{"id":106091,"date":"2026-07-22T19:34:55","date_gmt":"2026-07-22T19:34:55","guid":{"rendered":"https:\/\/youzum.net\/shape-shifting-mirrors-on-nasas-new-space-telescope-could-unveil-jupiters-like-our-own\/"},"modified":"2026-07-22T19:34:55","modified_gmt":"2026-07-22T19:34:55","slug":"shape-shifting-mirrors-on-nasas-new-space-telescope-could-unveil-jupiters-like-our-own","status":"publish","type":"post","link":"https:\/\/youzum.net\/de\/shape-shifting-mirrors-on-nasas-new-space-telescope-could-unveil-jupiters-like-our-own\/","title":{"rendered":"Shape-shifting mirrors on NASA\u2019s new space telescope could unveil Jupiters like our own"},"content":{"rendered":"<div data-chronoton-summary=\"&lt;ul&gt;&lt;br&gt;&lt;li&gt;&lt;strong&gt;A disappearing act:&lt;\/strong&gt; NASA's Roman telescope carries the first space-bound &quot;active&quot; coronagraph, which doesn't just block starlight\u2014it measures and suppresses glare, improving sensitivity to exoplanets by up to 1,000 times over current instruments.&lt;\/li&gt;&lt;br&gt;&lt;li&gt;&lt;strong&gt;Shape-shifting mirrors:&lt;\/strong&gt; Two deformable mirrors, each controlled by thousands of tiny actuators, can sculpt their surfaces in increments as small as a tenth the diameter of a hydrogen atom to cancel out unwanted light\u2014like noise-canceling headphones, but for starlight.&lt;\/li&gt;&lt;br&gt;&lt;li&gt;&lt;strong&gt;Jupiters we've never seen before:&lt;\/strong&gt; Nearly every exoplanet directly photographed so far is an oversized, still-glowing youngster nothing like our solar system's planets. Roman could change that, capturing reflected light from true Jupiter-like worlds\u2014mature, cool gas giants orbiting sunlike stars at realistic distances.&lt;\/li&gt;&lt;br&gt;&lt;li&gt;&lt;strong&gt;A stepping stone to finding Earth 2.0:&lt;\/strong&gt; Even a planet reduced to a handful of pixels carries real scientific weight\u2014Roman can analyze its light across wavelengths to probe atmospheric chemistry.&lt;\/li&gt;&lt;\/ul&gt;\" data-chronoton-post-id=\"1140701\" data-chronoton-expand-collapse=\"1\" data-chronoton-analytics-enabled=\"1\"><\/div>\n<p>When NASA\u2019s Nancy Grace Roman Space Telescope launches, as early as the end of next month, it will attempt one of astronomy\u2019s most precise disappearing acts to date. The telescope will carry the first space-bound \u201cactive\u201d coronagraph, an instrument that effectively erases most of the light from a star during photography. <\/p>\n<p>It will allow astronomers to take the first pictures of planets orbiting other stars that are similar to those in our solar system. Ultimately, it could pave the way for a future mission that could snap the first photos of Earth-like worlds.<\/p>\n<p>\u201cI hope it\u2019s remembered for it being that critical stepping stone for \u2026 finding Earth 2.0,\u201d says Brandon Creager, the instrument\u2019s lead mechanical engineer at NASA\u2019s Jet Propulsion Laboratory (JPL).<\/p>\n<p>Named after Nancy Grace Roman, NASA\u2019s first chief of astronomy, this new telescope will carry a roughly 300-megapixel wide-field camera that will enable it to capture images about 100 times larger than the Hubble Space Telescope\u2019s widest exposures at a similar resolution. <\/p>\n<p>These capabilities will help astronomers unpack the mysterious identities of dark matter and dark energy\u2014and to detect <a href=\"https:\/\/science.nasa.gov\/universe\/exoplanets\/roman-telescope-predicted-to-find-100000-transiting-planets\/\">around 100,000 new<\/a> exoplanets, planets outside our solar system, whose presence can be inferred from the way they distort the starlight of more distant stars. Javier Via\u00f1a, a research scientist at Harvard who has had two projects selected for Roman\u2019s highly competitive first year of observing, compares the leap to moving from \u201cinterviewing a handful of people\u201d to \u201cconducting a global census.\u201d<\/p>\n<p>Another camera will use the coronagraph, blocking out a star\u2019s light as it observes one stellar system at a time. The instrument will allow astronomers an unprecedented look at the space <em>around<\/em> stars, enabling them to see smaller, dimmer, and more close-in exoplanets. \u201cIt\u2019s giving us the ability to see planets that we haven\u2019t been able to physically see before,\u201d says Creager.<\/p>\n<h3 class=\"wp-block-heading\"><strong>The anatomy of a vanishing trick<\/strong><\/h3>\n<p>Coronagraphs in space aren\u2019t new. But earlier incarnations, such as those currently aboard Hubble and the James Webb Space Telescope, use a stationary system to block a star\u2019s blinding light. The approach does help, but it\u2019s a bit like putting your thumb over a flashlight while searching a dark room for a firefly. Though the bulb vanishes, stray glare can still escape and overwhelm the light of the insect. Inside a telescope, that glare can come from light leaking around the edges of machinery or from minuscule imperfections in mirrors and coatings that can scatter starlight into speckles. All this can hide, or even impersonate, a planet.<\/p>\n<p>Roman\u2019s coronagraph, however, will attempt something completely unseen in space telescopes until this year: Before each observation, it will measure that leftover light and try to suppress it, a technique known as active wavefront control.<\/p>\n<p>The telescope is able to do this because it contains two deformable mirrors. Each has a 48-by-48 checkerboard of actuators (tiny pistons) beneath a thin, deformable sheet of glass. Applying a small amount of voltage makes the actuators contract and tug their patches of mirror slightly backward, like thousands of microscopic fingers delicately sculpting a surface. <\/p>\n<p>The effect is very subtle: Each patch of mirror can deform by up to 0.5 micrometers, or about one-fourth the size of an <em>E. coli<\/em> bacterium, and in increments as small as approximately 10 picometers. That\u2019s about a tenth the diameter of a hydrogen atom, says Ilya Poberezhskiy, the instrument\u2019s project systems engineer at JPL.<\/p>\n<p>The actuators allow the mirrors to create an \u201cactive wavefront,\u201d where each component is moved to the perfect position to cancel out incoming waves of unwanted light\u2014a bit like a pair of noise-canceling headphones, but for light instead of sound. The \u201ccanceled-out\u201d light creates a \u201cdoughnut-shaped region around the star where we suppress starlight and where we\u2019re hoping to see exoplanets,\u201d says Poberezhskiy. <\/p>\n<p>Compared with current space-based coronagraphs, the system is expected to improve sensitivity to exoplanets against the glare of their host stars by a factor of up to 1,000, revealing planets that would have been far too faint to detect before.<\/p>\n<p>Like Hubble and JWST, Roman also uses masks, patterned plates placed in the path of the light that are designed to block the photons that run into them. One tool in Roman\u2019s mask arsenal is \u201csilicon grass,\u201d a thicket of microscopic spikes on some masks that can be used in certain configurations to absorb photons so they don\u2019t bounce around the telescope and accidentally reach a detector.<\/p>\n<p>Light entering the forest bounces deeper and deeper between the blades and gets trapped instead of reflecting back toward the camera. \u201cOnce the light gets into there, it never gets out,\u201d Poberezhskiy says. The mirrors and masks form a succession of gates and hedges to guide as much of the preserved planetary light as possible toward the final detector.<\/p>\n<h3 class=\"wp-block-heading\"><strong>Alien Jupiters<\/strong><\/h3>\n<p>This elaborate setup could open a new chapter in the direct imaging of exoplanets. Nearly all exoplanets photographed so far are oversize youngsters that are nothing like the residents of our solar system: several times the mass of Jupiter, still glowing with the heat left over from their birth, and orbiting tens or hundreds of times farther from their star than the Earth is from the sun. This is because they are relatively easy to see. Their size, warmth, and distance from their parent star makes them shine brightly in infrared light, far away from the worst of the stellar glare.<\/p>\n<p>Roman, however, could directly image a true Jupiter analogue\u2014a planet similar to Jupiter in mass and circling a sunlike star a few times farther out than Earth is from our sun. Unlike the hot Jupiters we can see now, this one would be a much more mature gas giant like ours, primarily reflecting its parent star\u2019s light after billions of years of cooling instead of heavily emitting its own.<\/p>\n<p>Astronomers have been able to infer the existence of such planets from the gravitational wobble they impart to the star. Roman instead will collect starlight reflected from the planet itself. \u201cWe\u2019re not looking at the star. We\u2019re not looking at the effect of the planet on the star,\u201d says Meredith MacGregor, a professor of astronomy at Johns Hopkins who has also secured an observing program. \u201cWe are actually looking at the planet, and that is super powerful.\u201d<\/p>\n<p>Once this instrument becomes available, it will become the scientists\u2019 turn to do their jobs. \u201cI\u2019m honestly a little terrified about how we\u2019re all going to deal with it, because I think it\u2019s just so much data,\u201d MacGregor says. \u201cI think people will legitimately still be working on Roman data for decades.\u201d<\/p>\n<p>But don\u2019t expect to see a 4K photo of an alien Jupiter in the coming months. Roman will not be able to resolve such a planet into a solid globe\u2014at best, it will likely resemble <a href=\"https:\/\/en.wikipedia.org\/wiki\/List_of_directly_imaged_exoplanets#\/media\/File:HR_8799_Orbiting_Exoplanets.gif\">a smattering of pixels<\/a>. Still, that will be enough, MacGregor says, as Roman can then use the coronagraph to get information on the various wavelengths of light from the planet, which can tell astronomers about its atmospheric chemistry.<\/p>\n<p>\u201cYou\u2019re taking something that\u2019s a point of light and turning it into an actual world,\u201d she says, \u201cbecause if you know that about its atmosphere, now you know something about the surface of the planet and the possibility of life being on that planet, right? So that\u2019s a big step.\u201d<\/p>\n<p>During its first observations, scientists and engineers will see whether they can hold a star at the very center of the coronagraph\u2019s masks, shape the mirrors, \u201cdig\u201d the dark doughnut (as Poberezhskiy describes it), and then maintain everything as the spacecraft moves through space and actively changes temperature.<\/p>\n<p>The results will inform NASA\u2019s proposed Habitable Worlds Observatory, the daydream of many an exoplanet astronomer, which will in theory be able to separate the light of an Earthlike planet from that of a sunlike star, over 10 billion times brighter.<\/p>\n<p>Creager, who has worked on the instrument since 2018, is proud of the achievement: \u201cNot too many people get to say, \u2018I built something and it\u2019s taking a picture of a planet that\u2019s at a star that\u2019s 50 light-years away or 100 light-years away.\u2019\u201d He imagines the moment he and his team will be able to look at the first image as it arrives: \u201cYes, we did that.\u201d While the planet may show up only as a tiny dot, Roman\u2019s achievement will be the darkness engineered around it.<\/p>","protected":false},"excerpt":{"rendered":"<p>When NASA\u2019s Nancy Grace Roman Space Telescope launches, as early as the end of next month, it will attempt one of astronomy\u2019s most precise disappearing acts to date. The telescope will carry the first space-bound \u201cactive\u201d coronagraph, an instrument that effectively erases most of the light from a star during photography. It will allow astronomers to take the first pictures of planets orbiting other stars that are similar to those in our solar system. Ultimately, it could pave the way for a future mission that could snap the first photos of Earth-like worlds. \u201cI hope it\u2019s remembered for it being that critical stepping stone for \u2026 finding Earth 2.0,\u201d says Brandon Creager, the instrument\u2019s lead mechanical engineer at NASA\u2019s Jet Propulsion Laboratory (JPL). Named after Nancy Grace Roman, NASA\u2019s first chief of astronomy, this new telescope will carry a roughly 300-megapixel wide-field camera that will enable it to capture images about 100 times larger than the Hubble Space Telescope\u2019s widest exposures at a similar resolution. These capabilities will help astronomers unpack the mysterious identities of dark matter and dark energy\u2014and to detect around 100,000 new exoplanets, planets outside our solar system, whose presence can be inferred from the way they distort the starlight of more distant stars. Javier Via\u00f1a, a research scientist at Harvard who has had two projects selected for Roman\u2019s highly competitive first year of observing, compares the leap to moving from \u201cinterviewing a handful of people\u201d to \u201cconducting a global census.\u201d Another camera will use the coronagraph, blocking out a star\u2019s light as it observes one stellar system at a time. The instrument will allow astronomers an unprecedented look at the space around stars, enabling them to see smaller, dimmer, and more close-in exoplanets. \u201cIt\u2019s giving us the ability to see planets that we haven\u2019t been able to physically see before,\u201d says Creager. The anatomy of a vanishing trick Coronagraphs in space aren\u2019t new. But earlier incarnations, such as those currently aboard Hubble and the James Webb Space Telescope, use a stationary system to block a star\u2019s blinding light. The approach does help, but it\u2019s a bit like putting your thumb over a flashlight while searching a dark room for a firefly. Though the bulb vanishes, stray glare can still escape and overwhelm the light of the insect. Inside a telescope, that glare can come from light leaking around the edges of machinery or from minuscule imperfections in mirrors and coatings that can scatter starlight into speckles. All this can hide, or even impersonate, a planet. Roman\u2019s coronagraph, however, will attempt something completely unseen in space telescopes until this year: Before each observation, it will measure that leftover light and try to suppress it, a technique known as active wavefront control. The telescope is able to do this because it contains two deformable mirrors. Each has a 48-by-48 checkerboard of actuators (tiny pistons) beneath a thin, deformable sheet of glass. Applying a small amount of voltage makes the actuators contract and tug their patches of mirror slightly backward, like thousands of microscopic fingers delicately sculpting a surface. The effect is very subtle: Each patch of mirror can deform by up to 0.5 micrometers, or about one-fourth the size of an E. coli bacterium, and in increments as small as approximately 10 picometers. That\u2019s about a tenth the diameter of a hydrogen atom, says Ilya Poberezhskiy, the instrument\u2019s project systems engineer at JPL. The actuators allow the mirrors to create an \u201cactive wavefront,\u201d where each component is moved to the perfect position to cancel out incoming waves of unwanted light\u2014a bit like a pair of noise-canceling headphones, but for light instead of sound. The \u201ccanceled-out\u201d light creates a \u201cdoughnut-shaped region around the star where we suppress starlight and where we\u2019re hoping to see exoplanets,\u201d says Poberezhskiy. Compared with current space-based coronagraphs, the system is expected to improve sensitivity to exoplanets against the glare of their host stars by a factor of up to 1,000, revealing planets that would have been far too faint to detect before. Like Hubble and JWST, Roman also uses masks, patterned plates placed in the path of the light that are designed to block the photons that run into them. One tool in Roman\u2019s mask arsenal is \u201csilicon grass,\u201d a thicket of microscopic spikes on some masks that can be used in certain configurations to absorb photons so they don\u2019t bounce around the telescope and accidentally reach a detector. Light entering the forest bounces deeper and deeper between the blades and gets trapped instead of reflecting back toward the camera. \u201cOnce the light gets into there, it never gets out,\u201d Poberezhskiy says. The mirrors and masks form a succession of gates and hedges to guide as much of the preserved planetary light as possible toward the final detector. Alien Jupiters This elaborate setup could open a new chapter in the direct imaging of exoplanets. Nearly all exoplanets photographed so far are oversize youngsters that are nothing like the residents of our solar system: several times the mass of Jupiter, still glowing with the heat left over from their birth, and orbiting tens or hundreds of times farther from their star than the Earth is from the sun. This is because they are relatively easy to see. Their size, warmth, and distance from their parent star makes them shine brightly in infrared light, far away from the worst of the stellar glare. Roman, however, could directly image a true Jupiter analogue\u2014a planet similar to Jupiter in mass and circling a sunlike star a few times farther out than Earth is from our sun. Unlike the hot Jupiters we can see now, this one would be a much more mature gas giant like ours, primarily reflecting its parent star\u2019s light after billions of years of cooling instead of heavily emitting its own. Astronomers have been able to infer the existence of such planets from the gravitational wobble they impart to the star. Roman instead will collect starlight reflected from the planet itself. \u201cWe\u2019re not looking<\/p>","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"pmpro_default_level":"","site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"_pvb_checkbox_block_on_post":false,"footnotes":""},"categories":[52,5,7,1],"tags":[],"class_list":["post-106091","post","type-post","status-publish","format-standard","hentry","category-ai-club","category-committee","category-news","category-uncategorized","pmpro-has-access"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v25.3 - 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