Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals

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Perseverance rover - SHERLOC Mars2020Rover-SHERLOC-20140731.jpg
SHERLOC's calibration target aboard the Perseverance Mars rover with Mars Meteorite in the centre of top row PIA24261-MarsPerseveranceRover-SHERLOC-CalibrationTarget-20201208.jpg
SHERLOC's calibration target aboard the Perseverance Mars rover with Mars Meteorite in the centre of top row

Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) is an ultraviolet Raman spectrometer that uses fine-scale imaging and an ultraviolet (UV) laser to determine fine-scale mineralogy, and detect organic compounds designed for the Perseverance rover as part of the Mars 2020 mission. [1] [2] [3] It was constructed at the Jet Propulsion Laboratory with major subsystems being delivered from Malin Space Science Systems and Los Alamos National Laboratory.

Contents

SHERLOC has a calibration target with possible Mars suit materials, and it will measure how they change over time in the Martian surface environment. [4]

Goals

According to a 2017 Universities Space Research Association (USRA) report: [2]

The goals of the SHERLOC investigation are to:

To do this SHERLOC does the following:

— Beegle, L.W., et al., USRA (2017) [2]

Construction

There are three locations on the rover where SHERLOC components are located. The SHERLOC Turret Assembly (STA) is mounted at the end of the rover arm. The STA contains spectroscopy and imaging components. The SHERLOC Body Assembly (SBA) is located on the rover chassis and acts as the interface between the STA and the Mars 2020 rover. The SBA deals with command and data handling, along with power distribution. The SHERLOC Calibration Target (SCT) is located on the front of the rover chassis and hold spectral standards.

SHERLOC consists of both imaging and spectroscopic elements. It has two imaging components consisting of heritage hardware from the MSL MAHLI instrument. The Wide Angle Topographic Sensor for Operations and eNgineering (WATSON) is a built to print re-flight that can generate color images over multiple scales. The other, Autofocus Context Imager (ACI), acts as the mechanism that allows the instrument to get a contextual image of a sample and to autofocus the laser spot for the spectroscopic part of the SHERLOC investigation.

For Spectroscopy, it utilizes a NeCu laser to generate UV photons (248.6 nm) which can generate characteristic Raman and fluorescence photons from a scientifically interesting sample. The deep UV laser is co-boresighted to a context imager and integrated into an autofocusing/scanning optical system that allows correlation of spectral signatures to surface textures, morphology and visible features. The context imager has a spatial resolution of 30 μm and currently is designed to operate in the 400-500 nm wavelength range. [5]

SHERLOC
PIA23894-MarsPerseveranceRover-SHERLOC-20200526.jpg
instrument – outside>
PIA23621-Mars2020Rover-SHERLOC-20200220.jpg
instrument – inside
PIA23895-MarsPersevranceRover-SHERLOC-TestImage-20200526.jpg
Test image
(26 May 2020)
Test – WATSON camera focus
(Mars; video; 0:05; 10 May 2021)
PIA25245-Mars-PerseveranceRover-SHERLOC-Test-20220722.jpg
Test rock study
(22 July 2022)
PIA25919-MarsPerseveranceRover-QuartierRock-SHERLOC-20230712.jpg
Quartier rock (context)
(12 July 2023)
PIA25919-MarsPerseveranceRover-QuartierRock-Closeup-20230712.png
Quartier rock study
(12 July 2023)

Results from Mars

WATON Selfie image of Perseverance rover and Ingenuity helicopter Mars 2020 selfie containing both perseverance rover and ingenuity.gif
WATON Selfie image of Perseverance rover and Ingenuity helicopter

Over the course of three years, SHERLOC and WATSON have been successfully collecting spectra and images of minerals and organics on the surface of Mars [6] [7] . Utilizing WATSON and ACI images, there was confirmation that the crafter floor consists of aqueously altered mafic material with various igneous origins [8] .In addition, WATSON has been used to collect selfies of the Perseverance rover and the Ingenuity helicopter [9] .

See also

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References

  1. ↑ Webster, Guy (31 July 2014). "SHERLOC to Micro-Map Mars Minerals and Carbon Rings". NASA . Retrieved 31 July 2014.
  2. 1 2 3 Beegle, L.W.; et al. (2017). "The SHERLOC Investigation For MARS 2020 (SHERLOC: Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals, an Investigation for 2020)" (PDF). Universities Space Research Association . Retrieved 30 August 2017.
  3. ↑ Bhartia, Rohit; Beegle, Luther W.; DeFlores, Lauren; Abbey, William; Razzell Hollis, Joseph; Uckert, Kyle; Monacelli, Brian; Edgett, Kenneth S.; Kennedy, Megan R.; Sylvia, Margarite; Aldrich, David; Anderson, Mark; Asher, Sanford A.; Bailey, Zachary; Boyd, Kerry (25 May 2021). "Perseverance's Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) Investigation". Space Science Reviews. 217 (4): 58. doi:10.1007/s11214-021-00812-z. ISSN   1572-9672.
  4. ↑ "The next NASA rover could lead to safer space suits for astronauts exploring Mars". The Mercury News. 20 February 2018. Retrieved 24 February 2018.
  5. ↑ Beegle, L.; Bhartia, R.; White, M.; DeFlores, L.; Abbey, W.; Wu, Yen-Hung; Cameron, B.; Moore, J.; Fries, M. (1 March 2015). "SHERLOC: Scanning habitable environments with Raman & luminescence for organics & chemicals". 2015 IEEE Aerospace Conference. pp. 1–11. doi:10.1109/AERO.2015.7119105. ISBN   978-1-4799-5379-0. S2CID   28838479.
  6. ↑ Scheller, Eva L.; Razzell Hollis, Joseph; Cardarelli, Emily L.; Steele, Andrew; Beegle, Luther W.; Bhartia, Rohit; Conrad, Pamela; Uckert, Kyle; Sharma, Sunanda; Ehlmann, Bethany L.; Abbey, William J.; Asher, Sanford A.; Benison, Kathleen C.; Berger, Eve L.; Beyssac, Olivier (9 December 2022). "Aqueous alteration processes in Jezero crater, Mars—implications for organic geochemistry". Science. 378 (6624): 1105–1110. doi:10.1126/science.abo5204. ISSN   0036-8075.
  7. ↑ Sharma, Sunanda; Roppel, Ryan D.; Murphy, Ashley E.; Beegle, Luther W.; Bhartia, Rohit; Steele, Andrew; Hollis, Joseph Razzell; Siljeström, Sandra; McCubbin, Francis M.; Asher, Sanford A.; Abbey, William J.; Allwood, Abigail C.; Berger, Eve L.; Bleefeld, Benjamin L.; Burton, Aaron S. (July 2023). "Diverse organic-mineral associations in Jezero crater, Mars". Nature. 619 (7971): 724–732. doi:10.1038/s41586-023-06143-z. ISSN   1476-4687.
  8. ↑ Wogsland, B. V.; Minitti, M. E.; Kah, L. C.; Yingst, R. A.; Abbey, W.; Bhartia, R.; Beegle, L.; Bleefeld, B. L.; Cardarelli, E. L.; Conrad, P. G.; Edgett, K.; Hickman‐Lewis, K.; Hugget, J.; Imbeah, S.; Kennedy, M. R. (November 2023). "Science and Science‐Enabling Activities of the SHERLOC and WATSON Imaging Systems in Jezero Crater, Mars". Earth and Space Science. 10 (11). doi:10.1029/2022EA002544. ISSN   2333-5084.
  9. ↑ "Perseverance's Selfie with Ingenuity - NASA Science". science.nasa.gov. Retrieved 8 June 2024.
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