1 00:00:01,500 --> 00:00:04,000 We live in a Universe of unimaginable scale 2 00:00:04,000 --> 00:00:06,500 and almost incomprehensible beauty. 3 00:00:06,500 --> 00:00:10,000 How is the light from stars, galaxies and nebulae 4 00:00:10,000 --> 00:00:12,000 fashioned into the spectacular images 5 00:00:12,000 --> 00:00:14,500 that have so inspired us over the years? 6 00:00:37,500 --> 00:00:39,500 This is the Hubblecast. 7 00:00:39,500 --> 00:00:43,500 News and images from the NASA / ESA Hubble Space Telescope. 8 00:00:43,500 --> 00:00:46,500 Travelling through time and space with our host, Dr. J 9 00:00:46,500 --> 00:00:49,000 EPISODE 10: Making the Universe come to life. Behind the Hubble images a.k.a. Dr. Joe Liske. 10 00:00:49,000 --> 00:00:51,000 Welcome to the Hubblecast. 11 00:00:51,000 --> 00:00:53,000 Do you ever look at this beautiful Hubble images 12 00:00:53,000 --> 00:00:55,000 and wonder how they were made? 13 00:00:55,000 --> 00:00:58,500 What exactly happens after the faint light from distant objects 14 00:00:58,500 --> 00:01:00,000 is detected by Hubble? 15 00:01:00,000 --> 00:01:03,000 How are these cosmic photons captured in space 16 00:01:03,000 --> 00:01:05,500 transformed into the glorious coloured images 17 00:01:05,500 --> 00:01:08,500 down here on you wall or your computer screen? 18 00:01:09,500 --> 00:01:11,500 On a clear night when we look up into the heavens 19 00:01:11,500 --> 00:01:14,000 we can see the light from thousands of stars. 20 00:01:14,000 --> 00:01:16,000 Our eyes are fantastic detectors 21 00:01:16,000 --> 00:01:18,500 but in reality they are actually very limited. 22 00:01:18,500 --> 00:01:22,000 They aren't sensitive enough to peer out very far into space. 23 00:01:22,500 --> 00:01:25,000 Also, we can only see visible light, 24 00:01:25,000 --> 00:01:28,500 but not ultraviolet or infrared light like Hubble can. 25 00:01:28,500 --> 00:01:32,000 That's why for professional astronomers the Hubble Space Telescope 26 00:01:32,000 --> 00:01:34,500 is such an exciting tool to probe the Universe. 27 00:01:36,000 --> 00:01:39,500 Sitting at its vantage point 600 km. above the Earth 28 00:01:39,500 --> 00:01:41,500 Hubble is a window on the Universe. 29 00:01:41,500 --> 00:01:43,500 The journey to make a Hubble image 30 00:01:43,500 --> 00:01:45,500 begins when light from a distant object 31 00:01:45,500 --> 00:01:48,000 starts on its way towards us. 32 00:01:48,000 --> 00:01:51,000 After travelling across the vast distances of space 33 00:01:51,000 --> 00:01:55,000 it is captured by Hubble with its 2.4 metre wide mirror. 34 00:01:55,500 --> 00:01:58,500 The light is then sent to one of Hubble several cameras 35 00:01:58,500 --> 00:02:01,500 where the photons are turned into an electrical charge 36 00:02:01,500 --> 00:02:05,000 by a CCD chip rather similar to the ones in digital cameras. 37 00:02:05,000 --> 00:02:07,500 The Advanced Camera for Surveys, for example, 38 00:02:07,500 --> 00:02:11,000 contains over 16 million picture elements or 'pixels'. 39 00:02:11,500 --> 00:02:14,500 These act as miniature 'buckets' to collect the light. 40 00:02:15,000 --> 00:02:17,000 The camera then reads out how much light 41 00:02:17,000 --> 00:02:19,000 has been captured in each bucket, 42 00:02:19,000 --> 00:02:21,500 the charge within each of the pixels, 43 00:02:21,500 --> 00:02:23,000 and that puts an image. 44 00:02:23,500 --> 00:02:26,500 This readout is then beamed back to the Earth 45 00:02:26,500 --> 00:02:28,000 as a series of encoded numbers 46 00:02:28,000 --> 00:02:31,000 that are stored in archives in the US and Europe. 47 00:02:33,000 --> 00:02:36,500 Hubble's cameras image the Universe through different filters, 48 00:02:37,500 --> 00:02:39,000 like this one. 49 00:02:41,500 --> 00:02:43,500 These select specific wavelengths of light 50 00:02:43,500 --> 00:02:46,500 that are characteristic of different physical processes 51 00:02:46,500 --> 00:02:48,500 which may be going on in different parts 52 00:02:48,500 --> 00:02:50,500 of distant galaxies and nebulae. 53 00:02:51,000 --> 00:02:54,500 Each of these filters results in a single gray-scale image 54 00:02:54,500 --> 00:02:56,500 which is then assigned a colour. 55 00:02:56,500 --> 00:03:00,000 This colour is usually chosen to more or less correspond 56 00:03:00,000 --> 00:03:03,500 to the actual colour of the filter, although this is not always true. 57 00:03:04,000 --> 00:03:07,000 Anywhere between two and six of these images 58 00:03:07,000 --> 00:03:10,000 are then combined to create the final colour image. 59 00:03:12,000 --> 00:03:14,500 Take this view of the colliding Antennae Galaxies. 60 00:03:14,500 --> 00:03:16,500 Hubble imaged this merging pair 61 00:03:16,500 --> 00:03:19,000 through red, green and blue filters 62 00:03:19,000 --> 00:03:22,500 to reveal the different components inside the galaxies. 63 00:03:22,500 --> 00:03:25,500 For example, the red light is coming from old stars 64 00:03:25,500 --> 00:03:28,500 and glowing hydrogen gas, while the blue light 65 00:03:28,500 --> 00:03:30,500 is showing the violent star formation 66 00:03:30,500 --> 00:03:32,500 triggered by the cosmic collision. 67 00:03:33,500 --> 00:03:36,500 The red, green and blue images are then combined 68 00:03:36,500 --> 00:03:39,000 to create the final multi-colour image. 69 00:03:42,000 --> 00:03:44,000 One of the challenges in making images 70 00:03:44,000 --> 00:03:47,000 is that there is a huge range of brightness in nature 71 00:03:47,000 --> 00:03:49,000 from faint to bright objects 72 00:03:49,000 --> 00:03:52,000 and astronomical images are so rich in information 73 00:03:52,000 --> 00:03:55,500 that our eyes and computer screens cannot show their full content. 74 00:03:56,000 --> 00:03:59,500 Nature can be difficult to capture in a single photograph 75 00:03:59,500 --> 00:04:02,500 and most of us have encountered situations like the following. 76 00:04:03,000 --> 00:04:05,500 Imagine you try to take a picture of a landscape. 77 00:04:06,000 --> 00:04:10,000 When you do so you can either capture the bright parts of the sky 78 00:04:10,000 --> 00:04:14,000 or the darker parts of the vegetation, but rarely both together. 79 00:04:14,500 --> 00:04:17,000 The job of the image processing specialists 80 00:04:17,000 --> 00:04:20,000 is to compress this range of brightnesses together 81 00:04:20,000 --> 00:04:22,000 so that we can see all the nuances. 82 00:04:24,000 --> 00:04:27,500 Image experts use the program FITS Liberator, 83 00:04:27,000 --> 00:04:30,000 pioneered be ESA, ESO and NASA, 84 00:04:30,000 --> 00:04:32,000 to produce the magnificent rich image 85 00:04:32,000 --> 00:04:34,500 which can be interpreted by our eyes. 86 00:04:40,500 --> 00:04:42,000 Warning! 87 00:04:44,000 --> 00:04:47,000 10 x slower in reality! 88 00:04:48,000 --> 00:04:51,000 Making Hubble images is fun & highly addictive! 89 00:04:52,000 --> 00:04:55,000 Google FITS LIBERATOR 90 00:05:02,000 --> 00:05:04,500 But is this what we would see with our eyes 91 00:05:04,500 --> 00:05:06,000 if we could look through Hubble? 92 00:05:06,500 --> 00:05:08,000 Well, not really. 93 00:05:08,000 --> 00:05:10,500 Look at this image of the Cigar Galaxy. 94 00:05:10,500 --> 00:05:13,500 This is what Hubble sees in visible light. 95 00:05:13,500 --> 00:05:16,500 Our eyes aren't actually sensitive enough 96 00:05:16,500 --> 00:05:19,500 to be able to detect the faint light from this distant object 97 00:05:19,500 --> 00:05:21,500 even when looking through a telescope. 98 00:05:21,500 --> 00:05:23,500 The reason why Hubble's instruments can do it 99 00:05:23,500 --> 00:05:26,000 is because they can gather and add up the light 100 00:05:26,000 --> 00:05:28,000 over an extended period of time, 101 00:05:28,000 --> 00:05:31,000 which is something our eyes can't do. 102 00:05:32,000 --> 00:05:34,500 Furthermore, some telescopes can 'see' wavelengths 103 00:05:34,500 --> 00:05:36,500 that we can't see with our eyes. 104 00:05:36,500 --> 00:05:39,000 This multi-wavelength view shows us much more 105 00:05:39,000 --> 00:05:42,000 than our eyes or anyone telescope can see. 106 00:05:43,000 --> 00:05:47,000 Parts of this image were made with the Chandra X-ray observatory in X-rays 107 00:05:47,000 --> 00:05:50,500 and part with the Spitzer Space Telescope in infrared light. 108 00:05:52,500 --> 00:05:55,000 In this episode we have seen how the images 109 00:05:55,000 --> 00:05:58,000 that have amazed and intrigued us are created. 110 00:05:58,000 --> 00:06:00,500 You too can have a go at making your own images, 111 00:06:00,500 --> 00:06:03,000 just Google for 'FITS Liberator'. 112 00:06:03,500 --> 00:06:06,000 This is Dr. J signing off for the Hubblecast. 113 00:06:06,000 --> 00:06:10,200 Once again, nature has surprised us beyond our wildest imagination... 114 00:06:12,000 --> 00:06:14,000 Hubblecast is produced by ESA / Hubble 115 00:06:14,000 --> 00:06:16,000 at the European Southern Observatory in Germany. 116 00:06:17,000 --> 00:06:19,000 The Hubble mission is a project of international cooperation 117 00:06:19,000 --> 00:06:21,000 between NASA and the European Space Agency.