{"id":520072,"date":"2026-08-26T05:44:55","date_gmt":"2026-08-25T19:44:55","guid":{"rendered":"https:\/\/www.nasa.gov\/?p=1041093"},"modified":"2026-08-26T05:44:55","modified_gmt":"2026-08-25T19:44:55","slug":"nasa-ames-contributions-to-romans-mission","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=520072","title":{"rendered":"NASA Ames\u2019 Contributions to Roman\u2019s Mission"},"content":{"rendered":"<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png\"><img fetchpriority=\"high\" decoding=\"async\" width=\"2000\" height=\"1125\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?w=2000\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"eager\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png 2000w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/roman-beautypass2026-med.png?resize=1200,675 1200w\" sizes=\"auto, (max-width: 2000px) 100vw, 2000px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">The Nancy Grace Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics.<\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\">Set to launch on Sunday, Aug. 30, NASA\u2019s Nancy Grace Roman Space Telescope will empower astronomers to explore vast regions of the cosmos and settle essential questions in the areas of dark energy, dark matter, planets outside our solar system, and the formation and growth of galaxies over cosmic time. Key contributions to Roman\u2019s mission made by researchers at NASA\u2019s Ames Research Center in California\u2019s Silicon Valley will advance Roman\u2019s science using the center\u2019s facilities, expertise, and innovations.<\/p>\n<p class=\"wp-block-paragraph\"><strong>Tools to predict, remove glare<\/strong><\/p>\n<p class=\"wp-block-paragraph\">Roman\u2019s main camera, the Wide Field Instrument, will capture expansive high-resolution pictures of the universe in optical and near-infrared light. These unprecedented images will enable astronomers to decode some of the deepest mysteries of the cosmos.<\/p>\n<p class=\"wp-block-paragraph\">Forms of glare that Roman\u2019s camera collects diminish image quality and thereby reduce the ability of astronomers to characterize certain cosmic structures. Innovative software developed by a team at NASA Ames, with collaborators at NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland, and IPAC\/Caltech in Pasadena, California, will improve Roman\u2019s images and optimize observing plans. Called ROSALIA (Roman Sky Analyst for Low Surface Brightness Imaging and Astronomy), the software predicts and removes unwanted light from astronomical images captured by Roman\u2019s Wide Field Instrument.<\/p>\n<p class=\"wp-block-paragraph\">Contaminating stray light occurs when photons scatter inside the telescope\u2019s optical system. Resulting light glints can produce deceptive image artifacts that mimic the appearance of real planets or nebulae. The ROSALIA software will allow astronomers to adjust their observation plans to limit glints from contaminating science targets in Roman\u2019s images.<\/p>\n<p class=\"wp-block-paragraph\">In addition to bright glints, stray light can also appear as a diffuse background. This form of stray light interferes with observations of the darkest regions of the universe, which is critical to understanding how large structures in the universe were formed.<\/p>\n<p class=\"wp-block-paragraph\">Another major contributor to obscuring background light is produced by nature itself: zodiacal light. Zodiacal emission originates from the scattering of sunlight by interplanetary dust particles in our solar system. The ROSALIA software predicts and strips away background contamination, including zodiacal and stray light from images, exposing the faint, diffuse emissions at galaxy edges where cosmic evolutionary histories are hidden.<\/p>\n<div id=\"\" class=\"hds-media hds-module hds-module-full alignfull wp-block-nasa-blocks-image-before-after\">\n<div class=\"NasaBlocksImageBeforeAfterBlock grid-container grid-row grid-container-block bg-spacesuit-white padding-x-0 padding-y-6 margin-x-auto nasa-block-align-full\">\n<div class=\"padding-x-0 grid-col-12\">\n<p>\t\t\t<!-- curtain view --><\/p>\n<div class=\"img-comparison-slider-parent comparison-view-active\">\n\t\t\t\t<img-comparison-slider><br \/>\n\t\t\t\t\t<img decoding=\"async\" slot=\"first\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png\" alt=\"\"><br \/>\n\t\t\t\t\t<img decoding=\"async\" slot=\"second\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png\" alt=\"\"><br \/>\n\t\t\t\t<\/img-comparison-slider><\/p>\n<div class=\"curtain-view-label-wrapper curtain-view-before\">\n\t\t\t\t\t<span class=\"curtain-view-label\">Simulated, unprocessed<\/span>\n\t\t\t\t<\/div>\n<div class=\"curtain-view-label-wrapper curtain-view-after\">\n\t\t\t\t\t<span class=\"curtain-view-label\">Simulated, processed<\/span>\n\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t<!-- toggle view --><\/p>\n<div class=\"toggle-comparison-parent\">\n\t\t\t\t<!-- if image_1 is active the show image_1 --><\/p>\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover toggle-view-image toggle-view-before-image toggle-view-active\"><img decoding=\"async\" width=\"768\" height=\"471\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?w=768\" class=\"attachment-medium_large size-medium_large\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png 10100w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=300,184 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=768,471 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1024,628 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1536,943 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=2048,1257 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=400,246 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=600,368 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=900,552 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1200,737 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=2000,1228 2000w\" sizes=\"auto, (max-width: 768px) 100vw, 768px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Simulated unprocessed image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument, showing two interacting galaxies<\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<p>\t\t\t\t<!-- if image_2 is active the show image_2 --><\/p>\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover toggle-view-image toggle-view-after-image\"><img decoding=\"async\" width=\"768\" height=\"471\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?w=768\" class=\"attachment-medium_large size-medium_large\" alt=\"Simulated image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument and then processed to remove glare, showing two interacting galaxies.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png 10100w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=300,184 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=768,471 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1024,628 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1536,943 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=2048,1257 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=400,246 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=600,368 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=900,552 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1200,737 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=2000,1228 2000w\" sizes=\"auto, (max-width: 768px) 100vw, 768px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Simulated image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument and then processed using NASA\u2019s Roman Sky Analyst for Low Surface Brightness Imaging and Astronomy tools to remove glare, showing two interacting galaxies. <\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<div class=\"toggle-button-container padding-1\">\n\t\t\t\t\t<button class=\"toggle-view-before-button toggle-comparison-view-active margin-right-1px\"><span class=\"toggle-view-before-label\">Simulated, unprocessed<\/span><\/button><button class=\"toggle-view-after-button margin-left-1px\"><span class=\"toggle-view-after-label\">Simulated, processed<\/span><\/button>\n\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t<!-- 2-up view --><\/p>\n<div class=\"two-up-view position-relative bg-carbon-10\">\n<div class=\"grid-row\">\n<div class=\"grid-col flex-3 padding-top-4 padding-bottom-4\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"768\" height=\"471\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?w=768\" class=\"attachment-medium_large size-medium_large\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png 10100w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=300,184 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=768,471 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1024,628 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1536,943 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=2048,1257 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=400,246 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=600,368 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=900,552 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=1200,737 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-zodi-thermal-stray-stars-rgb.png?resize=2000,1228 2000w\" sizes=\"auto, (max-width: 768px) 100vw, 768px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Simulated unprocessed image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument, showing two interacting galaxies<\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<\/p><\/div>\n<div class=\"bg-spacesuit-white width-2px\"><\/div>\n<div class=\"grid-col flex-3 padding-top-4 padding-bottom-4\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"768\" height=\"471\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?w=768\" class=\"attachment-medium_large size-medium_large\" alt=\"Simulated image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument and then processed to remove glare, showing two interacting galaxies.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png 10100w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=300,184 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=768,471 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1024,628 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1536,943 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=2048,1257 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=400,246 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=600,368 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=900,552 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=1200,737 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/base-rgb.png?resize=2000,1228 2000w\" sizes=\"auto, (max-width: 768px) 100vw, 768px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Simulated image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument and then processed using NASA\u2019s Roman Sky Analyst for Low Surface Brightness Imaging and Astronomy tools to remove glare, showing two interacting galaxies. <\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<\/p><\/div>\n<div class=\"curtain-view-label-wrapper curtain-view-before\">\n\t\t\t\t\t\t<span class=\"curtain-view-label\"><br \/>\n\t\t\t\t\t\t\tSimulated, unprocessed\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/div>\n<div class=\"curtain-view-label-wrapper curtain-view-after\">\n\t\t\t\t\t\t<span class=\"curtain-view-label\"><br \/>\n\t\t\t\t\t\t\tSimulated, processed\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/div>\n<\/p><\/div>\n<\/p><\/div>\n<p>\t\t\t<!-- Under image content --><\/p>\n<div class=\"grid-row flex-row title-row padding-x-2 desktop:padding-x-0 padding-top-2\">\n<div class=\"grid-col-12 tablet:grid-col-6\">\n<p class=\"before-after-heading margin-bottom-1\">\n\t\t\t\t\t\tBEFORE AND AFTER PROCESSING\t\t\t\t\t<\/p>\n<h2 class=\"before-after-title margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\tSimulated View From Roman&#8217;s Wide Field Instrument  \t\t\t\t\t<\/h2>\n<\/p><\/div>\n<div class=\"grid-col-12 tablet:grid-col-6 button-row margin-bottom-3 tablet:margin-bottom-0\">\n\t\t\t\t\t<!-- Update onClick handlers --><br \/>\n\t\t\t\t\t<button\n\t\t\t\t\t\taria-label=\"Curtain view\"\n\t\t\t\t\t\tclass=\"comparison-view curtain-view-button comparison-view-active padding-bottom-1 margin-left-1\"\n\t\t\t\t\t>Curtain<\/button><button\n\t\t\t\t\t\taria-label=\"Toggle view\"\n\t\t\t\t\t\tclass=\"comparison-view toggle-view-button padding-bottom-1 margin-left-1\"\n\t\t\t\t\t>Toggle<\/button><button\n\t\t\t\t\t\taria-label=\"Two-Up view\"\n\t\t\t\t\t\tclass=\"comparison-view two-up-view-button padding-bottom-1 margin-left-1\"\n\t\t\t\t\t>2-Up<\/button>\t\t\t\t<\/div>\n<\/p><\/div>\n<\/p><\/div>\n<p>\t\t<!-- Image detail area --><\/p>\n<div class=\"image-details-panel padding-x-0\">\n<div class=\"before-after-details-divider padding-y-2\">\n\t\t\t\t<!-- OnClick handleImageDetailsClick --><button class=\"image-details-toggle-button\"><span>Image Details<\/span><!-- style - if showImageDetails, then transform rotate(180deg), else none --><svg aria-hidden=\"true\" width=\"14\" height=\"15\" viewBox=\"0 0 14 15\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle cx=\"7\" cy=\"7.5\" r=\"6.5\" stroke=\"#58585B\" \/><path fill-rule=\"evenodd\" clip-rule=\"evenodd\" d=\"M7.0002 8.23854L9.26318 5.95996L9.80019 6.50067L7.0002 9.31996L4.2002 6.50067L4.73721 5.95996L7.0002 8.23854Z\" fill=\"#58585B\" \/><\/svg><\/button>\n\t\t\t<\/div>\n<p>\t\t\t<!-- if showImageDetails, then display --><\/p>\n<div id=\"image-details\" class=\" padding-x-0\">\n<div class=\"grid-row\">\n<div class=\"grid-col flex-2\">\n<div class=\"image-details-wrapper\">\n\t\t\t\t\t\t\tLeft: Simulated unprocessed image, as it would be captured by the Roman Space Telescope\u2019s Wide Field Instrument, showing two interacting galaxies. Right: Simulated image of the same view after stepwise processing, using NASA\u2019s Roman Sky Analyst for Low Surface Brightness Imaging and Astronomy (ROSALIA) tools, to remove four types of glare: zodiacal light, thermal background, stray-light, and stellar emission. The result is cleaner, sharper images where galaxies can be detected in greater detail. Image credits: NASA\/Borlaff, Sanchez-Alarcon, Nickerson, Marcum and ROSALIA team\/STScI\/FIRE\/DREAM\u00a0\t\t\t\t\t\t<\/div>\n<p>\t\t\t\t\t\t<!-- File List --><\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<p class=\"wp-block-paragraph\"><strong>New \u2018multi-star\u2019 tech to see exoplanets<\/strong><\/p>\n<p class=\"wp-block-paragraph\">The Roman Coronagraph Instrument is one of two instruments flying on Roman. It will demonstrate the most advanced technologies ever flown in space for directly imaging planets around other stars. The Roman Coronagraph uses a series of masks and mirrors, including two deformable mirrors, to suppress starlight. By precisely controlling the shape of the deformable mirrors, it creates a \u201cdark zone\u201d around the star where observers can see the faint reflected light from orbiting planets.<\/p>\n<p class=\"wp-block-paragraph\">The baseline operating mode of the Roman Coronagraph Instrument supports observation of exoplanets only in single star systems, as current coronagraph instruments cannot typically suppress the additional contaminating starlight in multi-star systems, such as binary star systems.<\/p>\n<p class=\"wp-block-paragraph\">Our solar system has a single star, the Sun. But roughly half of Sun-like stars are in multi-star systems. Having the ability to directly image exoplanets in multi-star systems will increase the likelihood of detecting life beyond our solar system and will expand our knowledge about how exoplanets form and evolve, since there are major differences in how those processes unfold in single star versus multi-star systems. Eliminating overlapping glares from multiple stars is the key challenge that must be overcome to image planets in such systems.<\/p>\n<p class=\"wp-block-paragraph\">Researchers at NASA Ames are meeting that challenge with an innovative technology called Multi-Star Wavefront Control (MSWC). This technology includes custom light-blocking masks and accompanying software designed to suppress the light from multiple stars and reveal hidden exoplanets. Through a collaboration with NASA\u2019s Jet Propulsion Laboratory in Southern California, the MSWC masks are included on the Roman Coronagraph\u2019s flight instrument as an added capability beyond Roman\u2019s baseline observation modes. They could be used if additional observation time is granted to the coronagraph team after the primary technology demonstration phase is completed.\u00a0<\/p>\n<p class=\"wp-block-paragraph\">The nearest star system to our solar system, Alpha Centauri, is one of the nearest multi-star systems to Earth, &nbsp;at only four light-years away. This triple-star system contains a binary of Sun-like stars \u2013 Alpha Centauri AB \u2013 orbited by a much smaller and dimmer star \u2013 Proxima Centauri. Although no exoplanets are confirmed around the Sun-like stars in this system, a planet candidate has been identified by NASA\u2019s James Webb Space Telescope in the habitable zone of Alpha Centauri A. Researchers, including the Ames MSWC team, are working to develop the capabilities needed to observe this system. &nbsp;<\/p>\n<p class=\"wp-block-paragraph\">NASA Ames also provides leadership and support for the hardware working group as part of the Roman Coronagraph Participation Program. This program allows international teams of researchers to enable additional capabilities to the Roman Coronagraph beyond its baseline modes; this includes the multi-star modes being developed at NASA Ames that use different masks beyond the baseline or new wavefront control and sensing algorithms.<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg\"><img decoding=\"async\" width=\"2048\" height=\"1365\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?w=2048\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Close-up shot of four of the coronagraph\u2019s masks. The masks are black shapes painted on a reflective silver square. The square is mounted on a metal rectangular box. The the top left and bottom right masks look like a flowers with six petals; the top right and bottom left masks look like insects with their wings spread open.\" style=\"transform: scale(1.2); transform-origin: 48% 48%; object-position: 48% 48%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg 8256w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=300,200 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=768,512 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=1024,683 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=1536,1024 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=2048,1365 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=400,267 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=600,400 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=900,600 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=1200,800 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/08\/52577820109-ed0bb44153-o.jpg?resize=2000,1333 2000w\" sizes=\"auto, (max-width: 2048px) 100vw, 2048px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Close-up view of four of the Roman Coronagraph\u2019s optical masks. The bottom-right mask, shaped like a six-petaled flower, is designed to suppress the light from multiple stars and reveal hidden exoplanets.<\/div>\n<div class=\"hds-credits\">NASA JPL\/Chris Gunn<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\"><strong>Advanced supercomputing<\/strong><\/p>\n<p class=\"wp-block-paragraph\">Experts at NASA\u2019s Advanced Supercomputing Division at Ames are advancing Roman\u2019s science by bringing extensive experience in&nbsp;data pipelines and mission operations to provide advice and guidance to the Roman project through key mission development phases. This ensures reliable performance of ground-based systems and operations so that science data processing is efficient and the quality and integrity of the resulting science data products is high.<\/p>\n<p class=\"wp-block-paragraph\">NASA Advanced Supercomputing researchers collaborated with the Ames MSWC team to develop high-performance computing tools for multi-star wavefront control simulations and to conduct studies to assess the feasibility of the MSWC technique.<\/p>\n<p class=\"wp-block-paragraph\"><strong>Learn more:<\/strong><\/p>\n<p class=\"has-text-align-center wp-block-paragraph\">The Nancy Grace Roman Space Telescope mission: <a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/\" rel=\"noopener\">https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/<\/a><\/p>\n<p class=\"wp-block-paragraph\"><strong>For news media:<\/strong>&nbsp;<\/p>\n<p class=\"wp-block-paragraph\">Roman&nbsp;media resources: <a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/roman-media-resources\/\" rel=\"noopener\">https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/roman-media-resources\/<\/a><\/p>\n<p class=\"wp-block-paragraph\">Members of the news media interested in covering this topic should reach out to the\u202f<a href=\"mailto:arc-dl-newsroom@mail.nasa.gov\"  rel=\"noreferrer noopener\">NASA Ames newsroom<\/a>.&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Set to launch on Sunday, Aug. 30, NASA\u2019s Nancy Grace Roman Space Telescope will empower astronomers to explore vast regions of the cosmos and settle essential questions in the areas of dark energy, dark matter, planets outside our solar system, and the formation and growth of galaxies over cosmic time. Key contributions to Roman\u2019s mission [\u2026]<\/p>\n","protected":false},"author":13,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[15621,15606],"tags":[],"class_list":["post-520072","post","type-post","status-publish","format-standard","hentry","category-ames-research-center","category-general"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO Pro 5.0.1 - aioseo.com -->\n\t<meta name=\"description\" content=\"Set to launch on Sunday, Aug. 30, NASA\u2019s Nancy Grace Roman Space Telescope will empower astronomers to explore vast regions of the cosmos and settle essential questions in the areas of dark energy, dark matter, planets outside our solar system, and the formation and growth of galaxies over cosmic time. 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Key contributions to Roman\u2019s mission [\u2026]","inLanguage":"en-AU","isPartOf":{"@id":"https:\/\/www.vibewire.com.au\/#website"},"breadcrumb":{"@id":"https:\/\/www.vibewire.com.au\/?p=520072#breadcrumblist"},"author":{"@id":"https:\/\/www.vibewire.com.au\/?author=13#author"},"creator":{"@id":"https:\/\/www.vibewire.com.au\/?author=13#author"},"datePublished":"2026-08-26T05:44:55+10:00","dateModified":"2026-08-26T05:44:55+10:00"},{"@type":"WebSite","@id":"https:\/\/www.vibewire.com.au\/#website","url":"https:\/\/www.vibewire.com.au\/","name":"VibreWire Online","description":"Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything","inLanguage":"en-AU","publisher":{"@id":"https:\/\/www.vibewire.com.au\/#organization"}}]},"og:locale":"en_US","og:site_name":"VibeWire Magazine - Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything","og:type":"article","og:title":"NASA Ames\u2019 Contributions to Roman\u2019s Mission - VibeWire Magazine","og:description":"Set to launch on Sunday, Aug. 30, NASA\u2019s Nancy Grace Roman Space Telescope will empower astronomers to explore vast regions of the cosmos and settle essential questions in the areas of dark energy, dark matter, planets outside our solar system, and the formation and growth of galaxies over cosmic time. Key contributions to Roman\u2019s mission [\u2026]","og:url":"https:\/\/www.vibewire.com.au\/?p=520072","article:published_time":"2026-08-25T19:44:55+00:00","article:modified_time":"2026-08-25T19:44:55+00:00","twitter:card":"summary_large_image","twitter:site":"@VibewireCentral","twitter:title":"NASA Ames\u2019 Contributions to Roman\u2019s Mission - VibeWire Magazine","twitter:description":"Set to launch on Sunday, Aug. 30, NASA\u2019s Nancy Grace Roman Space Telescope will empower astronomers to explore vast regions of the cosmos and settle essential questions in the areas of dark energy, dark matter, planets outside our solar system, and the formation and growth of galaxies over cosmic time. Key contributions to Roman\u2019s mission [\u2026]","twitter:creator":"@VibewireCentral"},"aioseo_meta_data":{"post_id":"520072","title":null,"description":null,"keywords":null,"keyphrases":null,"primary_term":null,"canonical_url":null,"og_title":null,"og_description":null,"og_object_type":"default","og_image_type":"default","og_image_url":null,"og_image_width":null,"og_image_height":null,"og_image_custom_url":null,"og_image_custom_fields":null,"og_video":null,"og_custom_url":null,"og_article_section":null,"og_article_tags":null,"twitter_use_og":false,"twitter_card":"default","twitter_image_type":"default","twitter_image_url":null,"twitter_image_custom_url":null,"twitter_image_custom_fields":null,"twitter_title":null,"twitter_description":null,"schema":{"blockGraphs":[],"customGraphs":[],"default":{"data":{"Article":[],"Course":[],"Dataset":[],"FAQPage":[],"Movie":[],"Person":[],"Product":[],"ProductReview":[],"Car":[],"Recipe":[],"Service":[],"SoftwareApplication":[],"WebPage":[]},"graphName":"","isEnabled":true},"graphs":[]},"schema_type":"default","schema_type_options":null,"pillar_content":false,"robots_default":true,"robots_noindex":false,"robots_noarchive":false,"robots_nosnippet":false,"robots_nofollow":false,"robots_noimageindex":false,"robots_noodp":false,"robots_notranslate":false,"robots_max_snippet":null,"robots_max_videopreview":null,"robots_max_imagepreview":"large","priority":null,"frequency":null,"local_seo":null,"seo_analyzer_scan_date":"2026-08-25 21:12:50","breadcrumb_settings":null,"limit_modified_date":false,"open_ai":null,"ai":null,"created":"2026-08-25 21:12:23","updated":"2026-08-25 21:12:50","focus_keyword":null,"additional_keywords":null,"truseo_locale":null},"aioseo_breadcrumb":"<div class=\"aioseo-breadcrumbs\"><span class=\"aioseo-breadcrumb\">\n\t<a href=\"https:\/\/www.vibewire.com.au\" title=\"Home\">Home<\/a>\n<\/span><span class=\"aioseo-breadcrumb-separator\">&raquo;<\/span><span class=\"aioseo-breadcrumb\">\n\t<a href=\"https:\/\/www.vibewire.com.au\/?cat=15606\" title=\"General\">General<\/a>\n<\/span><span class=\"aioseo-breadcrumb-separator\">&raquo;<\/span><span class=\"aioseo-breadcrumb\">\n\tNASA Ames\u2019 Contributions to Roman\u2019s Mission\n<\/span><\/div>","aioseo_breadcrumb_json":[{"label":"Home","link":"https:\/\/www.vibewire.com.au"},{"label":"General","link":"https:\/\/www.vibewire.com.au\/?cat=15606"},{"label":"NASA Ames\u2019 Contributions to Roman\u2019s Mission","link":"https:\/\/www.vibewire.com.au\/?p=520072"}],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/520072","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/13"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=520072"}],"version-history":[{"count":2,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/520072\/revisions"}],"predecessor-version":[{"id":520244,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/520072\/revisions\/520244"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=520072"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=520072"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=520072"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}