1 00:00:00,166 --> 00:00:05,105 Music 2 00:00:05,205 --> 00:00:09,442 The James Webb Space Telescope is exploring the universe 3 00:00:09,809 --> 00:00:13,480 and it's revealed sights humanity has never seen. 4 00:00:13,580 --> 00:00:17,017 Music 5 00:00:17,050 --> 00:00:21,554 So the goals of the first images were to showcase the impressive 6 00:00:21,554 --> 00:00:26,226 capabilities of JWST to the public and to the astronomical community 7 00:00:26,226 --> 00:00:27,127 at large. 8 00:00:27,127 --> 00:00:31,364 And the subsequent images have been taken more for specific science questions 9 00:00:31,364 --> 00:00:34,501 that have been asked by the various groups in the astronomical community. 10 00:00:34,768 --> 00:00:38,104 And so those pictures are much more tied to specific science questions. 11 00:00:38,605 --> 00:00:39,873 And still, they're beautiful. 12 00:00:41,274 --> 00:00:43,676 The JWST mission has taken a long time to get here. 13 00:00:43,676 --> 00:00:45,979 It's been 20, 25 years in production, 14 00:00:46,513 --> 00:00:49,549 and so it's been a lot of effort by a lot of people, 15 00:00:49,549 --> 00:00:53,319 including myself, over a decade and a half myself on the mission. 16 00:00:53,620 --> 00:00:54,988 And so to actually get to the point 17 00:00:54,988 --> 00:00:59,059 where we get to see the pictures, the fruits of all that work was really, 18 00:00:59,526 --> 00:01:02,262 really amazing for me to finally see that come through. 19 00:01:02,429 --> 00:01:04,264 And they were just so spectacular. 20 00:01:04,264 --> 00:01:05,832 It was excellent. 21 00:01:05,832 --> 00:01:08,468 It paid back all that effort and more for me. 22 00:01:09,269 --> 00:01:13,339 So for a team of scientists to get time to actually observe with Webb, 23 00:01:13,740 --> 00:01:15,909 the first thing they need to do is write a proposal. 24 00:01:16,376 --> 00:01:19,846 And so that proposal is a text, but it also comes 25 00:01:19,846 --> 00:01:23,183 with what they want to do, what targets they want to observe, 26 00:01:23,583 --> 00:01:27,787 and which instruments they want to use on JWST and which modes. 27 00:01:27,787 --> 00:01:31,658 And so then that gets put together and submitted, submits here to the Institute. 28 00:01:31,658 --> 00:01:34,294 But then the Institute convenes a panel of experts 29 00:01:34,494 --> 00:01:37,063 from outside the Institute for us all astronomers. 30 00:01:37,430 --> 00:01:40,633 And then they get to rank they look at all the proposals 31 00:01:40,633 --> 00:01:43,903 in a specific area and then rank them, and the top ranked proposals 32 00:01:44,170 --> 00:01:47,240 then get forwarded to actually take their observations. 33 00:01:48,675 --> 00:01:51,544 When a science team is awarded time to work with Webb. 34 00:01:52,011 --> 00:01:55,849 They start by using a special software to set the required parameters 35 00:01:56,015 --> 00:01:58,017 for the telescope to conduct their science. 36 00:01:58,918 --> 00:02:01,754 The software allow scientists to use different modes 37 00:02:01,754 --> 00:02:04,791 on Webb's instruments to achieve their scientific objectives. 38 00:02:05,992 --> 00:02:09,162 When it's time for the observation, the code instructs the telescope 39 00:02:09,229 --> 00:02:12,966 to locate the target object and capture several images of it. 40 00:02:13,199 --> 00:02:17,670 Light from the target object is processed through the instruments and the raw data 41 00:02:17,670 --> 00:02:21,441 the science team requires is stored onto Webb's onboard hard drive. 42 00:02:22,075 --> 00:02:25,845 Once the team's data is collected, their data and images are transmitted 43 00:02:25,845 --> 00:02:26,446 to Earth 44 00:02:26,446 --> 00:02:29,983 from Webb to NASA's Deep Space Network ground stations, 45 00:02:29,983 --> 00:02:34,087 where their data gets routed directly to the Space Telescope Science Institute. 46 00:02:34,888 --> 00:02:37,423 Once we get the data here in Baltimore at the Institute, 47 00:02:37,724 --> 00:02:39,559 then we run it through our pipeline. 48 00:02:39,559 --> 00:02:42,962 That is a series of steps that removes the artifacts 49 00:02:43,029 --> 00:02:45,732 from the instrument or the detectors that we know about, 50 00:02:45,999 --> 00:02:48,401 because we've taken extensive calibration observations 51 00:02:48,735 --> 00:02:52,205 and we now produce these cleaned images that are just about the 52 00:02:52,205 --> 00:02:54,174 astrophysical source we're interested in. 53 00:02:54,174 --> 00:02:57,010 And then the all those images go into an archive here 54 00:02:57,010 --> 00:03:00,547 at the Institute that's then available to the proposers 55 00:03:01,781 --> 00:03:04,417 that they can then download it and start doing their science on it. 56 00:03:04,951 --> 00:03:08,621 So if we're going to produce a color image out of the observations, 57 00:03:08,621 --> 00:03:12,225 then we take we've taken multiple images in different filters. 58 00:03:12,692 --> 00:03:15,461 And then those after they've been processed through 59 00:03:15,461 --> 00:03:17,297 and removed all the instrumental artifacts, 60 00:03:17,297 --> 00:03:21,401 then we pass them along to the experts in our public outreach office 61 00:03:21,734 --> 00:03:26,706 that then turn them into the really sensational color images that we all love. 62 00:03:27,740 --> 00:03:30,743 When you're processing any sort of astronomical image, 63 00:03:31,211 --> 00:03:33,780 those images are taken through different filters. 64 00:03:33,780 --> 00:03:37,050 So the light's captured through different filters and it starts out grayscale. 65 00:03:37,283 --> 00:03:40,220 And then so you actually get color information 66 00:03:40,220 --> 00:03:43,923 from taking the light in those filters, and then you assign colors afterwards 67 00:03:43,923 --> 00:03:46,159 like an image processor will assign colors. 68 00:03:46,326 --> 00:03:48,795 And we do this typically what we call chromatic ordering, 69 00:03:48,795 --> 00:03:51,164 which just means that the shortest wavelengths gets assigned. 70 00:03:51,164 --> 00:03:54,934 The blue color in between it's green, and then the longest wavelength 71 00:03:54,934 --> 00:03:56,269 gets assigned the red color. 72 00:03:56,269 --> 00:03:59,973 And then we additively combine those together to get our full color image. 73 00:04:00,073 --> 00:04:03,109 The reason we want to color the images is because there's actually more 74 00:04:03,109 --> 00:04:04,477 that you can get, more information 75 00:04:04,477 --> 00:04:06,579 that you can get from the image if you see it in color. 76 00:04:06,879 --> 00:04:09,649 If you're looking at a galaxy in optical light, 77 00:04:10,049 --> 00:04:12,318 we expect that they're going to be star forming regions 78 00:04:12,318 --> 00:04:14,887 and they're going to show up as these bright blue regions. 79 00:04:14,887 --> 00:04:18,758 And then if there's hydrogen gas around them, that will show up as bright red. 80 00:04:19,259 --> 00:04:22,028 And so if we can apply the color to the different filters 81 00:04:22,028 --> 00:04:25,164 and make an image in color, you can actually just see that right away. 82 00:04:25,164 --> 00:04:27,433 And you learn something new from the image by seeing it in color. 83 00:04:28,167 --> 00:04:31,537 Webb's imagery and science are revolutionary. 84 00:04:32,438 --> 00:04:36,209 It's challenging our theories of the universe and generating more 85 00:04:36,209 --> 00:04:37,910 questions we need to answer. 86 00:04:37,910 --> 00:04:45,718 Music