Arcus (satellite)

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Arcus
Arcus X-ray Spectrometer on orbit.jpg
Artist concept of the Arcus satellite on orbit.
Mission type X-ray space observatory
Operator NASA
Website www.arcusxray.org
Mission duration 2–5 years (proposed)
Spacecraft properties
Bus LEOStar-2 S/C [1]
Manufacturer Orbital ATK[2]
BOL mass 1,142 kg (2,518 lb)[1]
Power 405 W[1]
Start of mission
Launch date 2023 (proposed)[3]
Main telescope
Focal length 12 m (39 ft)[1]
Collecting area 500 cm2 (78 sq in)[1]
Wavelengths X-ray

Arcus is a proposed X-ray space observatory proposed to NASA's Explorer program, Medium Explorer (MIDEX) class.

The Arcus mission would study galaxies and galaxy clusters using high-resolution X-ray spectroscopy to characterize the interactions between these objects and the diffuse hot gas that permeates them. The Principal investigator is Randall Smith at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts; the project has significant contributions from the Massachusetts Institute of Technology, cosine Measurement Systems (Warmond NL), PennState, and the Max Planck Institute for Extraterrestrial Physics.[2][3]

Overview[edit]

Arcus's spectrograph was originally intended to fly on the cancelled International X-ray Observatory (IXO).[4] After the 2011 cancellation, Arcus was proposed as a mission in 2014 to the Small Explorer program (SMEX) but it was not selected for development. After numerous technological advances later, Arcus was again proposed to NASA in 2016 to the Medium Exproler program (MIDEX) and was awarded $2 million to refine their mission concept (Phase A study) over nine-months.[5] If selected, it would be funded $250 million for development.[6]

Arcus is an X-ray grating spectrometer space observatory that combines X-ray optics and gratings to disperse the X-rays, much like how a prism separates sunlight into the colors of the rainbow.[2] It would observe astrophysical phenomena in X-ray band over a broad target size range. Its mission includes investigations on the composition of cosmic dust grains, stellar evolution, identify the launching mechanisms of supermassive black hole winds, and structure formation of galaxy clusters. Using new technologies, it offers a resolution improvement of ten times better than existing X-ray observatories.[4][7]

The space observatory would orbit Earth in a 4:1 lunar resonance, which would allow significant stability for minimal propellant consumption, which could extend the mission life to about 10 years.[1]

It is competing for selection for the next Medium-Class Explorers mission, which will take place in 2019, between Arcus and SPHEREx.[5][2] If selected in 2019 and built, it would launch in 2023.[3]

References[edit]

  1. ^ a b c d e f Arcus: exploring the formation and evolution of clusters, galaxies, and stars. (PDF). Randall K. Smith, M. H. Abraham, S. J. Wolk, et al. Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, edited by Jan-Willem A. den Herder, Tadayuki Takahashi, Marshall Bautz, Proc. of SPIE, 2018. doi:10.1117/12.2231778.
  2. ^ a b c d NASA Selects the Arcus X-Ray Mission for Phase A Study. Harvard-Smithsonian Center for Astrophysics. Press release: 10 August 2017.
  3. ^ a b c NASA selects X-ray mission Arcus for phase A study. SRON. 23 August 2017.
  4. ^ a b Arcus Mission - Home page. Accessed: April 2018.
  5. ^ a b NASA Selects Proposals to Study Galaxies, Stars, Planets. Katherine Brown, NASA News. 9 August 2017.
  6. ^ NASA selects Arcus for Phase A studies. Penn State News. 31 August 2018.
  7. ^ High-resolution X-ray gratings enable state-of-the-art spectrometer. Phys Org. 9 January 2018.