Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals#Construction

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

{{quote|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.

|author=Beegle, L.W., et al. |source=USRA (2017)}}

{{redirect|WATSON|other uses|Watson (disambiguation)}}

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.{{Cite book|last1=Beegle|first1=L.|last2=Bhartia|first2=R.|last3=White|first3=M.|last4=DeFlores|first4=L.|last5=Abbey|first5=W.|last6=Wu|first6=Yen-Hung|last7=Cameron|first7=B.|last8=Moore|first8=J.|last9=Fries|first9=M.|title=2015 IEEE Aerospace Conference |chapter=SHERLOC: Scanning habitable environments with Raman & luminescence for organics & chemicals |date=2015-03-01|pages=1–11|doi=10.1109/AERO.2015.7119105|isbn=978-1-4799-5379-0|s2cid=28838479 }}{{multipleimage | caption_align=center |header=SHERLOC |direction=horizontal |align=center |width= |image1=PIA23894-MarsPerseveranceRover-SHERLOC-20200526.jpg |caption1=instrument – outside> |width1=190 |image2=PIA23621-Mars2020Rover-SHERLOC-20200220.jpg |caption2=instrument – inside |width2=190 |image3=PIA23895-MarsPersevranceRover-SHERLOC-TestImage-20200526.jpg |caption3=Test image
(26 May 2020) |width3=190 |image4=PIA24641-MarsPerseveranceRover-WatsonCameraViewsRocks-20210510.webm |caption4=Test – WATSON camera focus
(Mars; video; 0:05; 10 May 2021) |width4=191 |image5=PIA25245-Mars-PerseveranceRover-SHERLOC-Test-20220722.jpg |caption5=Test rock study
(22 July 2022) |width5=250 |image6=PIA25919-MarsPerseveranceRover-QuartierRock-SHERLOC-20230712.jpg ||caption6=Quartier rock (context)
(12 July 2023) |width6=190 |image7=PIA25919-MarsPerseveranceRover-QuartierRock-Closeup-20230712.png |caption7=Quartier rock study
(12 July 2023) |width7=190|footer= }}

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{{update section|date=October 2024}}

File:Mars 2020 selfie containing both perseverance rover and ingenuity.gif

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.{{Cite journal |last=Scheller |first=Eva L. |last2=Razzell Hollis |first2=Joseph |last3=Cardarelli |first3=Emily L. |last4=Steele |first4=Andrew |last5=Beegle |first5=Luther W. |last6=Bhartia |first6=Rohit |last7=Conrad |first7=Pamela |last8=Uckert |first8=Kyle |last9=Sharma |first9=Sunanda |last10=Ehlmann |first10=Bethany L. |last11=Abbey |first11=William J. |last12=Asher |first12=Sanford A. |last13=Benison |first13=Kathleen C. |last14=Berger |first14=Eve L. |last15=Beyssac |first15=Olivier |date=2022-12-09 |title=Aqueous alteration processes in Jezero crater, Mars—implications for organic geochemistry |url=https://www.science.org/doi/10.1126/science.abo5204 |journal=Science |language=en |volume=378 |issue=6624 |pages=1105–1110 |doi=10.1126/science.abo5204 |issn=0036-8075|url-access=subscription }}{{Cite journal |last=Sharma |first=Sunanda |last2=Roppel |first2=Ryan D. |last3=Murphy |first3=Ashley E. |last4=Beegle |first4=Luther W. |last5=Bhartia |first5=Rohit |last6=Steele |first6=Andrew |last7=Hollis |first7=Joseph Razzell |last8=Siljeström |first8=Sandra |last9=McCubbin |first9=Francis M. |last10=Asher |first10=Sanford A. |last11=Abbey |first11=William J. |last12=Allwood |first12=Abigail C. |last13=Berger |first13=Eve L. |last14=Bleefeld |first14=Benjamin L. |last15=Burton |first15=Aaron S. |date=July 2023 |title=Diverse organic-mineral associations in Jezero crater, Mars |url=https://www.nature.com/articles/s41586-023-06143-z |journal=Nature |language=en |volume=619 |issue=7971 |pages=724–732 |doi=10.1038/s41586-023-06143-z |issn=1476-4687|pmc=10371864 }} Utilizing WATSON and ACI images, there was confirmation that the Jezero Crater floor consists of aqueously altered mafic material with various igneous origins.{{Cite journal |last=Wogsland |first=B. V. |last2=Minitti |first2=M. E. |last3=Kah |first3=L. C. |last4=Yingst |first4=R. A. |last5=Abbey |first5=W. |last6=Bhartia |first6=R. |last7=Beegle |first7=L. |last8=Bleefeld |first8=B. L. |last9=Cardarelli |first9=E. L. |last10=Conrad |first10=P. G. |last11=Edgett |first11=K. |last12=Hickman‐Lewis |first12=K. |last13=Hugget |first13=J. |last14=Imbeah |first14=S. |last15=Kennedy |first15=M. R. |date=November 2023 |title=Science and Science‐Enabling Activities of the SHERLOC and WATSON Imaging Systems in Jezero Crater, Mars |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022EA002544 |journal=Earth and Space Science |language=en |volume=10 |issue=11 |doi=10.1029/2022EA002544 |issn=2333-5084|doi-access=free }} 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. {{Cite web |title=Perseverance's Selfie with Ingenuity - NASA Science |url=https://science.nasa.gov/resource/perseverances-selfie-with-ingenuity/ |access-date=2024-06-08 |website=science.nasa.gov |language=en-US}}

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• 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

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{{Reflist|30}}

• [http://mars.jpl.nasa.gov/mars2020 Mars 2020 Mission - Home Page - NASA/JPL]

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