{"id":24785,"date":"2021-11-22T00:28:58","date_gmt":"2021-11-21T16:28:58","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/unfolding-the-universe-the-commissioning-process-of-the-james-webb-space-telescope\/"},"modified":"2021-11-22T00:28:58","modified_gmt":"2021-11-21T16:28:58","slug":"unfolding-the-universe-the-commissioning-process-of-the-james-webb-space-telescope","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/unfolding-the-universe-the-commissioning-process-of-the-james-webb-space-telescope\/","title":{"rendered":"Unfolding the universe: the commissioning process of the James Webb Space Telescope"},"content":{"rendered":"<p>This December, an Ariane 5 rocket will launch from Kourou, French Guiana carrying the most complicated telescope ever developed \u2014 the joint NASA\/ESA\/CSA James Webb Space Telescope. However, when the telescope launches, it will not immediately be ready for scientific observations. In fact, the telescope won\u2019t perform any observations until about six months after launch.<\/p>\n<p>Following separation from the Ariane 5 second stage, James Webb will spend the next month deploying all of its instruments, mirrors, and structural systems that will be used for scientific observations. Once the telescope reaches its orbit at Earth-Sun Lagrange Point 2 (L2), it will spend up to six months performing tests and calibrating systems for observations.<\/p>\n<\/p>\n<p>This entire deployment and testing process is called commissioning and it&nbsp;is a vital part of a spacecraft\u2019s life and ultimately determines if a spacecraft will be able to properly function as expected. For James Webb, commissioning is an extremely important process that the entire telescope team will monitor.<\/p>\n<p>To gain insight into James Webb\u2019s commissioning process and what the process will be like for the team, NASASpaceflight spoke with Keith Parrish, James Webb\u2019s Observatory Manager and Commissioning Lead.<\/p>\n<p>\u201cCommissioning actually starts when the rocket leaves the ground. So once Ariane 5 takes off, that\u2019s when we say commissioning is starting,\u201d Parrish said.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-82131\" class=\" wp-image-82131\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-350x248.jpeg\" alt=\"\" width=\"827\" height=\"586\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-350x248.jpeg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-494x350.jpeg 494w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-768x544.jpeg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-1920x1360.jpeg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/Artist_s_view_of_Webb_on_an_Ariane_5_rocket-scaled-1-1170x829.jpeg 1170w\" sizes=\"(max-width: 827px) 100vw, 827px\"><\/p>\n<p id=\"caption-attachment-82131\" class=\"wp-caption-text\">Artist\u2019s depiction of Ariane 5 fairing seperation during the launch of JWST. (Credit: ESA)<\/p>\n<p>\u201cSo commissioning really starts with that first day of activities, which is getting safely on orbit. That\u2019s our entire goal. We\u2019re completely focused on just getting the observatory on orbit safely. We define \u2018safe\u2019 as Webb is talking to the ground, its solar arrays are deployed and generating power, and we\u2019re on our way to L2. It\u2019s a really fast compressed time period from the time that James Webb leaves the ground to it getting on orbit.\u201d<\/p>\n<p>\u201cSo now we\u2019re on orbit. Now we do a mid-course correction phase. That\u2019s where we will actually use Webb\u2019s thrusters to take out any of the errors that Ariane 5 gave us. We tell the Ariane 5 team to send us in a certain direction at a certain velocity, and they\u2019ll get us really, really close to that target. We\u2019re talking [40,200 km\/h], though, so we may have to put in a few meters per second of velocity [to get to the exact velocity and direction]. So we\u2019re talking little tiny puffs from our onboard thruster system.\u201d<\/p>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>\u201cWe do in that first day, about 12 and a half hours after launch. We\u2019ll see how that first mid-course correction went and then about two days later we\u2019ll do another small correction. The corrections will start getting smaller and really narrowing us down so that we\u2019re right on that track to get to L2.\u201d<\/p>\n<p>After this, perhaps the most critical aspect of James Webb\u2019s mission is up next \u2014 deployments.<\/p>\n<p>\u201cAbout three or four days after launch is actually when we go into our deployments phase.<\/p>\n<p>\u201cWe\u2019ll start our deployment phases with our sunshield deployment. We have very large pallets that are 20 to 30 feet tall that hold all of our membrane material [for the sunshield]. We have five small and very thin membranes that constitute our sunshield, and we have to unfold all that material and get it pulled into place. We start by lowering the front and back pallets down, and that takes about a day. Then over the next two to three days, we start releasing all of our release devices [on the sunshield and pallets]. We have about 170 released devices that we fire to actually release all this material and structures over the sunshield\u2019s deployment phase. Between day three and day six, we actually get the sunshield fully deployed.\u201d<\/p>\n<p>\u201cAlso in that period, we start to see rapid cooling of our telescope and its instruments once we get that sunshield out.\u201d<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-82133\" class=\" wp-image-82133\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-350x267.jpg\" alt=\"\" width=\"881\" height=\"672\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-350x267.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-459x350.jpg 459w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-768x586.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-1920x1465.jpg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/48936479373_aedba34e60_o-1170x893.jpg 1170w\" sizes=\"(max-width: 881px) 100vw, 881px\"><\/p>\n<p id=\"caption-attachment-82133\" class=\"wp-caption-text\">James Webb\u2019s sunshield fully deployed. (Credit: NASA\/Chris Gunn)<\/p>\n<p>Next up is the deployment of James Webb\u2019s 6.5 m diameter mirror \u2014 one of the largest mirrors ever flown into space, and the most complex space telescope mirror ever built.<\/p>\n<p>\u201cSo our telescope consists of our primary mirror, which is made of eighteen individual mirror segments. For launch, we fold back six of the segments so Webb will fit inside the launch vehicle. Then, we have a secondary mirror. That secondary mirror is actually what takes in all the light that gets collected by the main mirror and puts the light down into our cameras and our instrument systems.&nbsp; The secondary mirror is kind of mounted on a tripod that is broken up into different links and folded back onto the primary mirror. So we fold the secondary mirror out and then we fold out the two wings of the primary mirror.\u201d<\/p>\n<p>\u201cSomewhere around the 10 to 14-day range, we feel like we will have the primary and secondary mirror fully deployed,\u201d Parrish said.<\/p>\n<p>NASASpaceflight recently spoke with James Webb\u2019s Optical Telescope Element Manager about the mirror\u2019s systems and complexity.<\/p>\n<\/p>\n<p><iframe title=\"The Webb Telescope's Unfolding Secondary Mirror\" src=\"https:\/\/www.youtube.com\/embed\/DxQ3QI0s6sc?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen=\"\" name=\"fitvid0\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>Next, the James Webb mirror team will start working on aligning each of the 18 individual mirror segments. Each mirror features its own motor that allows the team to \u201cwiggle\u201d them all into alignment.<\/p>\n<p>\u201cThen we get into a period of time where our optical folks will take about two weeks to start [aligning] those 18 mirrors around. Also during this time, we\u2019re turning on a lot of other electronics on the telescope. We\u2019re getting the spacecraft more and more up and running as we bring more and more systems online.\u201d<\/p>\n<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>James Webb Space Telescope UPDATES<\/li>\n<li>L2 Future Spacecraft<\/li>\n<li>Click here to Join L2<\/li>\n<\/ul>\n<p>\u201cAnd then, somewhere about 30 days into the mission, we\u2019ve confirmed that everything moves and that everything is deployed.\u201d<\/p>\n<p>For James Webb and its teams back on Earth, the next step in commissioning is L2 orbital insertion.<\/p>\n<p>\u201cNext, we\u2019ll do one final mid-course correction burn that will insert us into our orbit at Lagrange Point 2, or L2,\u201d Parrish said.&nbsp;\u201cThat first 30 days is action-packed and very exciting. It doesn\u2019t stop; it\u2019s just one activity after another, but then it actually quiets down. Over the next, two to three months we\u2019re going to be focused on our instruments and the telescope.\u201d<\/p>\n<p>But to do that, the telescope needs to be properly cooled down.<\/p>\n<p>\u201cIt takes probably three to four months to get everything down to the 30 to 50 Kelvin temperature ranges that [most instruments] need. But during that time, our optical team is continuing to align the telescope. They\u2019re continuing to do something called a wavefront sensing exercise. That\u2019s where they\u2019ll use one of the cameras to actually retrieve what we call the wavefront, which is really an optical metric for how aligned the telescope is. Then, based on that data, it all comes down to the ground software to figure out all the little tiny movements that need to occur to get those 18 segments, perfectly aligned. We are really talking about nanometer precision at this point. We have small mechanisms that can move these mirrors in extremely small amounts.\u201d<\/p>\n<p><iframe id=\"twitter-widget-1\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: static; visibility: visible; width: 550px; height: 604px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-1&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1459261096011997185&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2021%2F11%2Fcommissioning-jwst-1%2F&amp;sessionId=175cec5e8da58142b12688a29b03d58f2d657517&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1459261096011997185\"><\/iframe><\/p>\n<p>\u201cWe do something called fine guiding during this period as well. That\u2019s actually where we bring our Canadian instrument, the fine guidance sensor,&nbsp;FGS, online. It\u2019s basically a really, really high precision star tracker which lets the telescope point to its astronomical targets. That takes about two to four months.\u201d<\/p>\n<p>At this point, the sunshield has allowed James Webb to cool to its expected temperatures for observations. But how does James Webb cool some of its instruments, and how do the instrument teams work to adapt their instruments to the temperatures?<\/p>\n<p>\u201cWe have a mechanical cryocooler that cools the instruments down to the temperature we need. We\u2019re getting very, very close to absolute zero on one of our instruments. It\u2019s the mid-infrared instrument (MIRI), and that instrument requires a mechanical cryocooler. So we\u2019re also bringing that cooler system online. That cooler system generates vibrations, so our optical team and our cooler team are working together to tune that cooler to make sure that those vibrations don\u2019t interfere with the optical performance of the telescope,\u201d Parrish said.<\/p>\n<p>After this, James Webb gets turned over to the instrument teams.<\/p>\n<p>\u201cWe have four instruments, and [those teams] will then go through a series of calibration exercises with those instruments. These exercises range from thermal stability measurements to looking at dark areas to just calibrating out all of the artifacts in the instruments that would interfere with science observations.\u201d<\/p>\n<p>This delicate work will take about two months, bringing the total commissioning phase to about six months total.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-82135\" class=\" wp-image-82135\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2-350x248.jpeg\" alt=\"\" width=\"869\" height=\"616\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2-350x248.jpeg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2-494x350.jpeg 494w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2-768x544.jpeg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2-1170x829.jpeg 1170w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/11\/isim2.jpeg 1200w\" sizes=\"(max-width: 869px) 100vw, 869px\"><\/p>\n<p id=\"caption-attachment-82135\" class=\"wp-caption-text\">The four instruments onboard the James Webb Space Telescope. (Credit: NASA)<\/p>\n<p>With such a complex commissioning and deployment process, redundancy is needed for a lot of instruments and spacecraft systems. So, how much redundancy is built into the deployment and commissioning sequence? What if a specific system fails to deploy? How long does the team have to fix the issue in the deployment\/commissioning timeframe before running into serious issues?<\/p>\n<p>\u201cRedundancy is important, and obviously we paid a lot of attention to what we implemented in our systems. Though the one thing we really wanted to make sure of is that when it comes to our deployments we are not on any clock. We can go as slow as we want to keep the entire Observatory safe,\u201d Parrish said.<\/p>\n<p>\u201cFor instance, we get one wing of the telescope out and the other one is being a little fussy. We\u2019re not in any rush to worry about that. We can stand down and take plenty of time to assess it and then get back to it. So one of the keys is that we can go as slow as necessary, and it doesn\u2019t have to be a big problem. It can just be \u2018this looks a little odd to us\u2019 and we can slow everything down and take our time.\u201d<\/p>\n<p>However, there\u2019s always an outlier.<\/p>\n<p>\u201cWe do have one deployment that we would call time-critical, and it\u2019s our solar array \u2014 which is all autonomous, though. That\u2019s typical of any spacecraft that\u2019s launched; you want to get that solar array unfurled, deployed, and producing power.\u201d<\/p>\n<p>\u201cBut remember those 170 release devices? In their natural state, mechanically they want to be released. So we did a lot of work to make sure they don\u2019t release prematurely. These release devices are also electrically redundant. We have two different systems that can actually release those devices.\u201d<\/p>\n<\/p>\n<p><iframe title=\"29 Days on the Edge\" src=\"https:\/\/www.youtube.com\/embed\/uUAvXYW5bmI?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen=\"\" name=\"fitvid1\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>And that electrical redundancy is true for the entire telescope as well.<\/p>\n<p>\u201cElectrically, we are fully redundant. We have two computers on board that control all of our deployments. We have one primary and then we have a complete secondary backup computer that can handle all of our deployments, so all of our wiring is completely redundant as well.\u201d<\/p>\n<p>This electrical redundancy fills a role that wasn\u2019t possible for a large part of James Webb \u2014 you can\u2019t be backups for every system on board.<\/p>\n<p>\u201cLet\u2019s just take the sunshield, for instance. You can\u2019t have two sunshields. So you can\u2019t have one sunshield that doesn\u2019t work and have a full backup of that. That\u2019s obviously not feasible at all. So we introduced mechanical redundancy into the system.\u201d<\/p>\n<p>\u201cWhat we ended up getting into is that the efforts we made to make something more reliable actually made it less reliable because we introduced more parts, so we\u2019ve actually had to balance that.&nbsp;So now, when it comes to something like a motor, we have what\u2019s called dual windings. There are two sets of windings in the motor that can be accessed by those two computers. There are also two sets of wiring. So we can always have redundancy in our motors electrically all the way through the system,\u201d Parrish said.<\/p>\n<p>James Webb is currently slated to launch atop an Ariane 5 rocket from Kourou, French Guiana on December 18, 2021.<\/p>\n<p><em>(Lead image: Engineers inspect the secondary mirror of James Webb following a deployment test. Credit: NASA\/Chris Gunn)<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This December, an Ariane 5 rocket will launch from Kourou, French Guiana carrying the most complicated telescope ever developed \u2014 the joint NASA\/ESA\/CSA James Webb Space Telescope. However, when the telescope launches, it will not immediately be ready for scientific observations. In fact, the telescope won\u2019t perform any observations until about six months after launch. [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[1540,1661,421,246,7970,1691,190],"class_list":["post-24785","post","type-post","status-publish","format-standard","hentry","category-news","tag-ariane-5","tag-astronomy","tag-csa","tag-esa","tag-james-webb","tag-jwst","tag-nasa"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24785"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=24785"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24785\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=24785"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=24785"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=24785"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}