1 00:00:05,390 --> 00:00:02,990 as a cosmic photographer NASA's Hubble 2 00:00:08,030 --> 00:00:05,400 Space Telescope has taken over a million 3 00:00:11,629 --> 00:00:08,040 snapshots documenting the universe 4 00:00:14,150 --> 00:00:11,639 these images illustrate explain and 5 00:00:15,829 --> 00:00:14,160 Inspire us with their Grandeur but may 6 00:00:16,910 --> 00:00:15,839 not match what we'd see with our own 7 00:00:19,070 --> 00:00:16,920 eyes 8 00:00:21,529 --> 00:00:19,080 that's because Hubble sees light beyond 9 00:00:24,470 --> 00:00:21,539 our sensitivity 10 00:00:25,970 --> 00:00:24,480 our eyes only sense a small fraction of 11 00:00:28,370 --> 00:00:25,980 the universe's light 12 00:00:30,710 --> 00:00:28,380 this tiny band of wavelengths called the 13 00:00:33,709 --> 00:00:30,720 visible spectrum holds every color in 14 00:00:35,810 --> 00:00:33,719 the rainbow light outside that span with 15 00:00:38,330 --> 00:00:35,820 longer or shorter wavelengths is 16 00:00:40,430 --> 00:00:38,340 invisible to our eyes but those 17 00:00:43,490 --> 00:00:40,440 invisible wavelengths can tell us so 18 00:00:45,590 --> 00:00:43,500 much more about the universe Hubble 19 00:00:47,150 --> 00:00:45,600 House's six scientific instruments that 20 00:00:49,369 --> 00:00:47,160 observe at different wavelengths 21 00:00:52,490 --> 00:00:49,379 together they expand our vision into 22 00:00:54,470 --> 00:00:52,500 infrared and ultraviolet light 23 00:00:57,529 --> 00:00:54,480 that doesn't mean Hubble can show us 24 00:00:59,689 --> 00:00:57,539 never before seeing colors in fact the 25 00:01:01,850 --> 00:00:59,699 telescope can only see the universe in 26 00:01:03,830 --> 00:01:01,860 Shades of Gray 27 00:01:05,870 --> 00:01:03,840 seeing in black and white allows Hubble 28 00:01:08,510 --> 00:01:05,880 to detect subtle differences in the 29 00:01:10,490 --> 00:01:08,520 light's intensity if one wavelength is 30 00:01:12,050 --> 00:01:10,500 brighter than another that tells us 31 00:01:12,969 --> 00:01:12,060 something about the science of that 32 00:01:16,010 --> 00:01:12,979 object 33 00:01:18,469 --> 00:01:16,020 but because color helps humans interpret 34 00:01:20,870 --> 00:01:18,479 what we see NASA Specialists work to 35 00:01:23,710 --> 00:01:20,880 process and colorize publicly available 36 00:01:26,450 --> 00:01:23,720 Hubble data into more accessible images 37 00:01:28,730 --> 00:01:26,460 when Hubble snaps a photo it puts a 38 00:01:31,070 --> 00:01:28,740 filter in front of its detector allowing 39 00:01:33,770 --> 00:01:31,080 specific wavelengths to pass through 40 00:01:34,609 --> 00:01:33,780 Broadband filters let in a wide range of 41 00:01:37,010 --> 00:01:34,619 light 42 00:01:39,649 --> 00:01:37,020 narrowband filters are more selective 43 00:01:42,830 --> 00:01:39,659 isolating light from Individual elements 44 00:01:45,289 --> 00:01:42,840 like hydrogen oxygen and sulfur 45 00:01:47,870 --> 00:01:45,299 Hubble observes the same object multiple 46 00:01:49,969 --> 00:01:47,880 times using different filters image 47 00:01:52,190 --> 00:01:49,979 processors then assign those images a 48 00:01:54,230 --> 00:01:52,200 color based on their filtered wavelength 49 00:01:56,749 --> 00:01:54,240 the longest wavelength becomes red 50 00:01:59,030 --> 00:01:56,759 medium becomes green and the shortest 51 00:02:00,410 --> 00:01:59,040 blue corresponding to the light sensors 52 00:02:02,810 --> 00:02:00,420 in our eyes 53 00:02:05,149 --> 00:02:02,820 combining them gives us a color image 54 00:02:07,789 --> 00:02:05,159 showcasing characteristics we can't make 55 00:02:10,309 --> 00:02:07,799 out in black and white 56 00:02:12,410 --> 00:02:10,319 adding color reveals the underlying 57 00:02:14,449 --> 00:02:12,420 science in every image 58 00:02:17,390 --> 00:02:14,459 it's like translating words into another 59 00:02:18,650 --> 00:02:17,400 language making sure no information is 60 00:02:21,350 --> 00:02:18,660 lost 61 00:02:22,970 --> 00:02:21,360 some words have an exact counterpart the 62 00:02:25,369 --> 00:02:22,980 meaning Remains the Same when you swap 63 00:02:28,369 --> 00:02:25,379 them couple's true color photos are like 64 00:02:32,030 --> 00:02:28,379 that they are a direct translation using 65 00:02:34,430 --> 00:02:32,040 broad filters and wavelengths we can see 66 00:02:37,550 --> 00:02:34,440 other words can't be translated directly 67 00:02:39,770 --> 00:02:37,560 when we use narrowband filters or peer 68 00:02:41,930 --> 00:02:39,780 outside the visible spectrum it's like 69 00:02:45,110 --> 00:02:41,940 translating words with no one word 70 00:02:46,850 --> 00:02:45,120 replacement easily done but requires 71 00:02:48,949 --> 00:02:46,860 more work 72 00:02:51,770 --> 00:02:48,959 narrowband images highlight the 73 00:02:54,050 --> 00:02:51,780 concentration of important elements 74 00:02:56,809 --> 00:02:54,060 infrared images are like heat Maps 75 00:02:59,750 --> 00:02:56,819 helping us spot newborn stars in dark 76 00:03:01,550 --> 00:02:59,760 Dusty clouds and peer further back in 77 00:03:04,430 --> 00:03:01,560 time and space 78 00:03:06,890 --> 00:03:04,440 in ultraviolet we uncover active aurorae 79 00:03:09,350 --> 00:03:06,900 on Jupiter and learn how young massive 80 00:03:12,350 --> 00:03:09,360 stars develop 81 00:03:14,330 --> 00:03:12,360 image processors also clean up artifacts 82 00:03:16,790 --> 00:03:14,340 signatures in an image that aren't 83 00:03:19,490 --> 00:03:16,800 produced by The observed Target as 84 00:03:22,250 --> 00:03:19,500 sensors age some pixels become imperfect 85 00:03:24,009 --> 00:03:22,260 returning too much electrical charge or 86 00:03:27,229 --> 00:03:24,019 not enough 87 00:03:29,290 --> 00:03:27,239 artifacts can leave behind odd shapes or 88 00:03:31,910 --> 00:03:29,300 return images without any true black 89 00:03:33,770 --> 00:03:31,920 these effects can be calibrated and 90 00:03:36,229 --> 00:03:33,780 removed 91 00:03:37,970 --> 00:03:36,239 other artifacts come from the dynamic 92 00:03:39,649 --> 00:03:37,980 environment of space 93 00:03:41,990 --> 00:03:39,659 even the best photographers get 94 00:03:44,809 --> 00:03:42,000 photobombed in Hubble's case the 95 00:03:47,449 --> 00:03:44,819 culprits are asteroids spacecraft or 96 00:03:50,570 --> 00:03:47,459 debris trails and high energy particles 97 00:03:53,030 --> 00:03:50,580 called cosmic rays by combining and 98 00:03:55,430 --> 00:03:53,040 aligning multiple observations image 99 00:03:58,369 --> 00:03:55,440 processors can identify them and piece 100 00:04:00,770 --> 00:03:58,379 together an artifact free image 101 00:04:03,050 --> 00:04:00,780 without processing many Hubble images 102 00:04:05,930 --> 00:04:03,060 would be divided down the middle 103 00:04:08,869 --> 00:04:05,940 this line called a chip Gap is the tiny 104 00:04:10,670 --> 00:04:08,879 space between some camera sensors Hubble 105 00:04:13,070 --> 00:04:10,680 moves slightly with each observation 106 00:04:15,470 --> 00:04:13,080 allowing image processors to fill the 107 00:04:18,229 --> 00:04:15,480 Gap and replace faulty pixels 108 00:04:20,990 --> 00:04:18,239 this process is called dithering 109 00:04:23,810 --> 00:04:21,000 and because there's no natural up or 110 00:04:27,050 --> 00:04:23,820 down in space processors decide how to 111 00:04:29,870 --> 00:04:27,060 rotate and frame the image 112 00:04:32,450 --> 00:04:29,880 it's a time consuming procedure simple 113 00:04:34,610 --> 00:04:32,460 images take about a week while large 114 00:04:39,650 --> 00:04:34,620 mosaics stitch together from many 115 00:04:45,230 --> 00:04:42,230 Hubble images may not be what we'd see 116 00:04:47,030 --> 00:04:45,240 firsthand instead they are tools for 117 00:04:49,610 --> 00:04:47,040 understanding science at a glance 118 00:04:52,990 --> 00:04:49,620 shedding light on otherwise invisible