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Nancy Grace Roman, shown here at NASA's Goddard Space Flight Center in approximately 1972, was the first female executive and the first Chief of Astronomy at NASACredit: NASAImage701.2 KBJPGnancy grace romanhttps://stsci.box.com/s/pjwtwa4q7z199puxppt3q4niwmae6whahttps://roman.gsfc.nasa.gov/aboutNGR.html


Learn about Nancy Grace Roman, her contribution to NASA missions, and how NASA has honored her.

Credit: NASA's Goddard Space Flight Center


Music: "Rising Tides" from Universal Production Music

Video956.8 MBMP4Roman_Biography_Best_1080https://stsci.box.com/s/i26zvhytv00tqiwu1yw1t4vsmbdn0w5whttps://svs.gsfc.nasa.gov/13608


The original prototypes of the LEGO® Ideas "Women of NASA" set displayed in front of the Apollo Lunar Module in the Boeing Milestones of Flight Hall at the Smithsonian’s National Air and Space Museum in Washington, DC, August 20, 2018. Credit: National Air and Space Museum

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Smithsonian's National Air and Space Museum

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Contact Smithsonian Institution

Image2 MBJPGNASM2018-02043https://stsci.box.com/s/rrcyydzfzkgvy2v299smf185edd6gxbjhttps://airandspace.si.edu/multimedia-gallery/nasm2018-02043jpg


Nancy Grace Roman, standing here in front of a 1/6-scale model of the Hubble Space Telescope at NASA's Goddard Space Flight Center, is known to many as the "Mother of Hubble" for her foundational role in the observatory's planning and program structure, paving the way for missions like the Roman Space Telescope (formerly WFIRST).Credit: NASAImage1 MBJPGNGR_Still_1https://stsci.box.com/s/cwp47ll85gode0u4fakyxeriklk5xw32https://roman.gsfc.nasa.gov/aboutNGR.html


Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team.Photographer: NASA/GSFC/Bill HrybykImage4 MBJPGGSFC_20170331_2017-11028_037_orighttps://stsci.box.com/s/wpbl1g90uren6f4iheg1cedv7105g1kphttps://images.nasa.gov/details-GSFC_20170331_2017-11028_037


Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team.Photographer: NASA/GSFC/Bill HrybykImage6 MBJPGGSFC_20170331_2017-11028_014_orighttps://stsci.box.com/s/2xg0hbfofxp3gubg345azk54st4sdvn5https://images.nasa.gov/details-GSFC_20170331_2017-11028_014


NASA's Associate Administrator of the Science Mission Directorate Dr. Edward J. Weiler presents the Women in Aerospace's Lifetime Achievement Award to retired NASA chief astronomer Nancy Grace Roman at the organization's annual awards ceremony and banquet held at the Ritz-Carlton Hotel in Arlington, VA on Tuesday, Oct. 26, 2010. Four current NASA leaders and one retiree were recognized for their work by Women in Aerospace. The event celebrates women's professional excellence in aerospace and honors women who have made outstanding contributions to the aerospace community. Photo Credit: (NASA/Bill Ingalls)Photographer: (NASA/Bill Ingalls)Image16.6 MBTIF201010260006HQ_orighttps://stsci.box.com/s/19s43nv877zxbglxflxgkww09hyhru7yhttps://images.nasa.gov/details-201010260006HQ


The history of women's contributions to the fields of science, technology, engineering, and math (STEM) is long and varied. But it has also often been overlooked or underrepresented. This series highlights only a very few of the women who have made important discoveries and have had a crucial impact on STEM fields. This, however, is not just a look into the past. Today, women are in every STEM discipline, in every type of job, and represent the widest range of background and experiences.


Download the free poster set to use in your space

Credit: NASA


Illustration: Kristin DiVona

Image3.4 MBPDFroman_posterhttps://stsci.box.com/s/qif9riups3ye1w650tg0u854dz62hcg9https://chandra.si.edu/women/images/roman.pdf


Nancy with a model of an Orbiting Solar Observatory.Credit: NASAImage1.2 MBPNGnancy-modelhttps://stsci.box.com/s/ewta914jgirwifgx4g4v7geynckws1rshttps://hackaday.com/2018/04/03/nancy-grace-roman-mother-of-the-hubble/










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

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


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


Stylized still frame of spacecraft animationCredit: 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 nameCredit: NASA's Goddard Space Flight CenterImage1.8 MBJPGRoman_Title_1https://stsci.box.com/s/de2mwgl5vg55u3zidr73ztyr498fobumhttps://svs.gsfc.nasa.gov/13621


Still frame of spacecraft animationCredit: 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 spacecraftCredit: 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 spacecraftCredit: 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.Credit: 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.Credits: 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.Credits: 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.Credits: 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.Credit: NASA's Goddard Space Flight CenterImage4 MBPNGWFIRSTNASAPhotohttps://stsci.box.com/s/2aj4xjo30g67or6pznpf9vrccmuevcmkhttps://svs.gsfc.nasa.gov/13295










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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.

Credit: NASA's Goddard Space Flight Center.


Music" "Horizon Ahead" from Killer Tracks

Video269.5 MBMP413235_WFI_Roman_Best_1080https://stsci.box.com/s/eb54z0uwxchl1re2zwz2nj5ogy44jcprhttps://svs.gsfc.nasa.gov/13235


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


Animated GIF of the Roman Wide Field Instrument.Credit: NASA's Goddard Space Flight CenterAnimation1.8 MBGIFWFIRST_WideFieldInstrumenthttps://stsci.box.com/s/itwbh12qrd21uc9ejmc6hugpv3txe8tqhttps://svs.gsfc.nasa.gov/13235










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

Credit: NASA's Goddard Space Flight Center


Music: "Concept of Motion" from Universe Production Music

Video96.8 MBMP413325_Roman_CGI_1080https://stsci.box.com/s/yh5oh6lxu1um85pvqsz0j32iokyxfiv0https://svs.gsfc.nasa.gov/13325




















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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.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Video30 MBMP413644_Rogue_Planet_1080https://stsci.box.com/s/m6pxbptqq1xwopul054cib53a8476k8bhttps://svs.gsfc.nasa.gov/13644




















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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 MBPNGEagle_Zoom_3840x2160https://stsci.box.com/s/vo03mnk2vky8kwm6w3sd2wnw1rxppcod

N/A


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


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.  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/news-2020-41


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-3840x2160https://stsci.box.com/s/0hdnebsckqiyi55segnf3wo5bov4hpbrhttps://hubblesite.org/contents/media/videos/2020/41/1282-Video?news=true


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://hubblesite.org/contents/media/videos/2020/41/1284-Video?news=true


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


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 MBPNGSTSCI-H-p2002b-q-7237x5121https://stsci.box.com/s/0d8yszqylp7oum3m4yvx1e885tsyh25khttps://hubblesite.org/contents/media/images/2020/02/4609-Image?news=true


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


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


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-5400x5400https://stsci.box.com/s/587tn7f4cpsbvxzs1a9c1cpujmn27wruhttps://hubblesite.org/contents/media/images/2020/02/4612-Image?news=true


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


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.

Credit: 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
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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


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: STScI

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

N/A


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: STScI

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

N/A


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


The footprint of the Nancy Grace Roman Space Telescope's Wide Field Instrument on top of the Hubble Legacy Survey.


Hubble Legacy Survey:

This Hubble Space Telescope image represents the largest, most comprehensive "history book" of galaxies in the universe.

The image, a combination of nearly 7,500 separate Hubble exposures, represents 16 years' worth of observations.

The ambitious endeavor, called the Hubble Legacy Field, includes several Hubble deep-field surveys, including the eXtreme Deep Field (XDF), the deepest view of the universe. The wavelength range stretches from ultraviolet to near-infrared light, capturing all the features of galaxy assembly over time.

The image mosaic presents a wide portrait of the distant universe and contains roughly 265,000 galaxies. They stretch back through 13.3 billion years of time to just 500 million years after the universe's birth in the big bang. The tiny, faint, most distant galaxies in the image are similar to the seedling villages from which today's great galaxy star-cities grew. The faintest and farthest galaxies are just one ten-billionth the brightness of what the human eye can see.

The wider view contains about 30 times as many galaxies as in the Hubble Ultra Deep Field, taken in 2004. The new portrait, a mosaic of multiple snapshots, covers almost the width of the full Moon. Lying in this region is the XDF, which penetrated deeper into space than this legacy field view. However, the XDF field covers less than one-tenth of the full Moon's diameter.


Hubble Legacy Field:
NASA, ESA, G. Illingworth and D. Magee (University of California, Santa Cruz), K. Whitaker (University of Connecticut), R. Bouwens (Leiden University), P. Oesch (University of Geneva,) and the Hubble Legacy Field team


Background Image: DSS


Image Composition: STScI

Image2.9 MBPNGHLF-Roman_1920x1080https://stsci.box.com/s/t41rs4u61b2rdjvq4iunkkstt87lfblh

N/A

Related Hubble Legacy Field Press Release - https://hubblesite.org/contents/news-releases/2019/news-2019-17.html?itemsPerPage=100


The footprint of the Nancy Grace Roman Space Telescope's Wide Field Instrument on top of the Hubble Legacy Survey.  Pullout- of the Hubble Ultra Deep Field is shown.


Hubble Legacy Survey:

This Hubble Space Telescope image represents the largest, most comprehensive "history book" of galaxies in the universe.

The image, a combination of nearly 7,500 separate Hubble exposures, represents 16 years' worth of observations.

The ambitious endeavor, called the Hubble Legacy Field, includes several Hubble deep-field surveys, including the eXtreme Deep Field (XDF), the deepest view of the universe. The wavelength range stretches from ultraviolet to near-infrared light, capturing all the features of galaxy assembly over time.

The image mosaic presents a wide portrait of the distant universe and contains roughly 265,000 galaxies. They stretch back through 13.3 billion years of time to just 500 million years after the universe's birth in the big bang. The tiny, faint, most distant galaxies in the image are similar to the seedling villages from which today's great galaxy star-cities grew. The faintest and farthest galaxies are just one ten-billionth the brightness of what the human eye can see.

The wider view contains about 30 times as many galaxies as in the Hubble Ultra Deep Field, taken in 2004. The new portrait, a mosaic of multiple snapshots, covers almost the width of the full Moon. Lying in this region is the XDF, which penetrated deeper into space than this legacy field view. However, the XDF field covers less than one-tenth of the full Moon's diameter.

Hubble Legacy Field:
NASA, ESA, G. Illingworth and D. Magee (University of California, Santa Cruz), K. Whitaker (University of Connecticut), R. Bouwens (Leiden University), P. Oesch (University of Geneva,) and the Hubble Legacy Field team


Hubble Ultra Deep Field (2004):   NASAESA, S. Beckwith (STScI) and the HUDF Team.


Background Image: DSS


Image Composition: STScI

Image2.9 MBPNGHLF-Roman_1920x1080_pullouthttps://stsci.box.com/s/nuhffgt5nzv4xej447a2efaiu7ufpv5w

N/A

Related Hubble Legacy Field Press Release - https://hubblesite.org/contents/news-releases/2019/news-2019-17.html?itemsPerPage=100


Related Hubble Ultra Deep Field (2004) Press Release - https://hubblesite.org/contents/news-releases/2004/news-2004-07.html











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(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.


Updated version in progress by STScI.

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.


Updated version using simulated Roman data in progress by STScI.

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










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


This infographic showcases the difference in data volume between the Nancy Grace Roman and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.Credit: NASA's Goddard Space Flight CenterImage39.3 MBPNGRoman_Data_Scale_HubbleOnly_Finalhttps://stsci.box.com/s/okmw15dblwmq4ajnmkfnivxdwb4e4p6shttps://svs.gsfc.nasa.gov/13667


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.

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


Image Composition: STScI

Image8.5 MBJPGRoman - Simulated Viewhttps://stsci.box.com/s/bceee8zopmvsq169n5tkndutfwnaezlu


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.

Credit: Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_Landscape_Texthttps://stsci.box.com/s/9fgfz4uyjmpa1io3yzow2w9kn2icigxghttps://svs.gsfc.nasa.gov/13667


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.

Credit: Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_Portrait_Texthttps://stsci.box.com/s/4wrzhvltn01mcpu2w238tddsvsx8fsmchttps://svs.gsfc.nasa.gov/13667


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.Credit: Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation TeamImage
PNGGreatfield_Simulated_Roman_Landscape_NoTexthttps://stsci.box.com/s/lnp2rumbiadldy6a6wrcj392qvbmhzvwhttps://svs.gsfc.nasa.gov/13667


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.Credit: 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/61cwd1r28a686qh1uze2v15ws3azc5rqhttps://svs.gsfc.nasa.gov/13667










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Comparison of Hubble, Webb, and Roman, including their unique strengths and synergies.Credit:  A. James (STScI)Image32.4 MBPNGRoman-Hubble-Webb_comparison

https://stsci.box.com/s/s2f0es38bw4kex10lhks2x58pubfo0k3

https://hubblesite.org/hubble-30th-anniversary/resources


Comparison of observatories in the 2020s and their windows into the electromagnetic spectrum.  



Credit: A. James (STScI)Image1.3 MBJPGmany_observatories_wavelength_graphhttps://stsci.box.com/s/1nbv554hcym2yjth9a5etnm9ebfzwqnq


NASA Astrophysics Fleet Mission ChartCredit: NASAimage3.5 MBPDFAstro Fleet2019-Feb21_TAGGEDhttps://stsci.box.com/s/ferl1fvl5q9j3nypo5t1lw17vcj4hm3ghttps://smd-prod.s3.amazonaws.com/science-pink/s3fs-public/atoms/files/Astro%20Fleet2019-Feb21_TAGGED.pdf


Comparison of Hubble and expected Rubin Observatory LSST data resolution. (L) BVz color image from the Hubble CANDELS field with θ = 0.1” and r ≈ 28.5. Roman will have comparable resolution. (R) Simulated Rubin LSST image made by degrading Hubble data to Rubin resolution of θ = 0.6”. In the Rubin image, the galaxy is blended with surrounding objects. Correlating overlapping Rubin and Roman imagery would make it possible to develop machine learning algorithms to deblend Rubin imagery that does not overlap with Roman.


Clean version.

Image from B.E. Robertson, et al. 2019, Nat Rev Phys, 1, 450



image2 MBPNGRoman_Deblending_clean



Comparison of Hubble and expected Rubin Observatory LSST data resolution. (L) BVz color image from the Hubble CANDELS field with θ = 0.1” and r ≈ 28.5. Roman will have comparable resolution. (R) Simulated Rubin LSST image made by degrading Hubble data to Rubin resolution of θ = 0.6”. In the Rubin image, the galaxy is blended with surrounding objects. Correlating overlapping Rubin and Roman imagery would make it possible to develop machine learning algorithms to deblend Rubin imagery that does not overlap with Roman.


Annotated version.

Image from B.E. Robertson, et al. 2019, Nat Rev Phys, 1, 450image2 MBPNGRoman_Deblending_annotated

https://ui.adsabs.harvard.edu/abs/2019NatRP...1..450R/abstract




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