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Thumbnail | Working Name | Description | Credit | File Type | File Size | File Extension | Filename | File Location | Source Location | Learn more about the Roman Space Telescope spacecraft with this short tour of the main systems. | Video | 807.1 MB | MP4 | 13295_Roman_360_Best_10809m81dvpe9zpfjc41zeml5hnq0o0kdh14
ewta914jgirwifgx4g4v7geynckws1rs | https://hackaday.com/2018/04/03/nancy-grace-roman-mother-of-the-hubble/ | ||||||
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Music: "Flight Impressions" from Universal Production Music
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Thumbnail | Working Name | Description | Credit | File Type | File Size | File Extension | Filename | File Location | Source 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 Image | 8.3 MB | PNG | Abell246_Zoom_3840x2160N/A Related Press Release -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 Image | 8.3 MB | PNG | Abell246_Zoom_RomanHubbleLabeled_3840x2160N/A Related Press Release -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 Video | 22.9 MB | MP4 | STScI-H-v2041b-3840x2160This 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 Video | 23.8 MB | MP4 | STScI-H-v2041d-3840x2160This image showcases one panel of an exhibit on UGC 2885 (Rubin's Galaxy), highlighting the unique strengths of Hubble, Webb, and Roman in observing galaxies. | Hubble's View of Rubin's Galaxy: NASA, ESA, and B. Holwerda (University of Louisville) Exhibit composition: STScI
Image | 2.9 MB | JPG | UGC2885_2019-exhibit-FINALN/A Hubble's Rubin Galaxy press release -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. Image being updated by STScI, will be available shortly! Hubble's View of Rubin's Galaxy: NASA, ESA, and B. Holwerda (University of Louisville) Image composition: STScI
Image | 29.9 MB | PNG | UGC2885_2020-article-FINALN/A Hubble's Rubin Galaxy press release - Expand |
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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 | https:
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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
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 |
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 |
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_NoText |
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