[0:00] There’s a bit of tension in the story for this video. [0:03] When I put out a call for interesting things that I could film in England, [0:06] one of the team from Jodrell Bank got in touch. [0:09] Tucked away in the Cheshire countryside, [0:11] it’s the home of the Lovell Telescope, a World Heritage Site, [0:14] the largest radio telescope in the country, [0:16] and one of the scientific and engineering icons of Britain. [0:19] And the tension is this. [0:21] They wanted to show off the new science they’re working on [0:23] all across their campus, [0:24] and we are going to do that, ’cos one of the big questions I had was, [0:28] is a 70-year-old telescope still useful? [0:31] But also, from my side, what I wanted very much [0:35] was to climb the giant telescope. [0:38] (bird twitters) [0:40] Well, there are definitely worse views than that to start the day, aren’t there? [0:43] There is a reason for that, [0:45] beyond my just being a massive nerd, [0:47] when I was young, probably about ten years old, [0:49] I went to Jodrell Bank as a visitor, [0:50] to see what was then called the Discovery Centre, [0:53] not on a school trip. [0:54] Young me, very much into space and science, [0:56] wanted to go see the big telescope. [0:58] But of course, they don’t let visitors onto, or even up close to the telescope, [1:02] it’s a working science thing. [1:04] And while I had a good day out, [1:06] I think I was a bit disappointed that I couldn’t get under it or... [1:10] up on it. [1:11] There’s no photos of that trip, by the way, it was the nineties, [1:13] people didn’t carry cameras around every minute of their lives. [1:15] Anyway, about 30 years later, I went back. [1:18] Adult-me parked up, checked in with the team at Jodrell Bank, and first up, [1:22] they took me to see the newly-updated visitor centre. [1:25] There’s a lot of screens and displays, [1:26] it’s far more impressive than it used to be, [1:28] but I was quite glad to see there were still a couple of things I remembered. [1:32] Do you still have the black hole table? [1:33] ’Cos I remember... -If you just go round here... [1:36] You still have the black hole table! [1:39] I spent like 15 minutes as a kid just playing with that black hole table. [1:43] I was really tempted to do that again, [1:45] but never mind. [1:46] Also, the old acoustic dishes are still there! [1:49] What you’re about to hear is the audio from the on-camera mics, by the way, [1:52] no trickery. [1:53] I have such a strong memory of these from when I was like ten years old. [1:58] (sotto voce) You can whisper very quietly... [1:59] And it turns up on the other side. [2:02] Core memory. Got to do that again 30 years later. [2:05] It’s not bad. [2:06] I couldn’t find the mock control room [2:08] where kids used to be able to sit down and pretend they were controlling the dish, [2:10] but still, happy with that. Nostalgia complete, on to the science. [2:14] Now, there are two sides behind the scenes at Jodrell Bank these days. [2:17] I did remember seeing the old university buildings from the ’60s and ’70s, [2:21] but in the last few years, there’s been a very shiny new headquarters built [2:24] next door for another project. [2:26] The Square Kilometre Array Observatory, the SKAO, [2:30] is a big intergovernmental organisation. [2:33] The actual telescopes are on the other side of the planet, [2:35] in South Africa and Australia, [2:36] but the headquarters is at Jodrell Bank. [2:39] I met William, who’s their director of communication, outreach and education, [2:43] and the first thing we went to seemed almost out of place. [2:46] That’s a very sci-fi sign, isn’t it? [2:48] You’ve picked a full science fiction font there. [2:50] Okay, you have a proper council chamber! [2:54] Well, so, that’s, you know, right there in the middle of Cheshire. [2:56] That’s quite unusual. -Yeah. [2:58] It’s an unusual setting. [2:59] Big picture, what is the SKAO? [3:02] So, maybe, you know, you should turn around, and this is the SKAO here. [3:06] You know, all these flags. -(laughs) [3:08] Oh, I can see why you’re head of outreach. That was smooth. [3:12] But this really embodies who we are as an international organisation. [3:16] What we are doing is really to build and to operate [3:20] the world’s largest radio telescopes. [3:21] And one will be observing lower frequencies, [3:25] so that’s the one in Australia. [3:26] That’s the one we will be using to really go back in time [3:29] to what we call the cosmic dawn. [3:31] The Cosmic Dawn, as in D-A-W-N, [3:34] is the period just after the Big Bang. [3:36] And by “just after”, I mean a quarter of a billion years, [3:40] because the numbers you encounter in astronomy are mind-boggling. [3:43] So, really observing, you know, these very first signals [3:46] which were emitted after the Big Bang. [3:49] And so, that will give us some clues about, you know, how all of it started. [3:54] We know that Nobel Prize discoveries will be made with our telescopes. [3:59] When? I don’t know, but, you know, that’s the goal. [4:03] I got to talk to their head of science operations. [4:06] One of the cool things about the SKA [4:08] is really that we’re building it [4:10] to be as flexible as possible to observe things that we don’t even know about yet. [4:14] We don’t know what our galaxy really looks like. [4:16] I mean, it’s quite bizarre to think about the fact that... [4:18] Do we not know that? [4:20] With all of the beautiful images of other galaxies out there, [4:23] we don’t really know what our own galaxy looks like [4:25] because it’s quite hard to observe. [4:27] -Yeah, you don’t have a mirror out there! -Exactly. [4:29] We don’t actually know how big stars form, [4:31] and when you’re talking about understanding galaxies [4:34] throughout the universe, [4:36] I mean, if you don’t understand how those building blocks are really being formed, [4:40] then how can you really know the detail of what’s going on in the galaxies? [4:44] I mean, how planets form. -Yeah. [4:46] I mean, we know that they form in the debris disc around stars. [4:50] But we actually don’t know the crucial phase of how things get from [4:54] really, really small particles through the centimetre scale [4:58] up to something that’s much larger, of course, to make a planet. [5:01] We just assume it happens. [5:03] It must happen. [5:04] -Yes. -We just don’t know how. [5:06] We know it happens, but our theory currently doesn’t support it. [5:09] And the SKA is really well-suited to that scale. [5:14] A lot of things that I assumed were pretty much proven and sorted [5:16] are still promising theories with data attached. [5:20] The SKAO is going to produce about a petabyte of science data every day [5:24] to help with a lot of astronomy. [5:26] But while that’s all coordinated at Jodrell Bank, [5:28] the actual receipt of signals is happening in other countries. [5:31] Because one of the problems with any radio telescope in the UK [5:34] is there isn’t much room for radio quiet zones. [5:37] And certainly not this close to cities. [5:39] Jodrell Bank does ask visitors to turn their phones off, [5:41] but there are still roads and train lines nearby, there will be interference. [5:46] So I still have the question... [5:48] is the Lovell Telescope, the famous one, still useful? [5:52] Or is it now more history than science? [5:54] To start answering that, I got taken into the telescope control room by Simon, [5:59] he’s a professor and the associate director of the observatory. [6:01] Five years to build? [6:03] Very rapid project, enormously ambitious in the early 1950s, [6:07] not long after the war, [6:09] to build a radio telescope [6:12] which was so much larger than anything that existed before. [6:16] How much? [6:18] So, it was ten times larger than the largest telescope that existed before. [6:21] Oh, okay. Right, sure. [6:23] And a leap in the dark. [6:25] They had no idea what they would discover. [6:28] There were big telescopes before [6:30] what became known as the Mark One 250-Foot Telescope, [6:33] they just weren’t steerable. [6:35] To this day, the big dish at Jodrell Bank [6:37] is still the third largest fully steerable telescope in the world. [6:40] It can be pointed at anywhere in the sky. [6:43] I cannot tell you how much the young version of me [6:47] that sat at the mock control room that the discovery centre had back then [6:52] is absolutely overjoyed. [6:56] Oh, my word. [6:58] (laughs) [7:00] So, that is the telescope. [7:01] That’s the 250-foot, 76-metre Lovell Telescope. [7:05] Pointing straight up, [7:06] ’cos we’re doing some painting and repair work on it at the moment. [7:10] I keep worrying that I’m getting in the way of science here. [7:12] And I’ve just realised that this is not an observing day. [7:15] There is literally a cherry picker with someone painting the telescope in there. [7:18] Alright, so, can I have a look? What’s it...? [7:20] So, this is Mirza, our controller today. [7:23] So, there’s somebody in here, [7:25] there’s a controller in this room 24 hours a day... [7:27] Right. It’s a lovely control desk, this. [7:29] I know that’s the nerdiest thing I’ve said in a while. [7:32] It’s a really nice control desk. -This is the original 1957 control desk. [7:38] -Right. -In terms of the steel. [7:39] But all the electronics that drives the telescope [7:41] and controls the telescope so precisely is new. [7:45] I am a little worried that, because the folks in that room [7:47] were explaining the very basics of their radio astronomy work to me, [7:51] I’m doing them a little bit of a disservice. [7:53] So, just to be clear, everyone you’re hearing from in that control room [7:57] has a PhD. [7:58] Anyway, Mirza, the telescope controller, [8:00] also showed me a more modern-looking bank of screens at the back of the room, [8:03] that connects the telescope to the E-MERLIN network, [8:06] a collection of smaller dishes across the UK. [8:08] So, you can remote control all of those as well? [8:11] We can remotely control from this station here. [8:13] As you can see, we have the names of all the telescopes. [8:17] You’ll see they’re pointing at the same position, [8:19] so they’re all on the same source. [8:22] That’s not an icon.... that’s not a static icon. [8:24] That’s literally the direction it’s pointing. [8:26] That’s live. That’s live data coming through. [8:29] You’ll see the Lovell is... -Lovell is pointed up, and it’s red? [8:32] It’s pointed straight up, and it’s red. [8:33] It’s pointing up, but not in a few hours’ time, hopefully. [8:36] Right. [8:36] So, you’re observing something right now. [8:40] I’m not sure what it is, but you’re definitely observing something. [8:43] That something was explained to me by Emmanuel. [8:46] Again PhD. [8:47] We are pointing on this particular target, 3C84, [8:51] which is one of the brightest radio sources in the sky. [8:53] And we use this source as a calibrator [8:56] to calibrate the instrument or the observation when it is done. [8:59] So, once it stays on this target [9:01] for some time in the sky, [9:03] all the telescopes will move to the science target [9:06] from the calibrator to the target and then observe. [9:09] And then once the data comes through the fibre-optics [9:11] from all the network of telescopes, [9:13] it is correlated right here in Jodrell Bank. [9:15] And someone’s going to earn their PhD off that, [9:17] or someone’s going to find some magical discovery. [9:21] -You never know. -You never know. [9:23] One of the advantages of radio astronomy is that scientists can take signals [9:26] from telescopes that are a long way apart, [9:28] correlate them all together with fibre-optic cables and computers, [9:31] and end up with the equivalent resolution [9:33] of a telescope the size of that entire network. [9:36] This is the ends of those optical fibres. [9:40] So, these optical fibres stretch out to the individual telescopes, [9:43] and then we have to focus them, [9:45] and we do that in the machine which is behind us. [9:47] Oh, there’s a... [9:49] (laughs) [9:51] Okay, you’ve got... [9:54] Oh! Okay. [9:55] Yep. [9:56] (whirring) [9:58] Little bit noisy. [10:00] So, this is the supercomputer which is doing the focusing. [10:04] It’s a correlator designed to multiply the raw signals [10:08] from each pair of telescopes, [10:09] accumulate those, [10:11] and then Emmanuel and colleagues turn those into images. [10:14] And the reason it’s in this rather weird room [10:17] is that this keeps any of the radio signals that this generates [10:21] away from the big dish. [10:22] So now we can go and see some of our young scientists working on the data. [10:26] The young scientists in question [10:28] all either have their PhDs or are working on them. [10:31] Sorry to interrupt. [10:32] I’ve been told you’ve all been briefed on who I am and what I’m doing here. [10:37] I’m worried that Simon just kind of opened the door and said, “Hi, here’s Tom.” [10:40] Benjamin is working on a live feed from the 42-foot telescope, [10:44] one of the other smaller dishes at Jodrell Bank, [10:46] which is picking up the signal from the rapidly rotating remnants [10:49] of a collapsed star, called a pulsar. [10:52] I have an animation of what one of those looks like here... [10:55] Someone has prepared a presentation here! [10:57] Simon’s been doing hard work here. [10:59] Thank you, folks. [11:00] So what we’re seeing here is a beam of radio emission, [11:03] a little bit like a lighthouse that is sweeping itself around the sky, [11:08] and the reason it sweeps around the sky like this is, [11:10] I actually have a little model here. [11:11] You have a model! [11:16] I knew you were coming. [11:18] As the star rotates, that beam, [11:20] that radio beam, like here that’s coming away from the magnetic pole, [11:24] is sweeping around the sky somewhat like a lighthouse. [11:26] And if we happen to be fortuitously located in the galaxy, [11:30] and that beam sweeps across Earth, [11:32] we will see a little pulse every time it does so, [11:35] and so we call them pulsars. [11:37] A pulsar is the size of a city, the mass of the Sun, [11:40] and the fastest one we know of rotates 716 times per second. [11:47] Like I said, astronomy includes mind-boggling numbers. [11:50] The idea really is to unambiguously account [11:52] for every single rotation of these stars. [11:55] Right. [11:56] Because if we can do that, then we can do all kinds of experiments [11:59] because what we have is effectively clocks in the sky, [12:02] and if you have clocks in the sky, [12:04] that’s a fantastic way to test general relativity [12:07] to find the limits of Einstein’s theory. [12:10] Next up is Phoebe, who was bouncing radio signals off asteroids. [12:14] So, there’s a radar in Madrid that’ll be transmitting, [12:18] and then all the radio telescopes in this network [12:20] will then be listening to the echo of that radar pulse, [12:24] like, bouncing off the asteroid. -Wow. [12:26] And you do that a few times, and you can work out how fast it’s moving, [12:29] what direction it’s going, everything like that, or...? [12:31] -Hopefully, with just one observation. -Just one? [12:33] With the multiple telescopes at the same time, [12:36] you should get an idea of the speed from that as well. [12:38] Resolution is much better than optical. [12:41] We can get down to about a metre, [12:44] sort of, with the imaging that we’re going to do. [12:47] Hopefully. [12:48] This is, sort of, quite new, and we’ve not tried it before. [12:51] This is the first VLBI observation [12:55] to get this level of detail. [12:57] VLBI there is Very Long Baseline Interferometry, [13:02] which is the name for that process of combining multiple telescopes [13:04] in different locations. [13:06] I mean, do I just ask what everyone’s working on? [13:08] Like, I’m assuming Simon has prepared all of you with something, but... [13:11] Uh, no. This is my regular office. [13:13] Okay! (all laugh) [13:15] Thank you! [13:16] That was a little unfair to Justin, [13:18] who I later found out specialises in researching cosmic rays [13:21] and high-energy particles, [13:22] and was actively working there. I’m sorry, Justin. [13:25] But all this research is based on data coming in from other dishes. [13:28] We still haven’t talked about the Lovell Telescope itself. [13:31] My question remains... [13:33] can a 70-year-old telescope still be useful? [13:36] Or is it just a heritage landmark now? [13:39] Because it has a huge amount of heritage. [13:41] Perhaps most famously, it intercepted photos [13:43] that were transmitted from the first Soviet lander on the moon. [13:47] Those pictures were in the British press [13:48] well before the Soviets ever wanted them released. [13:51] [announcer] The Western World had their first word of the successful probe [13:54] from an English source. [13:55] The Jodrell Bank Observatory near Manchester. [13:58] It was now time to head out to the telescope itself, [14:01] while the maintenance teams were also out there, [14:02] and I wasn’t disrupting science. [14:04] I put on a climbing harness... [14:06] (harness clips and zips) Yeah, alright. [14:07] ...and then went out to the dish, accompanied by Simon, [14:10] plus telescope supervisor, Phil, [14:11] who’s worked on the site for decades, [14:13] and also, hastily-recruited and quite excited, Megan, [14:17] one of Jodrell Bank’s comms team, [14:18] who was very happy to volunteer to hold another camera. [14:21] Lead the way! Thank you very much. [14:23] Oh shades. [14:25] Definitely going to need them. [14:26] I’ve never encountered safety sunglasses before, [14:28] but when you’ve got not only the sky, [14:30] but also the sky reflected off the bowl of a bright-white telescope, [14:34] they’re a good idea. [14:35] I thought razor burn was just a part of life [14:38] that I had to deal with. [14:39] But recently, I have unlearned a bad habit [14:42] and it’s got better. [14:43] I used to instinctively push down when I shaved. [14:46] Most folks who shave do that without even thinking about it, [14:49] because most modern cartridge razors are built with pivots or springs. [14:53] Or if you use disposables, like I did, [14:55] the whole thing just flexes a tiny amount. [14:58] Because the blade can move, it feels a little unstable [15:00] when you're shaving and it meets the resistance of your hair. [15:02] It tugs. So you push just a little harder [15:06] to try and stabilise it against your skin. [15:07] That doesn't actually stop the blade flexing. [15:09] It just increases friction, and that’s one of the causes of razor burn. [15:13] Just bad design. [15:15] A few weeks ago, Henson Shaving sent me their razor. [15:18] It’s machined out of solid aerospace-grade aluminum, [15:21] the tolerances are as tight as 13 microns in places, [15:25] the blade is held completely rigid. [15:27] Which means I had to learn not to apply so much force, and [15:30] let the weight of the razor do most of the work. [15:32] And now I have less razor burn! [15:34] There’s no subscription model or proprietary blades here: [15:37] this takes the inexpensive, international- standard, double-edge blades. [15:41] If you want to use a different brand of blade, you can, [15:43] so it also works out much cheaper long-term. [15:47] If you use the link in the description or scan the QR code on screen, [15:50] you too can get a Henson razor, hopefully end up with less razor burn, [15:53] plus they’ll throw in a hundred free blades, [15:56] which should last you a long time. [15:58] It’s still impressive. [15:59] It really is. [16:00] 3,000 tonnes, able to move from one part of the sky to another fairly quickly, [16:06] but also able to track things across the sky [16:08] to within a thousandth of a degree. [16:11] And that’s a challenge now. [16:13] It was a challenge in 1957... -Right! [16:16] ...before computers! -(laughs) [16:18] I came here as a kid, [16:20] and remember looking up at this when I was about this tall, [16:24] and wanting to do this. [16:25] Where do we go from here? [16:26] -We’ll head up towards the lift. -Alright. [16:29] We just take care stepping over the rails, you can see they’re quite oily and greasy. [16:34] Oh okay. [16:34] And we don’t want greasy boots to go climbing with. [16:37] Oh! Yeah. [16:39] So, are these railway tracks? [16:41] Yep, standard railway tracks. [16:42] Huh! [16:44] That makes sense, because it was built, what, 70 years ago? [16:47] And you use the technology you have, if it works and it’s proven. [16:50] It’s about 50-100 tonnes per wheel, is the load. [16:54] -Yep. -64 wheels it runs on. [16:57] -(exhales) -So... [16:59] -How on earth? -When you change the wheels, [17:00] you jack the telescope up. [17:01] Yep. [17:02] -Really? -Yep. [17:04] So yep... [17:05] Just a hydraulic jack. [17:07] -Wow. -About 200 tonnes to lift it up. [17:10] Slide it out and put another one in. [17:12] The telescope is named after Sir Bernard Lovell, [17:15] first director of the observatory, [17:16] the driving force behind building the telescope. [17:18] And the painting job is apparently never-ending. [17:21] You can see the blue cherry picker in the background there. [17:23] It’s a steel structure, it relies on painting to protect it. [17:28] And, you know, it’s been operating for nearly 70 years, [17:32] and we want to keep it going for another 70 years. [17:34] Bit cosy, but it does take four people. [17:37] (laughter) [17:38] And as we headed out onto the catwalks, [17:40] I was a little bit lost for words. [17:43] (laughs) [17:46] Oh wow! [17:52] -You okay? -Yeah! [17:54] This is very, very cool. [17:55] We didn’t check that you’re okay with heights before coming up here, did we? [17:58] (laughs) [17:59] Megan was absolutely fine with heights. [18:01] Also, you can see two of the other, smaller Jodrell Bank dishes there, [18:04] those were the ones actively listening and doing science at that moment. [18:07] From there, it was up onto the first surface of the dish. [18:10] The telescope does look a bit different compared to the early days. [18:13] It’s been shored up and upgraded over years, [18:15] and it gained a brand new surface in the early 2000s. [18:18] Oh! [18:19] The first stop was between those two surfaces, [18:22] and then it was up onto the dish. [18:25] (laughing) [18:28] Thank you! [18:29] The telescope’s been standing for 70 years, [18:33] this floor has been standing for 25 years, [18:35] and it’s made of steel, and yet, [18:37] somehow I’m still just a little bit worried as I go up here. [18:41] So, the idea of the parabola is to focus the radio waves that land on the telescope [18:46] to the focus, which is what you can see at the top. [18:48] Yes, because there’s all sorts of bad graphics [18:50] where the beam is coming into that directly, [18:53] and it’s not, it comes into this bowl... [18:55] -Yes. -...and gets bounced up to there. [18:58] Yep. [18:59] And the property of a parabola is, wherever it hits this surface, [19:03] it ends up in that hole in the middle. [19:05] And moreover, the path length from each ray is the same. [19:09] So, if you like, all those radio waves add up coherently, in step, at the focus. [19:14] -Oh! -That is the property of a parabola. [19:16] Right. [19:17] Radio has a wavelength anywhere from a few centimetres to kilometres, [19:21] so thankfully, the dish surface doesn’t have to be too precise. [19:23] We’re not going to cause any damage walking on it. [19:26] To see nothing but dish and the sky is magic. [19:30] Okay, if you’re ready for the next challenge, [19:32] we can have a go at heading up to the top and have a look. [19:35] Yeah, this is where I leave you two behind. [19:38] Let’s do it. [19:43] And the sun’s come out! [19:45] And it’s blinding! [19:46] You were right about those shades. [19:48] I’m going to put those on. [19:49] I know, I look like a dork... [19:51] Oh, my word! [19:52] ...and you can’t see my eyes. [19:54] I take the shades off again in a bit, [19:55] but with the sun out and that light being reflected up towards us, [19:58] it was bright. [20:00] There is a reason that you do not point a telescope at the sun. [20:03] Even well off-axis, like it was, it felt so bright. [20:07] But we were high enough that I could see the horizon again. [20:10] I am so incredibly lucky. Right. [20:13] Where do I go from here? [20:14] Climbing harness hooked in, [20:16] up the ladder to the focal point. [20:18] That is the very top of the telescope. [20:23] (laughs) [20:27] Oh, it wobbles! [20:30] Course it does. [20:31] What an incredible view. [20:34] Something special, isn’t it, up here? [20:36] It really is. [20:39] So, is it still doing science? [20:43] I don’t know what I was expecting. [20:44] Some mirror system, some fancy little thing? [20:46] No, you’re literally moving the entire detector. [20:49] Yep. Because there’s only one focal point to the whole dish. [20:54] So, to use that same focal point twice... -Yeah. [20:58] ...it requires to move one out of the way and put the other one into the same slot. [21:04] The telescope is 70 years old. [21:06] It’s now a Grade I listed historical site, [21:08] which is probably going to give them all sorts of trouble [21:10] refitting it in future. [21:12] But the surface is only 25 years old, [21:14] and those multiple detectors, the different science packages [21:17] that can be moved into the focal point are much more recent than that. [21:21] The Lovell Telescope is still doing world-class science, [21:24] on its own, as part of networks, [21:26] because it turns out that as long as you do the upkeep, [21:28] the scientific concept of [21:30] “massive parabolic dish that you can point anywhere” [21:34] doesn’t really go out of date. [21:36] But there is one more thing. [21:38] I spent a while admiring the view, [21:40] and then headed back down, and back in the control room, [21:42] I got to do something that my ten-year-old self, [21:45] playing at the controls in the mock control room in the discovery centre, [21:49] would never have dreamed was possible. [21:51] Alright. [21:53] Five seconds on the siren? [21:54] Five seconds on the siren, yes. [21:56] (siren wails) [22:02] (siren fades) [22:05] That got their attention, right? And then... [22:08] Return. [22:09] -Enter on here. -Yeah. [22:13] With slow grace, [22:15] the Lovell Telescope began to turn [22:17] and pointed at its first science target for the day. [22:22] There’s a kid, um, on the fence there, [22:24] he’s going to be, like, a few pixels in the final footage. [22:27] And he’s just staring up at the machine, [22:30] and he’s about the age I would have been when I got here. [22:35] I wonder if the same thing’s just sparked off in his head? [22:39] (chuckles) [22:43] The ten-year-old version of me is so happy. [22:46] Your dream’s come true. [22:50] Next time, or right now on Nebula, [22:51] I visit a school where the students have four legs [22:54] and a bendy backbone, to see how they outperform robots.