S
S. W. Squyres
Researcher at Cornell University
Publications - 210
Citations - 10570
S. W. Squyres is an academic researcher from Cornell University. The author has contributed to research in topics: Mars Exploration Program & Meridiani Planum. The author has an hindex of 48, co-authored 210 publications receiving 9646 citations. Previous affiliations of S. W. Squyres include California Institute of Technology.
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Journal ArticleDOI
Distribution of Hydrogen in the Near-Surface of Mars: Evidence for Subsurface Ice Deposits
William V. Boynton,W. C. Feldman,S. W. Squyres,Thomas H. Prettyman,J. Brückner,Larry G. Evans,R. C. Reedy,R. C. Reedy,R. D. Starr,James R. Arnold,D. M. Drake,P. Englert,Albert E. Metzger,I. G. Mitrofanov,Jacob I. Trombka,Claude d’Uston,Heinrich Wänke,Olivier Gasnault,D. K. Hamara,Daniel M. Janes,Robert L. Marcialis,Sylvestre Maurice,I. Mikheeva,G. J. Taylor,R. L. Tokar,C. Shinohara +25 more
TL;DR: The Gamma-Ray Spectrometer on the Mars Odyssey has identified two regions near the poles that are enriched in hydrogen, and it is suggested that the host of the hydrogen in the subsurface layer is ice, which constitutes 35 ± 15% of the layer by weight.
Supporting Online Material for Cassini Observes the Active South Pole of Enceladus
C. C. Porco,P. Helfenstein,P. C. Thomas,Andrew P. Ingersoll,J. Wisdom,R. West,Gerhard Neukum,Tilmann Denk,R. Wagner,T. Roatsch,S. Kieffer,Elizabeth P. Turtle,A. McEwen,T. V. Johnson,Julie A. Rathbun,J. Veverka,Daren Wilson,Jason Perry,J. Spitale,André Brahic,J. Burns,A. D. DelGenio,Luke Dones,C. D. Murray,S. W. Squyres +24 more
TL;DR: The shape of Enceladus suggests a possible intense heating epoch in the past by capture into a 1:4 secondary spin/orbit resonance.
Journal ArticleDOI
A habitable fluvio-lacustrine environment at Yellowknife Bay, Gale crater, Mars.
John P. Grotzinger,Dawn Y. Sumner,Linda C. Kah,K. M. Stack,Sanjeev Gupta,Lauren A. Edgar,David M. Rubin,Kevin W. Lewis,Juergen Schieber,Nicolas Mangold,Ralph E. Milliken,Pamela G. Conrad,David J. DesMarais,Jack D. Farmer,Kirsten L. Siebach,Fred Calef,Joel A. Hurowitz,Scott M. McLennan,Douglas W. Ming,David T. Vaniman,Joy A. Crisp,Ashwin R. Vasavada,Kenneth S. Edgett,Michael C. Malin,David F. Blake,Ralf Gellert,Paul R. Mahaffy,Roger C. Wiens,Sylvestre Maurice,John A. Grant,Sharon A. Wilson,Robert C. Anderson,Luther W. Beegle,Raymond E. Arvidson,Bernard Hallet,R. S. Sletten,Melissa S. Rice,James F. Bell,J. L. Griffes,Bethany L. Ehlmann,Ryan B. Anderson,Thomas F. Bristow,William E. Dietrich,Gilles Dromart,Jennifer L. Eigenbrode,Abigail A. Fraeman,Craig Hardgrove,K. E. Herkenhoff,Louise Jandura,Gary Kocurek,Seungwon Lee,Laurie A. Leshin,Richard Leveille,Daniel Limonadi,Justin N. Maki,Scott McCloskey,M. A. Meyer,Michelle E. Minitti,Horton E. Newsom,Dorothy Z. Oehler,Avi Okon,Marisa C. Palucis,T. J. Parker,Scott K. Rowland,Mariek E. Schmidt,S. W. Squyres,Andrew Steele,Edward M. Stolper,Roger E. Summons,Allan H. Treiman,Rebecca M. E. Williams,A. Yingst +71 more
TL;DR: The Curiosity rover discovered fine-grained sedimentary rocks, which are inferred to represent an ancient lake and preserve evidence of an environment that would have been suited to support a martian biosphere founded on chemolithoautotrophy.
Journal ArticleDOI
Cassini imaging of Jupiter's atmosphere, satellites, and rings.
Carolyn Porco,Robert A. West,Alfred S. McEwen,Anthony D. Del Genio,Andrew P. Ingersoll,Peter C. Thomas,S. W. Squyres,Luke Dones,Carl D. Murray,Torrence V. Johnson,Joseph A. Burns,André Brahic,Gerhard Neukum,Joseph Veverka,J. Barbara,Tilmann Denk,Michael W. Evans,Joseph Ferrier,Paul Geissler,Paul Helfenstein,Thomas Roatsch,Henry B. Throop,Matthew S. Tiscareno,Ashwin R. Vasavada +23 more
TL;DR: Findings on Jupiter's zonal winds, convective storms, low-latitude upper troposphere, polar stratosphere, and northern aurora are reported, including previously unseen emissions arising from Io and Europa in eclipse, and a giant volcanic plume over Io's north pole are described.
Journal ArticleDOI
Volatile, Isotope, and Organic Analysis of Martian Fines with the Mars Curiosity Rover
Laurie A. Leshin,Paul R. Mahaffy,Christopher R. Webster,Michel Cabane,Patrice Coll,Pamela G. Conrad,P. D. Archer,S. K. Atreya,A. E. Brunner,A. E. Brunner,Arnaud Buch,Jennifer L. Eigenbrode,G. Flesch,Heather B. Franz,Heather B. Franz,Caroline Freissinet,Daniel P. Glavin,Amy McAdam,Kristen E. Miller,Douglas W. Ming,Richard V. Morris,Rafael Navarro-González,Paul B. Niles,T. C. Owen,Robert O. Pepin,S. W. Squyres,Andrew Steele,Jennifer C. Stern,Roger E. Summons,Dawn Y. Sumner,B. Sutter,Cyril Szopa,Samuel Teinturier,Melissa G. Trainer,James J. Wray,John P. Grotzinger +35 more
TL;DR: Samples from the Rocknest aeolian deposit were heated to ~835°C under helium flow and evolved gases analyzed by Curiosity's Sample Analysis at Mars instrument suite, suggesting that oxygen is produced from thermal decomposition of an oxychloride compound.