XRISM

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] ||

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.mov (3840x2160) [21.6 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || 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] ||

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] || Spectroscopy,_Explained_Final_ProRes.mov (3840x2160) [43.3 GB] || Spectroscopy,_Explained_Final_Best_4k.mp4 (3840x2160) [2.5 GB] || Spectroscopy_Explained.mp4 (3840x2160) [1.1 GB] || Spectroscopy_Explained.webm (3840x2160) [125.6 MB] || SpectroscopyExplainedAdjustedCaptions.en_US.srt [11.1 KB] || SpectroscopyExplainedAdjustedCaptions.en_US.vtt [10.5 KB] ||

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] ||

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] ||

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] ||

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] ||

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 (320x180) [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_4444ProRes.mov (3840x2160) [1.7 GB] || frames/3840x2160_16x9_30p/XRISM_360_4k_30fps/ (3840x2160) [32.0 KB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || frames/3840x2160_16x9_60p/XRISM_360_4k_60fps/ (3840x2160) [128.0 KB] || 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.webm (0x0) [0 bytes] ||

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] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || 3840x2160_16x9_60p (3840x2160) [64.0 KB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] ||

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] ||

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] ||

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] ||