X-Ray Imaging and Spectroscopy Mission

Last updated

X-Ray Imaging and Spectroscopy Mission (X線分光撮像衛星)
XRISM in a nutshell (cropped).png
Diagram of the XRISM observatory
NamesXRISM
ASTRO-H Successor
ASTRO-H2
XARM
Mission type X-ray astronomy
Operator JAXA
COSPAR ID 2023-137A OOjs UI icon edit-ltr-progressive.svg
SATCAT no. 57800
Website xrism.isas.jaxa.jp/en
www.nasa.gov/content/goddard/xrism-x-ray-imaging-and-spectroscopy-mission
Mission durationPlanned:
3 years
Elapsed:
11 months, 17 days
Spacecraft properties
Spacecraft typeASTRO
Bus ASTRO-H
Launch mass2,300 kg (5,100 lb)
Start of mission
Launch date6 September 2023, 23:42:11 UTC [1]
Rocket H-IIA 202
Launch site Tanegashima, LA-Y1
Contractor Mitsubishi Heavy Industries
Orbital parameters
Reference system Geocentric orbit
Regime Low Earth orbit
Perigee altitude 550 km
Apogee altitude 550 km
Inclination 31.0°
Period 96.0 minutes
Main telescope
NameSoft X-ray Telescope
Diameter45 cm (18 in) [2]
Focal length5.6 m (18 ft)
←  Hitomi (ASTRO-H)
XRISM XRISM Additional Images (SVS14389 - xrism in bay may 2022).jpeg
XRISM

The X-Ray Imaging and Spectroscopy Mission (XRISM, pronounced "crism"), formerly the X-ray Astronomy Recovery Mission (XARM), is an X-ray space telescope mission of the Japan Aerospace Exploration Agency (JAXA) in partnership with NASA to provide breakthroughs in the study of structure formation of the universe, outflows from galaxy nuclei, and dark matter. [3] [4] As the only international X-ray observatory project of its period, XRISM will function as a next generation space telescope in the X-ray astronomy field, similar to how the James Webb Space Telescope, Fermi Space Telescope, and the Atacama Large Millimeter Array (ALMA) Observatory are placed in their respective fields. [2] [5]

Contents

The mission is a stopgap for avoiding a potential period of observation loss between the current X-ray telescopes (Chandra and XMM-Newton), and those of the future (Advanced Telescope for High Energy Astrophysics (ATHENA)). Without XRISM, there could be a time period during with no X-ray data was collected. This would arise in the early 2020s as these two reach the end of their missions, due to the loss, in 2016, of the Hitomi X-ray telescope, which was launched to be the follow-on to the Chandra and Newton telescopes. [2] [5]

During its early design phase, XRISM was also known as the "ASTRO-H Successor" or "ASTRO-H2". After the loss of Hitomi, the name XARM was used, the R in the acronym refers to recovering the ability to do X-ray spectroscopy and its benefits. The name changed to XRISM in 2018 when JAXA formally initiated the project team. [6]

Overview

XRISM spacecraft XRISM 001.png
XRISM spacecraft

With the retirement of Suzaku in September 2015, and the detectors onboard Chandra X-ray Observatory and XMM-Newton operating for more than 15 years and gradually aging, the failure of Hitomi meant that X-ray astronomers would have a 13-year blank period in soft X-ray observation, until the launch of ATHENA in 2035. [Note 1] [2] [5] [7] This would result in a major setback for the international community, [8] as studies performed by large scale observatories in other wavelengths, such as the James Webb Space Telescope and the Thirty Meter Telescope will commence in the early 2020s, while there would be no telescope to cover the most important part of X-ray astronomy. [2] [5] A lack of new missions could also deprive young astronomers a chance to gain hands-on experience from participating in a project. [2] [5] Along with these reasons, motivation to recover science that was expected as results from Hitomi, became the rationale to initiate the XRISM project. XRISM has been recommended by ISAS's Advisory Council for Research and Management, the High Energy AstroPhysics Association in Japan, NASA Astrophysics Subcommittee, NASA Science Committee, NASA Advisory Council. [5] [9]

With its successful launch in September 2023, [1] XRISM is expected to cover the science that was lost with Hitomi, such as the structure formation of the universe, feedback from galaxies/active galaxy nuclei, and the history of material circulation from stars to galaxy clusters. [4] The space telescope will also take over Hitomi's role as a technology demonstrator for the European Advanced Telescope for High Energy Astrophysics (ATHENA) telescope. [7] [10] [11] Multiple space agencies, including NASA and the European Space Agency (ESA) are participating in the mission. [12] In Japan, the project is led by JAXA's Institute of Space and Astronautical Science (ISAS) division, and U.S. participation is led by NASA's Goddard Space Flight Center (GSFC). The U.S. contribution is expected to cost around US$80 million, which is about the same amount as the contribution to Hitomi. [13] [14]

Changes from Hitomi

203 foils assembled in the X-ray Mirror Assembly XMA XRISM s X-ray mirror assembly.jpg
203 foils assembled in the X-ray Mirror Assembly XMA

The X-ray Imaging and Spectroscopy Mission will be one of the first projects for ISAS to have a separate project manager (PM) and primary investigator (PI). This measure was taken as part of ISAS's reform in project management to prevent the recurrence of the Hitomi accident. [5] In traditional ISAS missions, the PM was also responsible for tasks that would typically be allocated to PIs in a NASA mission.

While Hitomi had an array of instruments spanning from soft X-ray to soft gamma ray, XRISM will focus around the Resolve instrument (equivalent to Hitomi's soft X-ray spectrometer), [15] as well as Xtend (SXI), which has a high affinity to Resolve. [16] The elimination of a hard X-ray telescope was justified by the 2012 launch of NASA's NuSTAR satellite, something that did not exist when Hitomi (then known as the New X-Ray Telescope, NeXT) was initially formulated. [17] [Note 2] NuSTAR's spatial and energy resolution is analogous to Hitomi's hard X-ray instruments. [17] Once XRISM's operation starts, collaborative observations with NuSTAR will likely be essential. [4] Meanwhile, the scientific value of the soft and hard X-ray band width boundary has been noted; therefore the option of upgrading XRISM's instruments to be partially capable of hard X-ray observation is under consideration. [16] [17] [ needs update ]

A hard X-ray telescope proposal with abilities surpassing Hitomi was proposed in 2017. [18] The FORCE (Focusing On Relativistic universe and Cosmic Evolution) space telescope is a candidate for the next ISAS competitive medium class mission. If selected, FORCE would be launched after the mid-2020s, with an eye towards conducting simultaneous observations with ATHENA. [18] [4]

History

Following the premature termination of the Hitomi mission, on 14 June 2016 JAXA announced their proposal to rebuild the satellite. [19] The XARM pre-project preparation team was formed in October 2016. [20] In the U.S. side, formulation began in the summer of 2017. [3] In June 2017, ESA announced that they would participate in XARM as a mission of opportunity. [12]

Instruments

An illustration of the range of cosmic temperatures including the temperature at which XRISM will work to ensure the optimal functioning of its instruments A Guide to Cosmic Temperatures (SVS14374 - Cosmic Temperatures Infographic Final Full).jpg
An illustration of the range of cosmic temperatures including the temperature at which XRISM will work to ensure the optimal functioning of its instruments

XRISM carries two instruments for studying the soft X-ray energy range, Resolve and Xtend. The satellite has telescopes for each of the instruments, SXT-I (Soft X-ray Telescope for Imager) and SXT-S (Soft X-ray Telescope for Spectrometer). [5] The pair of telescopes have a focal length of 5.6 m (18 ft). [2]

Resolve

Resolve is an X-ray micro calorimeter developed by NASA and the Goddard Space Flight Center. [22] The instrument is a duplicate version of its Hitomi predecessor. It used some space-qualified hardware left from the manufacture of Hitomi's SXS. [23]

Xtend

Xtend is an X-ray CCD camera. Xtend improves on the energy resolution of Hitomi's SXI. [24]

Launch

JAXA launched XRISM on 6 September 2023 at 23:42 UTC (7 September 08:42 Japan Standard Time) using an H-IIA rocket from Tanegashima Space Center. XRISM was successfully inserted into orbit on the same day, and the accompanying launch payload, SLIM, began its multi-month journey to the Moon. [1]

A protective shutter over the Resolve instrument's detector has failed to open. This does not prevent the instrument from operating, but limits it to observing X-rays of energy 1800  eV and above, as opposed to the planned 300 eV. [25] [26] A similar shutter over Xtend has opened normally.

See also

Notes

  1. ↑ Saku Tsuneta, director general of ISAS describes ATHENA as being a "super ASTRO-H"
  2. ↑ Hitomi/ASTRO-H was known as New X-ray Telescope (NeXT) during its proposal stage

Related Research Articles

<span class="mw-page-title-main">Chandra X-ray Observatory</span> NASA space telescope launched in 1999

The Chandra X-ray Observatory (CXO), previously known as the Advanced X-ray Astrophysics Facility (AXAF), is a Flagship-class space telescope launched aboard the Space ShuttleColumbia during STS-93 by NASA on July 23, 1999. Chandra was sensitive to X-ray sources 100 times fainter than any previous X-ray telescope, enabled by the high angular resolution of its mirrors. Since the Earth's atmosphere absorbs the vast majority of X-rays, they are not detectable from Earth-based telescopes; therefore space-based telescopes are required to make these observations. Chandra is an Earth satellite in a 64-hour orbit, and its mission is ongoing as of 2024.

<span class="mw-page-title-main">JAXA</span> Japans national air and space agency

The Japan Aerospace Exploration Agency (JAXA) is the Japanese national air and space agency. Through the merger of three previously independent organizations, JAXA was formed on 1 October 2003. JAXA is responsible for research, technology development and launch of satellites into orbit, and is involved in many more advanced missions such as asteroid exploration and possible human exploration of the Moon. Its motto is One JAXA and its corporate slogan is Explore to Realize.

<span class="mw-page-title-main">SELENE</span> Japanese lunar orbiter spacecraft

SELENE, better known in Japan by its nickname Kaguya (かぐや), was the second Japanese lunar orbiter spacecraft following the Hiten probe. Produced by the Institute of Space and Astronautical Science (ISAS) and the National Space Development Agency (NASDA), the spacecraft was launched on September 14, 2007. After orbiting the Moon for a year and eight months, the main orbiter was instructed to impact on the lunar surface near the crater Gill on June 10, 2009.

<span class="mw-page-title-main">Advanced Satellite for Cosmology and Astrophysics</span>

The Advanced Satellite for Cosmology and Astrophysics was the fourth cosmic X-ray astronomy mission by JAXA, and the second for which the United States provided part of the scientific payload. The satellite was successfully launched on 20 February 1993. The first eight months of the ASCA mission were devoted to performance verification. Having established the quality of performance of all ASCA's instruments, the spacecraft provided science observations for the remainder of the mission. In this phase the observing program was open to astronomers based at Japanese and U.S. institutions, as well as those located in member states of the European Space Agency.

<span class="mw-page-title-main">Suzaku (satellite)</span> Satellite

Suzaku was an X-ray astronomy satellite developed jointly by the Institute of Space and Aeronautical Science at JAXA and NASA's Goddard Space Flight Center to probe high-energy X-ray sources, such as supernova explosions, black holes and galactic clusters. It was launched on 10 July 2005 aboard the M-V launch vehicle on the M-V-6 mission. After its successful launch, the satellite was renamed Suzaku after the mythical Vermilion bird of the South.

<span class="mw-page-title-main">Akari (satellite)</span> Infrared astronomy satellite developed by Japan Aerospace Exploration Agency

AKARI (ASTRO-F) was an infrared astronomy satellite developed by Japan Aerospace Exploration Agency, in cooperation with institutes of Europe and Korea. It was launched on 21 February 2006, at 21:28 UTC by M-V rocket into Earth Sun-synchronous orbit. After its launch it was named AKARI (明かり), which means light in Japanese. Earlier on, the project was known as IRIS.

ASTRO-G was a planned radio telescope satellite by JAXA. It was expected to be launched into elliptic orbit around Earth.

XEUS was a space observatory plan developed by the European Space Agency (ESA) as a successor to the successful XMM-Newton X-ray satellite telescope. It was merged to the International X-ray Observatory (IXO) around 2008, but as that project ran into issues in 2011, the ESA component was forked off into Advanced Telescope for High Energy Astrophysics (Athena).

<span class="mw-page-title-main">Netherlands Institute for Space Research</span>

SRON Netherlands Institute for Space Research (SRON) is the Dutch national institute for space research. It develops and uses technology for analysis in space, This includes astrophysical research, Earth observation, and exoplanetary research. The SRON research focuses on sensors designed to detect X-rays, infrared radiation, and visible light.

<i>Hitomi</i> (satellite) Failed Japanese X-ray astronomy satellite

Hitomi, also known as ASTRO-H and New X-ray Telescope (NeXT), was an X-ray astronomy satellite commissioned by the Japan Aerospace Exploration Agency (JAXA) for studying extremely energetic processes in the Universe. The space observatory was designed to extend the research conducted by the Advanced Satellite for Cosmology and Astrophysics (ASCA) by investigating the hard X-ray band above 10 keV. The satellite was originally called New X-ray Telescope; at the time of launch it was called ASTRO-H. After it was placed in orbit and its solar panels deployed, it was renamed Hitomi. The spacecraft was launched on 17 February 2016 and contact was lost on 26 March 2016, due to multiple incidents with the attitude control system leading to an uncontrolled spin rate and breakup of structurally weak elements.

The Monitor of All-sky X-ray Image (MAXI) is an X-ray telescope mounted on the International Space Station since 2009. The instrument uses wide field of view X-ray detectors to perform a sky survey, measuring the brightness of X-ray sources every 96 minutes.

<span class="mw-page-title-main">Neutron Star Interior Composition Explorer</span> NASA telescope on International Space Station

The Neutron Star Interior Composition ExploreR (NICER) is a NASA telescope on the International Space Station, designed and dedicated to the study of the extraordinary gravitational, electromagnetic, and nuclear physics environments embodied by neutron stars, exploring the exotic states of matter where density and pressure are higher than in atomic nuclei. As part of NASA's Explorer program, NICER enabled rotation-resolved spectroscopy of the thermal and non-thermal emissions of neutron stars in the soft X-ray band with unprecedented sensitivity, probing interior structure, the origins of dynamic phenomena, and the mechanisms that underlie the most powerful cosmic particle accelerators known. NICER achieved these goals by deploying, following the launch, and activation of X-ray timing and spectroscopy instruments. NICER was selected by NASA to proceed to formulation phase in April 2013.

<span class="mw-page-title-main">Hinotori (satellite)</span> Japanese satellite

Hinotori, also known as ASTRO-A before launch, was a Japanese X-ray astronomy satellite. It was developed by the Institute of Space and Astronautical Science (ISAS). Its primary mission was to study of solar flares emanating from the Sun during the solar maximum. It was launched successfully on February 21, 1981 using a M-3S rocket as the vehicle from Uchinoura Space Center. After the start of normal operation, it observed a large solar flare and, a month later, succeeded in observing 41 flares of many sizes from the Sun. It reentered the atmosphere on July 11, 1991. The name Hinotori is the Japanese word for Phoenix.

<span class="mw-page-title-main">Smart Lander for Investigating Moon</span> Japanese lunar lander mission (2023–2024)

Smart Lander for Investigating Moon (SLIM) is a lunar lander mission of the Japan Aerospace Exploration Agency (JAXA). The lander's initial launch date in 2021 was postponed until 2023 due to delays in its rideshare, the X-Ray Imaging and Spectroscopy Mission (XRISM). On 6 September 2023 at 23:42 UTC, XRISM launched, and SLIM separated from it later that day.

Orbiting Binary Black Hole Investigation Satellite (ORBIS) is a small space telescope still in development by Japan that will study binary black holes in the X-ray region.

The Innovative Satellite Technology Demonstration Program is a series of spacecraft missions for testing technology and ideas put forward by universities and private companies. The program demonstrates various experimental devices and technology in space by providing flight opportunities. It is managed by the JAXA Research and Development Directorate. According to JAXA, the goal of this program is to test high risk, innovative technology that will lead to the space industry gaining competitiveness in the international field.

Cosmic Vision is the third campaign of space science and space exploration missions in the Science Programme of the European Space Agency (ESA). Formulated in 2005 as Cosmic Vision: Space Science for Europe 2015–2025, the campaign succeeded the Horizon 2000 Plus campaign and envisioned a number of missions in the fields of astronomy and solar system exploration beyond 2015. Ten missions across four funding categories are planned to be launched under Cosmic Vision, with the first being CHEOPS in December 2019. A mission to the Galilean moons (JUICE), the first deep space mission with an opportunistic target, and one of the first gravitational-wave space observatories (LISA), are planned for launch as part of the Cosmic Vision campaign.

<span class="mw-page-title-main">Compton Spectrometer and Imager</span> Space observatory to study gamma rays

The Compton Spectrometer and Imager (COSI) is a NASA SMEX astrophysics mission that will launch a soft gamma-ray telescope in 2027. It is a wide-field compact Compton telescope (CCT) that is uniquely suited to investigate the "MeV gap". It provides imaging, spectroscopy, and polarimetry of astrophysical sources, and its germanium detectors provide excellent energy resolution for emission line measurements.

References

  1. 1 2 3 Davenport, Justin (6 September 2023). "Japanese H-IIA launches X-ray telescope and lunar lander". NASASpaceFlight. Retrieved 7 September 2023.
  2. 1 2 3 4 5 6 7 Tsuneta, Saku (14 July 2016). "Ｘ線天文衛星ASTRO‐H「ひとみ」の後継機の検討について" (PDF) (Press release) (in Japanese). JAXA. Retrieved 1 July 2017.
  3. 1 2 Hertz, Paul (22 June 2017). "Astrophysics" (PDF). NASA. Retrieved 1 July 2017.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  4. 1 2 3 4 Fujimoto, Ryuichi; Tashiro, Makoto (5 January 2017). "ASTRO-Hに対する高エネルギーコミュニティの総括と今後の方向性について" (PDF) (in Japanese). JAXA. Retrieved 1 July 2017.
  5. 1 2 3 4 5 6 7 8 "Ｘ線天文衛星代替機の検討状況について" (PDF) (in Japanese). Ministry of Education, Culture, Sports, Science and Technology. 29 September 2016. Retrieved 1 July 2017.
  6. ↑ "X-Ray Imaging and Spectroscopy Mission: What's New". NASA Goddard Space Flight Center . Retrieved 22 January 2024.
  7. 1 2 "ISASニュース 2017.1 No.430" (PDF) (in Japanese). Institute of Space and Astronautical Science. 22 January 2017. Retrieved 23 March 2016.
  8. ↑ "Ｘ線天文衛星「ひとみ」の異常事象への対応と代替機の開発について" (PDF) (in Japanese). Committee on National Space Policy of Japan. 18 August 2016. Retrieved 1 July 2017.
  9. ↑ Craft, R.; Bautz, M.; Tomsick, J. (29 January 2017). "Probing the Hot and Energetic Universe: X-rays and Astrophysics" (PDF). NASA. Retrieved 28 June 2017.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  10. ↑ Takahashi, Tadayuki (27 November 2015). "X線天文衛星 ASTRO-Hの衛星概要" (PDF) (in Japanese). JAXA. Retrieved 13 July 2017.
  11. ↑ Dotani, Tadayasu (15 June 2011). "The 1st Athena Science Workshop JAXA Contribution" (PDF). Institute of Space and Astronautical Science. Retrieved 24 June 2017.
  12. 1 2 "GRAVITATIONAL WAVE MISSION SELECTED, PLANET-HUNTING MISSION MOVES FORWARD". ESA. 20 June 2017. Retrieved 24 June 2017.
  13. ↑ Foust, Jeff (21 July 2016). "NASA may build replacement instrument for Japanese astronomy mission". SpaceNews. Retrieved 30 June 2017.
  14. ↑ "第９回 宇宙科学・探査小委員会 議事要旨" (PDF) (in Japanese). Committee on National Space Policy of Japan. 1 November 2016. Retrieved 30 June 2017.
  15. ↑ Tashiro, Makoto; Kelley, Richard (8 June 2017). "X‐ray Astronomy Recovery Mission XARM" (PDF). ESA. Retrieved 5 October 2017.
  16. 1 2 "宇宙開発利用部会（第30回）議事録" (in Japanese). Ministry of Education, Culture, Sports, Science and Technology. 29 September 2016. Archived from the original on 9 July 2017. Retrieved 1 July 2017.
  17. 1 2 3 "宇宙開発利用部会（第29回）議事録" (in Japanese). Ministry of Education, Culture, Sports, Science and Technology. 14 July 2016. Archived from the original on 9 July 2017. Retrieved 1 July 2017.
  18. 1 2 Nakazawa, Kazuhiro; Mori, Koji (6 January 2017). "軟Ｘ線から硬Ｘ線の広帯域を高感度で撮像分光する小型衛星計画 FORCE - Focusing On Relativistic universe and Cosmic Evolution" (PDF) (in Japanese). JAXA. Retrieved 1 July 2017.
  19. ↑ "Astrophysics Implementation Plan: 2016 Update" (PDF). NASA. 15 December 2017. Retrieved 1 July 2017.
  20. ↑ "ISASニュース 2017.6 No.435" (PDF) (in Japanese). Institute of Space and Astronautical Science. 23 June 2017. Retrieved 4 July 2017.
  21. ↑ SVS (3 August 2023). "NASA Scientific Visualization Studio | A Guide to Cosmic Temperatures". SVS. Retrieved 6 August 2023.
  22. ↑ "Missions of Opportunity (MO) in Development – X-Ray Imaging and Spectroscopy Mission (XRISM) – Resolve". NASA. Retrieved 9 July 2019.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  23. ↑ Foust, Jeff (13 June 2016). "NASA and JAXA begin discussions on aftermath of Hitomi failure". SpaceNews. Retrieved 28 June 2017.
  24. ↑ "X線天文衛星ASTRO-Hのプロジェクト終了について" (PDF) (in Japanese). Ministry of Education, Culture, Sports, Science and Technology. 30 May 2017. Retrieved 1 July 2017.
  25. ↑ "XRISM's First Light and Operational Update" (Press release). Japan Aerospace Exploration Agency. 5 January 2024. ...Resolve's spectra are still limited to 1,800 eV and above because the Dewar aperture door to protect the sensitive detector has yet to be opened....
  26. ↑ Kazmierczak, Jeanette (5 January 2024). "NASA/JAXA XRISM Mission Reveals Its First Look at X-ray Cosmos" (Press release). NASA Goddard Space Flight Center. The door, designed to protect the detector before launch, has not opened as planned after several attempts. The door blocks lower-energy X-rays, effectively cutting the mission off at 1,700 electron volts compared to the planned 300.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.