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Geological, Multispectral, and Meteorological Imaging Results from the Mars 2020 Perseverance Rover in Jezero Crater

Authors :
James F. Bell, III
Justin N. Maki
Sanna Alwmark
Bethany L. Ehlmann
Sarah A. Fagents
John P. Grotzinger
Sanjeev Gupta
Alexander Hayes
Ken E. Herkenhoff
Briony H. N. Horgan
Jeffrey R. Johnson
Kjartan B. Kinch
Mark T. Lemmon
Morten B. Madsen
Jorge I. Núñez
Gerhard Paar
Melissa Rice
James W. Rice, Jr
Nicole Schmitz
Robert Sullivan
Alicia Vaughan
Mike J. Wolff
Andreas Bechtold
Tanja Bosak
Louise E. Duflot
Alberto G. Fairén
Brad Garczynski
Ralf Jaumann
Marco Merusi
Chase Million
Eleni Ravanis
David L. Shuster
Justin Simon
Michael St. Clair
Christian Tate
Sebastian Walter
Benjamin Weiss
Alyssa M. Bailey
Tanguy Bertrand
Olivier Beyssac
Adrian J. Brown
Piluca Caballo-Perucha
Michael A. Caplinger
Christy M. Caudill
Francesca Cary
Ernest Cisneros
Edward Cloutis
Nathan Cluff
Paul Corlies
Kelsie Crawford
Sabrina Curtis
Robert Deen
Darian Dixon
Christopher Donaldson
Megan Barrington
Michelle Ficht
Stephanie Fleron
Michael Hansen
David Harker
Rachel Howson
Joshua Huggett
Samantha Jacob
Elsa Jensen
Ole B Jensen
Mohini Jodhpurkar
Jonathan Joseph
Christian Juarez
Linda C Kah
Oak Kanine
Jessica Kristensen
Tex Kubacki
Kristiana Lapo
Angela Magee
Michael Maimone
Greg L Mehall
Laura Mehall
Jess Mollerup
Daniel Viúdez-Moreiras
Kristen Paris
Kathryn E Powell
Frank Preusker
Jon Proton
Corrine Rojas
Danny Sallurday
Kim Saxton
Eva Scheller
Christina H Seeger
Mason Starr
Nathan Stein
Nathalie Turenne
Jason Van Beek
Andrew G Winhold
Rachel Yingling
Source :
Science Advances. 8(47)
Publication Year :
2022
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2022.

Abstract

Perseverance’s Mastcam-Z instrument provides high-resolution stereo and multispectral images with a unique combination of spatial resolution, spatial coverage, and wavelength coverage along the rover’s traverse in Jezero crater, Mars. Images reveal rocks consistent with an igneous (including volcanic and/or volcaniclastic) and/or impactite origin and limited aqueous alteration, including polygonally fractured rocks with weathered coatings; massive boulder-forming bedrock consisting of mafic silicates, ferric oxides, and/or iron-bearing alteration minerals; and coarsely layered outcrops dominated by olivine. Pyroxene dominates the iron-bearing mineralogy in the fine-grained regolith, while olivine dominates the coarse-grained regolith. Solar and atmospheric imaging observations show significant intra- and intersol variations in dust optical depth and water ice clouds, as well as unique examples of boundary layer vortex action from both natural (dust devil) and Ingenuity helicopter–induced dust lifting. High-resolution stereo imaging also provides geologic context for rover operations, other instrument observations, and sample selection, characterization, and confirmation.

Details

Language :
English
ISSN :
23752548
Volume :
8
Issue :
47
Database :
NASA Technical Reports
Journal :
Science Advances
Notes :
Mars Exploration Program, , 203959, , 1511125, , 2017-06388, , 19PACOI04, , RGPIN-2021-02995, , RGPIN-2015-04582, , PEA 4000117520, , CF19-0023, , 801199, , 818602
Publication Type :
Report
Accession number :
edsnas.20230016428
Document Type :
Report
Full Text :
https://doi.org/10.1126/sciadv.abo4856