{"id":251897,"date":"2025-07-15T23:49:16","date_gmt":"2025-07-15T13:49:16","guid":{"rendered":"https:\/\/www.nasa.gov\/?p=885607"},"modified":"2025-07-15T23:49:16","modified_gmt":"2025-07-15T13:49:16","slug":"one-survey-by-nasas-roman-could-unveil-100000-cosmic-explosions","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=251897","title":{"rendered":"One Survey by NASA\u2019s Roman Could Unveil 100,000 Cosmic Explosions"},"content":{"rendered":"

Scientists predict one of the major surveys by NASA\u2019s upcoming Nancy Grace Roman Space Telescope may reveal around 100,000 celestial blasts, ranging from exploding stars to feeding black holes. Roman may even find evidence of some of the universe\u2019s first stars, which are thought to completely self-destruct without leaving any remnant behind.<\/p>\n

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\"Simulated<\/a><\/figure>
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This simulation showcases the dynamic universe as NASA\u2019s Nancy Grace Roman Space Telescope could see it over the course of its five-year primary mission. The video sparkles with synthetic supernovae from observations of the OpenUniverse simulated universe taken every five days (similar to the expected cadence of Roman’s High-Latitude Time-Domain Survey, which OpenUniverse simulates in its entirety). On top of the static sky of stars in the Milky Way and other galaxies, more than a million exploding stars flare into visibility and then slowly fade away. To highlight the dynamic physics happening and for visibility at this scale, the true brightness of each transient event has been magnified by a factor of 10,000 and no background light has been added to the simulated images. The video begins with Roman\u2019s full field of view, which represents a single pointing of Roman\u2019s camera, and then zooms into one square.<\/div>\n
Credit: NASA\u2019s Goddard Space Flight Center and M. Troxel<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

Cosmic explosions offer clues to some of the biggest mysteries of the universe. One is the nature of dark energy<\/a>, the mysterious pressure thought to be accelerating the universe\u2019s expansion.<\/p>\n

\u201cWhether you want to explore dark energy, dying stars, galactic powerhouses, or probably even entirely new things we\u2019ve never seen before, this survey will be a gold mine,\u201d said Benjamin Rose, an assistant professor at Baylor University in Waco, Texas, who led a study about the results. The paper is published in The Astrophysical Journal<\/a><\/em>.<\/p>\n

Called the <\/a>High-Latitude Time-Domain Survey<\/a>, this observation program will scan the same large region of the cosmos every five days for two years. Scientists will stitch these observations together to create movies that uncover all sorts of cosmic fireworks.<\/p>\n

Chief among them are exploding stars<\/a>. The survey is largely geared toward finding a special class of supernova called type Ia<\/a>. These stellar cataclysms allow scientists to measure cosmic distances and trace the universe\u2019s expansion because they peak at about the same intrinsic brightness. Figuring out how fast the universe has ballooned during different cosmic epochs offers clues to dark energy.<\/p>\n

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\"High-Latitude<\/a><\/figure>
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This infographic describes the High-Latitude Time-Domain Survey that will be conducted by NASA\u2019s Nancy Grace Roman Space Telescope. The survey\u2019s main component will cover over 18 square degrees \u2014 a region of sky as large as 90 full moons \u2014 and see supernovae that occurred up to about 8 billion years ago. Smaller areas within the survey will pierce even farther, potentially back to when the universe was around a billion years old. The survey will be split between the northern and southern hemispheres, located in regions of the sky that will be continuously visible to Roman. The bulk of the survey will consist of 30-hour observations every five days for two years in the middle of Roman\u2019s five-year primary mission.<\/div>\n
Credit: NASA’s Goddard Space Flight Center<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

In the new study, scientists simulated Roman\u2019s entire High-Latitude Time-Domain Survey. The results suggest Roman could see around 27,000 type Ia supernovae\u2014about 10 times more than all previous surveys combined.<\/p>\n

Beyond dramatically increasing our total sample of these supernovae, Roman will push the boundaries of how far back in time we can see them. While most of those detected so far occurred within approximately the last 8 billion years, Roman is expected to see vast numbers of them earlier in the universe\u2019s history, including more than a thousand that exploded more than 10 billion years ago and potentially dozens from as far back as 11.5 billion years. That means Roman will almost certainly set a new record for the farthest type Ia supernova while profoundly expanding our view of the early universe and filling in a critical gap in our understanding of how the cosmos has evolved over time.<\/p>\n

\u201cFilling these data gaps could also fill in gaps in our understanding of dark energy,\u201d Rose said. \u201cEvidence is mounting that dark energy has changed over time, and Roman will help us understand that change by exploring cosmic history in ways other telescopes can\u2019t.\u201d<\/p>\n

But type Ia supernovae will be hidden among a much bigger sample of exploding stars Roman will see once it begins science operations in 2027. The team estimates Roman will also spot about 60,000 core-collapse supernovae, which occur when a massive star runs out of fuel and collapses under its own weight.<\/p>\n

That\u2019s different from type Ia supernovae, which originate from binary star systems that contain at least one white dwarf \u2014 the small, hot core remnant of a Sun-like star \u2014 siphoning material from a companion star. Core-collapse supernovae aren\u2019t as useful for dark energy studies as type Ias are, but their signals look similar from halfway across the cosmos.<\/p>\n

\u201cBy seeing the way an object\u2019s light changes over time and splitting it into spectra \u2014 individual colors with patterns that reveal information about the object that emitted the light\u2014we can distinguish between all the different types of flashes Roman will see,\u201d said Rebekah Hounsell<\/a>, an assistant research scientist at the University of Maryland-Baltimore County working at NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland and a co-author of the study.<\/p>\n

\u201cWith the dataset we\u2019ve created, scientists can train machine-learning algorithms to distinguish between different types of objects and sift through Roman\u2019s downpour of data to find them,\u201d Hounsell added. \u201cWhile searching for type Ia supernovae, Roman is going to collect a lot of cosmic \u2018bycatch\u2019\u2014other phenomena that aren\u2019t useful to some scientists, but will be invaluable to others.\u201d<\/p>\n

Hidden Gems<\/strong><\/p>\n

Thanks to Roman\u2019s large, deep view of space, scientists say the survey should also unearth extremely rare and elusive phenomena, including even scarcer stellar explosions and disintegrating stars.<\/p>\n

Upon close approach to a black hole, intense gravity can shred a star in a so-called tidal disruption event. The stellar crumbs heat up as they swirl around the black hole, creating a glow astronomers can see from across vast stretches of space-time. Scientists think Roman\u2019s survey will unveil 40 tidal disruption events, offering a chance to learn more about black hole physics.<\/p>\n

The team also estimates Roman will find about 90 superluminous supernovae, which can be 100 times brighter than a typical supernova. They pack a punch, but scientists aren\u2019t completely sure why. Finding more of them will help astronomers weigh different theories.<\/p>\n

Even rarer and more powerful, Roman could also detect several kilonovae<\/a>. These blasts occur when two neutron stars \u2014 extremely dense cores leftover from stars that exploded as supernovae \u2014 collide. To date, there has been only one definitive kilonova detection<\/a>. The team estimates Roman could spot five more.<\/p>\n

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\"An<\/a><\/figure>
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This artist’s concept visualizes a kilonova \u2013 an explosion\u00a0that happens when two neutron stars or a neutron star and a black hole collide and merge. When these collisions happen, a fraction of the resulting debris is ejected as jets, which move near the speed of light. The remaining debris produces hot, glowing, neutron-rich clouds that forge heavy elements, like gold and platinum.\u00a0Researchers will mine data from\u00a0NASA\u2019s Nancy Grace Roman Space Telescope, which will survey the same areas of the sky every few days, to identify kilonovae. Roman\u2019s extensive data will help astronomers better identify how often these events occur, how much energy they give off, and how near or far they are.<\/div>\n
Credit: NASA, ESA, J. Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

That would help astronomers learn much more about these mysterious events, potentially including their fate. As of now, scientists are unsure whether kilonovae result in a single neutron star, a black hole, or something else entirely.<\/p>\n

Roman may even spot the detonations of some of the first stars that formed in the universe. These nuclear furnaces were giants, up to hundreds of times more massive than our Sun, and unsullied by heavy elements that hadn\u2019t yet formed<\/a>.<\/p>\n

They were so massive that scientists think they exploded differently than modern massive stars do. Instead of reaching the point where a heavy star today would collapse, intense gamma rays inside the first stars may have turned into matter-antimatter pairs (electrons and positrons). That would drain the pressure holding the stars up until they collapsed, self-destructing in explosions so powerful they\u2019re thought to leave nothing behind.<\/p>\n

So far, astronomers have found about half a dozen candidates of these \u201cpair-instability\u201d supernovae, but none have been confirmed.<\/p>\n

\u201cI think Roman will make the first confirmed detection of a pair-instability supernova,\u201d Rose said \u2014 in fact the study suggests Roman will find more than 10. \u201cThey\u2019re incredibly far away and very rare, so you need a telescope that can survey a lot of the sky at a deep exposure level in near-infrared light, and that\u2019s Roman.\u201d<\/p>\n

A future rendition of the simulation could include even more types of cosmic flashes, such as variable stars and active galaxies. Other telescopes may follow up on the rare phenomena and objects Roman discovers to view them in different wavelengths of light to study them in more detail.<\/p>\n

\u201cRoman\u2019s going to find a whole bunch of weird and wonderful things out in space, including some we haven\u2019t even thought of yet,\u201d Hounsell said. \u201cWe\u2019re definitely expecting the unexpected.\u201d<\/p>\n

For more information about the Roman Space Telescope visit www.nasa.gov\/roman<\/a>.<\/p>\n

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 & Imaging in Thousand Oaks, California.<\/p>\n

By Ashley Balzer<\/strong>
NASA\u2019s Goddard Space Flight Center<\/strong><\/a>, Greenbelt, Md.<\/strong><\/p>\n

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