{"id":915,"date":"2019-12-18T03:11:40","date_gmt":"2019-12-18T03:11:40","guid":{"rendered":"http:\/\/jwst.astro.umontreal.ca\/?page_id=915"},"modified":"2022-03-07T21:35:55","modified_gmt":"2022-03-07T21:35:55","slug":"canadas-role","status":"publish","type":"page","link":"https:\/\/jwst.astro.umontreal.ca\/?page_id=915","title":{"rendered":"Canada&#8217;s Role"},"content":{"rendered":"<div id=\"attachment_916\" style=\"width: 574px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-916\" class=\"wp-image-916\" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/JWST-300x169.png\" alt=\"\" width=\"564\" height=\"318\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/JWST-300x169.png 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/JWST-1024x576.png 1024w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/JWST-768x432.png 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/JWST.png 1280w\" sizes=\"auto, (max-width: 564px) 100vw, 564px\" \/><p id=\"caption-attachment-916\" class=\"wp-caption-text\">Credit: Northrop Grumman.<\/p><\/div>\n<p><span style=\"color: #000000;\">The Webb Telescope is set to be the most important space telescope of the next decade.\u00a0<\/span><span style=\"color: #000000;\">As a collaborating member of the mission, Canada has a unique opportunity to highlight its technical and scientific expertise in space astronomy through its instrument contributions to the mission and continued support to scientists from Canadian institutions working on the Webb team.<\/span><\/p>\n<p><span style=\"color: #000000;\">In exchange for its contributions, Canada receives a <a href=\"http:\/\/jwst.astro.umontreal.ca\/?page_id=915#Canada_Programs\">guaranteed share of Webb\u2019s observing time<\/a>, ensuring immediate scientific discoveries for Canadian scientists.<\/span><\/p>\n<p>&nbsp;<\/p>\n<h3 id=\"Canada_Instruments\"><span style=\"color: #000000;\"><strong>CANADIAN INSTRUMENTS<\/strong><\/span><\/h3>\n<div id=\"attachment_917\" style=\"width: 606px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-917\" class=\"wp-image-917\" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/FGS_NIRISS-300x169.png\" alt=\"\" width=\"596\" height=\"336\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/FGS_NIRISS-300x169.png 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/FGS_NIRISS-1024x576.png 1024w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/FGS_NIRISS-768x432.png 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/FGS_NIRISS.png 1280w\" sizes=\"auto, (max-width: 596px) 100vw, 596px\" \/><p id=\"caption-attachment-917\" class=\"wp-caption-text\">Canada\u2019s contributions to the Webb Telescope, the Fine Guidance Sensor (FGS) and the Near-Infrared Imager and Slitless Spectrograph (NIRISS), was delivered in a single unit to NASA\u2019s Goddard Space Flight Center in 2012. Credit: NASA.<\/p><\/div>\n<p><span style=\"color: #000000;\">Canada contributed both the Fine Guidance Sensor (FGS) and the Near-Infrared Imager and Slitless Spectrograph(NIRISS) instrument to the Webb telescope. Both components have been packaged together into a single unit the size of a washing machine that weighs about 150 kilograms.<\/span><\/p>\n<h5><span style=\"color: #000000;\"><strong>Fine Guidance Sensor<\/strong><strong>\u00a0<\/strong><\/span><\/h5>\n<p><span style=\"color: #000000;\">When a telescope wants to take clear images, it needs to point towards the object it is studying and carefully track it in the sky. Webb will move into position for observations using a system of gyroscopes, but it will also need to know where to look.<\/span><\/p>\n<p><span style=\"color: #000000;\">The Canadian-made Fine Guidance Sensor is an infrared camera that acts as Webb\u2019s eyes. To get clear and detailed pictures of the Universe, Webb uses the FGS to lock on a star position with very high precision.<\/span><\/p>\n<p><span style=\"color: #000000;\">The FGS and Webb\u2019s system of gyroscopes work together with the final optical piece in Webb called the fine steering mirror (FSM) to stabilise the light beam coming from deep space objects. With input from the FGS, the FSM can tip and tilt tiny amounts very quickly to correct for a jittery lightbeam without having to move the entire telescope. All scientific observations taken by Webb involve the use of the FGS.<\/span><\/p>\n<h5><span style=\"color: #000000;\"><strong>Near-Infrared Imager and Slitless Spectrograph<\/strong><\/span><\/h5>\n<p><span style=\"color: #000000;\">Canada\u2019s Near-Infrared Imager and Slitless Spectrograph photographs and gathers spectra from many types of celestial objects. A spectrum shows exactly how bright an object is at many different wavelengths, or colours. This gives detailed information on the characteristics of the observed object. NIRISS uses an infrared camera sensitive to infrared light between 0.6 and 5.0 microns. Once it has captured the infrared light of an object, the light can be broken up into a spectrum using a tool called a grism which is similar to the prisms used to break up sunlight into a rainbow.<\/span><\/p>\n<p><span style=\"color: #000000;\">NIRISS also has another mode that allows it to take an image and spectra simultaneously using a technique called interferometry which allows scientists to examine objects that are very close together.<\/span><\/p>\n<p><span style=\"color: #000000;\">NIRISS and all the other scientific instruments will be turned on when they are needed for specific science programs. Commands to do this will be sent from the Webb Science and Operation Center at the Space Telescope Science Institute in Baltimore, USA.<\/span><\/p>\n<p><span style=\"color: #000000;\">NIRISS will be able to study the atmospheres of exoplanets and determine their composition, observe distant galaxies and examine objects that are very close together in the sky.<\/span><\/p>\n<p>&nbsp;<\/p>\n<h3 id=\"Canada_Team\"><span style=\"color: #000000;\"><strong>THE CANADIAN TEAM<\/strong><\/span><\/h3>\n<div id=\"attachment_918\" style=\"width: 519px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-918\" class=\"wp-image-918\" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/IMG_1866-300x200.jpg\" alt=\"\" width=\"509\" height=\"339\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/IMG_1866-300x200.jpg 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/IMG_1866.jpg 720w\" sizes=\"auto, (max-width: 509px) 100vw, 509px\" \/><p id=\"caption-attachment-918\" class=\"wp-caption-text\">Part of the Canadian JWST Team at a meeting at Honeywell in Kanata, Ontario in 2019.<\/p><\/div>\n<p><span style=\"color: #000000;\">The Webb science project in Canada is led by:<\/span><\/p>\n<ul>\n<li><span style=\"color: #000000;\"><strong>Principal Investigator<\/strong>: Prof. Ren\u00e9 Doyon, Universit\u00e9 de Montr\u00e9al<\/span><\/li>\n<li><span style=\"color: #000000;\"><strong>Project Scientist<\/strong>: Dr. Chris Willott, NRC-Herzberg Astronomy &amp; Astrophysics<\/span><\/li>\n<\/ul>\n<p><span style=\"color: #000000;\">Researchers from a number of other universities and institutes also make up the <a href=\"http:\/\/jwst.astro.umontreal.ca\/?page_id=485\">Canadian Webb science team<\/a>:<\/span><\/p>\n<ul>\n<li><span style=\"color: #000000;\">NRC-Herzberg Astronomy &amp; Astrophysics<\/span><\/li>\n<li><span style=\"color: #000000;\">Saint-Mary\u2019s University<\/span><\/li>\n<li><span style=\"color: #000000;\">Universit\u00e9 de Montr\u00e9al<\/span><\/li>\n<li><span style=\"color: #000000;\">University of Toronto<\/span><\/li>\n<li><span style=\"color: #000000;\">York University<\/span><\/li>\n<li><span style=\"color: #000000;\">Cornell University<\/span><\/li>\n<li><span style=\"color: #000000;\">Space Telescope Science Institute<\/span><\/li>\n<li><span style=\"color: #000000;\">University of Michigan<\/span><\/li>\n<li><span style=\"color: #000000;\">University of Rochester<\/span><\/li>\n<\/ul>\n<p><span style=\"color: #000000;\"><strong>Instrument Team<\/strong><\/span><\/p>\n<p><span style=\"color: #000000;\">Funding for the Canadian portion of the Webb mission is provided by the Canadian Space Agency. The FGS\/NIRISS unit was built, tested and maintained by Honeywell. Scientists from a number of other institutes have also worked on the Canadian instrument and guidance sensor:<\/span><\/p>\n<ul>\n<li><span style=\"color: #000000;\">NASA<\/span><\/li>\n<li><span style=\"color: #000000;\">Space Telescope Science Institute<\/span><\/li>\n<li><span style=\"font-size: 0.9em; color: #000000;\">Universit\u00e9 de Montr\u00e9al<\/span><\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<h3 id=\"Canada_Science\"><span style=\"color: #000000;\"><strong>CANADIAN SCIENCE PROGRAMS<\/strong><\/span><\/h3>\n<p><span style=\"color: #000000;\">Canadian scientists will be some of the first to use data taken by the Webb Telescope to make new discoveries about the Universe.<\/span><\/p>\n<p><span style=\"color: #000000;\">Thanks to the CSA\u2019s important contribution to the mission, Canada has guaranteed access to approximately 5% of Webb\u2019s observing time reserved for programs selected through a competitive process for the<strong> General Observations (GO) program<\/strong>. These science programs will be chosen on a yearly basis while Webb is operational.<\/span><\/p>\n<p><span style=\"color: #000000;\">Canada\u2019s contribution of the NIRISS scientific instrument and the Fine Guidance Sensor has also secured 450 hours of Webb time through the <strong>Guaranteed Time Observations (GTO)<\/strong> program during the first few years of the mission.<\/span><\/p>\n<p><span style=\"color: #000000;\">Finally, one Canadian-led science programs has been selected for the competitive <strong>Early Release Science (ERS)<\/strong> program which will have priority time during Webb\u2019s first year of observing.<\/span><\/p>\n<h5 class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">Guaranteed Time Observations (GTO) Programs<\/span><\/b><\/span><\/h5>\n<p class=\"Body\"><span style=\"color: #000000;\"><span lang=\"EN-US\">In exchange for the Canadian instrument contributions, the Canadian Webb science team have been allotted 450 hours of guaranteed observing time on the Canadian NIRISS instrument and Webb\u2019s other instruments.<\/span><span lang=\"EN-US\">\u00a0<\/span><\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">Seven small programs tackling subjects such as rogue planets, brown dwarfs and exoplanets will account for 47 of these hours. The remaining 403 hours will be split between two main programs. Click <a href=\"http:\/\/jwst.astro.umontreal.ca\/?page_id=523\">here<\/a> for a full list of the Canadian GTO programs.<\/span><\/p>\n<p class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">CANUCS: CAnadian NIRISS Unbiased Cluster Survey<\/span><\/b><\/span><\/p>\n<div id=\"attachment_920\" style=\"width: 467px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-920\" class=\"wp-image-920 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ChrisWillott_CANUCS-300x216.jpg\" alt=\"\" width=\"457\" height=\"329\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ChrisWillott_CANUCS-300x216.jpg 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ChrisWillott_CANUCS-1024x736.jpg 1024w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ChrisWillott_CANUCS-768x552.jpg 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ChrisWillott_CANUCS.jpg 1200w\" sizes=\"auto, (max-width: 457px) 100vw, 457px\" \/><p id=\"caption-attachment-920\" class=\"wp-caption-text\">Dr. Chris Willott, JWST Project Scientist, presents the CANUCS program. Credit: RASC Victoria.<\/p><\/div>\n<p class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">Lead<\/span><\/b><span lang=\"EN-US\">: Dr. Chris Willott, NRC-Herzberg<br \/>\n<\/span><b><span lang=\"EN-US\">Program time<\/span><\/b><span lang=\"EN-US\">: 199 hours<br \/>\n<\/span><b><span lang=\"EN-US\">Instruments used:\u00a0<\/span><\/b><span lang=\"EN-US\">NIRISS, NIRCam, NIRSpec<br \/>\n<\/span><b><span lang=\"EN-US\">Goal<\/span><\/b><span lang=\"EN-US\">: Study some of the first galaxies ever formed; understand the evolution of dwarf galaxies across time<\/span><\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">The CANUCS program will observe very early galaxies using a technique called gravitational lensing. Massive groups of galaxies called clusters can warp and magnify light from very early galaxies, making them easier to observe.<\/span><\/p>\n<div id=\"attachment_921\" style=\"width: 553px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-921\" class=\"wp-image-921 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/GravLensing-300x225.jpg\" alt=\"\" width=\"543\" height=\"407\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/GravLensing-300x225.jpg 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/GravLensing-1024x768.jpg 1024w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/GravLensing-768x576.jpg 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/GravLensing.jpg 1280w\" sizes=\"auto, (max-width: 543px) 100vw, 543px\" \/><p id=\"caption-attachment-921\" class=\"wp-caption-text\">Large masses such as galaxy clusters can deform spacetime. They act like a gravitational lens that deforms the light emitted by background galaxies. The background galaxies can also be magnified, making them easier to observe. Credit: NASA\/ESA\/L. Cal\u00e7ada.<\/p><\/div>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">The NIRISS instrument will collect images and spectra from these galaxies at different periods of the Universe&#8217;s history. This will help scientists better understand how galaxies evolved over time.<\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">Webb\u2019s large mirror will be especially useful to observe very small galaxies called dwarf galaxies. The CANUCS program will also help us better understand dark matter and star formation in very large galaxy clusters.<\/span><\/p>\n<p class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">NEAT: NIRISS Exploration of the Atmospheric diversity of Transiting exoplanets<\/span><\/b><\/span><\/p>\n<div id=\"attachment_922\" style=\"width: 391px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-922\" class=\"wp-image-922 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-300x290.jpg\" alt=\"\" width=\"381\" height=\"368\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-300x290.jpg 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-1024x990.jpg 1024w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-768x743.jpg 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-1536x1486.jpg 1536w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/DavidLafreniere_UdeM-2048x1981.jpg 2048w\" sizes=\"auto, (max-width: 381px) 100vw, 381px\" \/><p id=\"caption-attachment-922\" class=\"wp-caption-text\">Prof. David Lafreni\u00e8re, a member of the JWST Science Team, is leading the NEAT science program. Credit: Luc Turbide\/Universit\u00e9 de Montr\u00e9al.<\/p><\/div>\n<p class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"FR\">Lead<\/span><\/b><span lang=\"FR\">: Prof. David Lafreni\u00e8re, Universit\u00e9 de Montr\u00e9al<br \/>\n<\/span><b><span lang=\"EN-US\">Program time<\/span><\/b><span lang=\"EN-US\">: 204 hours<br \/>\n<\/span><b><span lang=\"EN-US\">Instrument used:\u00a0<\/span><\/b><span lang=\"EN-US\">NIRISS<br \/>\n<\/span><b><span lang=\"EN-US\">Goal<\/span><\/b><span lang=\"EN-US\">: Observe and study the atmospheres of exoplanets, including their composition and temperature<\/span><\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">The NEAT program will study exoplanets, planets that orbit stars other than the Sun. Exoplanets are often detected when they pass, or transit, in front of their parent star and dim its light.<\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">While the exoplanet itself blocks the star\u2019s light, some of the starlight passes through the exoplanet\u2019s atmosphere. The NIRISS instrument will collect the spectra of this starlight which will show signatures of certain molecules found in the exoplanets\u2019 atmospheres. This method is called transit spectroscopy.<\/span><\/p>\n<div id=\"attachment_923\" style=\"width: 589px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-923\" class=\"wp-image-923 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/TransitSpectroscopy-300x200.jpg\" alt=\"\" width=\"579\" height=\"386\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/TransitSpectroscopy-300x200.jpg 300w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/TransitSpectroscopy-768x512.jpg 768w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/TransitSpectroscopy.jpg 948w\" sizes=\"auto, (max-width: 579px) 100vw, 579px\" \/><p id=\"caption-attachment-923\" class=\"wp-caption-text\">When starlight passes through a planet\u2019s atmosphere, certain parts of the light are absorbed by the atmosphere\u2019s elements. By studying the starlight with these absorption lines, scientists can determine the composition of the planet\u2019s atmosphere. Credit: Christine Daniloff\/MIT, Julien de Wit.<\/p><\/div>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">Some of the NEAT program\u2019s targets are rocky planets like Earth. The NEAT team hopes to make the very first detection of an atmosphere on such a planet. This could give us clues on whether or not these planets are habitable.<\/span><\/p>\n<h5 class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">Early Release Science (ERS) Programs<\/span><\/b><\/span><\/h5>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">To quickly make the most of Webb\u2019s full science potential, a part of Webb\u2019s first five months of operations has been dedicated to special Early Release Science (ERS) programs.<\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">The proposed ERS programs went through a competitive process before being chosen based on their scientific merit and benefit for the global astronomical community.<\/span><\/p>\n<p class=\"Body\"><span lang=\"EN-US\" style=\"color: #000000;\">One of the 13 chosen ERS programs is led by a Canadian astronomer.<\/span><\/p>\n<p class=\"Body\"><span style=\"color: #000000;\"><b><span lang=\"EN-US\">Radiative Feedback from Massive Stars as Traced by Multiband Imaging and Spectroscopic Mosaics<\/span><\/b><\/span><\/p>\n<div id=\"attachment_924\" style=\"width: 316px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-924\" class=\"wp-image-924 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ElsPeeters-200x300.jpg\" alt=\"\" width=\"306\" height=\"459\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ElsPeeters-200x300.jpg 200w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/ElsPeeters.jpg 585w\" sizes=\"auto, (max-width: 306px) 100vw, 306px\" \/><p id=\"caption-attachment-924\" class=\"wp-caption-text\">Prof. Els Peeters leads one of 13 ERS programs on Webb during its first year. Credit: Western University.<\/p><\/div>\n<p><span style=\"color: #000000;\"><strong>Lead<\/strong>: Prof. Els Peeters, Western University<\/span><br \/>\n<span style=\"color: #000000;\"><strong>Program time<\/strong>: 28 hours<\/span><br \/>\n<span style=\"color: #000000;\"><strong>Instruments used:\u00a0<\/strong>NIRCam, NIRSpec, MIRI<\/span><br \/>\n<span style=\"color: #000000;\"><strong>Goal<\/strong>: Study the interaction between light emitted by very massive stars and their surrounding environment and how this affects the material between stars called the interstellar medium (ISM)<\/span><\/p>\n<p><span style=\"color: #000000;\">The space between stars is often filled with gas and dust that can be heated by the light produced by these stars. This heating can be so intense that the gas and dust\u2019s chemistry will change and the molecules will break down \u2014 or dissociate. These regions are called Photodissociation Regions (PDRs).<\/span><\/p>\n<div id=\"attachment_925\" style=\"width: 518px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-925\" class=\"wp-image-925 \" src=\"http:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/OrionBar-279x300.jpg\" alt=\"\" width=\"508\" height=\"546\" srcset=\"https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/OrionBar-279x300.jpg 279w, https:\/\/jwst.astro.umontreal.ca\/wp-content\/uploads\/OrionBar.jpg 586w\" sizes=\"auto, (max-width: 508px) 100vw, 508px\" \/><p id=\"caption-attachment-925\" class=\"wp-caption-text\">The Great Nebula in Orion is a region of space where stars are being formed from clouds of dust. The bar visible in the lower left quarter of the image is Orion\u2019s Bar, a photodissociation region (PDR), where starlight is heating up and changing the nearby gas. Credit: NASA\/C. O\u2019Dell\/S. Wong.<\/p><\/div>\n<p><span style=\"color: #000000;\">One well known example of a PDR is Orion\u2019s Bar, which is part of Orion\u2019s Nebula located in the Orion constellation.<\/span><\/p>\n<p><span style=\"color: #000000;\">A large part of the infrared light in galaxies is produced by these PDRs. Studying the chemical and physical processes happening in these regions will allow scientists to better understand how stars interact with their environment.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The Webb Telescope is set to be the most important space telescope of the next decade.\u00a0As a collaborating member of the mission, Canada has a unique opportunity to highlight its technical and scientific expertise in space astronomy through&#8230; <a class=\"read-more\" href=\"https:\/\/jwst.astro.umontreal.ca\/?page_id=915\">Read More<\/a><\/p>\n","protected":false},"author":3,"featured_media":0,"parent":893,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-915","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/pages\/915","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=915"}],"version-history":[{"count":12,"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/pages\/915\/revisions"}],"predecessor-version":[{"id":1441,"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/pages\/915\/revisions\/1441"}],"up":[{"embeddable":true,"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=\/wp\/v2\/pages\/893"}],"wp:attachment":[{"href":"https:\/\/jwst.astro.umontreal.ca\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=915"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}