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GSFC_20190626_WFIRST_m13235_widefield_Animation
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titleNancy Grace Roman Space Telescope


NASA's Goddard Space Flight Center.

Music" "Horizon Ahead" from Killer Tracks

Expand
titleRoman Space Telescope


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The Nancy Grace Roman Space Telescope is a next-generation space telescope that will survey the infrared universe from beyond the orbit of the Moon. The spacecraft's giant camera, the Wide Field Instrument (WFI), will be fundamental to this exploration. The WFI features the same angular resolution as Hubble but with 100 times the field of view. Data it gathers will enable scientists to discover new and uniquely detailed information about planetary systems around other stars. The WFI will also map how matter is structured and distributed throughout the cosmos, which should ultimately allow scientists to discover the fate of the universe. Watch this video to see a simplified version of how it works.

Video269.5 MBMP413235_WFI_Roman_Best_1080
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Learn more about the Roman Space Telescope spacecraft with this short tour of the main systems.

NASA's Goddard Space Flight Center


Music: “Phenomenon" from Above and Below Written and produced by Lars Leonhard

Video807.1 MBMP413295_Roman_360_Best_1080https://stsci.box.com/s/9m81dvpe9zpfjc41zeml5hnq0o0kdh14https://svs.gsfc.nasa.gov/13295

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage48.4 KBJPGTurntableRev01A_ProRes_Alpha.00001_printhttps://stsci.box.com/s/e5mcy7dm5i4cp48feffpktv9fscmto0shttps://roman.gsfc.nasa.gov/gallery-spacecraftillustrations.html

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage191.4 KBJPGRoman_Space_Telescope_Still_1https://stsci.box.com/s/iddn4cojy0peaq68urgiv2m5xvautwiwhttps://svs.gsfc.nasa.gov/13621

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage172.2 KBJPGRoman_Space_Telescope_Still_2https://stsci.box.com/s/axgzqky3u55uwjv3iwaags1gvewdz332https://svs.gsfc.nasa.gov/13621

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage178.3 KBJPGRoman_Space_Telescope_Still_3https://stsci.box.com/s/3hr4ctcz7b61j6b14g4lh43ejcfx7wvkhttps://svs.gsfc.nasa.gov/13621

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage507.8 KBJPGRST_2020_Stillhttps://stsci.box.com/s/l6dcfm49nydoschci88jnvmn8o5d75q8https://svs.gsfc.nasa.gov/13621

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage755.2 KBJPGRoman_Space_Telescope_Animation1_Still2https://stsci.box.com/s/qy3f9jyhy3aqxpn1su9qx9vjon0pid1ghttps://svs.gsfc.nasa.gov/13621

Stylized still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage2 MBJPGTrailer_still_1https://stsci.box.com/s/g526b9ntswvm4iovkiqjuksswa8jtodqhttps://svs.gsfc.nasa.gov/13621

Stylized still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage1.5 MBJPGRoman_Still_2https://stsci.box.com/s/h7k7y22w2rpqr0w3q46fdqrp5atysh1fhttps://svs.gsfc.nasa.gov/13621

Stylized still frame of spacecraft animation and name

NASA's Goddard Space Flight CenterImage1.8 MBJPGRoman_Title_1https://stsci.box.com/s/de2mwgl5vg55u3zidr73ztyr498fobumhttps://svs.gsfc.nasa.gov/13621

Still frame of spacecraft animation

NASA's Goddard Space Flight CenterImage38.3 KBJPGTurntableWithBarrelRollA_4k.00738_printhttps://stsci.box.com/s/ckg6p2ta4vpw1nlsuk2xlpllt5n55w21https://svs.gsfc.nasa.gov/13621

"Beauty pass" animation of the Roman Space Telescope spacecraft

NASA's Goddard Space Flight CenterVideo45.4 MBMP4Roman_Space_Telescope_Beauty1_1080https://stsci.box.com/s/5sg8hzhiya6mm8r799fpul6w36wuuh7xhttps://svs.gsfc.nasa.gov/13621

"Beauty pass" animation of the Roman Space Telescope spacecraft

NASA's Goddard Space Flight CenterVideo45.5 MBMP4Roman_Space_Telescope_Beauty2_1080https://stsci.box.com/s/frk2ko9hk4ydq2k8uxkohxvvhk6sy8uzhttps://svs.gsfc.nasa.gov/13621

Welcome to NASA's upcoming infrared survey mission, taking a wider view of the cosmos.

NASA's Goddard Space Flight CenterVideo281.5 MBMP4Roman_Space_Telescope_Trailer_Best_1080https://stsci.box.com/s/ai1fe4kjh29ao3gcqbi93xrku2u9b5uihttps://svs.gsfc.nasa.gov/13606

The Roman Space Telescope’s primary mirror reflects an American flag. Its surface is figured to a level hundreds of times finer than a typical household mirror.

L3Harris TechnologiesImage9 MBJPGpm10https://stsci.box.com/s/xzo05oilxq7upj38wg1gdvitxa111y95https://www.nasa.gov/feature/goddard/2020/primary-mirror-for-nasas-roman-space-telescope-completed

The Nancy Grace Roman Space Telescope’s primary mirror, which will collect and focus light from cosmic objects near and far, has been completed. Using this mirror, Roman will capture stunning space vistas with a field of view 100 times greater than Hubble images.

L3Harris TechnologiesImage1.7 MBJPGpm2_1https://stsci.box.com/s/bou373c30lnu38zn7bcrshm8rie56656https://www.nasa.gov/feature/goddard/2020/primary-mirror-for-nasas-roman-space-telescope-completed

Crane operators lower the support equipment to move the Roman Space Telescope’s primary mirror. Using this mirror, Roman will provide a new view into the universe, helping scientists solve cosmic mysteries related to dark matter, dark energy, and planets around other stars.

L3Harris TechnologiesImage43.7 KBJPGpm3https://stsci.box.com/s/ozwncqvt4ml3idufa4rt00rjvwkikkamhttps://www.nasa.gov/feature/goddard/2020/primary-mirror-for-nasas-roman-space-telescope-completed

Members of the Roman Space Telescope team pose with the telescope’s primary mirror at L3 Harris Technologies in Rochester, New York. The telescope just passed a key milestone review, permitting the team to move on to finalizing the telescope design.

NASA's Goddard Space Flight CenterImage4 MBPNGWFIRSTNASAPhotohttps://stsci.box.com/s/2aj4xjo30g67or6pznpf9vrccmuevcmkhttps://svs.gsfc.nasa.gov/13295

This photo shows the setup for space environment testing of the engineering development unit for Roman’s Solar Array Sun Shield, which will serve two purposes. First, it will supply electrical power to the observatory. Second, it will shield the Optical Telescope Assembly, the Wide Field Instrument, and the Coronagraph Instrument from sunlight.

NASA/Chris GunnImage133.2KBJPGromamsassjpg_1https://stsci.box.com/s/k0g8m3yj3s9y1u949jr5a8q4yhnhdmpqhttps://www.nasa.gov/feature/goddard/2021/nasa-confirms-roman-missions-flight-design-in-milestone-review

This photo shows 18 of Roman's detectors mounted in an engineering test unit of the mission's focal plane array. The focal plane array will be incorporated into Roman's Wide Field Instrument – a 300-megapixel camera that will capture enormous images of the cosmos.

NASA/Chris GunnImage113 KBJPEGromandet-1681946https://stsci.box.com/s/lzh8v5cdxogmio7jwx4uq1qh55twmbi1https://www.nasa.gov/feature/goddard/2021/nasa-s-roman-space-telescope-selects-24-flight-quality-heat-vision-eyes
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titleWide Field Instrument (WFI)

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Greg Mosby holds one of Roman’s detectors (left) and an entire cell phone camera (right) for size comparison. The best modern cell phone cameras can provide around 12-megapixel images, while each of Roman’s detectors contains 16 megapixels. Since Roman’s camera contains 18 detectors, it will capture 300-megapixel panoramas. The mission will conduct sweeping cosmic surveys with the same sharp resolution that the Hubble Space Telescope provides.

eb54z0uwxchl1re2zwz2nj5ogy44jcpr
https://svs.gsfc.nasa.gov/13235

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4k animation of the telescope and Wide Field Instrument, showing a simplified exploded view of how it works.

NASA's Goddard Space Flight Center/CI LabVideo384.5 MBMP4
NASA/Chris GunnImage92.4 KBJPGRoman-detector-phone-camerahttps://stsci.box.com/s/
tltx2mth63vklcet8jxj3k9fbk7n9ifu
5aysqk0z947ldqyw08jlgr9wt5j2kdgshttps://
svs.gsfc
www.nasa.gov
/13235

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Animated GIF of the Roman Wide Field Instrument.

NASA's Goddard Space Flight CenterAnimation1.8 MBGIFWFIRST_WideFieldInstrumenthttps://stsci.box.com/s/itwbh12qrd21uc9ejmc6hugpv3txe8tqhttps://svs.gsfc.nasa.gov/13235
/feature/goddard/2021/nasa-s-roman-space-telescope-selects-24-flight-quality-heat-vision-eyes



NASA's Goddard Space Flight Center

Music: "Concept of Motion" from Universe Production Music

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titleWide Field Instrument (WFI
Expand
titleCoronagraph Instrument (CGI)


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Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.

Image Added

The Nancy Grace Roman Space Telescope is a next-generation space telescope that will survey the infrared universe from beyond the orbit of the Moon. The spacecraft's giant camera, the Wide Field Instrument (WFI), will be fundamental to this exploration. The WFI features the same angular resolution as Hubble but with 100 times the field of view. Data it gathers will enable scientists to discover new and uniquely detailed information about planetary systems around other stars. The WFI will also map how matter is structured and distributed throughout the cosmos, which should ultimately allow scientists to discover the fate of the universe. Watch this video to see a simplified version of how it works.

NASA's Goddard Space Flight Center.


Music" "Horizon Ahead" from Killer Tracks

Video269.5 MBMP413235_WFI_Roman_Best
Video96.8 MBMP413325_Roman_CGI
_1080https://stsci.box.com/s/
yh5oh6lxu1um85pvqsz0j32iokyxfiv0
eb54z0uwxchl1re2zwz2nj5ogy44jcprhttps://svs.gsfc.nasa.gov/
13325
13235
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titleRoman Science

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4k animation of the telescope and Wide Field Instrument, showing a simplified exploded view of how it works.

NASA's Goddard Space Flight Center/CI LabVideo384.5 MBMP4GSFC_20190626_WFIRST_m13235_widefield_Animationhttps://stsci.box.com/s/tltx2mth63vklcet8jxj3k9fbk7n9ifuhttps://svs.gsfc.nasa.gov/13235

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Animated GIF of the Roman Wide Field Instrument.

NASA's Goddard Space Flight CenterAnimation1.8 MBGIFWFIRST_WideFieldInstrumenthttps://stsci.box.com/s/itwbh12qrd21uc9ejmc6hugpv3txe8tqhttps://svs.gsfc.nasa.gov/13235










Exoplanets13644_Rogue_Planet
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titleCoronagraph Instrument (CGI)
Expand
titlePlanets by the Thousands
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titleSolar System
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title


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Rogue planets are free-floating planets that do not orbit a star and instead travel through space. Scientists think they are outcasts from developing planetary systems and may be very numerous throught the galaxy.  This illustration shows a rogue planet traveling through space.

NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Video30 MBMP4

Image Added

Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.

NASA's Goddard Space Flight Center


Music: "Concept of Motion" from Universe Production Music

Video96.8 MBMP413325_Roman_CGI_1080https://stsci.box.com/s/
m6pxbptqq1xwopul054cib53a8476k8b




Eagle_Zoom_3840x2160
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titleRoman Science


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titlePlanets by the Thousands


Expand
titleSolar System


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This Roman simulated image is 1/140th a Roman field of view. There are so many stars at the center of our galaxy that in other telescopes’ views they may blur together, but Roman will see them with high clarity, distinguishing stars in the center bulge from those in the surrounding disk. Tracking the precise positions and colors of individual stars over time will provide insight on the star-formation processes in the Milky Way bulge, bar, and disk.

Matthew T. Penny (Ohio State University)Image5.5 MBPNGSimulated_Bulge_image-WZcolor
Box Live Link
url
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titleExoplanets


13644https://stsci.box.com/s/pqvjc0d4wzp8lkgqyk3od99l9xpd1whb
ThumbnailCreditFile TypeFile SizeFile ExtensionFilenameFile LocationSource Location

Image Added

Rogue planets are free-floating planets that do not orbit a star and instead travel through space. Scientists think they are outcasts from developing planetary systems and may be very numerous throught the galaxy.  This illustration shows a rogue planet traveling through space.

NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Video30 MBMP413644_Rogue_Planet_1080

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HR 8799 is a system that harbors four super-Jupiters orbiting with periods that range from decades to centuries. This footage consists of 7 images of HR 8799 taken with the Keck Telescope over 7 years. 

Jason Wang (Caltech)/Christian Marois (NRC Herzberg)Video1.6 MBMP4hr8799_orbit_hd_crophttps://jasonwang.space/orbits.html

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This animation shows how a planet can disappear in a star’s bright light, and how a coronagraph, such as the one that will be used on Roman, can reveal it.

NASA's Goddard Space Flight Center/CI LabVideo29.5 MBMOVWFIRST_exoplanet_Coronagraph_V2_H264_1080phttps://roman.gsfc.nasa.gov/exoplanets_direct_imaging.html

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The Roman surveys will search for planets toward the center of our Milky Way galaxy, which is heavily populated with stars. The higher density of stars will yield more microlensing events, including those that reveal exoplanets.

NASA's Goddard Space Flight Center/CI LabVideo15.1 MBMP4WFIRST_Microlensing_S4_4k_30fps_h264https://stsci.box.com/s/gu4h9c72e1x4utvlvy7wx8ebif4auqk2m6pxbptqq1xwopul054cib53a8476k8bhttps://romansvs.gsfc.nasa.gov/exoplanets_microlensing.html

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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.

13644

Image Added

HR 8799 is a system that harbors four super-Jupiters orbiting with periods that range from decades to centuries. This footage consists of 7 images of HR 8799 taken with the Keck Telescope over 7 years. 

Jason Wang (Caltech)/Christian Marois (NRC Herzberg)Video1.6 MBMP4hr8799_orbit_hd_cropNASA's Goddard Space Flight CenterVideo20.7 MBMP4WFIRST_Microlensing_S1a_4k_30fps_h264https://stsci.box.com/s/pqvjc0d4wzp8lkgqyk3od99l9xpd1whb
fbcyykftizf6vkqysrefk6o2nd4xx0oc


https://roman.gsfc.nasa.gov/exoplanets_microlensingjasonwang.space/orbits.html

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This animation shows how a planet can disappear in a star’s bright light, and how a coronagraph, such as the one that will be used on Roman, can reveal it.

NASA's Goddard Space Flight Center/CI LabVideo29.5 MBMOVWFIRST_exoplanet_Coronagraph_V2_H264_1080p

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Kepler and other exoplanet search efforts have discovered thousands of large planets with small orbits, represented by the red and black dots on this chart. Roman will find planets with a much wider range of masses orbiting farther from their host star, shown by the blue dots.

NASA’s Goddard Space Flight Center, adapted from Penny et al. (2019)Image1.2 MBPNGRoman_expected_planets-lghttps://roman.gsfc.nasa.gov/exoplanets_direct_microlensingimaging.html

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The Roman surveys will search for planets toward the center of our Milky Way galaxy, which is heavily populated with stars. The higher density of stars will yield more microlensing events, including those that reveal exoplanets.

NASA's Goddard Space Flight Center/CI LabVideo15.1 MBMP4WFIRST_Microlensing_S4_4k_30fps_h264

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This animation shows a planet crossing in front of, or transiting, its host star and the corresponding light curve astronomers would see. Using this technique, scientists anticipate Roman could find 100,000 new worlds.

Credits: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Video884.9 KBMP4Transit-Method-For-Detecting-Planetshttps://roman.gsfc.nasa.gov/exoplanets_transit_methodmicrolensing.html

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This animation illustrates two ways a the concept of gravitational microlensing event could look to an observer. At top is the way it could appear to a telescope able to resolve the features. The source star appears to move and distort as its light is warped by the closer lensing star and its planet. At bottom is a light curve showing the intensity of light from the event. As the two stars reach best alignment, the signal reaches its peak. The planet orbiting the lensing star is detectable as a brief change in brightness.. 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.

NASA's Goddard Space Flight Center/CI LabVideo23 20.7 MBMP4WFIRST_Microlensing_S1bS1a_4k_30fps_h264https://svsroman.gsfc.nasa.gov/20315exoplanets_microlensing.html

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Kepler and other exoplanet search efforts have discovered thousands of large planets with small orbits, represented by the red and black dots on this chart. Roman will find planets with a much wider range of masses orbiting farther from their host star, shown by the blue dots.

NASA’s Goddard Space Flight Center, adapted from Penny et al. (2019)Image1.2 MBPNGRoman_expected_planets-lg

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This pair of animations compare signals from two planet detection methods – microlensing (top) and transit (bottom) – for high- and low-mass planets. Microlensing signals from small planets are rare and brief, but they’re stronger than the signals from other methods.

NASA's Goddard Space Flight Center/CI LabVideo19.9 MBMP4WFIRST_Microlensing_S2_4k_30fps_h264https://svsroman.gsfc.nasa.gov/20315exoplanets_microlensing.html

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This animation shows a planet crossing in front of, or transiting, its host star and the corresponding light curve astronomers would see. Using this technique, scientists anticipate Roman could find 100,000 new worlds.

Credits: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Video884.9 KBMP4Transit-Method-For-Detecting-Planets

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The Roman Space Telescope will have Hubble-like angular resolution since it will orbit above Earth’s atmosphere, enabling it to separate host and source stars from microlensing events. Its wide field of view will allow the Roman Space Telescope to classify planets’ stars on an unprecedented scale, adding to our understanding of the type of systems throughout the galaxy – including those like our own.

NASA's Goddard Space Flight Center/CI LabVideo21.8 MBMP4WFIRST_Microlensing_S5_4k_30fps_h264https://svsroman.gsfc.nasa.gov/20315
Expand
titleStars by the Billions
exoplanets_transit_method.html

Image Added

This animation illustrates two ways a gravitational microlensing event could look to an observer. At top is the way it could appear to a telescope able to resolve the features. The source star appears to move and distort as its light is warped by the closer lensing star and its planet. At bottom is a light curve showing the intensity of light from the event. As the two stars reach best alignment, the signal reaches its peak. The planet orbiting the lensing star is detectable as a brief change in brightness.

NASA's Goddard Space Flight Center/CI LabVideo23 MBMP4WFIRST_Microlensing_S1b_4k_30fps_h264
sxudzjo0bp3528cncsqw6iwch6dkzfdp
Published article:
iopscience
iop.org/article/10.3847/1538-4365/aafb69/pdf 

Penny, M. T., 2019, ApJS, 241, 3P

gsfc.nasa.gov/20315

Image Added

This pair of animations compare signals from two planet detection methods – microlensing (top) and transit (bottom) – for high- and low-mass planets. Microlensing signals from small planets are rare and brief, but they’re stronger than the signals from other methods.

NASA's Goddard Space Flight Center/CI LabVideo19.9 MBMP4WFIRST_Microlensing_S2_4k_30fps_h264https://svs.gsfc.nasa.gov/20315

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The Roman Space Telescope will have Hubble-like angular resolution since it will orbit above Earth’s atmosphere, enabling it to separate host and source stars from microlensing events. Its wide field of view will allow the Roman Space Telescope to classify planets’ stars on an unprecedented scale, adding to our understanding of the type of systems throughout the galaxy – including those like our own.

NASA's Goddard Space Flight Center/CI LabVideo21.8 MBMP4WFIRST_Microlensing_S5_4k_30fps_h264

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This image of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. In the center is Hubble's view of the Pillars of Creation - superimposed on a ground-based image.  Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.

The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Image9.7 MBPNG
vo03mnk2vky8kwm6w3sd2wnw1rxppcod

N/A

Related Press Release - 
hubblesite.org/contents/news-releases/2020/news-2020-41

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This image of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s
svs.gsfc.nasa.gov/20315

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This graphic highlights the search areas of three planet-hunting missions: the upcoming Nancy Grace Roman Space Telescope, the Transiting Exoplanet Survey Satellite (TESS), and the retired Kepler Space Telescope. Astronomers expect Roman to discover roughly 100,000 transiting planets, worlds that periodically dim the light of their stars as they cross in front of them. While other missions, including Kepler's extended K2 survey (not pictured in this graphic), have unveiled relatively nearby planets, Roman will reveal a wealth of worlds much farther from home.

NASA's Goddard Space Flight CenterImage96.1 KBJPEGmission_observations-transit-_mkvhttps://www.nasa.gov/feature/goddard/2021/nasa-s-roman-mission-predicted-to-find-thousands-of-transiting-planets




Expand
titleStars by the Billions


. In the center is Hubble's view of the Pillars of Creation - superimposed on a ground-based image.  Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.  This version has labels.

The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

N/A

Related Press Release - https://hubblesite.org/contents/news-releases/2020/news-2020-41

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This video of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the famous Pillars of Creation superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.

The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

hubblesitecontentsmedia/videos/2020/41/1282-Video?news=true

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This video It begins with a Hubble image famous The view then zooms out to show the full field of view of   This version has labels.Video423 STScI-H-v2041c-d45dk6epga6vje40o7wzgrnmzdura80amediavideos/41/1284-Video?news=trueImage Removed simulated of a portion Andromeda galaxy highlights the high resolution, large , and unique footprint of NASA’s

NASA, STScI, and B.F. Williams (University of Washington)

Image composition: STScI

NASA, STScI, and B. F. Williams (University of Washington)

Image composition: STScI

STSCI-H-p2002b-q-7237x51210d8yszqylp7oum3m4yvx1e885tsyh25kmedia/images02/4609-Image?news=true

NASA, STScI, and B. F. Williams (University of Washington)

Image composition: STScI

STSCI-H-p2002c-q-7237x5121g7nhs7jr4g5s9pmpmbmsvf1c8af866xtimages024610Image

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A composite figure of the Andromeda galaxy (M31) highlights the extremely large

Background image: Digitized Sky Survey and R. Gendler

Moon image: NASA, GSFC, and Arizona State UniversityRoman simulation images: NASA, STScI, and B. F. Williams (University of Washington)

Image composition: STScI

https://hubblesiteimages024611Image

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A composite figure of the Andromeda galaxy (M31) highlights the extremely .  This version has additional labels.Background image: Digitized Sky Survey and R GendlerMoon image: , GSFC and Arizona State UniversityRoman simulation images :NASA, 38p2002ef5400x5400587tn7f4cpsbvxzs1a9c1cpujmn27wru4612

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A composite figure (M31) highlights the extremely large field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.  Inside the Roman footprint is simulated Roman data, which you can see more clearly in the three pull-outs - each one being a Hubble field-of-view.

In addition to the resolved stars in Andromeda, the insets reveal:

The top inset:  star cluster and background galaxy

Middle inset: dust cloud

Bottom inset: young star cluster

Background image: Digitized Sky Survey and R. Gendler

Roman simulation images: 505 andromeda_context_sim_and_pulloutsgjvtupzzyulw41a7lx5u4ckfmitfoere

N/A

Related press-release:  4612

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NASA’s Nancy Grace Roman Space Telescope, will capture the equivalent of 100 high-resolution Hubble images in a single shot, imaging large areas of the sky 1,000 times faster than Hubble. In several months, the Roman Space Telescope could survey as much of the sky in near-infrared light—in just as much detail—as Hubble has over its entire three decades.
Although Roman has not yet opened its wide, keen eyes on the universe, astronomers are already running simulations to demonstrate what it will be able to see and plan their observations.
This simulated image of a portion of our neighboring galaxy Andromeda (M31) provides a preview of the vast expanse and fine detail that can be covered with just a single pointing of the Roman Space Telescope. Using information gleaned from hundreds of Hubble observations, the simulated image covers a swath roughly 34,000 light-years across, showcasing the red and infrared light of more than 50 million individual stars detectable with Roman.

Watch the video to learn more about the Roman Space Telescope's simulated image.

NASA's Goddard Space Flight Center

Music: "Flight Impressions" from Universal Production Music

13497_Simulated_Image_Roman_Best_1080ad3bo5j1m9p5ubjnkz1h5iku0n5pliypsvs.gsfc.nasa.gov/13497

Background image: Nathan Smith, University of Minnesota/NOIRLab/NOAO/AURA/NSFHubble

Mosaic: Hubble Image: NASAESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF

Mystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)Trumpler 14: NASAESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of Arizona)

Composition:  A. Pagan (STScI)

zxxhv4ugl0ou46y7btw1zkf9trp4ecvoRoman Overview Presentationstscieduroman/documentation/technical-documentation

Background image: Nathan Smith, University of Minnesota/NOIRLab/NOAO/AURA/NSFHubble

Mosaic: Hubble Image: NASAESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF

Mystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)Trumpler 14: NASAESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of Arizona)

Composition:  A. Pagan (STScI)

Roman_: Hubble Image N Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image California, Berkeley) and NOAO/AURA/NSFMystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)Trumpler 14: NASAESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of Arizona)

Composition:  A. Pagan (STScI)

url4aupbau6u1mizd6n2xcl7ubio1r3yo18Roman Overview Presentationstsci.edu/roman/documentation/technical-documentation
Thumbnail and DescriptionCreditFile TypeFile SizeFile ExtensionFilenameFile LocationSource Location

Image Added

This Roman simulated image is 1/140th a Roman field of view. There are so many stars at the center of our galaxy that in other telescopes’ views they may blur together, but Roman will see them with high clarity, distinguishing stars in the center bulge from those in the surrounding disk. Tracking the precise positions and colors of individual stars over time will provide insight on the star-formation processes in the Milky Way bulge, bar, and disk.

Matthew T. Penny (Ohio State University)Image5.5 MBPNGSimulated_Bulge_image-WZcolor

Box Live Link
url

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Image9.7 MBPNGEagle_Zoom_RomanHubbleLabeled_3840x2160https://stsci.box.com/s/ybkkkyed2qoqgsph2zsmp8k7olgz7ji0

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Video41.7 MBMP4STScI-H-v2041a-3840x2160

https://stsci.box.com/s/

0hdnebsckqiyi55segnf3wo5bov4hpbr

sxudzjo0bp3528cncsqw6iwch6dkzfdp


Published article: https://

iopscience.iop.org/

article/

10.3847/1538-4365/aafb69/pdf 

Penny, M. T., 2019, ApJS, 241, 3P

Image Added

This image

of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.

In the center is Hubble's view of the

Pillars of Creation - superimposed on a ground-based image.

  Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.


The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Image9.7 MBMP4PNGEagle_Zoom_3840x2160https://stsci.box.com/s/vo03mnk2vky8kwm6w3sd2wnw1rxppcod

N/

A


Related Press Release - https://hubblesite.org/contents/

news-releases/

2020/news-2020

-41

Image Added

This

image

of the

Eagle Nebula showcases the superb resolution and wide field of view

of NASA’s upcoming Nancy Grace Roman Space Telescope.

Image45.4 MBPNGSTSCI-H-p2002a-q-7237x4453https://stsci.box.com/s/tu9i8tuiqnyhoizcd8x6gwubasg788kmhttps://hubblesite.org/contents/media/images/2020/02/4608-Image?news=true

Image Removed

Details of a simulated image of the Andromeda galaxy highlight the high resolution of Roman imagery. Unlike a typical wide field camera, which can cover a large area of sky but cannot reveal fine details, Roman will provide both a large field of view and high resolution. The details shown here each cover about 0.0013 square degrees of sky, the equivalent to a single infrared image from Hubble’s WFC3 camera. The pixel scale is 0.11 arcseconds/pixel.

Image56.1 MBPNG

In the center is Hubble's view of the Pillars of Creation - superimposed on a ground-based image.  Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.  This version has labels.


The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Image9.7 MBPNGEagle_Zoom_RomanHubbleLabeled_3840x2160https://stsci.box.com/s/ybkkkyed2qoqgsph2zsmp8k7olgz7ji0

N/

A


Related Press Release - https://hubblesite.org/contents/

news-releases/2020/

Image Removed

Details of a simulated image of the Andromeda galaxy highlight the high resolution of Roman imagery. Unlike a typical wide field camera, which can cover a large area of sky but cannot reveal fine details, Roman will provide both a large field of view and high resolution. The details shown here each cover about 0.0013 square degrees of sky, the equivalent to a single infrared image from Hubble’s WFC3 camera. The pixel scale is 0.11 arcseconds/pixel.  This version has additional labels.

news-2020-41

Image Added

This video of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the famous Pillars of Creation superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.


The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)

Video41.7 MBMP4STScI-H-v2041a-3840x2160Image56.1 MBPNGhttps://stsci.box.com/s/0hdnebsckqiyi55segnf3wo5bov4hpbrhttps://hubblesite.org/contents/media/videos/2020/41/1282-Video?news=true

Image Added

This video of the Eagle Nebula showcases the superb resolution and wide

field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.

It begins with a Hubble image of the famous Pillars of Creation superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.  This version has labels.


The wide field image for the Eagle nebula is a combination between an image taken by NSF’s 0.9-meter telescope at Kitt Peak National Observatory (Credit: T.A.Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A.Wolpa (NOIRLab/NSF/AURA)) and an image by amateur astronomer Liam Murphy.

L. Hustak (STScI)

Acknowledgement: L. Murphy, T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and B.A.Wolpa (NOAO/AURA/NSF)


Video42.3 MBMP4STScI-H-v2041c-3840x2160https://stsci.box.com/s/d45dk6epga6vje40o7wzgrnmzdura80ahttps://hubblesiteImage38.3 MBPNGSTSCI-H-p2002d-f-5400x5400https://stsci.box.com/s/v0dn04p7uzemp5zis8im8wmqq52npc46.org/contents/media/videos/2020/41/1284-Video?news=true

Image Added

This simulated image of a portion of the Andromeda galaxy highlights the high resolution, large field of view, and unique footprint of NASA’s upcoming Nancy Grace Roman Space Telescope

.

NASA

,

 

STScI, and B.F. Williams (University of Washington)


Image composition: STScI

Image45.4 MBPNGSTSCI-H-p2002a-q-7237x4453https://stsci.box.com/s/tu9i8tuiqnyhoizcd8x6gwubasg788kmhttps://hubblesite.org/contents/media/images/2020/02/4608-Image?news=true

Image Added

Details of a simulated image of the Andromeda galaxy

highlight the high resolution of Roman imagery. Unlike a typical wide field camera, which can cover a large area of sky but cannot reveal fine details, Roman will provide both a large field of view and high resolution. The details shown here each cover about 0.0013 square degrees of sky, the equivalent to a single infrared image from Hubble’s WFC3 camera. The pixel scale is 0.11 arcseconds/pixel.

NASA, STScI, and B. F. Williams (University of Washington)


Image composition: STScI

Image56.1 MBTIFPNGSTSCI-H-p2002b-q-7237x5121https://stsci.box.com/s/0d8yszqylp7oum3m4yvx1e885tsyh25khttps://hubblesite.org/contents/media/images/2020/02/4609-Image?news=trueVideo936.5 MBMP4

Image Added

Details of a simulated image of the Andromeda galaxy highlight the high resolution of Roman imagery. Unlike a typical wide field camera, which can cover a large area of sky but cannot reveal fine details, Roman will provide both a large field of view and high resolution. The details shown here each cover about 0.0013 square degrees of sky, the equivalent to a single infrared image from Hubble’s WFC3 camera. The pixel scale is 0.11 arcseconds/pixel.  This version has additional labels.

NASA, STScI, and B. F. Williams (University of Washington)


Image composition: STScI

Image56.1 MBPNGSTSCI-H-p2002c-q-7237x5121https://stsci.box.com/s/g7nhs7jr4g5s9pmpmbmsvf1c8af866xthttps://

Image Removed

The Carina Nebula is an example of a star-forming region with many stages of the stellar lifecycle captured by Hubble. There is no guarantee that Roman will be studying this same area.

This is the clean version of the image.

hubblesite.org/contents/media/images/2020/02/4610-Image?news=true

Image Added

A composite figure of the Andromeda galaxy (M31) highlights the extremely large field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.

Background image: Digitized Sky Survey and R. Gendler


Moon image: NASA, GSFC, and Arizona State University


Roman simulation images: NASA, STScI, and B. F. Williams (University of Washington)


Image composition: STScI

Image38.3 MBPNGSTSCI-H-p2002d-f-5400x5400https://stsci.box.com/s/v0dn04p7uzemp5zis8im8wmqq52npc46https://hubblesite.org/contents/media/images/2020/02/4611-Image?news=true

Image Added

A composite figure of the Andromeda galaxy (M31) highlights the extremely large field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.  This version has additional labels.

Background image: Digitized Sky Survey and R. Gendler


Moon image: NASA, GSFC, and Arizona State University


Roman simulation images : NASA, STScI, and B. F. Williams (University of Washington)


Image composition: STScI

Image38.4 MBPNGSTSCI-H-p2002e-f-5400x5400Image2.9 MBPNGRoman_Stellar_LC_slide_clean_1920x1080
Box Live Link
urlhttps://stsci.box.com/s/587tn7f4cpsbvxzs1a9c1cpujmn27wruhttps://hubblesite.org/

Image Removed

The Carina Nebula is an example of a star-forming region with many stages of the stellar lifecycle captured by Hubble. There is no guarantee that Roman will be studying this same area.

This is the annotated version of the image.

contents/media/images/2020/02/4612-Image?news=true

Image Added

A composite figure of the Andromeda galaxy (M31) highlights the extremely large field of view of NASA’s upcoming Nancy Grace Roman Space Telescope.  Inside the Roman footprint is simulated Roman data, which you can see more clearly in the three pull-outs - each one being a Hubble field-of-view.


In addition to the resolved stars in Andromeda, the insets reveal:

The top inset:  star cluster and background galaxy

Middle inset: dust cloud

Bottom inset: young star cluster

Background image: Digitized Sky Survey and R. Gendler


Roman simulation images: NASA, STScI, and B. F. Williams (University of Washington)


Image composition: STScI

Image50.5 MBTIFandromeda_context_sim_and_pulloutshttps://stsci.box.com/s/gjvtupzzyulw41a7lx5u4ckfmitfoere

N/A


Related press-release:  https://hubblesite.org/contents/media/images/2020/02/4612-Image?news=true

Image Added

NASA’s Nancy Grace Roman Space Telescope, will capture the equivalent of 100 high-resolution Hubble images in a single shot, imaging large areas of the sky 1,000 times faster than Hubble. In several months, the Roman Space Telescope could survey as much of the sky in near-infrared light—in just as much detail—as Hubble has over its entire three decades.

Although Roman has not yet opened its wide, keen eyes on the universe, astronomers are already running simulations to demonstrate what it will be able to see and plan their observations.

This simulated image of a portion of our neighboring galaxy Andromeda (M31) provides a preview of the vast expanse and fine detail that can be covered with just a single pointing of the Roman Space Telescope. Using information gleaned from hundreds of Hubble observations, the simulated image covers a swath roughly 34,000 light-years across, showcasing the red and infrared light of more than 50 million individual stars detectable with Roman.

Watch the video to learn more about the Roman Space Telescope's simulated image.

NASA's Goddard Space Flight Center


Music: "Flight Impressions" from Universal Production Music

Video936.5 MBMP413497_Simulated_Image_Roman_Best_1080https://stsci.box.com/s/ad3bo5j1m9p5ubjnkz1h5iku0n5pliyphttps://svs.gsfc.nasa.gov/13497

Image Added

The Carina Nebula is an example of a star-forming region with many stages of the stellar lifecycle captured by Hubble. There is no guarantee that Roman will be studying this same area.

This is the clean version of the image.

Background image: Nathan Smith, University of Minnesota/NOIRLab/NOAO/AURA/NSFHubble

Mosaic: Hubble Image: NASAESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF


Mystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)


Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)


Trumpler 14: NASAESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of Arizona)

Composition:  A. Pagan (STScI)

Image2.9 MBPNGRoman_Stellar_LC_slide_clean_1920x1080

Box Live Link
urlhttps://stsci.box.com/s/zxxhv4ugl0ou46y7btw1zkf9trp4ecvo

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Image Added

The Carina Nebula is an example of a star-forming region with many stages of the stellar lifecycle captured by Hubble. There is no guarantee that Roman will be studying this same area.

This is the annotated version of the image.

Background image: Nathan Smith, University of Minnesota/NOIRLab/NOAO/AURA/NSFHubble

Mosaic: Hubble Image: NASAESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF


Mystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)


Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)


Trumpler 14: NASAESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of Arizona)

Composition:  A. Pagan (STScI)

Image2.9 MBPNGRoman_Image2.9 MBPNGStellar_LC_slide_annotated_wo_Title_1920x1080

Box Live Link
urlhttps://stsci.box.com/s/0ow02ukb622hey5s8zt911fqagqvfkz0

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Image Modified

The Carina Nebula is an example of a star-forming region with many stages of the stellar lifecycle captured by Hubble. There is no guarantee that Roman will be studying this same area.

This is the full annotated version of the image, including title and Hubble instruments used in the pull-out Hubble images.

Background image: Nathan Smith, University of Minnesota/NOIRLab/NOAO/AURA/NSFHubble

Mosaic

: Hubble Image: NASAESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF


Mystic Mt.: NASAESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)


Eta Carina: NASAESA, N. Smith (University of Arizona), and J. Morse (BoldlyGo Institute)


Trumpler 14NASAESA,

and J.

Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain);
Acknowledgment: N. Smith (University of

Arizona)

Composition:  A. Pagan (STScI)

Image2.9 MBPNGRoman_Stellar_LC_slide_annotated_wInstruments_1920x1080

Box Live Link
urlhttps://stsci.box.com/s/4aupbau6u1mizd6n2xcl7ubio1r3yo18

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Image Added

NASA’s upcoming Nancy Grace Roman Space Telescope will see thousands of exploding stars called supernovae across vast stretches of time and space. Using these observations, astronomers aim to shine a light on several cosmic mysteries, providing a window onto the universe’s distant past and hazy present.

NASA's Goddard Space Flight Center

Music: "Relentless Data" from Universal Production Music

Video654.2 MBMP413852_Roman_Standard_Candle_Supernovae_1080_BestImage2.9 MBPNGRoman_Stellar_LC_slide_annotated_wInstruments_1920x1080
Box Live Link

https://

svs.gsfc.nasa.gov/13852



Expand
titleGalaxies by the Millions


Thumbnail and DescriptionCreditFile TypeFile SizeFile ExtensionFilenameFile LocationSource Location

This image of galaxy cluster Abell 426 showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It highlights Hubble's view of the galaxy NGC 1275 superimposed on a ground-based image. Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.


The wide field image for Abell 426 is composed of a combination of the Digitized Sky Survey and an image by Petri Kehusmaa.

L. Hustak (STScI)

Acknowledgement: Digitized Sky Survey and P. Kehusmaa

Image8.3 MBPNGAbell246_Zoom_3840x2160https://stsci.box.com/s/r6deulxldsro4vvfk8uu6owem39hm78y

N/A


Related Press Release - https://hubblesite.org/contents/news-releases/2020/news-2020-41

This image of galaxy cluster Abell 426 showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It highlights Hubble's view of the galaxy NGC 1275 superimposed on a ground-based image. Roman’s Wide Field Instrument field of view is highlighted. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.  This version has labels.


The wide field image for Abell 426 is composed of a combination of the Digitized Sky Survey and an image by Petri Kehusmaa.

L. Hustak (STScI)

Acknowledgement: Digitized Sky Survey and P. Kehusmaa

Image8.3 MBPNGAbell246_Zoom_RomanHubbleLabeled_3840x2160https://stsci.box.com/s/38thedm791ragzsrbixdnbq1yczt6cq6

N/A


Related Press Release - https://hubblesite.org/contents/news-releases/2020/news-2020-41

This video of galaxy cluster Abell 426 showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the galaxy NGC 1275 superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.


The wide field image for Abell 426 is composed of a combination of the Digitized Sky Survey and an image by Petri Kehusmaa.

L. Hustak (STScI)

Acknowledgement: Digitized Sky Survey and P. Kehusmaa

Video22.9 MBMP4STScI-H-v2041b-3840x2160https://stsci.box.com/s/omngflj4hxisfa39wsp858gjacgg34a0https://hubblesite.org/contents/media/videos/2020/41/1283-Video?news=true

This video of galaxy cluster Abell 426 showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the galaxy NGC 1275 superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing.  This version has labels.


The wide field image for Abell 426 is composed of a combination of the Digitized Sky Survey and an image by Petri Kehusmaa.

L. Hustak (STScI)

Acknowledgement: Digitized Sky Survey and P. Kehusmaa

Video23.8 MBMP4STScI-H-v2041d-3840x2160https://stsci.box.com/s/v0dmg4druro82sk89tfnqtbsu58tvfkshttps://hubblesite.org/contents/media/videos/2020/41/1285-Video?news=true

Roman will find a diversity of galaxies at different stages of their evolution—galaxies in small groups and in large clusters, merging galaxies, and newborn galaxies.  

By capturing both volume and detail, Roman will greatly advance knowledge about galaxies and their variety of forms, and also their evolution over the history of the universe.

This image showcases separate Hubble observations of select galaxies in the Coma Cluster, within a single Roman field of view.

This version has basic annotations.

Background Image: Digitized Sky Survey

Galaxy Images:  NASAESA, M. Sun (University of Alabama), W. Cramer and J. Kenney (Yale University), J. Mack (STScI), and J. Madrid (Australian Telescope National Facility) and Hubble Heritage Team (STScI/AURA).

Image Composition:  A. Pagan (STScI)

Image3.8 MBPNGComaCluster_Roman_Galaxy_Morphology_1920x1080_clean

Box Live Link
urlhttps://stsci.box.com/s/1onr0dd73jzk9i06oqzi6t8a3ntxworo

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Roman will find a diversity of galaxies at different stages of their evolution—galaxies in small groups and in large clusters, merging galaxies, and newborn galaxies.  

By capturing both volume and detail, Roman will greatly advance knowledge about galaxies and their variety of forms, and also their evolution over the history of the universe.

This image showcases separate Hubble observations of select galaxies in the Coma Cluster, within a single Roman field of view.

This version has additional annotations.

Background Image: Digitized Sky Survey

Galaxy Images:  NASAESA, M. Sun (University of Alabama), W. Cramer and J. Kenney (Yale University), J. Mack (STScI), and J. Madrid (Australian Telescope National Facility) and Hubble Heritage Team (STScI/AURA).

Image Composition:  A. Pagan (STScI)

Image3.8 MBPNGGalaxyMorphology_RomanSlide_1920x1080_annotated_woTitle

Box Live Link
urlhttps://stsci.box.com/s/lazffh86z22f8sw3s5eusbufcf7xpug5

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

This image showcases UGC 2885 (Rubin's Galaxy), with Hubble's view in inset and the Roman field of view.  Roman will be able to capture the entire halo of galaxies like Rubin in a single pointing, which is about 100 times larger than a Hubble pointing.

Hubble's View of Rubin's Galaxy:  NASA, ESA, and B. Holwerda (University of Louisville)


Background Image: DSS


Image Composition: J. DePasquale (STScI)

Image46.5 MBTIFrubins_pullouthttps://stsci.box.com/s/dq5r4xkqoahwsh8st12405alxna1iztq

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation


Hubble's Rubin Galaxy press release - https://hubblesite.org/contents/news-releases/2020/news-2020-1

This image showcases UGC 2885 (Rubin's Galaxy), with Hubble's view in inset and the Roman field of view.  Roman will be able to capture the entire halo of galaxies like Rubin in a single pointing, which is about 100 times larger than a Hubble pointing.


In this version, an estimate of the extent of the halo of Rubin's Galaxy is shown.

Hubble's View of Rubin's Galaxy:  NASA, ESA, and B. Holwerda (University of Louisville)


Background Image: DSS


Image composition: J. DePasquale (STScI)

Image46.5 MBTIFrubins_pullout_withHalohttps://stsci.box.com/s/05rcljanmdjnw504os94t4fw31v8tmns

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation


Hubble's Rubin Galaxy press release - https://hubblesite.org/contents/news-releases/2020/news-2020-1

This composite image illustrates the possibility of a Roman Space Telescope “ultra deep field” observation. In a deep field, astronomers collect light from a patch of sky for an extended period of time to reveal the faintest and most distant objects. This view centers on the Hubble Ultra Deep Field (outlined in blue), which represents the deepest portrait of the universe ever achieved by humankind, at visible, ultraviolet and near-infrared wavelengths. Two insets reveal stunning details of the galaxies within the field.

Beyond the Hubble Ultra Deep Field, additional observations obtained over the past two decades have filled in the surrounding space. These wider Hubble observations reveal over 265,000 galaxies, but are much shallower than the Hubble Ultra Deep field in terms of the most distant galaxies observed.

These Hubble images are overlaid on an even wider view using ground-based data from the Digitized Sky Survey. An orange outline shows the field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. Roman’s 18 detectors will be able to observe an area of sky at least 100 times larger than the Hubble Ultra Deep Field at one time, with the same crisp sharpness as Hubble.

NASA, ESA, and A. Koekemoer (STScI)

Acknowledgement: Digitized Sky Survey

Image6 MBTIFSTScI-R-p2103a-f-1920x1080

Box Live Link
urlhttps://stsci.box.com/s/b4wwoszzf369tdq1vjt80ihlsbax39cj

https://hubblesite.org/contents/media/images/2021/03/4797-Image?news=true

This composite annotated image illustrates the possibility of a Roman Space Telescope “ultra deep field” observation. In a deep field, astronomers collect light from a patch of sky for an extended period of time to reveal the faintest and most distant objects. This view centers on the Hubble Ultra Deep Field (outlined in blue), which represents the deepest portrait of the universe ever achieved by humankind, at visible, ultraviolet and near-infrared wavelengths. Two insets reveal stunning details of the galaxies within the field.

Beyond the Hubble Ultra Deep Field, additional observations obtained over the past two decades have filled in the surrounding space. These wider Hubble observations reveal over 265,000 galaxies, but are much shallower than the Hubble Ultra Deep field in terms of the most distant galaxies observed.

These Hubble images are overlaid on an even wider view using ground-based data from the Digitized Sky Survey. An orange outline shows the field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. Roman’s 18 detectors will be able to observe an area of sky at least 100 times larger than the Hubble Ultra Deep Field at one time, with the same crisp sharpness as Hubble.

NASA, ESA, and A. Koekemoer (STScI)

Acknowledgement: Digitized Sky Survey

Image6 MBTIFSTScI-R-p2103b-f-1920x1080

Box Live Link
urlhttps://stsci.box.com/s/vrvjy3fsvly4d22gyco0myt8ifutzux2


https://hubblesite.org/contents/media/images/2021/03/4798-Image?news=true

This zoom-out animation begins with a view of the Hubble Ultra Deep Field (outlined in blue), which represents the deepest portrait of the universe ever achieved by humankind, at visible, ultraviolet and near-infrared wavelengths. The view then expands to show a wider Hubble survey of that area of sky (white outline), which captured about 265,000 galaxies in a large mosaic. Expanding further, we see the Hubble data overlaid on a ground-based view using data from the Digitized Sky Survey.

An orange outline shows the field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. Roman’s 18 detectors will be able to observe an area of sky at least 100 times larger than the Hubble Ultra Deep Field at one time, with the same crisp sharpness as Hubble.

NASA, ESA, A. Koekemoer (STScI), and A. Pagan (STScI)Video20.2 MBMP4STScI-R-v2103a-1920x1080

Box Live Link
urlhttps://stsci.box.com/s/l1np584ffk80dt6h0aivgfrbufstay57


https://hubblesite.org/contents/media/videos/2021/03/1303-Video?news=true

This zoom-out annotated animation begins with a view of the Hubble Ultra Deep Field (outlined in blue), which represents the deepest portrait of the universe ever achieved by humankind, at visible, ultraviolet and near-infrared wavelengths. The view then expands to show a wider Hubble survey of that area of sky (white outline), which captured about 265,000 galaxies in a large mosaic. Expanding further, we see the Hubble data overlaid on a ground-based view using data from the Digitized Sky Survey.

An orange outline shows the field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. Roman’s 18 detectors will be able to observe an area of sky at least 100 times larger than the Hubble Ultra Deep Field at one time, with the same crisp sharpness as Hubble.

NASA, ESA, A. Koekemoer (STScI), and A. Pagan (STScI)Video20.4 MBMP4STScI-R-v2103b-1920x1080

Box Live Link
urlhttps://stsci.box.com/s/25389q0wj13xfnu8g5gaf80p1ed1m9gc


https://hubblesite.org/contents/media/videos/2021/03/1304-Video?news=true










Expand
titleCosmology


Thumbnail and DescriptionCreditFile TypeFile SizeFile ExtensionFilenameFile LocationSource Location

(2011) Astronomers have pushed NASA's Hubble Space Telescope to its limits by finding what they believe is the most distant object ever seen in the universe. Its light traveled 13.2 billion years to reach Hubble, roughly 150 million years longer than the previous record holder. The age of the universe is 13.7 billion years.

Illustration: NASA, ESA, and A. Feild (STScI);


Science: NASA, ESA, G. Illingworth (University of California, Santa Cruz), R. Bouwens (University of California, Santa Cruz, and Leiden University), and the HUDF09 Team

Image3.4 MBJPGEarly-Universehttps://stsci.box.com/s/ah83zdbpqtv46ci932imgv209yfh1rr7https://hubblesite.org/contents/media/images/2011/05/2815-Image.html?news=true

The SDSS map of the Universe. Each dot is a galaxy; the color bar shows the local density.

SDSSImage173.1 KBJPGorangepiehttps://stsci.box.com/s/6xfec4uos1147czkkz3epuydta4p647yhttps://www.sdss.org/science/

Visualization of simulated Roman emission-line galaxy distribution data used to measure BAO and RSD. The wedge shown covers an RA sweep of 45° with a DEC thickness of 1°, and includes more than 215,000 galaxies.


Data provided by Z. Zhai and Y. Wang, Caltech/IPAC, and A. Benson, Carnegie Observatories

Data Visualization: J. DePasquale, STScI.

Image3.7 MBPNGstatic_wedge-rev

Box Live Link
urlhttps://stsci.box.com/s/0k41nxrwkkkun4niexke9ee9lgonkwvk

"Cosmology with Roman" Fact Sheet

https://stsci.edu/roman/documentation/technical-documentation

Visualization of simulated Roman emission-line galaxy distribution data used to measure BAO and RSD. The wedge shown covers an RA sweep of 45° with a DEC thickness of 1°, and includes more than 215,000 galaxies of a much larger 5-million galaxy simulated galaxy catalog.

This version developed for experts in cosmology.

Data provided by Z. Zhai and Y. Wang, Caltech/IPAC, and A. Benson, Carnegie Observatories

Data Visualization: J. DePasquale and D. Player, STScI.

Image10.8 MBPNGLSS_Roman_Version1_Final

Box Live Link
urlhttps://stsci.box.com/s/8vx2iiipqqo7qtnwvsbzu57gjcqow9qi

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Visualization of simulated Roman emission-line galaxy distribution data used to measure BAO and RSD. The wedge shown covers an RA sweep of 45° with a DEC thickness of 1°, and includes more than 215,000 galaxies of a much larger 5-million galaxy simulated galaxy catalog.

This version developed for those not experts in cosmology.

Data provided by Z. Zhai and Y. Wang, Caltech/IPAC, and A. Benson, Carnegie Observatories

Data Visualization: J. DePasquale and D. Player, STScI.

Image10.3 MBPNGLSS_Roman_Version2_Final

Box Live Link
urlhttps://stsci.box.com/s/uirf16r1uy09gd7yoractn45bbtfp6zx

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

This animation explains how BAOs arose in the early universe and how astronomers can study the faint imprint they made on galaxy distribution to probe dark energy’s effects over time. In the beginning, the cosmos was filled with a hot, dense fluid called plasma. Tiny variations in density excited sound waves that rippled through the fluid. When the universe was about 400,000 years old, the waves froze where they were. Slightly more galaxies formed along the ripples. These frozen ripples stretched as the universe expanded, increasing the distance between galaxies. Astronomers can study this preferred distance between galaxies in different cosmic ages to understand the expansion history of the universe.

NASA's Goddard Space Flight Center


Music: "Pulse and Glow" from Adrift in Time. Written and Produced by Lars Leonhard.

Video250 MBMP413768_BAO_Narr_4k

Box Live Link
urlhttps://stsci.box.com/s/yvpr37k2q9ioupb46e7vb6wrjrn6wnl8

https://svs.gsfc.nasa.gov/13768

Shorter, unnarrated version of the animation above.

This animation explains how BAOs arose in the early universe and how astronomers can study the faint imprint they made on galaxy distribution to probe dark energy’s effects over time. In the beginning, the cosmos was filled with a hot, dense fluid called plasma. Tiny variations in density excited sound waves that rippled through the fluid. When the universe was about 400,000 years old, the waves froze where they were. Slightly more galaxies formed along the ripples. These frozen ripples stretched as the universe expanded, increasing the distance between galaxies. Astronomers can study this preferred distance between galaxies in different cosmic ages to understand the expansion history of the universe.

NASA's Goddard Space Flight CenterVideo66.2 MBMP4BAO_Short_4k

Box Live Link
urlhttps://stsci.box.com/s/0hkg1xr1qyth907vg2jrfu77s9v4qrbx

https://svs.gsfc.nasa.gov/13768

The small peak near the center of the graph in this video shows how BAOs subtly influenced galaxy distribution. Today, there is a slight bump in the probability of finding galaxies about 500 million light-years away from each other. This distance shrinks as we look farther out into space, to earlier cosmic times.

NASA's Goddard Space Flight CenterVideo23.2 MBMP4BAO_Bump_Graph_4k

Box Live Link
urlhttps://stsci.box.com/s/4vv36lx5bndzct48jx5rtwvs01vidzro

https://svs.gsfc.nasa.gov/13768

Waves of sound – BAOs – ripple through the primordial cosmic sea in this animated gif.

NASA's Goddard Space Flight CenterAnimation4.6 MBGIFBAO_Ripples

Box Live Link
urlhttps://stsci.box.com/s/3wn2mmlalw9yof1bh0wolgxcbh9bslah

https://svs.gsfc.nasa.gov/13768

Dark Energy Expansion Graph: Animation illustrating the changing rate of expansion due to dark energy.

NASA's Goddard Space Flight CenterVideo53.8 69MBMOVDark_Energy_Expansion_Graph_FINAL-1080phttps://roman.gsfc.nasa.gov/dark_energy.html

This visualization shows how dark matter (blue-gray threads) provided the framework for normal matter (bright spots) to build up into large cosmic structures, like galaxies and galaxy clusters.

KIPAC/StanfordAnimation69 MBGIFDark_Matter_Simulationhttps://roman.gsfc.nasa.gov/dark_matter.html

NASA's Wide Field Infrared Survey Telescope will explore how dark energy has affected the universe's expansion in the past. 

NASA's Goddard Space Flight CenterVideo14.4 MBMP4Unraveling_the_Mysteries_of_Dark_Energy_with_NASA's_WFIRST.mp4https://roman.gsfc.nasa.gov/newsroom_2019.html



...

Expand
titleBig Data and Archive


https://stsci.box.com/s/0ajh7iv14086w4dlfo9mok75dlorogxlRoman Overview Presentationokmw15dblwmq4ajnmkfnivxdwb4e4p6s
Thumbnail and DescriptionCreditFile TypeFile SizeFile ExtensionFilenameFile LocationSource Location

Image Removed

This infographic showcases the difference in data volume between the Nancy Grace Roman, Webb and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.

NASA's Goddard Space Flight CenterImage38.9 MBPNGRoman_Data_Scale_Finalhttps://stsci.box.com/s/iqmluwt2j2dyeexzpv8vyfdo4kkristphttps://svs.gsfc.nasa.gov/13667
File LocationSource Location

Image AddedImage Removed

This infographic showcases the difference in data volume between the Nancy Grace Roman, Webb and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.

NASA's Goddard Space Flight CenterImage3938.3 9 MBPNGRoman_Data_Scale_HubbleOnly_Finalhttps://stsci.box.com/s/okmw15dblwmq4ajnmkfnivxdwb4e4p6siqmluwt2j2dyeexzpv8vyfdo4kkristphttps://svs.gsfc.nasa.gov/13667

Image RemovedImage Added

This infographic showcases the difference in data volume between the Nancy Grace Roman and Hubble space telescopes, using hard drives to symbolize data volume.   Each day, Roman will send over 500 times more data back to Earth than Hubble.  This version gives the time baseline by which these archival data are collected (30 years for Hubble, 5 years for Roman).

Z. Levy (STScI)

.

NASA's Goddard Space Flight CenterImage139.7 3 MBJPGPNGBig Data - with timeRoman_Data_Scale_HubbleOnly_Final
Box Live Link
urlhttps://stsci.edu/roman/documentation/technical-documentationsvs.gsfc.nasa.gov/13667

Image AddedImage Removed

This infographic showcases the difference in data volume between the Nancy Grace Roman and Hubble space telescopes, using hard drives to symbolize data volume.  Each day, Roman will send over 500 times more data back to Earth than Hubble.  This version leaves off the time baseline by which these archival data are collected (30 years for Hubble, 5 years for Roman).

Z. Levy (STScI)Image1.6 MBJPGBig Datahttps://stsci.box.com/s/n89dvdu344h7br3j09udbet76w5mxh2t

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Hubble.  This version gives the time baseline by which these archival data are collected (30 years for Hubble, 5 years for Roman).

Z. Levy (STScI)Image1.7 MBJPGBig Data - with time

Box Live Link
urlhttps://stsci.box.com/s/0ajh7iv14086w4dlfo9mok75dlorogxl

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Image Added
This infographic showcases the difference in data volume between the Nancy Grace Roman and Hubble space telescopes, using hard drives to symbolize data volume.  Each day, Roman will send over 500 times more data back to Earth than Hubble.  This version leaves off the time baseline by which these archival data are collected (30 years for Hubble, 5 years for Roman).

Image Removed

This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The yellow squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. A blue square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team

Image Composition: Z. Levy (STScI)
Image81.5 6 MBJPGRoman - Simulated ViewBig Datahttps://stsci.box.com/s/bceee8zopmvsq169n5tkndutfwnaezlun89dvdu344h7br3j09udbet76w5mxh2t

Roman Overview Presentation

https://stsci.edu/roman/documentation/technical-documentation

Image RemovedImage Added

This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The purple yellow squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. An orange A blue square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team

ImagePNG


Image Composition: Z. Levy (STScI)

Image8.5 MBJPGRoman - Simulated ViewGreatfield_Simulated_Roman_Landscape_Texthttps://stsci.box.com/s/9fgfz4uyjmpa1io3yzow2w9kn2icigxgbceee8zopmvsq169n5tkndutfwnaezlu

Roman Overview Presentation

https://

svs.gsfc.nasa.gov/13667

stsci.edu/roman/documentation/technical-documentation

Image AddedImage Removed

This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The purple squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. An orange square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_PortraitLandscape_Texthttps://stsci.box.com/s/4wrzhvltn01mcpu2w238tddsvsx8fsmc9fgfz4uyjmpa1io3yzow2w9kn2icigxghttps://svs.gsfc.nasa.gov/13667

Image RemovedImage Added

This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The purple squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. An orange square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_LandscapePortrait_NoTextTexthttps://stsci.box.com/s/lnp2rumbiadldy6a6wrcj392qvbmhzvw4wrzhvltn01mcpu2w238tddsvsx8fsmchttps://svs.gsfc.nasa.gov/13667

Image RemovedImage Added

This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The purple squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. An orange square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_PortraitLandscape_NoTexthttps://stsci.box.com/s/61cwd1r28a686qh1uze2v15ws3azc5rqlnp2rumbiadldy6a6wrcj392qvbmhzvwhttps://svs.gsfc.nasa.gov/13667

Image RemovedImage Added

This video of the Eagle Nebula showcases the superb resolution and simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the famous Pillars of Creation superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing. This video contains labels.

L. Hustak (STScI)Video41.3 MBMP4STScI-H-v2041c-3840x2160-Labels
Box Live Link
urlhttps://stsci.box.com/s/05sxlj6trikhcgimb89bxo98dyhmprpx
https://svs.gsfc.nasa.gov/13672

Image Removed

This video of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s upcoming Nancy Grace Roman Space Telescope. It begins with a Hubble image of the famous Pillars of Creation superimposed on a ground-based image. The view then zooms out to show the full field of view of Roman’s Wide Field Instrument. Roman’s images will have the resolution of Hubble while covering an area about 100 times larger in a single pointing. This video does not contain labels.

L. Hustak (STScI)Video40.7 MB MP4STScI-H-v2041a-3840x2160-NoLabels

and exquisite resolution. The purple squares, which all contain background imagery simulated using data from Hubble’s Cosmic Assembly Near-infrared Deep Extragalactic Survey (CANDELS) program, outline the area Roman can capture in a single observation. An orange square shows the field of view of Hubble’s Wide Field Camera 3 for comparison. While the CANDELS program took Hubble nearly 21 days to survey in near-infrared light, Roman’s large field of view and higher efficiency would allow it to survey the same area in less than half an hour. Top left: This view illustrates a region of the large nearby spiral galaxy M83. Top right: A hypothetical distant dwarf galaxy appears in this magnified view, demonstrating Roman’s ability to detect small, faint galaxies at large distances. Bottom left: This magnified view illustrates how Roman will be able to resolve bright stars even in the dense cores of globular star clusters. Bottom right: A zoom of the CANDELS-based background shows the density of high-redshift galaxies Roman will detect.

Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_Portrait_NoTexthttps://stsci.box.com/s/4kh1m1h6rpi2dtxe4229vyty4db5oe3o61cwd1r28a686qh1uze2v15ws3azc5rqhttps://svs.gsfc.nasa.gov/1367213667

This illustration compares the relative sizes of the areas of sky covered by two surveys: Roman’s High Latitude Wide Area Survey, outlined in blue, and the largest mosaic led by Hubble, the Cosmological Evolution Survey (COSMOS), shown in red. In current plans, the Roman survey will be more than 1,000 times broader than Hubble’s. Roman will also explore more distant realms of space than most other telescopes have probed in previous efforts to study why the expansion of the universe is speeding up.

NASA's Goddard Space Flight CenterImage3.8 MBJPEGroman_hls_mkiii_2https://stsci.box.com/s/x8gtecqqdonl5zdm3nkxq4pw75l20wa9https://www.nasa.gov/feature/goddard/2021/nasa-s-roman-mission-will-help-empower-a-new-era-of-cosmological-discovery




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