NASA's Nancy Grace Roman Space Telescope is gliding toward its distant observation post on a pinpoint trajectory so precise that engineers estimate the spacecraft's fuel load will last twice as long as their initial expectations, the space agency confirmed Monday.
The $4.3 billion observatory's designers originally planned to load enough propellant into Roman's four fuel tanks for a minimum lifetime of five years, plus a potential five-year mission extension. That was a conservative estimate. NASA officials knew an on-target launch and perfect execution of the observatory's first post-launch course correction maneuver would leave Roman with a hearty fuel reserve.
"As a result of exquisite planning by our orbital dynamics team, brilliant execution by the operations team, and a precise launch from SpaceX, Roman has fuel for at least 22 years of potential science operations," Jamie Dunn, center director at NASA's Goddard Space Flight Center, said in a press release.
© SpaceX
NASA's Nancy Grace Roman Space Telescope is gliding toward its distant observation post on a pinpoint trajectory so precise that engineers estimate the spacecraft's fuel load will last twice as long as their initial expectations, the space agency confirmed Monday.
The $4.3 billion observatory's designers originally planned to load enough propellant into Roman's four fuel tanks for a minimum lifetime of five years, plus a potential five-year mission extension. That was a conservative estimate. NASA officials knew an on-target launch and perfect execution of the observatory's first post-launch course correction maneuver would leave Roman with a hearty fuel reserve.
"As a result of exquisite planning by our orbital dynamics team, brilliant execution by the operations team, and a precise launch from SpaceX, Roman has fuel for at least 22 years of potential science operations," Jamie Dunn, center director at NASA's Goddard Space Flight Center, said in a press release.
© SpaceX
Now that NASA’s Nancy Grace Roman Space Telescope is on its way toward its Lagrange Point 2 (L2) destination, more of its mission goals are coming into focus, including the possibility that it could detect an Earth-like planet orbiting a star like our own Sun using gravitational microlensing.
The Roman team said such a detection could identify targets for the proposed Habitable Worlds Observatory project, including scanning their atmospheres for signs of extraterrestrial life.
In NASA’s mission fact sheet, Roman’s planners pose several questions. These include:
Although scientists have used several methods to detect exoplanets, including Earth-like planets, Roman will employ three. These include the transit method, microlensing, and direct imaging. NASA said the combination of approaches will allow mission scientists to conduct a “sweeping search expected to uncover around 100,000 new exoplanets — a staggering leap compared to the nearly 6,200 currently known.”
“It is hoped that Roman will discover thousands of new exoplanets and significantly expand our knowledge of the diversity of planetary systems in our Galaxy,” explained Associate Professor Edita Stonkutė, an astrophysicist at Vilnius University unconnected to the Roman team, in a statement emailed to The Debrief.
Most exoplanets have been detected by the dimming of their host star when they transit between it and Earth, giving the transit method its name. Roman plans to use that same method for most of its larger planetary detections. However, among the expected tens of thousands of transit-method detections, mission planners expect a small but sizeable percentage to come from microlensing.
NASA said the “light-bending” microlensing phenomenon occurs when two distant stars “align closely from our vantage point.” Due to the strength of the nearer star’s gravity, the light from the more distant one is “warped” around the nearer one, essentially focusing it very briefly for a distant observer.
“If the alignment is especially close, the nearer star acts like a cosmic lens, focusing and magnifying light from the background star.” Professor Stonkutė explained. “By analysing these changes, astronomers can determine that the planet exists and estimate its mass and orbital characteristics.”
Critically, Professor Stonkutė also noted that microlensing can occur with objects other than stars, including exoplanets.
Using its Wide-Field Array, Roman will monitor hundreds of millions of stars. NASA said the observatory will monitor these target stars for “tiny surges in starlight” that typically signal a microlensing event.
Although the transit method is employed to detect larger exoplanets, NASA noted that microlensing “specializes in finding planets like those in our solar system.” The space agency added that this includes “worlds as lightweight as Mars in their star’s habitable zone or farther out.”
A star’s habitable zone is typically defined as the orbital plane where an exoplanet could sustain liquid water on its surface, a key ingredient for life as we know it.
Professor Stonkutė described microlensing as “particularly valuable” since it can detect planets that are difficult to spot with other planet-hunting methods. The professor said this includes “small Earth-like planets located far from their star.” The Roman team hopes to find “more than 1,000 microlensing planets.”
The professor warned that “most microlensing events cannot be predicted in advance.” As a result, telescopes need to actively scan large areas of the sky to increase the chances of a microlensing detection
“This is precisely where Roman has the edge over other telescopes that have searched for exoplanets using different methods,” the professor added.
While Roman is tasked with directly imaging exoplanets, finding another Earth around a Sun-like star will still require an indirect detection, most likely from a microlensing event. However, the Roman team notes that their observatory “will provide a crucial stepping stone for NASA’s Habitable Worlds Observatory concept.”
According to the space agency, that “flagship” telescope, still awaiting final approval, “would be designed to photograph Earth-like planets for the first time ever.”
Roman may also be able to scan the atmospheres of planets detected with the transit method. The space agency said Roman “would also look for signs of life called biosignatures by measuring atmospheric gases like oxygen and ozone that could signal the presence of living things.”
Christopher Plain is a Science Fiction and Fantasy novelist and has spent the last six years as Associate News Editor and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him at christopher@thedebrief.org.
When NASA announced that the new Nancy Grace Roman Space Telescope will perform its science duties from a point in space known as Lagrange 2, many observers noted that the space agency’s current state-of-the-art space observatory, the James Webb Space Telescope, shares this same orbital location.
Due to the extremely sensitive nature of both satellites and their sensors, and the irreplaceable scientific value they will provide in the future, it might seem natural to wonder whether these two space observatories are at risk of a deep-space collision.
Fortunately, that’s a very unlikely prospect, and here’s a look at all the space separating Roman and Webb—and how NASA will ensure the two observatories remain safely apart.
Many scientific satellites reside a little over 200 miles above Earth in an orbital plane called Low Earth Orbit (LEO). This proximity enables communication with Earth and offers the potential for future servicing missions.
For example, NASA’s groundbreaking Hubble Space Telescope orbits LEO at about 300 miles above Earth. This proximity enabled servicing missions that have kept Hubble delivering valuable scientific data for over three and a half decades since its 1990 launch. Still, LEO also limits which missions Hubble can undertake.
More recently, NASA launched JWST. However, unlike Hubble, Webb rocketed roughly one million miles from Earth before arriving at Lagrange 2. According to a NASA fact sheet detailing the Roman Space Telescope’s mission, this location offers several benefits over LEO.
“At L2, the gravity of the Sun and Earth, together with an object’s motion around the Sun, let it stay lined up with Earth as they orbit,” NASA explains, “allowing Roman to have a relatively steady orbit without using much fuel.”
NASA also notes that heat from Earth, the Sun, and the Moon has less impact on infrared telescopes designed to “see” heat. L2 also offers JWST and Roman, “a constant, unobstructed view of a wide swath of the sky.”
“Earth won’t block much of Roman’s view since it will be so distant,” NASA explains.
Instead of sitting still at the heart of L2, NASA notes that Webb “traces out a large orbit around the actual L2 point.” For comparison, the space agency noted that JWST’s orbit around L2 is “much larger than the Moon’s orbit around Earth.”
Like Webb, the Nancy Grace Roman Space Telescope is also destined for L2. The new space telescope will also trace out an orbit around L2 rather than remaining comparatively stationary.
Because of the wide orbits of both spacecraft and the efforts of the mission’s controllers, NASA said the two valuable space telescopes “will easily be kept far apart.”
Like previous NASA missions, Roman will have a primary lifetime and a backup plan if the observatory remains viable after the first mission ends. For Roman, both the primary and secondary missions are slated for five years, bringing the observatory’s planned potential lifetime up to a possible ten years.
Notably, several NASA missions have continued to deliver scientific data well beyond their planned primary and secondary missions. Perhaps the most famous example is Voyager 1. Launched in 1977, the interplanetary mission has since left the solar system and continues to return data from beyond the heliopause, an area of deep space over 14 billion miles from Earth.
When discussing what obstacles may result in a shorter mission profile, NASA said that “fuel is expected to be the mission’s life-limiting resource.”
“While NASA does not currently have an ability to service observatories at L2, Roman is designed to be refuellable,” they added.
Christopher Plain is a Science Fiction and Fantasy novelist and has spent the last six years as Associate News Editor and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him at christopher@thedebrief.org.
Before NASA’s Nancy Grace Roman Space Telescope arrives at its Lagrange 2 destination and begins performing years of observations, the cutting-edge observatory that started life as a National Reconnaissance Office (NRO) spy satellite will deploy and calibrate its suite of instruments.
These include a primary mirror, a Wide Field Array sensor, and a Coronograph Instrument technology demonstration designed to block out starlight to enable direct imaging of exoplanets.
Here is a quick peek at those instruments, which will help Roman image exoplanets, search for signs of dark matter and dark energy, and add huge amounts of raw scientific data that will keep scientists busy for years to come.
Designed and built at L3Harris Technologies in Rochester, New York. Roman’s primary is 7.9 feet across (2.4 meters). That is the same size as the one on NASA’s legacy Hubble Space Telescope.
However, NASA said Roman’s main mirror, which weighs 410 pounds (186 kilograms), is just one-fourth the weight of Hubble’s, “thanks to major improvements in technology.” They also noted that the weight difference was critical to the Lagrange Point 2 mission’s viability.
While the main mirror will gather light, Roman’s Wide Field Instrument, or WFI, will gather digital images of the cosmos. According to NASA’s mission fact sheet, the 300-megapixel infrared camera “will give Roman the same angular resolution as Hubble but with a field of view at least 100 times larger.”
“Using this instrument, each Roman image will capture a patch of the sky bigger than the apparent size of a full moon,” the space agency explained.
Unlike many telescopes designed to focus incoming light toward a central point, NASA said Roman is designed to “see the most detail in a ring around the center.” That’s because the WFI’s millions of detectors are laid out in an arch shape. The space agency said this design “helps Roman capture a much wider area with equally sharp imaging and also lets both instruments operate simultaneously.”
Due to the hardware and software improvements, NASA said the WFI will gather data “up to 1,000 times faster than Hubble. When Roman’s five-year mission is completed, mission planners said they expect to gather “up to 20,000 terabytes (20 petabytes)” of data.
“Its sweeping cosmic surveys will help scientists discover new information about planets beyond our solar system, untangle mysteries like dark energy, and map how matter is structured and distributed throughout the cosmos,” the agency said when detailing WFI’s capabilities, adding that the mission’s “broad, crisp view will produce an extraordinary resource for a wide range of additional investigations.”
In a fact sheet, NASA said that the detector array at the heart of Roman’s WFI contains 18 “saltine cracker-sized” detectors. The space agency also said that each detector contains roughly 16.8 million tiny pixels (for a total of 300 million), “providing the mission with exquisite image resolution.”
Each cutting-edge detector comprises millions of photodiodes, which convert light into electrical current. NASA said this number of detectors, made from mercury-cadmium-telluride photodiodes (sensors that convert light into an electrical current), provides “one for each pixel.”
The space agency also noted that individual detectors are secured to a silicon electronics board that will help process the light signals using indium. Unlike steel, indium is a soft metal that has roughly the same consistency as chewing gum.
When they are working together, NASA said that these ultra-sensitive detectors “can capture vast areas of sky in a single shot while still revealing incredibly fine detail, allowing Roman to map the cosmos faster and more precisely than ever before.”
Astronomers typically infer the existence of exoplanets by the gravitational effects they exert on their host star or the dimming of the star’s light. However, directly imaging exoplanets has remained challenging because the star’s extremely bright light dwarfs the much dimmer light reflected by the planet. As a result, only a few of the largest, young “super Jupiters” have been directly imaged to date.
To block enough of a star’s light to capture an image of an exoplanet, Roman’s engineers have installed a novel Coronagraph. NASA describes this experimental device as “a system of optics, masks, self-flexing mirrors, and sensors designed to demonstrate the most advanced technologies ever flown in space for directly imaging planets around other stars.”
After its mid-flight deployment, Roman’s Coronagraph team will begin conducting a series of pre-planned observations. Mission planners said these observations “are scheduled for a total of three months spread across the mission’s first year-and-a-half of operations.”
“The Coronagraph aims to photograph worlds and dusty disks around nearby stars in visible light to help us see giant worlds that are older, colder, and in closer orbits than the hot, young super-Jupiters direct imaging has mainly revealed so far,” the space agency explained.
The Roman team expects to release new images by early 2027. For detailed updates, follow the
Roman blog at science.nasa.gov/blogs/roman.
Christopher Plain is a Science Fiction and Fantasy novelist and has spent the last six years as Associate News Editor and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him at christopher@thedebrief.org.
The innovative technology behind NASA’s new premier space observatory, the Nancy Grace Roman Space Telescope, has a secret side.
That’s because the optical technologies that will propel the search for dark matter and exoplanets in the coming years have roots in one of America’s spy agencies.
The clandestine side of the Roman telescope’s story begins in 2012, with a surprise that landed on NASA’s doorstep at the agency’s Goddard Space Flight Center: a pair of once-classified spy satellites.
The satellites were gifted to NASA by the U.S. National Reconnaissance Office (NRO), the military agency tasked with the design and construction of the U.S. federal government’s intelligence-gathering satellites.
The Roman Telescope is a modified version of one of those two former spy satellites NASA received in 2012, which were originally developed for looking back toward Earth, rather than scouring the cosmos for signs of exoplanets and signs of some of the universe’s most elusive phenomena.
However, the original NRO project that led to the development of its satellites ended up being cancelled due to budgetary issues. So as not to allow the technology to go to waste, the orphaned satellites were soon handed over to NASA.
Before the new Roman telescope that has astronomers so excited would take shape, NASA had to take the existing satellite frames provided by the NRO and attach special instruments that would equip it for cosmic observations, rather than just the clandestine ones it was originally designed for with its observations of Earth.
These additions included an infrared camera similar to the one on NASA’s James Webb Space Telescope (JWST), which allows it to observe phenomena at infrared wavelengths and spot phenomena across great cosmic distances that may not be discernible from Earth at normal visible wavelengths.
Along with the addition of new instruments, the satellite was also fitted for deployment further from Earth at the same Lagrange Point currently occupied by Webb.
The telescope is named after Nancy Roman, NASA’s first female executive, who served as its first chief of astronomy and was an influential astronomer in the development of classifications for stellar objects and their motion.
Even with its original development by another government agency, the Roman Telescope’s mission was nearly cancelled because of proposals in 2018 and 2019 under the first Trump administration.
Fortunately, with its launch scheduled for Sunday morning, Roman has already overcome several hurdles on its way from its original development for one of America’s spy agencies to becoming NASA’s newest milestone in astrophysics studies.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached at micah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
After several years of preparation, the Nancy Grace Roman Space Telescope is about to launch.
Here’s a look at the steps, tests, and deployments that NASA’s mission planners hope happen in the hours, days, and weeks after launch.
According to the mission site, once Roman has left Earth’s atmosphere, it will spend the next 90 days going through “a carefully orchestrated series of deployments, calibrations, and tests.”
Within the first hours of launch, NASA says the rocket boosters and main stage of the 18,000-pound (8,000-kilogram) dry-mass spacecraft, which is “about the mass of a Tyrannosaurus rex,” will separate. Soon thereafter, the rocket’s reusable side boosters will return to the area around the launch site and attempt to land.
In space, the rocket’s second stage will separate from the nose cone, which is jettisoned into space. This is followed by Roman separating from the launch vehicle.
To generate power and protect the spacecraft’s sensitive payload, Roman’s solar panels and sunshade will be deployed. According to NASA’s mission fact sheet, each of the space telescope’s six solar panels measures about 7 by 10 feet (2 by 3 meters) and is covered in a total of 3,902 solar cells.
When fully deployed, the panels will combine to provide up to 4 kilowatts of power. For comparison, the mission site says that it is “about the same rate that a modest rooftop solar panel system produces during the daytime.”
Roman will spend the next 30 days speeding toward its final destination, a relatively stable location in the solar system called Lagrange 2, located roughly 930,000 to 1 million miles (1.5 to 1.6 million kilometers) from Earth.
During that journey, the craft’s antenna and deployable aperture will deploy. NASA says the carbon composite radio dish is 5.6 feet (1.7 meters) in diameter. For comparison, the space organization compared its height to an average refrigerator but noted it “weighs only 24 pounds (10.9 kilograms).”
“Its large size will help Roman send radio signals across a million miles of intervening space to Earth,” NASA explained.
One band of the dual-band antenna will receive commands from mission control and return information about the spacecraft’s location and overall health. The second band will communicate what NASA termed “a deluge of data at up to 500 megabits per second.”
About halfway through its voyage, Roman will make a course correction. During that same phase, the spacecraft’s Coronograph instrument will power up. The telescope’s other primary sensor, the Wide Field Instrument, will activate a few weeks later.
“With all components fully deployed, NASA said Roman is over 42 feet (12.7 meters long) and over 14 feet (4.4 meters) wide. The space agency said these dimensions make Roman “about the size of a tour bus.”
Finally, NASA said that throughout the rest of its 90-day commissioning period, both the antenna and Coronagraph “will run through a series of calibrations and tests.”
Although the agency did not specify an exact date for the space telescope’s first light, the Roman team said it “anticipates releasing new images by early 2027.” For detailed updates, you can also follow NASA’s official Roman blog.
Christopher Plain is a Science Fiction and Fantasy novelist and has spent the last six years as Associate News Editor and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him at christopher@thedebrief.org.
Welcome to this special edition of The Intelligence Brief… This week, NASA is preparing to launch the Nancy Grace Roman Space Telescope, its next flagship space observatory and a mission poised to transform our understanding of distant worlds and some of the universe’s greatest mysteries. In our analysis, we’ll be looking at 1) how Roman’s powerful Wide Field and Coronagraph instruments will survey the cosmos on an unprecedented scale, 2) how the telescope could discover thousands of new exoplanets—including elusive rogue worlds—and directly image planets around other stars, 3) how Roman will survey more than a billion galaxies in search of new clues about dark matter and dark energy, and 4) why its combination of Hubble-like image quality and an enormously wider field of view could usher in a new era of astronomical discovery.
“We are poised at the brink of unfathomable scientific discovery.”
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On Sunday morning, NASA will set a new milestone with the launch of the Nancy Grace Roman Space Telescope, setting the course for discoveries that may include new insights into some of the universe’s greatest mysteries.
As NASA’s next flagship space observatory, this powerful new telescope is designed to discover thousands of distant worlds while also probing the lingering mysteries of dark matter and dark energy. Named after Nancy Grace Roman, NASA’s first chief of astronomy and an early advocate for the efforts that led to the launch of the Hubble Space Telescope, the new space observatory bearing her name is poised to offer one of the most detailed views of our universe ever captured.
Scheduled to lift off aboard a SpaceX Falcon Heavy rocket on August 30, 2026, at 7:26 a.m. EDT, the Roman telescope’s mission is comparable in ambition to those of the Hubble and James Webb Space Telescopes, but also very different in many respects. Here’s a look at what to know about this historic mission, what it may help researchers uncover, and why it could set the pace for a range of important scientific advancements in the coming years.
At the heart of its mission, Roman will offer astronomers a remarkably wide view of the cosmos. Surveying immense portions of the sky, the powerful instruments on board the telescope will capture high-resolution imagery comparable to Hubble at certain optical and infrared wavelengths—imagery that could dramatically reshape scientists’ understanding of both planets and the universe they inhabit.
In terms of the technologies it will carry with it into space, Nancy Grace Roman Space Telescope will rely on two primary instruments: its Wide Field Instrument (WFI) and Coronagraph Instrument. The WFI is equipped with a 300-megapixel near-infrared camera enabling wide-area imaging and spectroscopy, allowing Roman to conduct large-scale surveys with great precision and sensitivity—all of which make it ideal for use in the hunt for dark energy, exoplanets, and other hard-to-spot cosmic phenomena.
Meanwhile, Roman’s Coronagraph Instrument is designed specifically for imaging and studying exoplanets. Equipped for both imaging and spectroscopy, the coronagraph will suppress the overwhelming glare of distant stars, potentially making much fainter planets orbiting nearby visible. According to NASA, Roman’s powerful Coronagraph will be the first instrument deployed on a space observatory to leverage “numerically optimized, precision-fabricated coronagraph masks.”
By suppressing the overwhelming glare of distant stars so that much fainter planets around them become visible, Roman’s Coronagraph could achieve as much as 100 times the performance of existing facilities, offering a promising chance that some of the faintest planets in the cosmos—some as much as a billion times fainter than their host stars—could become visible.
With a little luck, Roman could also break new ground with the first direct imagery of an exoplanet possessing rings. Going beyond its immediate discoveries, the coronagraph will also demonstrate technologies that could eventually be incorporated into future observatories, including NASA’s proposed Habitable Worlds Observatory.
Presently, astronomers have confirmed roughly 6,000 planets beyond our Solar System. However, once Roman’s mission gets underway, that number could see a dramatic increase.
One of the ways it will achieve such landmark detections will be with the help of gravitational microlensing, which relies on detecting how the gravity of a foreground object can magnify light from a source much farther away. Using microlensing alone, there is a good chance Roman may discover several hundred—but more likely thousands—of planets, which may include worlds small enough that they have eluded previous detection using existing methods.
Along with the planets it discovers, astronomers anticipate that Roman will also find several new additions to the growing catalog of “rogue planets,” mysterious planetary bodies that wander through the cosmos without orbiting a star.
Additionally, NASA says that anywhere from 60,000 to 200,000 additional candidate planets could be revealed through transit observations, though only a fraction of these are expected to be confirmed through additional observations.
Arguably, one of the most significant components of Roman’s mission involves its study of the unseen side of the cosmos: the mysterious phenomena known as dark energy and dark matter.
In search of answers to such mysteries, Roman will soon begin scanning more than a billion galaxies as it maps the structure and evolution of the universe throughout cosmic history, providing data that will at the very least help researchers narrow down the most promising interpretations among a range of competing explanations for dark energy.
Simultaneously, the telescope will probe dark matter, the unseen material whose gravitational effects are currently needed to explain phenomena in our universe that include the motions of galaxies, as well as the evolution of some of the largest structures in the cosmos.
In many ways, what Roman is expected to achieve will be comparable to its predecessor, the Hubble Space Telescope, although at a far greater scale.
At some wavelengths, Roman will be capable of producing images that approach the clarity of Hubble’s iconic views of our universe, all while capturing as much as 100 times more of the sky with each observation. By capturing more of the sky with each image it produces, Roman’s efforts to map the universe could occur at a remarkable pace—perhaps a thousand times faster than those of its predecessor.
If all goes according to plan, Roman will be launched aboard a SpaceX Falcon Heavy rocket at 7:26 a.m. EDT this Sunday, Aug. 30. NASA will begin live coverage of Roman’s launch on Sunday at 6:20 a.m. Eastern Time, and you can follow the updates online with NASA’s free streaming platforms.
Once it lifts off, Roman will be carried 930,000 miles from Earth to the Sun-Earth Lagrange Point 2 region, which is the same location where the James Webb Space Telescope is currently operating. After it reaches orbit, for the next 90 days, Roman will undergo commissioning, after which science operations are expected to begin sometime in early 2027.
The observatory’s primary mission will last five years, although Roman could potentially remain operational for more than a decade, offering astronomers an unprecedented look at our universe and possibly a few answers to some of the most baffling questions about our universe.
That concludes this week’s installment of The Intelligence Brief. You can read past editions of our newsletter at our website, or if you found this installment online, don’t forget to subscribe and get future email editions from us here. Also, if you have a tip or other information you’d like to send along directly to me, you can email me at micah [@] thedebrief [dot] org, or reach me on X: @MicahHanks.
Here are the top stories we’re covering right now…
NASA engineering teams are preparing for the launch of the Nancy Grace Roman Space Telescope, which will soon begin the first phase of its historic mission to help scientists unlock the mysteries of dark energy.
On Wednesday, the American space agency reported that the completed telescope, presently contained within its payload fairing, has been transported from NASA’s Payload Hazardous Servicing Facility to a SpaceX hangar located at the famous Launch Complex 39A at NASA’s Kennedy Space Center.
If all goes according to plan, the telescope will be launched aboard a SpaceX Falcon Heavy rocket at 7:26 a.m. EDT this Sunday, Aug. 30.
The telescope’s unique science instruments make Roman a different breed of space observatory from its predecessors, like the James Webb Space Telescope and Hubble Telescope, as they are designed with the special focus of advancing the search for dark energy.
Roman is equipped with two primary capabilities, which involve its Wide Field Instrument (WFI) and Coronagraph Instrument. With a 300-megapixel, near-infrared camera designed for large area image capture and spectroscopy, the WFI will enable astronomers to observe a 0.281 square degree field of view and includes a special imaging mode with two slitless spectroscopy modes.
“The instrument provides a sharp point spread function, precision photometry, and stable observations for implementing the Dark Energy, Exoplanet Microlensing, and NIR surveys,” according to a NASA FAQ page detailing Roman’s primary instrument.
Meanwhile, the telescope’s Coronagraph Instrument also features both imaging and spectroscopy modes, with capabilities fine-tuned for imaging exoplanets.
“The Coronagraph will be the first instrument on a space telescope to make use of numerically optimized, precision-fabricated coronagraph masks,” NASA’s FAQ page reads. This will be achieved by employing a combination of deformable mirrors that will enable high-order wavefront control, a low-order wavefront sensing and control system, and finally, CCD detectors designed for electron multiplication and counting low-flux photons.
Along with its search for dark energy and exoplanets, Roman will also provide NASA and researchers around the world with an unprecedented opportunity to study the formation of galaxies and the way that dark matter governs their evolution over time.
NASA will begin live coverage of Roman’s launch on Sunday morning at 6:20 a.m. Eastern Time, and you can follow the updates online with NASA’s free streaming platforms.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached at micah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
NASA is currently targeting August 30 for the launch of the Nancy Grace Roman Space Telescope from Florida. The date can move, as launch dates do, but the mission is close enough to the pad that its central idea deserves a clear look: Roman will survey huge stretches of the universe in one exposure, gathering […]
The post NASA Is Targeting an August Launch for Roman. Here’s What the Telescope Will See appeared first on Curiosmos.
On July 27, technicians at NASA’s Kennedy Space Center in Florida installed a memory card containing 1,350,144 names as part of a commemorative plaque on the Nancy Grace Roman Space Telescope. The names were submitted by people globally, including astronauts from Artemis II and Artemis III. The memory card will travel with the Roman observatory to the Sun-Earth Lagrange point 2, or L2, about one million miles from Earth, where the Sun’s and Earth’s gravity balance out.
Roman is named after Dr. Nancy Grace Roman, NASA’s first chief astronomer and one of the architects of the agency’s modern science program. Roman championed space-based observatories that could study the universe from above Earth’s hazy atmosphere while making their data broadly available to the scientific community.
NASA and SpaceX are targeting launch for no earlier than 7:26 a.m. EDT Sunday, Aug. 30 aboard a SpaceX Falcon Heavy from Launch Complex 39A at Kennedy.
To learn more about the Roman mission, visit:
Image credit: NASA/Jolearra Tshiteya
Downloads
The post Download a Roman Poster! appeared first on NASA Science.
Are you ready for a new view of the universe? The Nancy Grace Roman Space Telescope will reveal distant worlds, dark energy, and the structure of the cosmos, and we want you to be a part of it!
Digital creators and social media users are invited to register to our NASA Social for the Nancy Grace Roman Space Telescope launch. Roman is NASA’s next flagship astrophysics mission, designed to explore everything from our outer solar system to the edge of the observable universe. This mission is scheduled to launch on Aug. 30, 2026, aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Are you passionate about social media and communications? Do you love to create content for an audience? Are you a fan of new, unique experiences? If you said yes, this NASA Social event is for you! This is your opportunity to be on the front lines of this historic mission.
The NASA Social event will take place over two days, including the day of launch. A maximum of 50 digital creators will be selected to attend this two-day event and will be given access similar to news media.
NASA Social participants will have the opportunity to:
NASA Social events are intended for members of the public. Current or former NASA civil servants, NASA contractors, NASA interns, and individuals or organizations currently under contract to provide products or services to NASA are not eligible to apply or participate in NASA Social events.
NASA Social registration for the Roman launch opens on this page on Monday, June 15 and the deadline to apply is at 11:59 p.m. EDT on Sunday, June 28. All applications will be considered on a case-by-case basis.
Do I need to have a social media account to register?
Yes. This event is designed for people who:
Users are encouraged to follow @NASARoman for Roman updates on X, Facebook, and @NASAGoddard and @NASAUniverse on Instagram. Updates and information about the event will be shared on X via @NASA_Events
How do I register?
Registration for this event opens Monday, June 15 and closes at 11:59 p.m. EDT on Sunday, June 28. Registration is for one person only (you) and is non-transferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis.
Can I register if I am not a U.S. citizen?
Yes, this event is open for all to apply.
When will I know if I am selected?
After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the first notifications on July 17 and waitlist notifications on July 22.
What are NASA Social credentials?
All NASA social applications will be considered on a case-by-case basis. Those chosen must prove through the registration process they meet specific engagement criteria.
If you do not make the registration list for this NASA Social, you still can attend the launch off site and participate in the conversation online. Find out about ways to experience a launch at https://www.nasa.gov/kennedy/see-a-launch-up-close/.
What are the registration requirements?
Registration indicates your intent to travel to NASA Kennedy and attend the two-day event in person. You are responsible for your own expenses for travel, accommodation, food, and other amenities.
The schedule of events and special guest appearances are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is canceled with limited or no notice. Please plan accordingly.
Kennedy is a government facility. Those who are selected may need to complete additional steps to receive clearance to enter the secure areas.
IMPORTANT: Those without proper identification cannot be admitted.
For United States Citizens:
You will be required to present a REAL ID compliant identification or valid U.S. passport PLUS one of the following:
Acceptable documents to accompany federal or state identification:
For Foreign Nationals:
For Legal Resident Aliens:
The REAL ID Act was passed by Congress in 2005 to establish minimum security standards for state-issued driver’s licenses and identification cards.
All registrants must be at least 18 years old.
What if the launch date changes?
Hundreds of different factors can cause a scheduled launch date to change multiple times. The launch date will not be official until after the Flight Readiness Review. If the launch date changes prior to the review, NASA may adjust the date of the NASA Social accordingly to coincide with the new target launch date, and will notify registrants of any changes via email.
If the launch is postponed, attendees will be invited to attend a later launch date. If the launch is postponed beyond 72 hours, the NASA Social event may be canceled.
NASA Social attendees are responsible for any additional costs they incur related to any launch delay. We strongly encourage participants to make travel arrangements that are refundable and/or flexible.
What if I cannot come to the Kennedy Space Center?
If you cannot come to NASA Kennedy and attend in person, you should not register for the NASA Social. Join the conversation by following @NASARoman on X and Facebook, and @NASAGoddard and @NASAUniverse on Instagram. You can watch the launch at nasa.gov/live. NASA will provide regular launch and mission updates on @NASA.
If you cannot make this NASA Social, don’t worry; NASA is planning many other NASA Social events in the near future at various locations! Check for updates on NASA Socials.
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