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Thumbnail | Working Name | Description | Credit | File Type | File Size | File Extension | Filename | File Location | Source Location | 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 Technologies | Image | 9 MB | JPG | pm10xzo05oilxq7upj38wg1gdvitxa111y95wwwfeature/goddard/2020/primary-mirror-for-nasas-roman-space-telescope-completedThe 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 Technologies | Image | 1.7 MB | JPG |
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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 | Source:
Rights Usage:
| Image | 2 MB | JPG | NASM2018-02043 |
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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). | NASA | Image | 1 MB | JPG | NGR_Still_1 |
title | Wide Field Instrument (WFI) |
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title | Coronagraph Instrument (CGI) |
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title | Roman Science |
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Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team. | Photographer: NASA/GSFC/Bill Hrybyk | Image | 4 MB | JPG | GSFC_20170331_2017-11028_037_orig | https://stsci.box.com/s/wpbl1g90uren6f4iheg1cedv7105g1kp | https://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 Hrybyk | Image | 6 MB | JPG | GSFC_20170331_2017-11028_014_orig | https://stsci.box.com/s/2xg0hbfofxp3gubg345azk54st4sdvn5 | https://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) | Image | 16.6 MB | TIF | 201010260006HQ_orig | https://stsci.box.com/s/19s43nv877zxbglxflxgkww09hyhru7y | https://images.nasa.gov/details-201010260006HQ | ||||
Artwork of Nancy Grace Roman and Vera C. Rubin. Developed for a social media campaign during Women's History Month by STScI and the Vera C. Rubin Observatory. | Illustration by J. Kang/STScI | Image | 597 KB | PNG | Roman_Rubin_tw |
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Artwork of Nancy Grace Roman and Vera C. Rubin. Sized for Facebook posts. Developed for a social media campaign during Women's History Month by STScI and the Vera C. Rubin Observatory. | Illustration by J. Kang/STScI | Image | 2.3 MB | PNG | Roman_Rubin_fb |
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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 | NASA Illustration: Kristin DiVona | Image | 3.4 MB | roman_poster | https://stsci.box.com/s/qif9riups3ye1w650tg0u854dz62hcg9 | https://chandra.si.edu/women/images/roman.pdf | |||||
Nancy with a model of an Orbiting Solar Observatory. | NASA | Image | 1.2 MB | PNG | nancy-model |
title | Planets by the Thousands |
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title | Solar System |
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title | Exoplanets |
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title | Stars by the Billions |
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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)
N/A
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Thumbnail | Working Name | Description | Credit | File Type | File Size | File Extension | Filename | File Location | Source Location | 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 Center | Image | 38.9 MB | PNG | Roman_Data_Scale_Final
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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. New version will be available soon. Credit: 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/9fgfz4uyjmpa1io3yzow2w9kn2icigxg | 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. Credit: Benjamin Williams, David Weinberg, Anil Seth, Eric Bell, Dave Sand, Dominic Benford, and the WINGS Science Investigation Team | Image | PNG | Greatfield_Simulated_Roman_Portrait_TextThis 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 | PNG |
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 | PNG |
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