| Title: |
The SuperCam Instrument onboard Perseverance: Overview of efforts compiled for Mars X conference |
| Authors: |
Cousin, Agnès; Wiens, Roger, C.; Clegg, Samuel; Gasnault, Olivier; Anderson, Ryan B.; Bernard, Sylvain; Beck, Pierre; Beyssac, Olivier; Broz, Adrian; Caravaca, Gwénaël; Chide, Baptiste; Clavé, Elise; Coloma, Leire; Comellas, Jade; Connell, Stephanie; Dehouck, Erwin; Forni, Olivier; Gillier, Martin; Johnson, Jeffrey; Kalucha, Hemani; Loche, Matteo; Madariaga, Juan, Manuel; Manelski, Henry; Mangold, Nicolas; Bouyssou Mann, Magali; García-Manrique, Juan Antonio; Maurice, Sylvestre; Mcconnochie, Timothy H.; Newell, R., T.; Ollila, Ann; Poblacion, Iratxe; Pilleri, Paolo; Poulet, François; Quantin-Nataf, Cathy; Robinson, Scott; Royer, Clément; Schröder, Susanne; Udry, Arya; Wolf, U; Zastrow, Allison; Team, The Supercam |
| Contributors: |
Institut de recherche en astrophysique et planétologie (IRAP); Université Toulouse III - Paul Sabatier (UT3); Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Department of Earth, Atmospheric, and Planetary Sciences West Lafayette (EAPS); Purdue University West Lafayette; Los Alamos National Laboratory (LANL); US Geological Survey Flagstaff (USGS); United States Geological Survey Reston (USGS); Research On Carbon-rich Key Samples IMPMC (IMPMC_ROCKS); Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC); Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement IRD : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement IRD : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); Institut de Planétologie et d'Astrophysique de Grenoble (IPAG); Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (Fédération OSUG)-Université Grenoble Alpes (UGA); Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement IRD : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); DLR Institute of Optical Sensor Systems (IOSS); Deutsches Zentrum für Luft- und Raumfahrt Berlin (DLR); Department of Analytical Chemistry Leioa; Universidad del País Vasco Espainia / Euskal Herriko Unibertsitatea España = University of the Basque Country Spain = Université du pays basque Espagne (UPV / EHU); University of Hawaii; Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE); École normale supérieure de Lyon (ENS de Lyon); Université de Lyon-Université de Lyon-Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS); Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO); Johns Hopkins University Applied Physics Laboratory Laurel, MD (APL); California Institute of Technology (CALTECH); Laboratoire de Planétologie et Géosciences UMR_C 6112 (LPG); Le Mans Université (UM)-Université d'Angers (UA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST); Nantes Université - pôle Sciences et technologie; Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie; Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ); Centre National d'Études Spatiales Toulouse (CNES); Universidad de Valladolid Valladolid (UVa); Space Science Institute Boulder (SSI); University of Maryland College Park (UMD); University System of Maryland; Institut d'astrophysique spatiale (IAS); Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES); PLANETO - LATMOS; Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS); Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); DLR Institut für Optische Sensorsyteme; University of Nevada Las Vegas (WGU Nevada); Lunar and Planetary Institute |
| Source: |
Tenth International Conference on Mars 2024 ; https://hal.science/hal-04650220 ; Tenth International Conference on Mars 2024, Lunar and Planetary Institute, Jul 2024, Pasadena (California), United States. LPI Contrib. No. 3007. 3169.pdf ; https://www.hou.usra.edu/meetings/tenthmars2024/ |
| Publisher Information: |
CCSD |
| Publication Year: |
2024 |
| Collection: |
Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ |
| Subject Terms: |
SuperCam; Mars; Mars2020; Perseverance; Jezero crater; [SDU]Sciences of the Universe [physics]; [SDU.STU]Sciences of the Universe [physics]/Earth Sciences; [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology; [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy |
| Subject Geographic: |
United States |
| Time: |
Pasadena (California), United States |
| Description: |
International audience ; The Perseverance rover landed at Jezero crater on February 18th, 2021. The choice of this landing site for the Mars2020 mission was motivated by its geological significance and the potential insights into Mars’ past habitability and search for past life. Indeed, Jezero crater once contained a lake, with a very well preserved delta on the west, making it an ideal location to search for signs of ancient microbial life. The Perseverance rover has four main objectives: 1. Search for traces of past microbial life 2. Characterize Mars’s climate and geology in the landing site 3. Collect samples for later return to Earth 4.Test technologies for future missions. Perseverance is equipped with seven scientific instruments, including the SuperCam suite [1,2]. SuperCam combines several remote-sensing techniques in order tostudy both the Martian surface and its atmosphere: 1. the LIBS (Laser-Induced Breakdown Spectroscopy) technique gives access to the chemical composition of the targets (up to 15m). All major elements are quantified (Si, Ti, Al, Fe, Mg, Ca, Na, K [3]) and the quantification of some minor elements is under progress [4]; 2. The Raman spectroscopy enables the identification of major mineral phases via the use of a 532nm pulsed laser, for Raman shifts between 150 and >4000cm-1; 3. The VISIR spectroscopy gives access to the mineralogy, via the reflection of sunlight to access the frequency of molecule bond vibrations of the targets. The VIS range covers the 379-464nm and 535-855nm range, and the IRS part is comprised in the 1.3-2.6 microns range using an Acousto-Optic Tunable Filter spectrometer [5]; 4. The Remote Micro Imager (RMI) uses a CMOS camera of 2048x2048 pixels, with an angular size of 10 microradians and a resolution of 50 microradians; 5. The microphone records air pressure fluctuations from 20 Hz to 12.5 or 50 KHz, at sampling rates of 25 or 100 KHz, respectively. |
| Document Type: |
conference object |
| Language: |
English |
| Relation: |
BIBCODE: 2024LPICo3007.3169C |
| Availability: |
https://hal.science/hal-04650220; https://hal.science/hal-04650220v1/document; https://hal.science/hal-04650220v1/file/3169.pdf |
| Rights: |
https://about.hal.science/hal-authorisation-v1/ ; info:eu-repo/semantics/OpenAccess |
| Accession Number: |
edsbas.7746DD63 |
| Database: |
BASE |