing its orbit significantly. 219 00:10:10,080 --> 00:10:12,080 But there are a few problems with this. 220 00:10:12,080 --> 00:10:14,640 Firstly, how much of a nudge do we need? 221 00:10:14,640 --> 00:10:17,560 If we don't nudge far enough, we'll still get an impact. 222 00:10:17,560 --> 00:10:20,280 And if we nudge too far, for smaller asteroids, 223 00:10:20,280 --> 00:10:22,320 they might crumble and break up into many pieces. 224 00:10:22,320 --> 00:10:23,360 Not good. 225 00:10:23,360 --> 00:10:27,240 The second technique I want to talk about involves this. 226 00:10:27,240 --> 00:10:30,560 Yeah, it's a tractor, but it's a gravity tractor. 227 00:10:30,560 --> 00:10:33,640 So this will actually be a spaceship which will fly 228 00:10:33,640 --> 00:10:35,200 alongside the asteroid. 229 00:10:35,200 --> 00:10:39,440 Its gravitational force will pull the asteroid towards it. 230 00:10:39,440 --> 00:10:41,960 This will again cause a deflection. 231 00:10:41,960 --> 00:10:44,960 The gravitational tractor technique is quite desirable 232 00:10:44,960 --> 00:10:47,760 because we don't actually impact the asteroid at all. 233 00:10:47,760 --> 00:10:49,680 It just sits alongside it 234 00:10:49,680 --> 00:10:51,760 and uses that gravitational force to deflect it. 235 00:10:51,760 --> 00:10:53,240 But the problem is, 236 00:10:53,240 --> 00:10:55,640 we can't put anything too massive in space. 237 00:10:55,640 --> 00:10:57,520 And so as it's causing the deflection, 238 00:10:57,520 --> 00:10:59,560 it needs to do that for quite some time 239 00:10:59,560 --> 00:11:02,640 to make sure that the asteroid will miss planet Earth. 240 00:11:02,640 --> 00:11:06,600 Now our last technique is usually what Hollywood go for. 241 00:11:06,600 --> 00:11:09,320 And it involves using a nuclear bomb. 242 00:11:09,320 --> 00:11:12,040 Now, if the asteroid is quite close to Earth and we don't 243 00:11:12,040 --> 00:11:15,880 have much time, using something like DART to move the asteroid away 244 00:11:15,880 --> 00:11:19,200 might not be enough. And that's where the nuke comes in. 245 00:11:19,200 --> 00:11:22,560 We can embed the nuke into the asteroid and then blow it up. 246 00:11:23,880 --> 00:11:26,160 We crush up the asteroid. 247 00:11:26,160 --> 00:11:27,800 SHE LAUGHS 248 00:11:27,800 --> 00:11:29,320 I'm making a bit of a mess! 249 00:11:29,320 --> 00:11:31,320 But we need to be careful with this technique, 250 00:11:31,320 --> 00:11:33,640 because now, instead of just one lump heading towards Earth, 251 00:11:33,640 --> 00:11:36,040 we have multiple lumps heading towards Earth, 252 00:11:36,040 --> 00:11:38,400 which means they'll have a greater impact area, 253 00:11:38,400 --> 00:11:40,360 potentially affecting many more people. 254 00:11:40,360 --> 00:11:43,840 Now, to understand which of these tools we can use 255 00:11:43,840 --> 00:11:46,560 for an asteroid strike, we need to get a better understanding 256 00:11:46,560 --> 00:11:49,320 of the asteroid. One I prepared earlier! 257 00:11:49,320 --> 00:11:52,400 And it's almost as if we need an eye in the sky. 258 00:11:52,400 --> 00:11:55,240 Cue the James Webb Space Telescope. 259 00:11:59,480 --> 00:12:01,800 When ground-based telescopes look up at space, 260 00:12:01,800 --> 00:12:04,200 they have the atmosphere to contend with. 261 00:12:04,200 --> 00:12:07,680 This means that images get blurred and measurements get distorted. 262 00:12:10,280 --> 00:12:12,280 But JWST gets around this. 263 00:12:12,280 --> 00:12:15,400 By sitting a million miles above the atmosphere, 264 00:12:15,400 --> 00:12:18,160 its highly specialised mirrors can capture even 265 00:12:18,160 --> 00:12:20,520 the faintest amounts of infrared light, 266 00:12:20,520 --> 00:12:23,280 allowing for incredible accuracy. 267 00:12:24,640 --> 00:12:28,280 It's further helped by an extreme cooling system. 268 00:12:28,280 --> 00:12:32,720 The spectrograph on board JWST is cooled to just seven degrees 269 00:12:32,720 --> 00:12:36,160 above absolute zero. All of this allows JWST 270 00:12:36,160 --> 00:12:39,880 to completely zone in on an object with minimal interference, 271 00:12:39,880 --> 00:12:43,840 which means astronomers can measure the sizes of incoming asteroids 272 00:12:43,840 --> 00:12:48,120 to a level of precision just not feasible from the ground. 273 00:12:50,280 --> 00:12:54,320 And in March, observations from JWST revealed why R4 274 00:12:54,320 --> 00:12:56,720 was about 60 metres across. 275 00:12:56,720 --> 00:13:00,400 A detail no ground-based telescope was able to supply. 276 00:13:02,280 --> 00:13:04,800 This key information will be invaluable 277 00:13:04,800 --> 00:13:08,080 for any future asteroid strikes. 278 00:13:08,080 --> 00:13:12,080 So, we know something's coming and we know what size. 279 00:13:12,080 --> 00:13:15,880 But another thing we might want to know is, what's it made of? 280 00:13:15,880 --> 00:13:19,760 Three, two, one, lift-off! 281 00:13:19,760 --> 00:13:23,440 Luckily, there is one mission that can provide some answers. 282 00:13:23,440 --> 00:13:25,360 Atlas V takes flight. 283 00:13:25,360 --> 00:13:29,200 Sending Lucy to uncover the fossils of our solar system. 284 00:13:29,200 --> 00:13:31,760 Launched in 2021, 285 00:13:31,760 --> 00:13:34,640 the Lucy mission is on a journey to explore 286 00:13:34,640 --> 00:13:37,880 a record breaking number of asteroids in our solar system. 287 00:13:39,280 --> 00:13:41,560 With 11 asteroids to explore, 288 00:13:41,560 --> 00:13:43,920 the Lucy mission is on course to provide us with 289 00:13:43,920 --> 00:13:47,480 a whole new understanding of the smorgasbord of asteroid types 290 00:13:47,480 --> 00:13:50,000 that could be headed our way. 291 00:13:52,120 --> 00:13:54,560 I'm meeting Dr Carly Howett, 292 00:13:54,560 --> 00:13:57,800 who has worked on the mission from the very beginning. 293 00:13:57,800 --> 00:14:00,240 - Let's talk about Lucy! - Let's. 294 00:14:00,240 --> 00:14:03,520 Now, obviously when we think about asteroids, we think asteroid belt. 295 00:14:03,520 --> 00:14:06,200 But that's not where Lucy's going to end up going? 296 00:14:06,200 --> 00:14:08,520 That's right. The asteroid belt's very cool. 297 00:14:08,520 --> 00:14:11,360 Lots of good science there. But we're going to a different set 298 00:14:11,360 --> 00:14:14,360 of asteroids. So these are known as Jupiter's trojan asteroids, 299 00:14:14,360 --> 00:14:16,080 but they're not orbiting Jupiter. 300 00:14:16,080 --> 00:14:18,080 They're sort of orbiting with Jupiter. 301 00:14:18,080 --> 00:14:19,640 So why these ones in particular? 302 00:14:19,640 --> 00:14:22,440 What's special about them versus the asteroid belt? 303 00:14:22,440 --> 00:14:25,480 Well, this region of space that they exist in are known as 304 00:14:25,480 --> 00:14:27,960 Lagrangian points. And they're really stable regions of space. 305 00:14:27,960 --> 00:14:30,560 If you get caught there, the gravity of the situation 306 00:14:30,560 --> 00:14:33,520 all sort of cancels out, basically, there's not a way, an easy way out. 307 00:14:33,520 --> 00:14:36,040 And so we think when the solar system was formed 308 00:14:36,040 --> 00:14:38,800 and debris was flying everywhere, anything that got caught 309 00:14:38,800 --> 00:14:41,400 in these regions of space got stuck there. 310 00:14:41,400 --> 00:14:44,040 And so they're sort of giving us a little glimpse back 311 00:14:44,040 --> 00:14:47,240 in what life could have been like in the very early solar system. 312 00:14:48,880 --> 00:14:51,440 By observing more and more asteroids, 313 00:14:51,440 --> 00:14:54,880 we can build our understanding of what could be heading our way. 314 00:14:54,880 --> 00:14:57,920 So what do we know already about these objects? 315 00:14:57,920 --> 00:15:00,440 - Are we able to categorise them at all? - A little bit, yeah. 316 00:15:00,440 --> 00:15:02,360 So we can see things from the Earth. 317 00:15:02,360 --> 00:15:04,960 We've got telescopes that point at the sky, and largely they fall into 318 00:15:04,960 --> 00:15:07,920 a certain number of categories. So there are things like iron asteroids 319 00:15:07,920 --> 00:15:11,560 that we think were probably the beginnings of a planet, 320 00:15:11,560 --> 00:15:15,480 but the outside got lost, and so we're left with this iron core, 321 00:15:15,480 --> 00:15:18,560 a bit like what would happen on the Earth if it lost everything 322 00:15:18,560 --> 00:15:22,400 above its core. You then have sort of stony, pebbly asteroids that, 323 00:15:22,400 --> 00:15:25,280 erm, that might be held together quite loosely. 324 00:15:25,280 --> 00:15:28,400 And then, what we're looking at with the Lucy mission, 325 00:15:28,400 --> 00:15:31,480 which are primitive asteroids. So asteroids that have stayed 326 00:15:31,480 --> 00:15:34,640 a long way from the Sun, they haven't had that thermal change 327 00:15:34,640 --> 00:15:38,720 that the Sun might produce, and we don't really know what's going on 328 00:15:38,720 --> 00:15:40,880 in their interior. And that's something we're going to go 329 00:15:40,880 --> 00:15:43,040 and try and find out. So when we understand more about 330 00:15:43,040 --> 00:15:45,800 each of those classes, we'll have a better idea of, in the future, 331 00:15:45,800 --> 00:15:48,560 if something is perhaps going to be a bit of a threat, 332 00:15:48,560 --> 00:15:49,920 how to categorise it. 333 00:15:49,920 --> 00:15:52,160 So how is Lucy going to be telling us more about 334 00:15:52,160 --> 00:15:54,440 what these asteroids are made of, then? 335 00:15:54,440 --> 00:15:57,320 So it's a difficult thing to see inside an asteroid, 336 00:15:57,320 --> 00:15:58,880 especially if you're doing a flyby. 337 00:15:58,880 --> 00:16:01,280 But we can tell a lot just by looking at the surface. 338 00:16:01,280 --> 00:16:03,680 So we have some cameras, we have black and white cameras 339 00:16:03,680 --> 00:16:06,040 and colour cameras, but we also have ways 340 00:16:06,040 --> 00:16:08,160 of understanding what the composition is. 341 00:16:08,160 --> 00:16:10,440 So we have an infrared spectrometer which measures 342 00:16:10,440 --> 00:16:12,200 those compositional fingerprints. 343 00:16:12,200 --> 00:16:15,280 And we can understand what the surface is made from, from that. 344 00:16:15,280 --> 00:16:17,600 And then we have a thermal camera on there as well. 345 00:16:17,600 --> 00:16:20,600 And so by putting all of these pieces of information together, 346 00:16:20,600 --> 00:16:22,800 along with the brightness and the shape, and all 347 00:16:22,800 --> 00:16:24,880 that sort of good stuff, we're going to be able to get 348 00:16:24,880 --> 00:16:27,160 a really good idea of what's going on in these asteroids 349 00:16:27,160 --> 00:16:29,400 in a way that we haven't been able to until now. 350 00:16:29,400 --> 00:16:31,960 How does this help us in the context of maybe 351 00:16:31,960 --> 00:16:36,360 - a future YR4-type threat? - So the more we know about asteroids, 352 00:16:36,360 --> 00:16:39,080 the better. So if we understand what they're made from, 353 00:16:39,080 --> 00:16:41,160 if we understand what they typically look like, 354 00:16:41,160 --> 00:16:44,240 all of those things can help us develop our models of how these 355 00:16:44,240 --> 00:16:47,400 asteroids evolve in their orbits over a matter of time. 356 00:16:47,400 --> 00:16:50,000 So when something starts threatening the Earth, 357 00:16:50,000 --> 00:16:52,440 it comes close to the Earth, the details matter. 358 00:16:52,440 --> 00:16:54,000 If we can know what they look like, 359 00:16:54,000 --> 00:16:56,640 if we know what their interiors are like, 360 00:16:56,640 --> 00:16:59,240 we can start modelling those very fine effects 361 00:16:59,240 --> 00:17:01,040 in a lot better detail. 362 00:17:01,040 --> 00:17:03,280 When we get all this information about these asteroids, 363 00:17:03,280 --> 00:17:06,840 how does it help us reduce the unknown unknowns? 364 00:17:06,840 --> 00:17:08,920 That's the $64 million question, right? 365 00:17:08,920 --> 00:17:10,880 One of the things that's really important, 366 00:17:10,880 --> 00:17:13,200 if you want to deflect an asteroid, is to think about how well 367 00:17:13,200 --> 00:17:15,120 the grains are in touch with each other. 368 00:17:15,120 --> 00:17:17,560 You can imagine if you have something that's basically 369 00:17:17,560 --> 00:17:20,120 like little polystyrene balls that are just touching, 370 00:17:20,120 --> 00:17:22,840 held together with gravity or maybe static, 371 00:17:22,840 --> 00:17:25,720 and you could just shove your way through them, right? But if you have 372 00:17:25,720 --> 00:17:28,040 something that's clumped together, if it's really sort of 373 00:17:28,040 --> 00:17:31,960 like an iron core, that's going to be a lot easier to move as one, 374 00:17:31,960 --> 00:17:34,240 right? If you shove it, the whole thing's going to move 375 00:17:34,240 --> 00:17:37,520 rather than collapse. And so when we start to think about how to deflect 376 00:17:37,520 --> 00:17:39,560 or how to interact with asteroids 377 00:17:39,560 --> 00:17:41,680 that are potentially a threat to Earth, 378 00:17:41,680 --> 00:17:44,160 understanding what they're made of and how they're held together 379 00:17:44,160 --> 00:17:46,000 is going to be really, really important. 380 00:17:49,120 --> 00:17:51,640 The Lucy spacecraft is currently passing through 381 00:17:51,640 --> 00:17:54,520 the asteroid belt towards Jupiter, and taking in some sights 382 00:17:54,520 --> 00:17:56,400 along the way. 383 00:17:57,960 --> 00:18:01,000 In 2023, it passed asteroid Dinkinesh, 384 00:18:01,000 --> 00:18:03,960 discovering it also had two moons. 385 00:18:05,120 --> 00:18:06,640 Not unknown for an asteroid, 386 00:18:06,640 --> 00:18:08,920 but new objects that further our knowledge. 387 00:18:10,760 --> 00:18:13,720 So what is the next big thing for Lucy, then? 388 00:18:13,720 --> 00:18:16,160 Well, on Easter Sunday, so easy to remember, 389 00:18:16,160 --> 00:18:18,920 we're going to be flying past our next main-belt asteroid. 390 00:18:18,920 --> 00:18:20,680 So this one is Donaldjohanson. 391 00:18:20,680 --> 00:18:24,120 It's larger than Dinkinesh that we flew by before. 392 00:18:24,120 --> 00:18:25,840 Why is Donaldjohanson exciting, then? 393 00:18:25,840 --> 00:18:27,880 Well, any time you see something new in the solar system, 394 00:18:27,880 --> 00:18:30,640 you learn lots of things that you didn't even know to ask. 395 00:18:30,640 --> 00:18:32,840 So there's just pure exploration, 396 00:18:32,840 --> 00:18:35,680 but we see that the way it reflects the light's really interesting. 397 00:18:35,680 --> 00:18:37,680 So we think it's either a really interesting shape 398 00:18:37,680 --> 00:18:39,720 or perhaps it has a moon, we'll find out. 399 00:18:39,720 --> 00:18:41,680 Very exciting, then! 400 00:18:44,800 --> 00:18:46,120 It's reassuring to know 401 00:18:46,120 --> 00:18:49,200 that our understanding of these potential threats is growing, 402 00:18:49,200 --> 00:18:52,520 but if an asteroid was on course to strike, 403 00:18:52,520 --> 00:18:54,960 who will do something about it? 404 00:18:54,960 --> 00:18:57,760 Or who are we going to call? 405 00:18:57,760 --> 00:19:00,320 Maggie's in Southampton to find out. 406 00:19:01,520 --> 00:19:04,240 It turns out that astronomy is pretty good 407 00:19:04,240 --> 00:19:06,920 at working out the odds of an asteroid strike, 408 00:19:06,920 --> 00:19:08,960 but that might be the easy bit. 409 00:19:08,960 --> 00:19:11,600 After that comes a complex discussion 410 00:19:11,600 --> 00:19:15,240 involving philosophy, ethics and geopolitics. 411 00:19:20,120 --> 00:19:22,240 I'm meeting Professor Hugh Lewis, 412 00:19:22,240 --> 00:19:26,080 who represents the UK on a global approach to asteroid threats. 413 00:19:26,080 --> 00:19:27,320 Nice to meet you. 414 00:19:27,320 --> 00:19:29,520 We're sitting here sort of surrounded by these flags. 415 00:19:29,520 --> 00:19:32,280 I guess this is a global threat, 416 00:19:32,280 --> 00:19:35,480 and so you are part of a network, a global network, 417 00:19:35,480 --> 00:19:37,680 that is considering this and looking at this 418 00:19:37,680 --> 00:19:40,680 and trying to assess these challenges. 419 00:19:40,680 --> 00:19:42,640 Yeah, so after the incident 420 00:19:42,640 --> 00:19:45,320 involving the asteroid over Russia, Chelyabinsk... 421 00:19:45,320 --> 00:19:47,440 - Yes. - ..more than a decade ago now, 422 00:19:47,440 --> 00:19:49,920 that really prompted the United Nations to take some action. 423 00:19:52,120 --> 00:19:55,240 The UN were reacting to an 18-metre asteroid 424 00:19:55,240 --> 00:19:58,400 that flashed across Chelyabinsk in 2013. 425 00:20:00,520 --> 00:20:04,200 It released the equivalent energy of 20 atomic bombs 426 00:20:04,200 --> 00:20:08,160 and created a shock wave that injured 1,500 people. 427 00:20:09,760 --> 00:20:13,400 It was a stark reminder of the threat that asteroids can pose. 428 00:20:14,440 --> 00:20:18,240 The United Nations recommended the creation of two groups. 429 00:20:18,240 --> 00:20:20,640 One was the International Asteroid Warning Network, 430 00:20:20,640 --> 00:20:23,800 and that's the group of scientists and facilities 431 00:20:23,800 --> 00:20:26,320 that would observe the solar system 432 00:20:26,320 --> 00:20:29,920 and identify the potentially hazardous objects 433 00:20:29,920 --> 00:20:31,360 and then issue warnings. 434 00:20:31,360 --> 00:20:32,840 And then the second group 435 00:20:32,840 --> 00:20:35,760 is the Space Mission Planning Advisory Group, 436 00:20:35,760 --> 00:20:38,880 commonly referred to as SMPAG, erm... 437 00:20:38,880 --> 00:20:41,920 and that's the group that I was a member of. 438 00:20:41,920 --> 00:20:44,920 - I see, yes. - And this was the group of engineers, scientists and experts 439 00:20:44,920 --> 00:20:49,440 who would consider how we would go about deflecting 440 00:20:49,440 --> 00:20:52,480 or mitigating the threat from an asteroid using a space mission. 441 00:20:52,480 --> 00:20:56,160 I think one of the challenges is that often many countries 442 00:20:56,160 --> 00:20:59,320 are exposed to a risk for an asteroid impact. 443 00:20:59,320 --> 00:21:01,280 - Yes. - And the problem is is that those countries 444 00:21:01,280 --> 00:21:04,480 don't necessarily have the capability to take action. 445 00:21:04,480 --> 00:21:07,720 - Yes. - So they have to rely upon other countries who do, 446 00:21:07,720 --> 00:21:10,880 and that means that we need to have that international response 447 00:21:10,880 --> 00:21:13,280 - and community that works together. - Yes. 448 00:21:13,280 --> 00:21:15,680 An asteroid is heading towards a country 449 00:21:15,680 --> 00:21:17,400 that doesn't have a space capability, 450 00:21:17,400 --> 00:21:19,720 so it's reliant on those that do, 451 00:21:19,720 --> 00:21:22,720 and any space capability will be quite expensive. 452 00:21:22,720 --> 00:21:25,960 - So weighing those two up seems a challenge. - Yeah. 453 00:21:25,960 --> 00:21:29,440 It is, and I think that's one of the key aspects 454 00:21:29,440 --> 00:21:32,640 of the involvement through the United Nations 455 00:21:32,640 --> 00:21:34,320 and the international community 456 00:21:34,320 --> 00:21:38,480 to understand that particular issue and to try and address it. 457 00:21:38,480 --> 00:21:40,720 Right. Gosh, it's a quagmire. 458 00:21:40,720 --> 00:21:43,160 Are there conferences on things like this? 459 00:21:43,160 --> 00:21:46,200 Yeah, so every two years, scientists and engineers 460 00:21:46,200 --> 00:21:49,800 get together for the Planetary Defence Conference. 461 00:21:49,800 --> 00:21:54,560 That sounds like...the Planetary Defence League, superheroes! 462 00:21:54,560 --> 00:21:57,200 Yeah, I guess you can see it in that way. 463 00:21:57,200 --> 00:21:59,000 These are people who are trying to 464 00:21:59,000 --> 00:22:01,120 understand the threat from asteroids 465 00:22:01,120 --> 00:22:02,760 and what to do about it. 466 00:22:02,760 --> 00:22:05,920 So, at these conferences, what sort of things do they do? 467 00:22:05,920 --> 00:22:08,920 This particular conference is really quite unusual, 468 00:22:08,920 --> 00:22:12,600 because they run a kind of a simulated exercise, 469 00:22:12,600 --> 00:22:15,480 where they create an asteroid, 470 00:22:15,480 --> 00:22:18,240 an asteroid that has a potential impact with Earth, 471 00:22:18,240 --> 00:22:23,680 and they ask the participants at the conference to play particular roles. 472 00:22:23,680 --> 00:22:26,960 It could be journalist, it could be scientist, erm... 473 00:22:26,960 --> 00:22:30,520 it could be, erm... you know, part of the government. 474 00:22:30,520 --> 00:22:34,360 And then they present you with the information about the asteroid 475 00:22:34,360 --> 00:22:37,560 in kind of pieces, they give you a little bit of information at a time, 476 00:22:37,560 --> 00:22:39,280 and you have to make decisions. 477 00:22:39,280 --> 00:22:43,040 Yes, so drip-feed the information, as it would be in a real situation. 478 00:22:43,040 --> 00:22:44,600 - Exactly right. - Right. 479 00:22:44,600 --> 00:22:47,520 And then in some cases, the asteroid ultimately misses, 480 00:22:47,520 --> 00:22:51,120 yet you still have to run through the scenarios 481 00:22:51,120 --> 00:22:53,000 and make sensible decisions. 482 00:22:53,000 --> 00:22:56,160 And in some cases, the asteroid does hit. 483 00:22:56,160 --> 00:22:58,520 And I think it really does showcase the fact 484 00:22:58,520 --> 00:23:01,600 that whenever we're dealing with this particular threat, 485 00:23:01,600 --> 00:23:03,200 it's never certain. 486 00:23:03,200 --> 00:23:06,240 There's always a chance that it misses us. 487 00:23:06,240 --> 00:23:09,320 But if we don't know that for absolute certain, 488 00:23:09,320 --> 00:23:11,760 an absolute certainty is a hard thing to get. 489 00:23:11,760 --> 00:23:13,440 And it's that kind of scenario that they use 490 00:23:13,440 --> 00:23:14,960 at the Planetary Defence Conference. 491 00:23:14,960 --> 00:23:16,880 It's never, "It's a huge asteroid, 492 00:23:16,880 --> 00:23:19,960 - "it's definitely going to hit, what do we do?" - Yes! 493 00:23:19,960 --> 00:23:22,320 You have to kind of really consider what the... 494 00:23:22,320 --> 00:23:24,240 ..not just what the numbers are telling you, 495 00:23:24,240 --> 00:23:28,120 but what the moral imperative is in terms of protecting the planet. 496 00:23:28,120 --> 00:23:31,920 That's why it's called "planetary defence", not UK defence. 497 00:23:31,920 --> 00:23:34,200 Yes! And so the fact that we are working together, 498 00:23:34,200 --> 00:23:35,960 I find quite comforting. 499 00:23:37,040 --> 00:23:40,080 While space can seem like a violent, scary place... 500 00:23:42,680 --> 00:23:45,400 ..it's good to stop, look up 501 00:23:45,400 --> 00:23:47,640 and enjoy our beautiful universe, 502 00:23:47,640 --> 00:23:49,120 asteroids and all. 503 00:23:52,560 --> 00:23:55,120 You can even see a few yourselves. 504 00:23:55,120 --> 00:23:58,160 Our resident stargazer, Pete, is on hand to guide us 505 00:23:58,160 --> 00:24:01,480 through some of the upcoming highlights in the night sky. 506 00:24:01,480 --> 00:24:04,640 For amateur astronomers, the big news while we were off air 507 00:24:04,640 --> 00:24:08,880 was the display of planets that were out in force. 508 00:24:08,880 --> 00:24:12,040 Now most of them are disappearing from view, 509 00:24:12,040 --> 00:24:15,240 but Jupiter and Mars are still there to spot, 510 00:24:15,240 --> 00:24:17,680 visible in the early evening sky. 511 00:24:18,840 --> 00:24:21,320 Jupiter is especially obvious, 512 00:24:21,320 --> 00:24:26,040 {\an8}low above the west-northwest horizon as darkness falls. 513 00:24:26,040 --> 00:24:28,960 {\an8}It can be seen in conjunction with a beautifully thin, 514 00:24:28,960 --> 00:24:33,400 13%-lit waxing crescent moon on the 30th of April. 515 00:24:33,400 --> 00:24:36,120 A wonderful sight if the weather is clear. 516 00:24:36,120 --> 00:24:40,160 Another easy spot this month is the Lyrid meteor shower, 517 00:24:40,160 --> 00:24:43,520 and this even has a tenuous link to asteroids, 518 00:24:43,520 --> 00:24:46,480 because the bodies which create the debris stream 519 00:24:46,480 --> 00:24:49,280 which passes through the Earth's atmosphere 520 00:24:49,280 --> 00:24:50,960 to create a meteor shower, 521 00:24:50,960 --> 00:24:53,840 are comets or sometimes asteroids. 522 00:24:55,000 --> 00:24:58,280 {\an8}A meteor shower's radiant is the small area of sky 523 00:24:58,280 --> 00:25:00,880 {\an8}its meteors appear to emanate from, 524 00:25:00,880 --> 00:25:04,160 {\an8}which in this case is near the bright star Vega. 525 00:25:04,160 --> 00:25:08,160 {\an8}The shower reaches its peak around midday on the 22nd of April, 526 00:25:08,160 --> 00:25:10,400 {\an8}meaning the best nights for a watch will be 527 00:25:10,400 --> 00:25:14,160 {\an8}the nights of the 21st of April into the morning of the 22nd, 528 00:25:14,160 --> 00:25:17,480 {\an8}and the 22nd of April into the morning of the 23rd, 529 00:25:17,480 --> 00:25:20,720 {\an8}with the most activity seen just before dawn. 530 00:25:20,720 --> 00:25:24,320 Watching Lyrid meteors is a fairly relaxed affair. 531 00:25:24,320 --> 00:25:26,560 All you have to do is make yourself comfortable, 532 00:25:26,560 --> 00:25:28,760 find a good dark location 533 00:25:28,760 --> 00:25:30,960 and keep watching the sky. 534 00:25:30,960 --> 00:25:35,440 Look at a height about two-thirds of the way up the sky in any direction. 535 00:25:35,440 --> 00:25:38,640 If you want to try your luck photographing Lyrid meteors, 536 00:25:38,640 --> 00:25:40,240 it's fairly easy to do. 537 00:25:40,240 --> 00:25:44,040 You just need a camera with a wide-angle fast lens. 538 00:25:44,040 --> 00:25:46,840 You need to set the camera's ISO fairly high 539 00:25:46,840 --> 00:25:49,040 and fully open the lens, 540 00:25:49,040 --> 00:25:51,240 and then just take continuous images, 541 00:25:51,240 --> 00:25:53,280 hoping to grab a meteor trail. 542 00:25:54,640 --> 00:25:56,960 If your sky is light-polluted and bright, 543 00:25:56,960 --> 00:25:59,440 your image may look like this. 544 00:25:59,440 --> 00:26:03,800 If so, reduce the exposure length until they aren't overexposed 545 00:26:03,800 --> 00:26:06,000 and you can still see stars. 546 00:26:06,000 --> 00:26:09,040 Then just let it run for as long as you are out, 547 00:26:09,040 --> 00:26:11,920 or your batteries allow, and see what happens. 548 00:26:11,920 --> 00:26:14,560 You never know, you might get lucky. 549 00:26:14,560 --> 00:26:17,080 But it's common to take thousands of images 550 00:26:17,080 --> 00:26:20,720 without a single meteor on any one of them. 551 00:26:20,720 --> 00:26:22,480 But if you have more advanced kit, 552 00:26:22,480 --> 00:26:25,840 there are two actual asteroids we'd like to point out. 553 00:26:25,840 --> 00:26:28,560 Neither of them are going to be hitting the Earth, 554 00:26:28,560 --> 00:26:31,160 but they are fairly easy to see. 555 00:26:31,160 --> 00:26:33,800 The first is 4 Vesta, 556 00:26:33,800 --> 00:26:36,960 which, with a diameter of 330 miles, 557 00:26:36,960 --> 00:26:39,080 is the largest asteroid 558 00:26:39,080 --> 00:26:43,760 in the main asteroid belt which lies between Mars and Jupiter. 559 00:26:45,600 --> 00:26:47,280 {\an8}To locate the asteroid, 560 00:26:47,280 --> 00:26:49,720 {\an8}use the two brightest stars in Libra, 561 00:26:49,720 --> 00:26:52,560 {\an8}Alpha Librae, or Zubenelgenubi, 562 00:26:52,560 --> 00:26:56,760 {\an8}and Beta Librae, or Zubeneschamali. 563 00:26:56,760 --> 00:26:59,600 {\an8}Vesta will be located in northern Libra, 564 00:26:59,600 --> 00:27:03,920 heading towards the border with Virgo as we head into next month. 565 00:27:03,920 --> 00:27:07,880 Record the suspected star field over several days 566 00:27:07,880 --> 00:27:10,000 where you think Vesta is located. 567 00:27:10,000 --> 00:27:12,360 If you've got it right, comparing the records 568 00:27:12,360 --> 00:27:16,400 should reveal Vesta as a moving star-like dot. 569 00:27:17,520 --> 00:27:20,480 Owners of smart telescopes have got it easy 570 00:27:20,480 --> 00:27:24,320 as all they have to do is search for Vesta and start imaging. 571 00:27:24,320 --> 00:27:26,440 For those that like a bit of a challenge, 572 00:27:26,440 --> 00:27:28,280 then there's 9 Metis, 573 00:27:28,280 --> 00:27:31,520 which comes to opposition on the 9th of May. 574 00:27:31,520 --> 00:27:33,800 "Opposition "is a term which describes 575 00:27:33,800 --> 00:27:37,960 when an object is in the opposite position in the sky to the Sun, 576 00:27:37,960 --> 00:27:40,800 so that means it's the best time to see it. 577 00:27:42,720 --> 00:27:45,080 It's currently also within Libra, 578 00:27:45,080 --> 00:27:48,440 and we can use the same two stars we used to locate Vesta 579 00:27:48,440 --> 00:27:50,360 to find 9 Metis. 580 00:27:50,360 --> 00:27:55,040 Just as with Vesta, record the star field over several nights. 581 00:27:55,040 --> 00:28:00,160 Align the stars and look for the moving object. 582 00:28:00,160 --> 00:28:02,360 Whether you're snapping Jupiter with your phone 583 00:28:02,360 --> 00:28:05,200 or you manage to track Metis across the sky, 584 00:28:05,200 --> 00:28:08,000 we'd love to see any photographs you've got, 585 00:28:08,000 --> 00:28:10,520 so send them in to our Flickr account. 586 00:28:10,520 --> 00:28:12,640 You can find details of this at 587 00:28:12,640 --> 00:28:17,440 www.bbc.co.uk/skyatnight 588 00:28:17,440 --> 00:28:20,520 and we'll show some of our favourites. 589 00:28:20,520 --> 00:28:23,400 Meanwhile, here are some of the pictures you've sent in 590 00:28:23,400 --> 00:28:25,000 while we were off air. 591 00:28:49,000 --> 00:28:52,160 Happy stargazing! Goodnight. 50245

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