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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 Lab | Video | 29.5 MB | MOV | WFIRST_exoplanet_Coronagraph_V2_H264_1080p | https://roman.gsfc.nasa.gov/exoplanets_direct_imaging.html |
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Penny, M. T., 2019, ApJS, 241, 3P
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) Image | 9.7 MB | PNG | Eagle_Zoom_3840x2160N/A Related Press Release -This image of the Eagle Nebula showcases the superb resolution and wide field of view of NASA’s
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) Image | 9.7 MB | PNG | Eagle_Zoom_RomanHubbleLabeled_3840x2160 | https://N/A Related Press Release -
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| NASA’s Nancy Grace Roman Space Telescope will be a powerful tool for studying galaxies throughout the cosmos. It will be able to provide spectra for every galaxy in its field of view. And with a field of view 200 times that of the Hubble Space Telescope at infrared wavelengths, Roman can capture thousands of objects of interest in a single observation. | VIDEO: Robert L. Hurt (IPAC) Music: "Red Giant" by Stellardrone | Video | 35.1 MB | MP4 | STScI-01G68DFH1Z4CB5FWSSE3CM5BK8wrqqwy5gvve8i0lqbtwvc9hli8624qifhubblesite.org/contents/news-releases/2022/news-2022-018.html?filterUUID=5f9d3684-88ed-4633-b385-93fd21831642
svs.gsfc.nasa.gov/13667 | ||||||
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) | Image | 1.7 MB | JPG | Big Data - with time |
This animation portrays the complementary nature of imaging and spectroscopy to understand galaxies. It begins with a portion of the Hubble GOODS-South field, a region of the sky containing hundreds of visible galaxies. Then rainbow-colored lines called spectra are added next to selected galaxies; in reality, every star and galaxy has its light spread out. The underlying image later fades away to highlight the galaxies’ spectra, which contain a wealth of information including distances (redshifts). The image and spectra were obtained by Hubble and illustrate what will be done with Roman, but over a vastly larger number of galaxies.
ANIMATION: NASA, ESA, Joseph DePasquale (STScI)
Roman Overview Presentation |
title | Big Data and Archive |
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Thumbnail and Description | Credit | File Type | File Size | File Extension | Filename | File Location | Source Location | ||||||||||||
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This infographic showcases the difference in data volume between the Nancy Grace Roman , Webb 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. | NASA's Goddard Space Flight Center | Image | 38.9 MB | PNG | 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) | Image | 1.6 MB | JPG | Big DataRoman_Data_Scale_Final | https://stsci.box.com/s/iqmluwt2j2dyeexzpv8vyfdo4kkristpn89dvdu344h7br3j09udbet76w5mxh2t | Roman Overview Presentation svsgsfc.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. | NASA's Goddard Space Flight Center | Image | 39.3 MB | PNG | Roman_Data_Scale_HubbleOnly_Final | https://stsci.box.com/s/okmw15dblwmq4ajnmkfnivxdwb4e4p6s | https://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 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: | 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) | Image | 18.7 5 MB | JPG | Big Data - with time | Roman Overview Presentation https://www.stsci.edu/roman/documentation/technical-documentation |
| Z. Levy (STScI) | Image | 1.6 MB | JPG | Big Data | Roman - Simulated View | https://stsci.box.com/s/bceee8zopmvsq169n5tkndutfwnaezlu | Roman Overview Presentation https://www.stsci.edu/roman/documentation/technical-documentation | ||
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 Team | Image | PNG | Greatfield_Simulated_Roman_Landscape_Text | https://stsci.box.com/s/n89dvdu344h7br3j09udbet76w5mxh2tRoman Overview Presentation9fgfz4uyjmpa1io3yzow2w9kn2icigxg | https://wwwsvs.gsfc.stscinasa.edu/roman/documentation/technical-documentationgov/13667 | |||||||||||||
This simulated image illustrates the wide range of science enabled by Roman's extremely wide field of view and exquisite resolution. The yellow 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. A blue 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 Team | Image Composition: Z. Levy (STScI) | Image | 8.5 MB | JPG | PNG | Greatfield_Simulated_Roman_Portrait_TextRoman - Simulated View | https://stsci.box.com/s/bceee8zopmvsq169n5tkndutfwnaezlu4wrzhvltn01mcpu2w238tddsvsx8fsmc Roman Overview Presentation | https://wwwsvs.gsfc.stscinasa.edu/roman/documentation/technical-documentationgov/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. | Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team | Image | PNG | Greatfield_Simulated_Roman_Landscape_TextNoText | https://stsci.box.com/s/9fgfz4uyjmpa1io3yzow2w9kn2icigxglnp2rumbiadldy6a6wrcj392qvbmhzvw | https://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. | Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team | Image | PNG | Greatfield_Simulated_Roman_Portrait_TextNoText | https://stsci.box.com/s/4wrzhvltn01mcpu2w238tddsvsx8fsmc61cwd1r28a686qh1uze2v15ws3azc5rq | https://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. | Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team | Image | PNG | 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 Center | Image | 3.8 MB | JPEG | roman_hls_mkiii_2Greatfield_Simulated_Roman_Landscape_NoText | https://stsci.box.com/s/lnp2rumbiadldy6a6wrcj392qvbmhzvwx8gtecqqdonl5zdm3nkxq4pw75l20wa9 | https://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. | Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team | Image | PNG | www.nasa.gov/feature/goddard/2021/nasa-s-roman-mission-will-help-empower-a-new-era-of-cosmological-discovery | |||
The Hubble image of a portion of the GOODS-South field (left) required multiple individual exposures that were stitched into a mosaic. The Roman Space Telescope will have a field of view (right) at least 100 times greater than Hubble, allowing it to capture data on thousands of galaxies in a single exposure. | IMAGE: NASA, ESA IMAGE PROCESSING: Joseph DePasquale (STScI) ACKNOWLEDGMENT: Pascal Oesch (University of Geneva), Mireia Montes (UNSW), DSS | Image | 32.8 MB | PNG | STScI-01FF85PY2TZSQRK1TVB7Y6NA0J | https://stsci.box.com/s/kza6zz7s7oo7l1svay3vw30bv00fo46t | https://hubblesite.org/contents/news-releases/2021/news-2021-048.html | ||||||||||||
The Roman Space Telescope is designed for large surveys of the sky. This animation gives a sense of the scale of just one of Roman’s potential survey areas, which would span an area of 2,000 square degrees – about 10,000 times the size of the full Moon. | NASA, IPAC, Robert L. Hurt (IPAC) Acknowledgement: This animation has made use of the Stellarium planetarium. | Video | 3.2 MB | MP4 | STScI-01FG2BZXPDVVSD26QQMSRGC7ZGGreatfield_Simulated_Roman_Portrait_NoText | https://stsci.box.com/s/61cwd1r28a686qh1uze2v15ws3azc5rq7t3gi35q8mkssf8cx170bg0xg6laft8d | https://svs.gsfc.nasa.gov/13667hubblesite.org/contents/media/videos/2021/048/01FG274RXS1QBDZA8WJ7MBAX99?news=true | ||||||||||||
The Nancy Grace Roman Space Telescope is a clue-hunter. As a survey mission, Roman will observe areas of the sky repeatedly, much like going back to the room multiple times to look for new details, or details that may have changed. It will cast a wide net with Hubble Space Telescope-quality data, but with 200 times Hubble’s infrared field of view! The infrared Roman mission will greatly expand our view of the universe, and it will provide many more clues to help solve some the greatest mysteries of astrophysics. | Illustration: J. Kang/STScI | Image | 682.2 KB | JPG | post_01 | 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 Center | Image | 3.8 MB | JPEG | roman_hls_mkiii_2 | https://stsci.box.com/s/x8gtecqqdonl5zdm3nkxq4pw75l20wa98r9v6y7137opysjc5ildaw66b9r1onl8 | https://wwwtwitter.nasa.govcom/featureSpaceTelescope/goddard/2021/nasa-s-roman-mission-will-help-empower-a-new-era-of-cosmological-discoverystatus/1562836961064538117 | ||||||
Like a detective who shares clues, the Nancy Grace Roman Space Telescope will provide open access and analysis of its data to scientists everywhere! | Illustration: J. Kang/STScI | Image | 480.5 KB | JPG | post_04 | The Hubble image of a portion of the GOODS-South field (left) required multiple individual exposures that were stitched into a mosaic. The Roman Space Telescope will have a field of view (right) at least 100 times greater than Hubble, allowing it to capture data on thousands of galaxies in a single exposure. | IMAGE: NASA, ESA IMAGE PROCESSING: Joseph DePasquale (STScI) ACKNOWLEDGMENT: Pascal Oesch (University of Geneva), Mireia Montes (UNSW), DSS | Image | 32.8 MB | PNG | STScI-01FF85PY2TZSQRK1TVB7Y6NA0J | https://stsci.box.com/s/kza6zz7s7oo7l1svay3vw30bv00fo46tcf1s5uejujolke3puxndi6hmtku9cb5u | https://hubblesitetwitter.orgcom/contentsSpaceTelescope/news-releases/2021/news-2021-048.html | The Roman Space Telescope is designed for large surveys of the sky. This animation gives a sense of the scale of just one of Roman’s potential survey areas, which would span an area of 2,000 square degrees – about 10,000 times the size of the full Moon. | status/1570452139985764352 | ||||
As a survey mission, the Nancy Grace Roman Space Telescope will collect Hubble-quality data but with 200 times Hubble’s infrared field of view. It will view planets by the thousands, galaxies by the millions, and stars by the billions. It will transmit almost 1,400 gigabytes of information to the ground each day—more than the storage space of an average home computer. For comparison, the Hubble Space Telescope sends less than 3 gigabytes a day, and the James Webb Space Telescope sends less than 60 gigabytes. After just five years of observing, Roman will have delivered 20,000 terabytes! All of this data will provide a treasure trove of information to scientists for many years to come. | Illustration: J. Kang/STScI | Image | 406 KB | JPG | post_05 | NASA, IPAC, Robert L. Hurt (IPAC) Acknowledgement: This animation has made use of the Stellarium planetarium. | Video | 3.2 MB | MP4 | STScI-01FG2BZXPDVVSD26QQMSRGC7ZG | https://stsci.box.com/s/7t3gi35q8mkssf8cx170bg0xg6laft8d5hf914jm0tnuxohtipwjeigtc31vnmkt | https://hubblesite.org/contents/media/videos/2021/048/01FG274RXS1QBDZA8WJ7MBAX99?news=true://twitter.com/SpaceTelescope/status/1572985338041098240 |
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