{"id":354351,"date":"2026-01-24T01:00:00","date_gmt":"2026-01-23T15:00:00","guid":{"rendered":"https:\/\/www.nasa.gov\/?p=946704"},"modified":"2026-01-24T01:00:00","modified_gmt":"2026-01-23T15:00:00","slug":"journey-to-center-of-milky-way-with-upcoming-nasa-roman-core-survey","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=354351","title":{"rendered":"Journey to Center of Milky Way With Upcoming NASA Roman Core Survey"},"content":{"rendered":"<p>At the heart of our own galaxy, there is a dense thicket of stars with a supermassive black hole at the very center. NASA\u2019s Nancy Grace Roman Space Telescope will provide the deepest-ever view of this zone, revealing stars, planets, and unique objects that resist definition.<\/p>\n<p>Based on the input of astronomers from across the globe, the Roman Space Telescope will spend three-quarters of its five-year primary mission conducting <a href=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasas-roman-mission-shares-detailed-plans-to-scour-skies\/\" data-type=\"link\" data-id=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasas-roman-mission-shares-detailed-plans-to-scour-skies\/\">three revolutionary surveys<\/a> of unprecedented scale. Their combined results will transform all areas of astronomy and answer longstanding questions about dark matter, dark energy, and planets outside of our solar system, called exoplanets.<\/p>\n<p>That last theme will be addressed by the Galactic Bulge Time-Domain Survey, which will peer into the center of our galaxy to study the stars and exoplanets that make up the densely populated region around the center of the Milky Way, known as the galactic bulge.<\/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-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg\"><img fetchpriority=\"high\" decoding=\"async\" width=\"2048\" height=\"1152\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?w=2048\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Galactic Bulge Time-Domain Survey infographic\" 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\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg 3840w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=2048,1152 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=1200,675 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-gbs.jpg?resize=2000,1125 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\">This infographic describes the Galactic Bulge Time-Domain Survey that will be conducted by NASA\u2019s Nancy Grace Roman Space Telescope. The smallest of Roman\u2019s core surveys, this observation program will consist of repeat visits to six fields covering 1.7 square degrees total. One field will pierce the very center of the galaxy, and the others will be nearby \u2014 all in a region of the sky that will be visible to Roman for two 72-day stretches each spring and fall. The survey will mainly consist of six seasons (three early on, and three toward the end of Roman\u2019s primary mission), during which Roman will view each field every 12 minutes. Roman will also view the six fields with less intensity at other times throughout the mission, allowing astronomers to detect microlensing events that can last for years, signaling the presence of isolated, stellar-mass black holes.<\/div>\n<div class=\"hds-credits\">Credit: NASA\u2019s Goddard Space Flight Center<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>The survey will observe six patches of the galactic bulge, one pinpointing the center and five nearby, every 12 minutes during 438 days of total observing time. The observations will be separated into six \u201cseasons\u201d spread out over five years.<\/p>\n<p>Spending so much time focusing on a relatively small area of the sky, the mission will be able to track changes in the motion and light of hundreds of millions of stars, and any planets that orbit them, over long periods \u2014 the \u201ctime-domain\u201d aspect of the survey.<\/p>\n<p>\u201cThis survey will be the highest precision, highest cadence, longest continuous observing baseline survey of our galactic bulge, where the highest density of stars in our galaxy reside,\u201d said Jessie Christiansen of Caltech\/IPAC, who served as co-chair of the committee that defined the Galactic Bulge Time-Domain Survey.<\/p>\n<p><strong>Exoplanet microlensing<\/strong><\/p>\n<p>Roman will use a method called microlensing to search for exoplanets, a technique that has so far identified just over 200 exoplanets, compared to more than 4,000 discovered with the <a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/transit-method\/\" rel=\"noopener\">transit method<\/a>, out of the greater than <a href=\"https:\/\/nexsci.caltech.edu\/\" rel=\"noopener\">6,000 currently confirmed<\/a>.<\/p>\n<p>With this survey, scientists expect to see over 1,000 new planets orbiting other stars just using microlensing alone. This would increase the number of exoplanets identified using this method by more than fivefold.<\/p>\n<p>A microlensing event is when light from a distant star in the background is warped slightly by a foreground object, like a star and its planet. This warping of light is called gravitational lensing, with the gravity from the star and planet bending the fabric of space that light is traveling through and focusing it like a magnifying glass.<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube\">\n<div class=\"wp-block-embed__wrapper\">\n<iframe loading=\"lazy\" title=\"How Gravitational Microlensing Works\" width=\"500\" height=\"281\" src=\"https:\/\/www.youtube.com\/embed\/kKf4jUoAzNQ?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/div><figcaption class=\"wp-element-caption\">This animation illustrates the concept of gravitational microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the warped space-time around the foreground star. This star is then a virtual magnifying glass, amplifying the brightness of the background source star, so we refer to the foreground star as the lens star. If the lens star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. Thus we discover the presence of exoplanets, and measure its mass and separation from its star.<br \/>Credit: NASA&#8217;s Goddard Space Flight Center\/CI Lab<\/figcaption><\/figure>\n<p>While the transit method is very good at identifying exoplanets that orbit close to their star, the microlensing method can discover exoplanets that orbit farther away from their star, and in planetary systems farther from Earth than ever studied before. Roman will be versatile enough to see exoplanets dwelling from the inner edge of the habitable zone out to great distances from their stars, with a wide range of masses from planets smaller than Mars to the size of gas giants like Jupiter and Saturn. It may even discover \u201crogue planets\u201d without host stars that either formed alone or were ejected from their host systems long ago.<\/p>\n<p>\u201cFor the first time, we will have a big picture understanding of Earth and our solar system within the broader context of the exoplanet population of the Milky Way galaxy,\u201d Christiansen said. \u201cWe still don\u2019t know how common Earth-like planets are, and the Roman Galactic Bulge Time-Domain Survey will provide us with this answer.\u201d<\/p>\n<p>This survey will create a census of exoplanets for scientists to draw statistical conclusions from, revealing common patterns found in exoplanets and furthering our understanding of planetary formation and habitability.<\/p>\n<p><strong>One survey; lots of science<\/strong><\/p>\n<p>Because of the immense amount of observing time and subsequent data produced, the Galactic Bulge Time-Domain Survey will advance not only the field of exoplanet microlensing, but other areas of astronomy, too.<\/p>\n<p>\u201cThere is an incredibly rich diversity of science that can be done with a high-precision, high-cadence survey like this one,\u201d said Dan Huber of the University of Hawaii, the other survey co-chair.<\/p>\n<p>The core survey was optimized not only for microlensing, but also to observe changes in brightness from small, fast blips to long-term trends. This property allows astronomers to discover and characterize transiting planets, red giant stars, stellar-mass black holes and other stellar remnants, and eclipsing binaries, and can lead to a deeper understanding about the physics of star formation and evolution.<\/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-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png\"><img decoding=\"async\" width=\"1316\" height=\"1319\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?w=1316\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Many thousands of bright, explosive looking stars speckle the screen. The smallest ones are white pinpoints, strewn across the screen like spilled salt. Larger ones are yellow and bluish white and they have spiky outer edges like sea urchins.\" 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\/2023\/10\/this-one.png 1316w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=150,150 150w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=300,300 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=768,770 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=1022,1024 1022w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=50,50 50w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=100,100 100w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=200,200 200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=400,400 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=600,600 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=898,900 898w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/10\/this-one.png?resize=1197,1200 1197w\" sizes=\"auto, (max-width: 1316px) 100vw, 1316px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">A simulated image of Roman&#8217;s observations toward the center of our galaxy, spanning only less than 1 percent of the total area of Roman\u2019s galactic bulge time-domain survey. The simulated stars were drawn from the Besan\u00e7on Galactic Model.<\/div>\n<div class=\"hds-credits\">Credit: Matthew Penny (Louisiana State University)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>&#8220;The stars in the bulge and center of our galaxy are unique and not yet well understood,\u201d Huber said. \u201cThe data from this survey will allow us to measure how old these stars are and how they fit into the formation history of our Milky Way galaxy.\u201d<\/p>\n<p>Roman\u2019s observing strategy in the Galactic Bulge Time-Domain Survey, as well as the <a href=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasa-roman-core-survey-will-trace-cosmic-expansion-over-time\/\" data-type=\"link\" data-id=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasa-roman-core-survey-will-trace-cosmic-expansion-over-time\/\">High-Latitude Time-Domain Survey<\/a> and the High-Latitude Wide-Area Survey, will allow astronomers to maximize scientific output, all with one telescope.<\/p>\n<p><strong>Abundance of data to explore<\/strong><\/p>\n<p>Roman will observe hundreds of millions of stars every 12 minutes during the survey period, providing an unprecedented volume of data for astronomers to parse through.<\/p>\n<p>The Roman Science Support Center at Caltech\/IPAC in Pasadena, California, will be responsible for the high-level science data processing for the Galactic Bulge Time Domain Survey, including exoplanet microlensing and general community outreach for Roman exoplanet science. The Science Support Center\u2019s monitoring of these stars has been automated to detect microlensing and variable events within the data. This helps scientists understand features like how frequently a star\u2019s brightness is changing, or if there are planets lurking near the lensed stars, or other sources of variability. The number of stars and frequency of the observations make the Roman data an ideal dataset for finding such sources.<\/p>\n<p>All Roman observations will be made publicly available after a short processing period. The mission is scheduled to launch no later than May 2027, with the team on track for launch in fall 2026.<\/p>\n<p>The Nancy Grace Roman Space Telescope is managed at NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA\u2019s Jet Propulsion Laboratory in Southern California; Caltech\/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific &amp; Imaging in Thousand Oaks, California.<\/p>\n<p><strong>By Isabel Swafford<br \/>Caltech\/IPAC, Pasadena, Calif.<\/strong><\/p>\n<p><strong>Media contact:<\/strong><\/p>\n<p><strong>Claire Andreoli<br \/><\/strong><a href=\"http:\/\/www.nasa.gov\/goddard\"><strong>NASA\u2019s Goddard Space Flight Center<\/strong><\/a><strong>, Greenbelt, Md.<br \/>301-286-1940<\/strong><\/p>\n<div id=\"\" class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 article_a hds-module hds-module-full alignfull wp-block-nasa-blocks-credits-and-details\">\n<section class=\"padding-x-0 padding-top-5 padding-bottom-2 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"grid-row grid-container maxw-widescreen padding-0\">\n<div class=\"grid-col-12 desktop:grid-col-2 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div 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class=\"margin-bottom-3\">\n<div>Ashley Balzer<\/div>\n<div><a href=\"mailto:&#97;s&#038;%23104;&#038;%23108;e&#038;%23121;.m.&#038;%2398;al&#038;%23122;er&#038;%2364;&#038;%23110;as&#038;%2397;&#038;%2346;&#038;%23103;ov\">&#97;&#115;&#104;ley&#46;m&#46;&#98;a&#108;&#122;&#101;r&#64;&#110;&#97;sa.&#103;&#111;&#118;<\/a><\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-row\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Location<\/div>\n<\/div>\n<div class=\"grid-col-8\">Goddard Space Flight Center<\/div>\n<\/div><\/div>\n<\/p><\/div>\n<div class=\"grid-col-12 desktop:grid-col-5 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black \">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Related Terms<\/h2>\n<\/div>\n<ul class=\"article-tags\">\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\" rel=\"noopener\">Nancy Grace Roman Space Telescope<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/universe\/exoplanets\/exoplanet-detection-methods\/\">Exoplanet Detection Methods<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/exoplanets\/\" rel=\"noopener\">Exoplanets<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/galaxies\/\" rel=\"noopener\">Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/goddard\/\">Goddard Space Flight Center<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/universe\/exoplanets\/exoplanet-detection-methods\/gravitational-microlensing\/\">Gravitational Microlensing<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/stars\/\" rel=\"noopener\">Stars<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/universe\/galaxies\/milky-way\/\">The Milky Way<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/\" rel=\"noopener\">The Universe<\/a><\/li>\n<\/ul>\n<\/div>\n<\/div><\/div>\n<\/section><\/div>\n<div id=\"\" class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 hds-module hds-module-full alignfull wp-block-nasa-blocks-related-articles\">\n<section class=\"hds-related-articles padding-x-0 padding-y-3 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"w-100 grid-row grid-container maxw-widescreen padding-0 text-align-left\">\n<div class=\"margin-bottom-4\">\n<h2 style=\"max-width: 100%;\" class=\"width-full w-full maxw-full\">Explore More<\/h2>\n<\/div><\/div>\n<div class=\"grid-row grid-container maxw-widescreen padding-0\">\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasa-roman-core-survey-will-trace-cosmic-expansion-over-time\/\" class=\"color-carbon-black\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"300\" height=\"113\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?w=300\" class=\"attachment-medium size-medium\" 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\/2025\/08\/snsn.jpg 5760w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=300,113 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=768,288 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=1024,384 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=1536,576 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=2048,768 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=400,150 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=600,225 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=900,338 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=1200,450 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/08\/snsn.jpg?resize=2000,750 2000w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">6 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA Roman Core Survey Will Trace Cosmic Expansion Over Time<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t5 months ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasas-roman-mission-shares-detailed-plans-to-scour-skies\/\" class=\"color-carbon-black\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"300\" height=\"188\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?w=300\" class=\"attachment-medium size-medium\" 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\/2025\/04\/roman-survey-infographic-mkiv-2.jpg 8000w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=300,188 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=768,480 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=1024,640 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=1536,960 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=2048,1280 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=400,250 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=600,375 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=900,563 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=1200,750 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/04\/roman-survey-infographic-mkiv-2.jpg?resize=2000,1250 2000w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">6 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA\u2019s Roman Mission Shares Detailed Plans to Scour Skies<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t9 months ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/www.nasa.gov\/missions\/roman-space-telescope\/nasa-announces-plan-to-map-milky-way-with-roman-space-telescope\/\" class=\"color-carbon-black\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"300\" height=\"169\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?w=300\" class=\"attachment-medium size-medium\" 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\/2025\/12\/roman-galacticplanesurvey-final-1.jpg 3840w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=2048,1152 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=1200,675 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/roman-galacticplanesurvey-final-1.jpg?resize=2000,1125 2000w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">7 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA Announces Plan to Map Milky Way With Roman Space Telescope<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t1 month ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<\/p><\/div>\n<\/section><\/div>\n","protected":false},"excerpt":{"rendered":"<p>At the heart of our own galaxy, there is a dense thicket of stars with a supermassive black hole at the very center. NASA\u2019s Nancy Grace Roman Space Telescope will provide the deepest-ever view of this zone, revealing stars, planets, and unique objects that resist definition. Based on the input of astronomers from across the [\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,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[19356,15636,15757,15614,19357,15619,15675,15769,15638],"tags":[],"class_list":["post-354351","post","type-post","status-publish","format-standard","hentry","category-exoplanet-detection-methods","category-exoplanets","category-galaxies","category-goddard-space-flight-center","category-gravitational-microlensing","category-nancy-grace-roman-space-telescope","category-stars","category-the-milky-way","category-the-universe"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/354351","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=354351"}],"version-history":[{"count":64,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/354351\/revisions"}],"predecessor-version":[{"id":356026,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/354351\/revisions\/356026"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=354351"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=354351"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=354351"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}