Lobster-eye optics

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Schematic diagram of lobster-eye lens. The green arrow represents the incident light and the red arrows represent the normal of the channel wall. Schematic diagram of lobster eye lens.jpg
Schematic diagram of lobster-eye lens. The green arrow represents the incident light and the red arrows represent the normal of the channel wall.

Lobster-eye optics are a biomimetic design, based on the structure of the eyes of a lobster with an ultra wide field of view, used in X-ray optics. This configuration allows X-ray light to enter from multiple angles, capturing more X-rays from a larger area than other X-ray telescopes. The idea was originally proposed for use in X-ray astronomy by Roger Angel in 1979, with a similar idea presented earlier by W. K. H. Schmidt in 1975. It was first used by NASA on a sub-orbital sounding rocket experiment in 2012. The Lobster Eye Imager for Astronomy, a Chinese technology demonstrator satellite, was launched in 2022. The Chinese Einstein Probe, launched in 2024, is the first major space telescope to use lobster-eye optics. Several other such space telescopes are currently under development or consideration.

Contents

Description

Close-up view of crustacean's (mantis shrimp's) eyes Odontodactylus scyllarus eyes.jpg
Close-up view of crustacean's (mantis shrimp's) eyes

While most animals have refractive eyes, lobsters and other crustaceans have reflective eyes. [2] The eyes of a crustacean contain clusters of cells, each reflecting a small amount of light from a particular direction. Lobster-eye optics technology mimics this reflective structure. This arrangement allows the light from a wide viewing area to be focused into a single image. The optics are made of microchannel plates. X-ray light can enter small tubes within these plates from multiple angles, and is focused through grazing-incidence reflection that gives a wide field of view. That, in turn, makes it possible to locate and image transient astronomical events that could not have been predicted in advance. [3]

The field of view (FoV) of a lobster-eye optic, which is the solid angle subtended by the optic plate to the curvature center, is limited only by the optic size for a given curvature radius. Since the micropore optics are spherically symmetric in essentially all directions, theoretically, an idealized lobster-eye optic is almost free from vignetting except near the edge of the FoV. [4] Micropore imagers are created from several layers of lobster-eye optics that creates an approximation of Wolter type-I optical design. [2]

History

Only three geometries that use grazing incidence reflection of X-rays to produce X-ray images are known: the Wolter system, the Kirkpatrick-Baez system, and the lobster-eye geometry. [5]

The lobster-eye X-ray optics design was first proposed in 1979 by Roger Angel. [6] [7] His design is based on Kirkpatrick-Baez optics, but requires pores with a square cross-section, and is referred to as the "Angel multi-channel lens". [5] This design was inspired directly by the reflective properties of lobster eyes. [1] [4] Before Angel, an alternative design involving a one-dimensional arrangement consisting of a set of flat reflecting surfaces had been proposed by W. K. H. Schmidt in 1975, known as the "Schmidt focusing collimator objective". [5] [8] [9] In 1989, physicists Keith Nugent and Stephen W. Wilkins collaborated to develop lobster-eye optics independently of Angel. Their key contribution was to open up an approach to manufacturing these devices using microchannel plate technology. This lobster-eye approach paved the way for X-ray telescopes with a 360-degree view of the sky. [10]

In 1992, Philip E. Kaaret and Phillip Geissbuehler proposed a new method for creating lobster-eye optics with microchannel plates. [11] Micropores required for lobster-eye optics are difficult to manufacture and have strict requirements. The pores must have widths between 0.01 and 0.5 mm and should have a length-to-width ratio of 20–200 (depends on the X-ray energy range); they need to be coated with a dense material for optimal X-ray reflection. The pore's inner walls must be flat and they should be organized in a dense array on a spherical surface with a radius of curvature of 2F, ensuring an open fraction greater than 50% and pore alignment accuracy between 0.1 and 5 arc minutes towards a common center. [5]

Similar optics designs include honeycomb collimators (used in NEAR Shoemaker's XGRS detectors and MESSENGER's XRS) and silicon pore imagers (developed by ESA for its planned ATHENA mission). [2]

Uses

Configuration of the focusing mirror system, focal detector array, and FoV of LEIA. The mirror assembly is divided into four individual quadrants, each consisting of 3 x 3 MPO plates and associated with one of the four detectors. Configuration of the focusing mirror system of LEIA.jpg
Configuration of the focusing mirror system, focal detector array, and FoV of LEIA. The mirror assembly is divided into four individual quadrants, each consisting of 3 × 3 MPO plates and associated with one of the four detectors.
The LEIA instrument undergoing on-ground X-ray calibration before being assembled onto the SATech satellite. LEIA instrument.jpg
The LEIA instrument undergoing on-ground X-ray calibration before being assembled onto the SATech satellite.

NASA launched the first lobster-eye imager on a Black Brant IX sub-orbital sounding rocket in 2012. The STORM/DXL instrument (Sheath Transport Observer for the Redistribution of Mass/Diffuse X-ray emission from the Local galaxy) had micropore reflectors arranged in an array to form a Kirkpatrick-Baez system. [12] [13] BepiColombo, a joint ESA and JAXA Mercury mission launched in 2018, has a non-imaging collimator MIXS-C, with a microchannel geometry similar to the lobster-eye micropore design. [8] [14]

CNSA launched the Lobster-Eye X-ray Satellite in 2020, the first in-orbit lobster-eye telescope. [15] In 2022, the Chinese Academy of Sciences built and launched the Lobster Eye Imager for Astronomy (LEIA), a wide-field X-ray imaging space telescope. It is a technology demonstrator mission that tests the sensor design for the Einstein Probe. [16] LEIA has a sensor module that gives it a field of view of 340 square degrees. [16] In August and September of 2022, LEIA conducted measurements to verify its functionality. A number of preselected sky regions and targets were observed, including the Galactic Center, the Magellanic Clouds, Sco X-1, Cas A, Cygnus Loop, and a few extragalactic sources. To eliminate interference from sunlight, the observations were obtained in Earth's shadow, starting 2 minutes after the satellite entered the shadow and ending 10 minutes before leaving it, resulting in an observational duration of ~23 minutes in each orbit. The CMOS detectors were operating in the event mode. [4]

Current and future space telescopes

The Einstein Probe, a joint mission by the Chinese Academy of Sciences (CAS) in partnership with the European Space Agency (ESA) and the Max Planck Institute for Extraterrestrial Physics, was launched on 9 January 2024. [17] It uses a 12-sensor module wide-field X-ray telescope for a 3600 square degree field of view, first tested by the Lobster Eye Imager for Astronomy mission. [16]

NASA's Goddard Space Center proposed an instrument that uses the lobster-eye design for the ISS-TAO mission (Transient Astrophysics Observatory on the International Space Station), called the X-ray Wide-Field Imager. [3] ISS-Lobster is a similar concept by ESA. [18]

Several space telescopes that use lobster-eye optics are under construction. The joint French-Chinese SVOM is expected to be launched in July 2024. [19] SMILE, a space telescope project by ESA and CAS, is planned to be launched in 2025. [20] ESA's THESEUS is now under consideration. [21]

Other uses

Lobster-eye optics can also be used for backscattering imaging for homeland security, detection of improvised explosive devices, nondestructive testing, and medical imaging. [1]

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References

  1. 1 2 3 Ma, Shizhang; Ouyang, Mingzhao; Fu, Yuegang; Hu, Yuan; Zhang, Yuhui; Yang, Yuxiang; Wang, Shengyu (September 2023). "Analysis of Imaging Characteristics of Wide-field Lobster Eye Lens". Journal of Physics: Conference Series. 2597 (1): 012010. Bibcode:2023JPhCS2597a2010M. doi: 10.1088/1742-6596/2597/1/012010 . ISSN   1742-6596. CC BY icon.svg Material was copied from this source, which is available under a Creative Commons Attribution 3.0 Archived 2011-02-23 at the Wayback Machine
  2. 1 2 3 Kitchin, C. R. (18 September 2017). Remote and Robotic Investigations of the Solar System. CRC Press. pp. 123–128. ISBN   978-1-4987-0494-6. Archived from the original on 14 February 2024. Retrieved 9 February 2024.
  3. 1 2 "Proposed NASA Mission Employs "Lobster-Eye" Optics to Locate Source of Cosmic Ripples - NASA". NASA. 26 October 2017. Archived from the original on 29 December 2023. Retrieved 29 December 2023.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  4. 1 2 3 4 5 6 7 Zhang, C.; et al. (1 December 2022). "First Wide Field-of-view X-Ray Observations by a Lobster-eye Focusing Telescope in Orbit". The Astrophysical Journal Letters. 941 (1): L2. arXiv: 2211.10007 . Bibcode:2022ApJ...941L...2Z. doi: 10.3847/2041-8213/aca32f . ISSN   2041-8205. CC BY icon.svg Material was copied from this source, which is available under a Creative Commons Attribution 4.0 Archived 2017-10-16 at the Wayback Machine
  5. 1 2 3 4 Richard Willingale (July 2021). "Lobster Eye Optics". In Sternberg, Amiel; Burrows, David N (eds.). The WSPC Handbook of Astronomical Instrumentation: Volume 4: X-Ray Astronomical Instrumentation. Vol. 4. World Scientific Publishing Co. Pte. Ltd. pp. 33–47, 85–106. Bibcode:2021hai4.book.....B. doi:10.1142/9446-vol4. ISBN   978-981-4644-38-9. Archived from the original on 14 February 2024. Retrieved 1 January 2024.
  6. ↑ Angel, J. R. P. (Oct 1, 1979). "Lobster eyes as X-ray telescopes". Astrophysical Journal. 233 (Part 1): 364–373. Bibcode:1979ApJ...233..364A. doi: 10.1086/157397 .
  7. ↑ Hartline, Beverly Karplus (4 January 1980). "Lobster-Eye X-ray Telescope Envisioned". Science. 207 (4426): 47. Bibcode:1980Sci...207...47K. doi:10.1126/science.207.4426.47. ISSN   0036-8075. Archived from the original on 29 December 2023. Retrieved 29 December 2023.
  8. 1 2 Hudec, Rene; Feldman, Charly (2022). "Lobster Eye X-ray Optics". Handbook of X-ray and Gamma-ray Astrophysics. Springer Nature. pp. 1–39. arXiv: 2208.07149 . doi:10.1007/978-981-16-4544-0_3-1. ISBN   978-981-16-4544-0. S2CID   260481363. Archived from the original on 2023-12-29. Retrieved 2023-12-29.
  9. ↑ Schmidt, W. K. H. (August 1, 1975). "A proposed X-ray focusing device with wide field of view for use in X-ray astronomy". Nuclear Instruments and Methods. 127 (2): 285–292. Bibcode:1975NucIM.127..285S. doi:10.1016/0029-554X(75)90501-7 – via ScienceDirect.
  10. ↑ "Scientist has an all-seeing eye on the future". The Age. 2004-08-19. Archived from the original on 2021-12-17. Retrieved 2021-12-17.
  11. ↑ Kaaret, Philip E.; Geissbuehler, Phillip (1992). Hoover, Richard B. (ed.). "Lobster-eye x-ray optics using microchannel plates". SPIE Proceedings. Multilayer and Grazing Incidence X-Ray/EUV Optics. 1546: 82. Bibcode:1992SPIE.1546...82K. doi:10.1117/12.51261. S2CID   121803620. Archived from the original on 2024-02-14. Retrieved 2024-02-01.
  12. ↑ Collier, Michael R.; et al. (1 July 2015). "Invited Article: First flight in space of a wide-field-of-view soft x-ray imager using lobster-eye optics: Instrument description and initial flight results". Review of Scientific Instruments. 86 (7). Bibcode:2015RScI...86g1301C. doi:10.1063/1.4927259. hdl: 1808/22116 . PMID   26233339. Archived from the original on 5 December 2023. Retrieved 9 February 2024.
  13. ↑ Keesey, Lori; Center, NASA's Goddard Space Flight. "NASA scientists build first-ever wide-field X-ray imager". phys.org. Archived from the original on 3 February 2024. Retrieved 9 February 2024.
  14. ↑ "MIXS - BepiColombo - Cosmos". www.cosmos.esa.int. Retrieved 16 February 2024.
  15. ↑ "Launch of the world's first soft X-ray satellite with 'Lobster-Eye' imaging technology". phys.org. Archived from the original on 2021-12-17. Retrieved 2021-12-17.
  16. 1 2 3 "Einstein Probe Time Domain Astronomical Information Center". ep.bao.ac.cn. Archived from the original on 28 December 2023. Retrieved 28 December 2023.
  17. ↑ The European Space Agency (January 9, 2024). "Einstein Probe lifts off on a mission to monitor the X-ray sky". www.esa.int. Archived from the original on January 9, 2024. Retrieved February 6, 2024.
  18. ↑ Camp, Jordan; et al. (12 May 2015). "ISS-Lobster: a low-cost wide-field x-ray transient detector on the ISS". Proceedings of SPIE: EUV and X-ray Optics. Synergy between Laboratory and Space IV. Vol. 9510. The International Society for Optical Engineering. p. 951007. doi:10.1117/12.2176745. ISBN   9781628416312. OCLC   923760787. S2CID   117082454.
  19. ↑ "The MXT and the lobster eye - Svom". China National Space Administration (CNSA); Chinese Academy of Sciences (CAS); French Space Agency (CNES). Archived from the original on 2023-10-04. Retrieved 2024-02-06.
  20. ↑ Branduardi-Raymont, G.; Wang, C.; Escoubet, C.P.; et al. (2018). ESA SMILE definition study report (PDF) (Technical report). European Space Agency. pp. 1–84. doi:10.5270/esa.smile.definition_study_report-2018-12. S2CID   239612452. ESA/SCI(2018)1. Archived (PDF) from the original on 2023-04-22.
  21. ↑ Amati, Lorenzo (December 2017). "The Transient High-Energy Sky and Early Universe Surveyor (THESEUS)". Proceedings of the Fourteenth Marcel Grossmann Meeting on General Realitivity. World Scientific Publishing. pp. 3295–3300. arXiv: 1907.00616 . doi:10.1142/9789813226609_0421. ISBN   978-981-322-659-3. Archived from the original on 2024-02-14. Retrieved 2024-02-06.
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