{
    "id": 40456,
    "url": "http://svs.gsfc.nasa.gov/gallery/xrism/",
    "page_type": "Gallery",
    "title": "XRISM",
    "description": "XRISM (X-ray Imaging and Spectroscopy Mission) is a JAXA/NASA collaborative mission with ESA participation. It launched from Japan in September of 2023 and is investigating the X-ray sky using high-resolution spectroscopy and imaging.",
    "release_date": "2023-02-03T00:00:00-05:00",
    "update_date": "2026-09-21T00:00:00-04:00",
    "main_image": {
        "id": 368686,
        "url": "http://svs.gsfc.nasa.gov/vis/a020000/a020300/a020374/XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png",
        "filename": "XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png",
        "media_type": "Image",
        "alt_text": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab",
        "width": 180,
        "height": 320,
        "pixels": 57600
    },
    "media_groups": [
        {
            "id": 371572,
            "url": "http://svs.gsfc.nasa.gov/gallery/xrism/#media_group_371572",
            "widget": "Basic text (large)",
            "title": "Overview",
            "caption": "",
            "description": "XRISM (X-ray Imaging and Spectroscopy Mission) is a JAXA/NASA collaborative mission with ESA participation. It launched from Japan in September of 2023 and is investigating the X-ray sky using high-resolution spectroscopy and imaging.",
            "items": [],
            "extra_data": {}
        },
        {
            "id": 371956,
            "url": "http://svs.gsfc.nasa.gov/gallery/xrism/#media_group_371956",
            "widget": "Tile gallery",
            "title": "News Stories",
            "caption": "",
            "description": "",
            "items": [
                {
                    "id": 525082,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 15099,
                        "url": "http://svs.gsfc.nasa.gov/15099/",
                        "page_type": "Produced Video",
                        "title": "NASA-JAXA XRISM Mission Sees Pulsar Accreting Companion's 'Wind'",
                        "description": "This artist’s concept of the BP Crucis system follows the pulsar on a passage through the dense stream of plasma flowing from its companion, a blue hypergiant 40 times the Sun’s mass. During each four-day passage, the pulsar’s X-ray brightness flares as it pulls in some of the gas. At first, the gas forms a messy, turbulent accretion disk around the pulsar, and plasma spirals down to it. But as the pulsar moves deeper into the stream, there’s not enough angular momentum to support the disk, and it breaks up. At this point, plasma falls straight onto the pulsar. Later, as the pulsar nears the end of its passage, a messy accretion disk rebuilds, this time spinning in the opposite direction of the earlier disk. Credit: NASA’s Goddard Space Flight Center Conceptual Image LaboratoryAlt text: Animation of the BP Crucis system0:00 A wide view, showing the giant star, its gas stream, and the pulsar nearing it.  0:08 The camera zooms into the pulsar as it encounters the stream.  0:10 Gas flowing past the pulsar forms a clockwise-spinning accretion disk.  0:17 The disk breaks up. The gas now flows directly onto the pulsar.  0:35 As the pulsar nears the end of its passage through the stream, a new disk, spinning counterclockwise, forms.  0:51 The disk breaks up and the pulsar exits the stream.  0:52 Return to a wide view of the system. || Still2.jpg (3840x2160) [1.6 MB] || XRISM2.mp4 (1920x1080) [73.7 MB] || XRISM.en_US.srt [49 bytes] || XRISM.en_US.vtt [59 bytes] || XRISM_1.mp4 (3840x2160) [184.3 MB] || XRISM.mp4 (3840x2160) [725.6 MB] || XRISMNO_TexT.mov (3840x2160) [3.7 GB] || XRISMFinalText.mov (3840x2160) [3.9 GB] || ",
                        "release_date": "2026-09-18T14:00:00-04:00",
                        "update_date": "2026-09-18T15:38:49-04:00",
                        "main_image": {
                            "id": 1205627,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a015000/a015099/BP_Crucis_concept_wide_large_ac_print.jpg",
                            "filename": "BP_Crucis_concept_wide_large_ac_print.jpg",
                            "media_type": "Image",
                            "alt_text": "In this artist’s concept of the BP Crucis system, the city-sized pulsar GX301-2 approaches a thick stream of gas flowing away from its massive partner, the blue hypergiant Wray 977. The pulsar flares up in X-rays twice each orbit when it encounters the stream. Credit: NASA’s Goddard Space Flight Center Conceptual Image LaboratoryAlt text: Artist’s concept of BP CrucisImage description: Against a hazy, star-filled sky, a brilliant bluish-white star shines near the center of this artist’s concept. From the star, at about 4 o’clock, an expanding stream of bluish gas arcs toward lower left and then sweeps toward bottom center as it moves into the foreground. Another bright star-like point, much smaller, shines near the stream, just right of the image’s center. It emits two long, thin, wedge-shaped beams of radiation. One emerges at about 2 o’clock and heads to the upper right, the other, emerging at 7 o’clock, heads toward lower left. Text reads “Artist’s concept.”  ",
                            "width": 1024,
                            "height": 683,
                            "pixels": 699392
                        }
                    }
                },
                {
                    "id": 525083,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14968,
                        "url": "http://svs.gsfc.nasa.gov/14968/",
                        "page_type": "Produced Video",
                        "title": "XRISM Clocks Hot Wind of Galaxy M82",
                        "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ",
                        "release_date": "2026-03-25T12:00:00-04:00",
                        "update_date": "2026-03-25T12:01:25-04:00",
                        "main_image": {
                            "id": 1202714,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014900/a014968/v3_XRISM_Resolve_M82_searchweb.png",
                            "filename": "v3_XRISM_Resolve_M82_searchweb.png",
                            "media_type": "Image",
                            "alt_text": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.\r\rCredit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026\r\rAlt text: Spectrum and image of galaxy M82\r\rImage description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center.",
                            "width": 320,
                            "height": 180,
                            "pixels": 57600
                        }
                    }
                },
                {
                    "id": 502905,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14933,
                        "url": "http://svs.gsfc.nasa.gov/14933/",
                        "page_type": "Produced Video",
                        "title": "XRISM Finds Elemental Bounty in Supernova Remnant",
                        "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ",
                        "release_date": "2025-12-04T09:00:00-05:00",
                        "update_date": "2025-12-04T09:50:10-05:00",
                        "main_image": {
                            "id": 1159933,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014900/a014933/cas_a_with_resolve_1_print.jpg",
                            "filename": "cas_a_with_resolve_1_print.jpg",
                            "media_type": "Image",
                            "alt_text": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. \rCredit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. Arcand\rAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of view\rImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left.",
                            "width": 1024,
                            "height": 825,
                            "pixels": 844800
                        }
                    }
                },
                {
                    "id": 489690,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14868,
                        "url": "http://svs.gsfc.nasa.gov/14868/",
                        "page_type": "Produced Video",
                        "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail",
                        "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ",
                        "release_date": "2025-07-23T00:00:00-04:00",
                        "update_date": "2025-07-23T11:18:33-04:00",
                        "main_image": {
                            "id": 1157083,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014800/a014868/GX_340+0_DECaPS_print.jpg",
                            "filename": "GX_340+0_DECaPS_print.jpg",
                            "media_type": "Image",
                            "alt_text": "This composite shows a section of the interstellar medium scientists X-rayed for sulfur using the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission). X-ray binary GX 340+0 is the blue dot in the center. The composite contains a blend of imagery in X-rays (represented in deep blue), infrared, and light.Credit: DSS/DECaPS/eRosita/NASA’s Goddard Space Flight CenterAlt text: Optical, infrared, and X-ray composite image of a portion of the interstellar gas and dust with an X-ray source at the centerImage description: A bright blue dot is at the center of this star field. Yellow, red, blue, and white dots speckle the rest of the image, some buried in green-tinted swirls of dust.",
                            "width": 1024,
                            "height": 603,
                            "pixels": 617472
                        }
                    }
                },
                {
                    "id": 446862,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14707,
                        "url": "http://svs.gsfc.nasa.gov/14707/",
                        "page_type": "Produced Video",
                        "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3",
                        "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ",
                        "release_date": "2024-11-25T11:00:00-05:00",
                        "update_date": "2025-01-21T16:25:27-05:00",
                        "main_image": {
                            "id": 1103695,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014700/a014707/Cyg_X3_spectrum_sml.png",
                            "filename": "Cyg_X3_spectrum_sml.png",
                            "media_type": "Image",
                            "alt_text": "XRISM’s Resolve instrument has captured the most detailed X-ray spectrum yet acquired of Cygnus X-3. Peaks indicate X-rays emitted by ionized gases, and valleys form where the gases absorb X-rays; many lines are also shifted to both higher and lower energies by gas motions. Top: The full Resolve spectrum, from 2 to 8 keV (kiloelectron volts), tracks X-rays with thousands of times the energy of visible light. Some lines are labeled with the names of the elements that produced them, such as sulfur, argon, and calcium, along with Roman numerals that refer to the number of electrons these atoms have lost. Bottom: A zoom into a region of the spectrum often dominated by features produced by transitions in the innermost electron shell (K shell) of iron atoms. These features form when the atoms interact with high-energy X-rays or electrons and respond by emitting a photon at energies between 6.4 and 7 keV. These details, clearly visible for the first time with XRISM’s Resolve instrument, will help astronomers refine their understanding of this unusual system.Credit: JAXA/NASA/XRISM CollaborationAlt text: XRISM Resolve X-ray spectrum of Cygnus X-3 Image description: Two graphs appear on a dark blue background. The text at the top reads “XRISM Resolve Spectrum of Cygnus X-3.” The top graph, which takes up the upper third of the image, has a lighter blue background that darkens from top to bottom, an even brighter squiggly line that arcs across the graph, and yellow text such as “Sulfur XV” and Calcium XX.” X-ray brightness increases from bottom to top, and X-ray energy (measured in thousands of electron volts, or keV) increases from left to right. An orange box labeled “Area of detail” surrounds a series of peaks and valleys near the right end and identifies the region shown in the bottom graph. The lower chart is labeled “Iron K-alpha region” and shows prominent emission and absorption features produced by iron. ",
                            "width": 1028,
                            "height": 800,
                            "pixels": 822400
                        }
                    }
                },
                {
                    "id": 525084,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14584,
                        "url": "http://svs.gsfc.nasa.gov/14584/",
                        "page_type": "Produced Video",
                        "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy",
                        "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ",
                        "release_date": "2024-05-08T09:00:00-04:00",
                        "update_date": "2024-05-08T09:26:33-04:00",
                        "main_image": {
                            "id": 1091980,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014500/a014584/Blazar.00550_print.jpg",
                            "filename": "Blazar.00550_print.jpg",
                            "media_type": "Image",
                            "alt_text": "Same as the above, but without labels. \rCredit: NASA's Goddard Space Flight Center Conceptual Image Lab\r",
                            "width": 1024,
                            "height": 576,
                            "pixels": 589824
                        }
                    }
                },
                {
                    "id": 426117,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14463,
                        "url": "http://svs.gsfc.nasa.gov/14463/",
                        "page_type": "Produced Video",
                        "title": "XRISM Mission Captures Unmatched Data With Just 36 Pixels",
                        "description": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XRISM_36_Pixels_Still.jpg (1920x1080) [959.9 KB] || XRISM_36_Pixels_Still_searchweb.png (320x180) [94.7 KB] || XRISM_36_Pixels_Still_thm.png (80x40) [7.0 KB] || 14463_XRISM_36Pixels_Good.mp4 (1920x1080) [148.9 MB] || 14463_XRISM_36Pixels_Best.mp4 (1920x1080) [514.8 MB] || 14463_XRISM_36Pixels_Captions.en_US.srt [4.6 KB] || 14463_XRISM_36Pixels_Captions.en_US.vtt [4.4 KB] || 14463_XRISM_36Pixels_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || ",
                        "release_date": "2024-04-30T11:00:00-04:00",
                        "update_date": "2024-04-26T12:18:10.001194-04:00",
                        "main_image": {
                            "id": 1091669,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014400/a014463/XRISM_36_Pixels_Still.jpg",
                            "filename": "XRISM_36_Pixels_Still.jpg",
                            "media_type": "Image",
                            "alt_text": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.",
                            "width": 1920,
                            "height": 1080,
                            "pixels": 2073600
                        }
                    }
                },
                {
                    "id": 417833,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14492,
                        "url": "http://svs.gsfc.nasa.gov/14492/",
                        "page_type": "Produced Video",
                        "title": "XRISM Reveals Its First Look at X-ray Cosmos",
                        "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ",
                        "release_date": "2024-01-05T08:50:00-05:00",
                        "update_date": "2024-01-04T14:59:46.354457-05:00",
                        "main_image": {
                            "id": 1088374,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014400/a014492/Resolve_N132D_Spectrum_searchweb.png",
                            "filename": "Resolve_N132D_Spectrum_searchweb.png",
                            "media_type": "Image",
                            "alt_text": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.\r\rCredit: JAXA/NASA/XRISM Resolve and Xtend",
                            "width": 320,
                            "height": 180,
                            "pixels": 57600
                        }
                    }
                },
                {
                    "id": 412362,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14405,
                        "url": "http://svs.gsfc.nasa.gov/14405/",
                        "page_type": "Produced Video",
                        "title": "XRISM: Exploring the Hidden X-ray Cosmos",
                        "description": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim || YTframe_XRISM_Exploring_XrayCosmos.jpg (1280x720) [668.5 KB] || YTframe_XRISM_Exploring_XrayCosmos_searchweb.png (320x180) [100.3 KB] || YTframe_XRISM_Exploring_XrayCosmos_thm.png (80x40) [7.6 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.srt [7.8 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.vtt [7.4 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mov (3840x2160) [21.6 GB] || ",
                        "release_date": "2023-08-25T10:00:00-04:00",
                        "update_date": "2023-08-25T11:16:34-04:00",
                        "main_image": {
                            "id": 858110,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014400/a014405/YTframe_XRISM_Exploring_XrayCosmos.jpg",
                            "filename": "YTframe_XRISM_Exploring_XrayCosmos.jpg",
                            "media_type": "Image",
                            "alt_text": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim",
                            "width": 1280,
                            "height": 720,
                            "pixels": 921600
                        }
                    }
                },
                {
                    "id": 417834,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 12956,
                        "url": "http://svs.gsfc.nasa.gov/12956/",
                        "page_type": "Produced Video",
                        "title": "Spectroscopy, Explained",
                        "description": "Video producer Sophia Roberts explains the basic principles behind spectroscopy, the science of reading light to determine the size, distance, spin and chemical composition of distant objects in space. Complete transcript available.Music Credits:Universal Production MusicOxygenate the Idea – by Amon Turner, Banksman, Eben StoneJungle Bounce – by Siddharth NadkarniSilent Patient – by Paul Reeves Background Story - by Peter LarsenData Dynamism – by Florian Moenks and Aron Wright Watch this video on the NASA Goddard YouTube channel. || Spectroscopy,_Explained_Thumbnail.jpg (3840x2160) [2.2 MB] || Spectroscopy,_Explained_Thumbnail_searchweb.png (320x180) [75.1 KB] || Spectroscopy,_Explained_Thumbnail_thm.png (80x40) [6.3 KB] || Spectroscopy,_Explained_Final_1080.mp4 (1920x1080) [412.9 MB] || SpectroscopyExplainedAdjustedCaptions.en_US.srt [11.1 KB] || SpectroscopyExplainedAdjustedCaptions.en_US.vtt [10.5 KB] || Spectroscopy_Explained.webm (3840x2160) [125.6 MB] || Spectroscopy_Explained.mp4 (3840x2160) [1.1 GB] || Spectroscopy,_Explained_Final_Best_4k.mp4 (3840x2160) [2.5 GB] || Spectroscopy,_Explained_Final_ProRes.mov (3840x2160) [43.3 GB] || ",
                        "release_date": "2023-08-15T10:00:00-04:00",
                        "update_date": "2023-08-16T11:38:20-04:00",
                        "main_image": {
                            "id": 857731,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a012900/a012956/Spectroscopy,_Explained_Thumbnail_searchweb.png",
                            "filename": "Spectroscopy,_Explained_Thumbnail_searchweb.png",
                            "media_type": "Image",
                            "alt_text": "Video producer Sophia Roberts explains the basic principles behind spectroscopy, the science of reading light to determine the size, distance, spin and chemical composition of distant objects in space. Complete transcript available.Music Credits:Universal Production MusicOxygenate the Idea – by Amon Turner, Banksman, Eben Stone\rJungle Bounce – by Siddharth NadkarniSilent Patient – by Paul Reeves \rBackground Story - by Peter Larsen\rData Dynamism – by Florian Moenks and Aron Wright\r Watch this video on the NASA Goddard YouTube channel.",
                            "width": 320,
                            "height": 180,
                            "pixels": 57600
                        }
                    }
                },
                {
                    "id": 412363,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14374,
                        "url": "http://svs.gsfc.nasa.gov/14374/",
                        "page_type": "Infographic",
                        "title": "A Guide to Cosmic Temperatures",
                        "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ",
                        "release_date": "2023-08-03T11:00:00-04:00",
                        "update_date": "2024-09-06T11:20:05-04:00",
                        "main_image": {
                            "id": 856133,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014300/a014374/Temperature_Infographic_Crop.jpg",
                            "filename": "Temperature_Infographic_Crop.jpg",
                            "media_type": "Image",
                            "alt_text": "Cropped image for thumbnail",
                            "width": 1920,
                            "height": 1080,
                            "pixels": 2073600
                        }
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 371573,
            "url": "http://svs.gsfc.nasa.gov/gallery/xrism/#media_group_371573",
            "widget": "Card gallery",
            "title": "Stills/Graphics",
            "caption": "",
            "description": "",
            "items": [
                {
                    "id": 417835,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14492,
                        "url": "http://svs.gsfc.nasa.gov/14492/",
                        "page_type": "Produced Video",
                        "title": "XRISM Reveals Its First Look at X-ray Cosmos",
                        "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ",
                        "release_date": "2024-01-05T08:50:00-05:00",
                        "update_date": "2024-01-04T14:59:46.354457-05:00",
                        "main_image": {
                            "id": 1088374,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014400/a014492/Resolve_N132D_Spectrum_searchweb.png",
                            "filename": "Resolve_N132D_Spectrum_searchweb.png",
                            "media_type": "Image",
                            "alt_text": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.\r\rCredit: JAXA/NASA/XRISM Resolve and Xtend",
                            "width": 320,
                            "height": 180,
                            "pixels": 57600
                        }
                    }
                },
                {
                    "id": 412364,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14374,
                        "url": "http://svs.gsfc.nasa.gov/14374/",
                        "page_type": "Infographic",
                        "title": "A Guide to Cosmic Temperatures",
                        "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ",
                        "release_date": "2023-08-03T11:00:00-04:00",
                        "update_date": "2024-09-06T11:20:05-04:00",
                        "main_image": {
                            "id": 856133,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014300/a014374/Temperature_Infographic_Crop.jpg",
                            "filename": "Temperature_Infographic_Crop.jpg",
                            "media_type": "Image",
                            "alt_text": "Cropped image for thumbnail",
                            "width": 1920,
                            "height": 1080,
                            "pixels": 2073600
                        }
                    }
                },
                {
                    "id": 412365,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14389,
                        "url": "http://svs.gsfc.nasa.gov/14389/",
                        "page_type": "Produced Video",
                        "title": "XRISM Additional Images",
                        "description": "The XRISM spacecraft during acoustic testing at JAXA's Tsukuba Space Center in December 2022. These and other tests confirm that the spacecraft can withstand the severe vibrations and sounds of its rocket launch.Credit: JAXA || XRISM_Acoustic_12_23_22.jpg (2832x4240) [6.9 MB] || ",
                        "release_date": "2023-08-01T13:00:00-04:00",
                        "update_date": "2023-07-31T19:53:23.924915-04:00",
                        "main_image": {
                            "id": 857083,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014300/a014389/XRISM_logo_searchweb.png",
                            "filename": "XRISM_logo_searchweb.png",
                            "media_type": "Image",
                            "alt_text": "XRISM mission mark.Credit: JAXA",
                            "width": 320,
                            "height": 180,
                            "pixels": 57600
                        }
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 371574,
            "url": "http://svs.gsfc.nasa.gov/gallery/xrism/#media_group_371574",
            "widget": "Card gallery",
            "title": "Animations",
            "caption": "",
            "description": "",
            "items": [
                {
                    "id": 412366,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 20374,
                        "url": "http://svs.gsfc.nasa.gov/20374/",
                        "page_type": "Animation",
                        "title": "XRISM Beauty Shots",
                        "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ",
                        "release_date": "2022-12-12T00:00:00-05:00",
                        "update_date": "2023-05-03T11:43:49.072206-04:00",
                        "main_image": {
                            "id": 368685,
                            "url": "http://svs.gsfc.nasa.gov/vis/a020000/a020300/a020374/XRISM_360_4k_30fps_4444ProRes.00001_print.jpg",
                            "filename": "XRISM_360_4k_30fps_4444ProRes.00001_print.jpg",
                            "media_type": "Image",
                            "alt_text": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab",
                            "width": 1024,
                            "height": 576,
                            "pixels": 589824
                        }
                    }
                },
                {
                    "id": 412367,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 14244,
                        "url": "http://svs.gsfc.nasa.gov/14244/",
                        "page_type": "Produced Video",
                        "title": "XRISM Resolve Animation",
                        "description": "This animation illustrates how the microcalorimeter array at the heart of XRISM's revolutionary Resolve soft X-ray spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to 50 millikelvins, just above absolute zero, detects this minute temperature change.Credit: NASA's Goddard Space Flight Center || XRISM_Calorimeter-STILL_print.jpg (1024x576) [64.0 KB] || XRISM_Calorimeter-STILL.jpg (3840x2160) [716.3 KB] || XRISM_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL_thm.png (80x40) [5.5 KB] || XRISM_Calorimeter-STILL_web.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || ",
                        "release_date": "2022-11-25T00:00:00-05:00",
                        "update_date": "2023-08-15T13:37:20-04:00",
                        "main_image": {
                            "id": 368140,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a014200/a014244/XRISM_Calorimeter-STILL_print.jpg",
                            "filename": "XRISM_Calorimeter-STILL_print.jpg",
                            "media_type": "Image",
                            "alt_text": "This animation illustrates how the microcalorimeter array at the heart of XRISM's revolutionary Resolve soft X-ray spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to 50 millikelvins, just above absolute zero, detects this minute temperature change.Credit: NASA's Goddard Space Flight Center",
                            "width": 1024,
                            "height": 576,
                            "pixels": 589824
                        }
                    }
                },
                {
                    "id": 525085,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 20417,
                        "url": "http://svs.gsfc.nasa.gov/20417/",
                        "page_type": "Animation",
                        "title": "Wind-Accreting Pulsar Visualization",
                        "description": "Visualization of the BP Crucis system showing the pulsar near closest approach to its companion, a blue hypergiant 40 times the Sun’s mass. Twice each orbit, the pulsar passes throuh a dense stream of plasma flowing from the companion, flaring up in X-rays as it does. In this sequence, the pulsar approaches, enters, and exits the stream. || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_print.jpg (1024x576) [84.0 KB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_searchweb.png (320x180) [62.1 KB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_thm.png (80x40) [5.0 KB] || XRISM_IM_SHOT_01_alt_30fps_1080p_proRes.mov (1920x1080) [352.2 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.mp4 (3840x2160) [26.2 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_proRes.webm (3840x2160) [5.9 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_proRes.mov (3840x2160) [1.3 GB] || ",
                        "release_date": "2026-09-18T14:00:00-04:00",
                        "update_date": "2026-10-05T11:21:01-04:00",
                        "main_image": {
                            "id": 1205653,
                            "url": "http://svs.gsfc.nasa.gov/vis/a020000/a020400/a020417/XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_print.jpg",
                            "filename": "XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_print.jpg",
                            "media_type": "Image",
                            "alt_text": "Visualization of the BP Crucis system showing the pulsar near closest approach to its companion, a blue hypergiant 40 times the Sun’s mass. Twice each orbit, the pulsar passes throuh a dense stream of plasma flowing from the companion, flaring up in X-rays as it does. In this sequence, the pulsar approaches, enters, and exits the stream.",
                            "width": 1024,
                            "height": 576,
                            "pixels": 589824
                        }
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 371575,
            "url": "http://svs.gsfc.nasa.gov/gallery/xrism/#media_group_371575",
            "widget": "Card gallery",
            "title": "Hardware Raw Footage/B-roll",
            "caption": "",
            "description": "",
            "items": [
                {
                    "id": 412368,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 13531,
                        "url": "http://svs.gsfc.nasa.gov/13531/",
                        "page_type": "Produced Video",
                        "title": "XRISM: Calorimeter Spectrometer Insert and Mirror Tests",
                        "description": "XRISM team members pose with the XRISM Calorimeter Spectrometer Insert in a NASA Goddard clean room. From left to right, they are Bryan James, Mike Sampson, Tomomi Watanabe, Pete Barfknecht, Scott Porter, and Sinclair Douglas.Credit: Larry Gilbert/NASA || GSFC_20191101__2020-2568_07.jpg (3000x1995) [3.6 MB] || GSFC_20191101__2020-2568_07_searchweb.png (320x180) [111.9 KB] || GSFC_20191101__2020-2568_07_thm.png (80x40) [7.7 KB] || ",
                        "release_date": "2020-01-31T00:00:00-05:00",
                        "update_date": "2023-05-03T13:45:14.185124-04:00",
                        "main_image": {
                            "id": 387810,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a013500/a013531/GSFC_20191101__2020-2568_07.jpg",
                            "filename": "GSFC_20191101__2020-2568_07.jpg",
                            "media_type": "Image",
                            "alt_text": "XRISM team members pose with the XRISM Calorimeter Spectrometer Insert in a NASA Goddard clean room. From left to right, they are Bryan James, Mike Sampson, Tomomi Watanabe, Pete Barfknecht, Scott Porter, and Sinclair Douglas.Credit: Larry Gilbert/NASA",
                            "width": 3000,
                            "height": 1995,
                            "pixels": 5985000
                        }
                    }
                },
                {
                    "id": 412369,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 13530,
                        "url": "http://svs.gsfc.nasa.gov/13530/",
                        "page_type": "Produced Video",
                        "title": "Mirror Quadrants for XRISM",
                        "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ",
                        "release_date": "2020-01-30T00:00:00-05:00",
                        "update_date": "2023-05-03T13:45:14.505303-04:00",
                        "main_image": {
                            "id": 387798,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a013500/a013530/GSFC_20190619_XRISM_XMA_11.jpg",
                            "filename": "GSFC_20190619_XRISM_XMA_11.jpg",
                            "media_type": "Image",
                            "alt_text": "Credit: Taylor Mickal/NASA",
                            "width": 3414,
                            "height": 2000,
                            "pixels": 6828000
                        }
                    }
                },
                {
                    "id": 412370,
                    "type": "details_page",
                    "extra_data": null,
                    "instance": {
                        "id": 13280,
                        "url": "http://svs.gsfc.nasa.gov/13280/",
                        "page_type": "Produced Video",
                        "title": "Assembling XRISM's X-ray Mirrors",
                        "description": "Team members Lawrence Lozipone of Stinger Ghaffarian Technologies, Inc. and Yang Soong, a researcher at the University of Maryland, College Park, work with flight mirrors for the X-ray Imaging and Spectroscopy Mission (XRISM). Nested aluminum mirror segments – 1,624 of them for each X-ray Mirror Assembly – focus the incoming X-rays for the satellite's science instruments. Credit: NASA's Goddard Space Flight Center || XRISM_Cleanroom_B-roll_1080Still.jpg (1920x1080) [727.5 KB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.mov (1920x1080) [7.0 GB] || XRISM_Cleanroom_B-roll_1080.mp4 (1920x1080) [991.6 MB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.webm (1920x1080) [52.0 MB] || ",
                        "release_date": "2020-08-19T00:00:00-04:00",
                        "update_date": "2023-05-03T13:44:44.935607-04:00",
                        "main_image": {
                            "id": 393903,
                            "url": "http://svs.gsfc.nasa.gov/vis/a010000/a013200/a013280/XRISM_Cleanroom_B-roll_4k_Still_print.jpg",
                            "filename": "XRISM_Cleanroom_B-roll_4k_Still_print.jpg",
                            "media_type": "Image",
                            "alt_text": "Shorter version of the above video.Credit: NASA's Goddard Space Flight Center",
                            "width": 1024,
                            "height": 576,
                            "pixels": 589824
                        }
                    }
                }
            ],
            "extra_data": {}
        }
    ]
}