XRISM (X-ray Imaging and Spectroscopy Mission)

Welcome & Introductions - Judy Black 00:00 Photo Montage - David Hoskin 3:12 Dr. Luigi Gallo - JAXA's XRISM X-Ray Observatory 13:28 Food for the Soul - Paul Heath 1:01:47 News from the Board - Tony McGrath 1:04:57 What's Up in Oct? - David Hoskin 1:10:33 sorry about the audio quality, we'll try and improve that.

At a time when phone cameras are capable of taking snapshots with millions of pixels, an instrument on the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) captures revolutionary science with just 36 of them. That may sound impossible, but it’s true. XRISM (pronounced “crism”) is led by JAXA (Japan Aerospace Exploration Agency) in collaboration with NASA, along with contributions from ESA (European Space Agency). It launched into orbit last September and has been scrutinizing the cosmos ever since. The mission detects “soft” X-rays, which have energies up to 5,000 times greater than visible light. It will probe the universe’s hottest regions, largest structures, and objects with the strongest gravity, like supermassive black holes in the cores of distant galaxies. XRISM accomplishes this with an instrument named Resolve. Resolve's detector takes the temperature of each X-ray that strikes it. Astronomers call Resolve a microcalorimeter spectrometer because each of its 36 pixels measures the tiny amount of heat delivered by each incoming X-ray. This lets astronomers see the chemical fingerprints of elements making up the sources in unprecedented detail. In order to accomplish this, the entire detector must be chilled to 459.58 degrees below zero Fahrenheit (minus 273.1 degrees Celsius), just a whisker above absolute zero. The instrument is so precise it can detect the motions of elements within a target, effectively providing a 3D view. Gas moving toward us glows at slightly higher energies than normal, while gas moving away from us emits slightly lower energies. This will, for example, allow scientists to better understand the flow of hot gas within clusters of galaxies and to track the movement of different elements in the debris of supernova explosions. Resolve is taking astronomers into a new era of cosmic exploration — and with only three-dozen pixels. Music credit: "Wading Through" and “Stop and Hide” from Universal Production Music Credit: NASA’s Goddard Space Flight Center Producer: Scott Wiessinger (KBR Wyle Services, LLC) Science writer: Francis Reddy (University of Maryland College Park) Animator:Adriana Manrique Gutierrez (KBR Wyle Services, LLC) Animator: Scott Wiessinger (KBR Wyle Services, LLC) Writer: Scott Wiessinger (KBR Wyle Services, LLC) Narrator: Sophia Roberts (Advocates in Manpower Management, Inc.) This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14463. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14463. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

Hi Spacecats, I'm Dr Maggie Lieu and welcome to my channel, where you can find all things space, astronomy and physics! In this week's video, we look at the XRISM's first release image and data. This video offers an in-depth look at the first images from JAXA's X-ray telescope, describing the galaxy cluster Abell2319 and the X-ray spectra captured of the bright supernova remnant N132D. We look at the instruments XTEND and RESOLVE that captured them and discuss the big issue XRISM is currently facing, that may make us believe there is a curse in X-ray astronomy after the previous loss of Hitomi and plagues of problems with previous telescopes like Suzaku. Links: https://www.isas.jaxa.jp/en/missions/spacecraft/current/slim.html https://global.jaxa.jp/activity/pr/jaxas/no088/03.html Media credits: XRISM results: JAXA XRISM craft: NASA GSFC Galaxy cluster: ESA/DOLAG Variable star: NASA/ESA/Kornmesser XTEND: JAXA Resolve: NASA GSFC N132D: NASA/STScI/CXC/SAO, processing by Judy Schmidt, CC BY-NC-SA Supernova remnant N132D: JAXA/NASA/XRISM Xtend; background, C. Smith, S. Points, the MCELS Team and NOIRLab/NSF/AURA Resolve detector: NASA/XRISM/Caroline Kilbourne XRISM combined: X-ray (JAXA), Optical (DSS*) *The Digitized Sky Survey Gatevalve: Esoe et al. 2020. https://www.sciencedirect.com/science/article/abs/pii/S0011227519302358?via%3Dihub GV: Sumitomo heavy industries Special thanks to my YouTube Members: Annex Celestial, Wheely Big Bike Trip, Steven Yee, Thomas Seiler, Anders Welander, Bill Fratt, David Brant, John Lewis, Kristóf Lovas & SpaceCatLuna. You can also sign up on my channel page! Support me through my shop: www.maggielieu.com/shop If you enjoyed the video, please consider by liking, sharing and subscribing! I'm also on: twitter: https://twitter.com/space_mog instagram: https://instagram.com/space_mog/ facebook: https://facebook.com/spacemog/

↓↓↓ Links and more in full description below ↓↓↓ Japan's brand new x-ray telescope, XRISM, has just releasd it's first ever images. They show a galaxy cluster called Abell 2319 and a supernova remnant called N132D. In this video we'll have a look at these images, how good they are and what they're showing, as well as looking at XRISM's mission in general. We also touch on how x-ray telescopes work and the risk we have of having no x-ray telescope in space at all. Enjoy, and leave me any questions or comments down below! You can buy me a coffee if you enjoyed this and want to support these videos. You don't have to though, no pressure. https://www.buymeacoffee.com/chrispattison How X Ray Telescopes work video: https://youtu.be/VDOm1IudAOo?si=Xx_4G1Ows2u04n3u How Gamma Ray Telescopes work: https://youtu.be/-1gRR9J8FZo LINKS and SOURCES: Xrism Specs and Tech: https://www.xrism.jaxa.jp/en/technology/ https://xrism.isas.jaxa.jp/en/technology/detail_02/ Xrism Factsheet: https://www.esa.int/Science_Exploration/Space_Science/XRISM_factsheet ESA Press Release (First Images): https://www.esa.int/Science_Exploration/Space_Science/XRISM_s_first_views_signal_shake-up_for_X-ray_astronomy#Anchor2 JAXA Press Release: https://global.jaxa.jp/press/2024/01/20240105-1_e.html Abell 2319 Image: https://www.esa.int/ESA_Multimedia/Images/2024/01/Galaxy_cluster_Abell_2319 Supernova Remnant N132D Image: https://www.esa.int/Science_Exploration/Space_Science/XRISM_s_first_views_signal_shake-up_for_X-ray_astronomy Supernova remnant 30 Doradus B Chandra Image: https://www.nasa.gov/image-article/nasa-telescopes-start-the-year-with-a-double-bang Chapters: 00:00 - Intro 00:27 - What is Xrism? 02:10 - The AMAZING way X-ray Telescopes Work 03:11 - NEW IMAGE 1 (Supernova Remnant N132D) 05:43 - NEW IMAGE 2 (Galaxy Cluster Abell 2319) 07:31 - Future Plans for XRISM 08:02 - Outro Hey team! If there is some other cool topic in physics you think we should learn about together, leave a comment down below! Until next time, stay safe. Please consider subscribing if you enjoyed the video, and you can also find me on Twitter and Instagram: https://twitter.com/chrisdpattison https://www.instagram.com/chrispattison22/

日本語 ⇒ https://youtube.com/live/voYZcThSWFE The live coverage of the launch of XRISM/SLIM. Broadcast schedule: 8:55 a.m. on August 28, 2023 (JST) Launch time: 9:26:22 a.m. (JST)

Hi Spacecats, I'm Dr Maggie Lieu and welcome to my channel, where you can find all things space, astronomy and physics! Today (with any luck) Japanese space agency JAXA will begin to face some of it's biggest challenges yet, another attempt at getting an X-ray space telescope in space and the launching the highest precision lunar lander ever. So let's talk about it! Links: Media credits: Chandrayaan 3 landing: ISRO Athena: SRON XRISM instruments: JAXA/NASA XRISM calorimeter: NASA/GSFC XRISM: NASA/GSFC Galaxy cluster: DOLAG Black hole: ESO/Kornmesser SLIM (various clips and images): JAXA Special thanks to my youtube perks members: Annex Celestial, Wheely Big Bike Trip, Steven Yee, Thomas Seiler, Anders Welander, Bill Fratt and Kristóf Lovas. You can also sign up on my channel page! Support me through my shop: www.maggielieu.com/shop If you enjoyed the video, please consider by liking, sharing and subscribing! I'm also on: twitter: https://twitter.com/space_mog instagram: https://instagram.com/space_mog/ facebook: https://facebook.com/spacemog/ onegarden: onegarden.com/?rfc=7wL

Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA. Music Credits: Universal Production Music Lights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan Jones Changing Tide by Rob Manning Wandering Imagination by Joel Goodman In Unison by Samuel Sim Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio Sophia Roberts (AIMM): Lead Producer Jeanette Kazmierczak (University of Maryland College Park): Lead Writer Adriana Manrique Gutierrez (KBRwyle): Lead Animator Scott Wiessinger (KBRwyle): Animator Rob Andreoli (AIMM): Videographer Harrison Bach (Intern): Videographer John D. Philyaw (AIMM: Videographer Aaron E. Lepsch (ADNET): Technical Support Francois Mernier (University of Maryland College Park): Research Astrophysicist Takashi Okajima (GSFC): Research Astrophysicist This video is public domain and along with other supporting visualizations can be downloaded from NASA Goddard's Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/14405 If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram: http://www.instagram.com/nasagoddard · X: http://twitter.com/NASAGoddard · Facebook: http://www.facebook.com/NASAGoddard · Flickr: http://www.flickr.com/photos/gsfc

The mission, abbreviated XRISM (pronounced “crism”), is a collaboration between the Japan Aerospace Exploration Agency (JAXA) and NASA, along with ESA (the European Space Agency) participation, to investigate the X-ray universe using high-resolution imaging and spectroscopy. XRISM features two instruments: Resolve, an X-ray calorimeter spectrometer, and Xtend, an X-ray imager. Cooled to a fraction of a degree above absolute zero, Resolve’s detector can measure the slight amount of heat generated when each pixel absorbs a single X-ray photon. Xtend will image a field of view about 60% larger than the apparent size of a full moon, giving it XRISM the widest view of any X-ray imaging satellite flown to date. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, developed the X-ray Mirror Assemblies used for both instruments, as well as the Resolve detector and many of its subsystems. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

The mission, abbreviated XRISM (pronounced “crism”), is a collaboration between the Japan Aerospace Exploration Agency (JAXA) and NASA, along with ESA (the European Space Agency) participation, to investigate the X-ray universe using high-resolution imaging and spectroscopy. XRISM features two instruments: Resolve, an X-ray calorimeter spectrometer, and Xtend, an X-ray imager. Cooled to a fraction of a degree above absolute zero, Resolve’s detector can measure the slight amount of heat generated when each pixel absorbs a single X-ray photon. Xtend will image a field of view about 60% larger than the apparent size of a full moon, giving it XRISM the widest view of any X-ray imaging satellite flown to date. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, developed the X-ray Mirror Assemblies used for both instruments, as well as the Resolve detector and many of its subsystems. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

The mission, abbreviated XRISM (pronounced “crism”), is a collaboration between the Japan Aerospace Exploration Agency (JAXA) and NASA, along with ESA (the European Space Agency) participation, to investigate the X-ray universe using high-resolution imaging and spectroscopy. XRISM features two instruments: Resolve, an X-ray calorimeter spectrometer, and Xtend, an X-ray imager. Cooled to a fraction of a degree above absolute zero, Resolve’s detector can measure the slight amount of heat generated when each pixel absorbs a single X-ray photon. Xtend will image a field of view about 60% larger than the apparent size of a full moon, giving it XRISM the widest view of any X-ray imaging satellite flown to date. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, developed the X-ray Mirror Assemblies used for both instruments, as well as the Resolve detector and many of its subsystems. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

The mission, abbreviated XRISM (pronounced “crism”), is a collaboration between the Japan Aerospace Exploration Agency (JAXA) and NASA, along with ESA (the European Space Agency) participation, to investigate the X-ray universe using high-resolution imaging and spectroscopy. XRISM features two instruments: Resolve, an X-ray calorimeter spectrometer, and Xtend, an X-ray imager. Cooled to a fraction of a degree above absolute zero, Resolve’s detector can measure the slight amount of heat generated when each pixel absorbs a single X-ray photon. Xtend will image a field of view about 60% larger than the apparent size of a full moon, giving it XRISM the widest view of any X-ray imaging satellite flown to date. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, developed the X-ray Mirror Assemblies used for both instruments, as well as the Resolve detector and many of its subsystems. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

開催日時：2023 年7 月21 日（金） 10 時30 分～11 時30 分 開催場所：JAXA 種子島宇宙センター竹崎展望台4 階記者会見室 および オンライン（Webex） 説明者： JAXA 宇宙科学研究所 X 線分光撮像衛星（XRISM）プロジェクトチーム プロジェクトマネージャ 前島 弘則（まえじま ひろのり） プリンシパルインベスティゲータ（研究主宰者） 田代 信（たしろ まこと） 配布資料： https://www.jaxa.jp/projects/files/youtube/xrism/xrism_doc_20230721.pdf ＊記者説明会内で流したインタビュー映像について ・XRISM Project Scientist (NASA)のBrian Williams（ブライアン・ウィリアムズ）氏によるインタビュー映像 クレジット ：NASA/JAXA ・XRISM Project Scientist (ESA)のMatteo Guainazzi（マッテオ・グアイナッツイ）氏によるインタビュー映像 クレジット ：ESA/JAXA 関連URL: XRISM/SLIM特設サイト　https://fanfun.jaxa.jp/countdown/xrism-slim/ XRISMプロジェクトサイト　https://xrism.isas.jaxa.jp/ ISAS　https://www.isas.jaxa.jp/ ▼JAXA公式チャンネルはこちら 〇JAXA Channel https://www.youtube.com/user/jaxachannel 〇JAXAイベントライブ配信専用チャンネル https://www.youtube.com/@JAXA-LiveEvent ▼関連再生リスト https://www.youtube.com/playlist?list=PLCQJJ3lTBuyB2XkiNRONJ3A_ecI1G4k4o https://www.youtube.com/playlist?list=PLCQJJ3lTBuyBfoORJP_wE7cCcdr4EVCRw ▼JAXA（国立研究開発法人宇宙航空研究開発機構/Japan Aerospace Exploration Agency） https://www.jaxa.jp/ https://global.jaxa.jp/ #jaxa #宇宙 #航空 #ISAS #宇宙探査 #XRISM

Video abstract for the paper "Limits from the grave: resurrecting Hitomi for decaying dark matter and forecasting leading sensitivity for XRISM" by Christopher Dessert, Orion Ning, Nicholas Rodd, and Benjamin Safdi.

Date: Mar 3, 2021 Presenters: Edmund Hodges-Kluck (Goddard) Description: This is a tutorial describing the XRISM x-ray space telescope instrument. Slides: https://drive.google.com/file/d/1bYoRuVDpSINUkedGz0vLO0osrKl5wO51/view?usp=sharing

This animation illustrates how the microcalorimeter array at the heart of XRISM’s Resolve instrument 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 near absolute zero, detects this minute temperature change. Credit: NASA's Goddard Space Flight Center This video is public domain and may be downloaded from NASA Goddard's Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/12160

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

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