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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. It was constructed at the Jet Propulsion Laboratory with major subsystems being delivered from Malin Space Science Systems and Los Alamos National Laboratory.

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

Goals

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

The goals of the SHERLOC investigation are to:

• Assess the habitability potential of a sample and its aqueous history.
• Assess the availability of key elements and energy source for life (C, H, N, O, P, S etc.).
• Determine if there are potential biosignatures preserved in Martian rocks and outcrops.
• Provide organic and mineral analysis for selective sample caching.

To do this SHERLOC does the following:

• Detects and classifies organics and astrobiologically relevant minerals on the surface and near subsurface of Mars.
• Bulk organic sensitivity of 10-5 to 10-6 w/w over a 7 x 7 mm spot.
• Fine scale organic sensitivity of 10-2 to 10-4 w/w spatially resolved at < 100 μm.
• Astrobiologically Relevant Mineral (ARM) detection and classification to < 100 μm resolution.

— Beegle, L.W., et al., USRA (2017)

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.

Results from Mars

This section needs to be updated. Please help update this article to reflect recent events or newly available information. (October 2024)

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. Utilizing WATSON and ACI images, there was confirmation that the Jezero Crater floor consists of aqueously altered mafic material with various igneous origins. In addition, WATSON has been used to collect selfies of the Perseverance rover and the Ingenuity helicopter. Recently, it successfully sealed and stored the first two rock samples from Mars. Because of it, We now know that these rocks derived from a volcanic environment, and that there was liquid water there in Mars's past, that formed salts that SHERLOC has seen.

See also

• Composition of Mars
• Curiosity rover
• Exploration of Mars
• Geology of Mars
• List of rocks on Mars
• Mars Science Laboratory
• MOXIE
• PIXL
• Scientific information from the Mars Exploration Rover mission
• Timeline of Mars Science Laboratory

References

1. Webster, Guy (31 July 2014). "SHERLOC to Micro-Map Mars Minerals and Carbon Rings". NASA. Retrieved 31 July 2014.
2. ^ 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. PMC 10371864.
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.

External links

• Mars 2020 Mission - Home Page - NASA/JPL

v t e Mars 2020
Timeline of Mars 2020
Payloads	Perseverance rover Ingenuity helicopter (list of flights)
Rover instruments	Hazcam Mastcam-Z MEDA MOXIE Navcam PIXL RIMFAX Rover embedded computers SHERLOC SuperCam
Features	MarsDial Multi-mission radioisotope thermoelectric generator Rocker-bogie Sky crane
Proposed landing sites	Selected Jezero crater Finalists Columbia Hills in Gusev crater Jezero crater Syrtis Major Planum Other Eberswalde crater Holden crater Mawrth Vallis Nili Fossae Melas Chasma
Related	Octavia E. Butler Landing Wright Brothers Field Cheyava Falls Exploration of Mars
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