Perseverance’s Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) Investigation

R. Bhartia(Photon Systems (United States)), L. W. Beegle(Jet Propulsion Laboratory), Lauren DeFlores(Jet Propulsion Laboratory), William Abbey(Jet Propulsion Laboratory), Joseph Razzell Hollis(Jet Propulsion Laboratory), Kyle Uckert(Jet Propulsion Laboratory), Brian Monacelli(Jet Propulsion Laboratory), K. S. Edgett(Malin Space Science Systems (United States)), M. R. Kennedy(Malin Space Science Systems (United States)), Margarite Sylvia(Jet Propulsion Laboratory), D. Aldrich(Jet Propulsion Laboratory), M. S. Anderson(Jet Propulsion Laboratory), Sanford A. Asher(Pittsburg State University), Zachary Bailey(Jet Propulsion Laboratory), Kerry Boyd(Los Alamos National Laboratory), Aaron S. Burton(Johnson Space Center), Michael Caffrey(Los Alamos National Laboratory), Michael J. Calaway(Johnson Space Center), Robert J. Calvet(Jet Propulsion Laboratory), Bruce Cameron(Jet Propulsion Laboratory), M. A. Caplinger(Malin Space Science Systems (United States)), Brandi L. Carrier(Jet Propulsion Laboratory), Nataly Chen(Jet Propulsion Laboratory), Amy Chen(Jet Propulsion Laboratory), Matthew J. Clark(Malin Space Science Systems (United States)), S. M. Clegg(Los Alamos National Laboratory), P. G. Conrad(Carnegie Institution for Science), Moogega Cooper(Jet Propulsion Laboratory), Kristine Davis(Johnson Space Center), B. L. Ehlmann(California Institute of Technology), Linda Facto(Jet Propulsion Laboratory), M. Fries(Johnson Space Center), D. H. Garrison(Johnson Space Center), Denine Gasway(Los Alamos National Laboratory), Ferial Ghaemi(Heinz Optical Engineering (United States)), Trevor G. Graff(Johnson Space Center), K. P. Hand(Jet Propulsion Laboratory), Cathleen M. Harris(Jet Propulsion Laboratory), J D Hein(Jet Propulsion Laboratory), Nicholas A. Heinz(Jet Propulsion Laboratory), Harrison Herzog(Jet Propulsion Laboratory), Eric B. Hochberg(Jet Propulsion Laboratory), Andrew Houck(Jet Propulsion Laboratory), William F. Hug(Photon Systems (United States)), Elsa Jensen(Malin Space Science Systems (United States)), Linda C. Kah(University of Tennessee at Knoxville), John M. Kennedy(Jet Propulsion Laboratory), Robert Krylo(Jet Propulsion Laboratory), Johnathan Lam(Jet Propulsion Laboratory), Mark Lindeman(Jet Propulsion Laboratory), Justin McGlown(Los Alamos National Laboratory), John Michel(Los Alamos National Laboratory), E. Miller(Jet Propulsion Laboratory), Zachary Mills(Jet Propulsion Laboratory), M. E. Minitti, Fai Mok(Jet Propulsion Laboratory), James D. Moore(Jet Propulsion Laboratory), Kenneth H. Nealson(University of Southern California), Anthony Nelson(Los Alamos National Laboratory), Raymond Newell(Los Alamos National Laboratory), Brian Nixon(Malin Space Science Systems (United States)), Daniel Nordman(Jet Propulsion Laboratory), D. L. Nuding(Johns Hopkins University Applied Physics Laboratory), Sonny Orellana(Jet Propulsion Laboratory), Michael Pauken(Jet Propulsion Laboratory), Glen Peterson(Los Alamos National Laboratory), Randy Pollock(Jet Propulsion Laboratory), Heather Quinn(Los Alamos National Laboratory), Claire Quinto(Jet Propulsion Laboratory), M. A. Ravine(Malin Space Science Systems (United States)), R. D. Reid(Photon Systems (United States)), Joe Riendeau(Jet Propulsion Laboratory), Amy Ross(Johnson Space Center), Joshua Sackos(Los Alamos National Laboratory), J. A. Schaffner(Malin Space Science Systems (United States)), Mark A. Schwochert(Jet Propulsion Laboratory), Molly O Shelton(Jet Propulsion Laboratory), Rufus Simon(Jet Propulsion Laboratory), C. L. Smith(Natural History Museum), P. Sobrón(Search for Extraterrestrial Intelligence), Kimberly Steadman(Jet Propulsion Laboratory), A. Steele(Carnegie Institution for Science), Dave Thiessen(Jet Propulsion Laboratory), Vinh D. Tran(Johnson Space Center), Tony Tsai(Jet Propulsion Laboratory), Michael Tuite(Jet Propulsion Laboratory), Eric Tung(Jet Propulsion Laboratory), Rami W. Wehbe(Jet Propulsion Laboratory), Rachel L. Weinberg(Jet Propulsion Laboratory), Ryan H. Weiner(Johnson Space Center), R. C. Wiens(Los Alamos National Laboratory), Kenneth H. Williford(Jet Propulsion Laboratory), Chris Wollonciej(Jet Propulsion Laboratory), Yen-Hung Wu(Jet Propulsion Laboratory), R. A. Yingst(Planetary Science Institute), Jason Zan(Jet Propulsion Laboratory)
Space Science Reviews
May 25, 2021
Cited by 236Open Access
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Abstract

Abstract The Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) is a robotic arm-mounted instrument on NASA’s Perseverance rover. SHERLOC has two primary boresights. The Spectroscopy boresight generates spatially resolved chemical maps using fluorescence and Raman spectroscopy coupled to microscopic images (10.1 μm/pixel). The second boresight is a Wide Angle Topographic Sensor for Operations and eNgineering (WATSON); a copy of the Mars Science Laboratory (MSL) Mars Hand Lens Imager (MAHLI) that obtains color images from microscopic scales (∼13 μm/pixel) to infinity. SHERLOC Spectroscopy focuses a 40 μs pulsed deep UV neon-copper laser (248.6 nm), to a ∼100 μm spot on a target at a working distance of ∼48 mm. Fluorescence emissions from organics, and Raman scattered photons from organics and minerals, are spectrally resolved with a single diffractive grating spectrograph with a spectral range of 250 to ∼370 nm. Because the fluorescence and Raman regions are naturally separated with deep UV excitation (<250 nm), the Raman region ∼ 800 – 4000 cm −1 (250 to 273 nm) and the fluorescence region (274 to ∼370 nm) are acquired simultaneously without time gating or additional mechanisms. SHERLOC science begins by using an Autofocus Context Imager (ACI) to obtain target focus and acquire 10.1 μm/pixel greyscale images. Chemical maps of organic and mineral signatures are acquired by the orchestration of an internal scanning mirror that moves the focused laser spot across discrete points on the target surface where spectra are captured on the spectrometer detector. ACI images and chemical maps (< 100 μm/mapping pixel) will enable the first Mars in situ view of the spatial distribution and interaction between organics, minerals, and chemicals important to the assessment of potential biogenicity (containing CHNOPS). Single robotic arm placement chemical maps can cover areas up to 7x7 mm in area and, with the < 10 min acquisition time per map, larger mosaics are possible with arm movements. This microscopic view of the organic geochemistry of a target at the Perseverance field site, when combined with the other instruments, such as Mastcam-Z, PIXL, and SuperCam, will enable unprecedented analysis of geological materials for both scientific research and determination of which samples to collect and cache for Mars sample return.


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