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Earth Science
USA
2026

D-Index & Metrics

Earth Science

D-Index
112
Citations
39005
World Ranking
63
National Ranking
27

Harry Y. McSween publication distribution in Earth Science in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Earth Science in 2026. The highlighted bar marks where Harry Y. McSween sits on this spectrum.

38–47 publications: 5 scientists 48–57 publications: 33 scientists 58–67 publications: 94 scientists 68–77 publications: 161 scientists 78–87 publications: 278 scientists 88–97 publications: 376 scientists 98–107 publications: 404 scientists 108–117 publications: 484 scientists 118–127 publications: 540 scientists 128–137 publications: 557 scientists 138–147 publications: 491 scientists 148–157 publications: 495 scientists 158–167 publications: 458 scientists 168–177 publications: 490 scientists 178–187 publications: 414 scientists 188–197 publications: 401 scientists 198–207 publications: 333 scientists 208–217 publications: 292 scientists 218–227 publications: 290 scientists 228–237 publications: 262 scientists 238–247 publications: 243 scientists 248–257 publications: 208 scientists 258–267 publications: 185 scientists 268–277 publications: 147 scientists 278–287 publications: 128 scientists 288–297 publications: 119 scientists 298–307 publications: 120 scientists 308–317 publications: 107 scientists 318–327 publications: 93 scientists 328–337 publications: 87 scientists 338–347 publications: 64 scientists 348–357 publications: 87 scientists 358–367 publications: 60 scientists 368–377 publications: 60 scientists 378–387 publications: 34 scientists 388–397 publications: 50 scientists 398–407 publications: 44 scientists 408–417 publications: 31 scientists 418–427 publications: 39 scientists 428–437 publications: 27 scientists 438–447 publications: 36 scientists 448–457 publications: 27 scientists 458–467 publications: 29 scientists 468–477 publications: 30 scientists 478–487 publications: 19 scientists 488–497 publications: 15 scientists 498–507 publications: 18 scientists 508–517 publications: 19 scientists 518–527 publications: 16 scientists 528–537 publications: 10 scientists 538–547 publications: 11 scientists 548–557 publications: 14 scientists 558–567 publications: 11 scientists 568–577 publications: 7 scientists 578–587 publications: 14 scientists 588–597 publications: 5 scientists 598–602 publications: 4 scientists 603+ publications: 100 scientists
38 publications 603+

This scientist: 623 publications — 99th percentile

99% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 603 publications or more.

Harry Y. McSween D-index placement in Earth Science in 2026

The chart shows the D-index (discipline H-index) distribution of Earth Science scientists ranked by Research.com in 2026. The highlighted bar marks where Harry Y. McSween sits on this spectrum.

30 D-Index: 144 scientists 31 D-Index: 215 scientists 32 D-Index: 278 scientists 33 D-Index: 379 scientists 34 D-Index: 366 scientists 35 D-Index: 372 scientists 36 D-Index: 389 scientists 37 D-Index: 366 scientists 38 D-Index: 344 scientists 39 D-Index: 349 scientists 40 D-Index: 296 scientists 41 D-Index: 289 scientists 42 D-Index: 277 scientists 43 D-Index: 279 scientists 44 D-Index: 248 scientists 45 D-Index: 257 scientists 46 D-Index: 212 scientists 47 D-Index: 202 scientists 48 D-Index: 207 scientists 49 D-Index: 204 scientists 50 D-Index: 183 scientists 51 D-Index: 178 scientists 52 D-Index: 182 scientists 53 D-Index: 178 scientists 54 D-Index: 163 scientists 55 D-Index: 117 scientists 56 D-Index: 163 scientists 57 D-Index: 120 scientists 58 D-Index: 113 scientists 59 D-Index: 136 scientists 60 D-Index: 135 scientists 61 D-Index: 96 scientists 62 D-Index: 103 scientists 63 D-Index: 83 scientists 64 D-Index: 103 scientists 65 D-Index: 83 scientists 66 D-Index: 89 scientists 67 D-Index: 92 scientists 68 D-Index: 89 scientists 69 D-Index: 78 scientists 70 D-Index: 75 scientists 71 D-Index: 53 scientists 72 D-Index: 62 scientists 73 D-Index: 54 scientists 74 D-Index: 35 scientists 75 D-Index: 52 scientists 76 D-Index: 50 scientists 77 D-Index: 32 scientists 78 D-Index: 37 scientists 79 D-Index: 20 scientists 80 D-Index: 33 scientists 81 D-Index: 36 scientists 82 D-Index: 34 scientists 83 D-Index: 34 scientists 84 D-Index: 24 scientists 85 D-Index: 19 scientists 86 D-Index: 18 scientists 87 D-Index: 26 scientists 88 D-Index: 30 scientists 89 D-Index: 17 scientists 90 D-Index: 21 scientists 91 D-Index: 19 scientists 92 D-Index: 15 scientists 93 D-Index: 14 scientists 94 D-Index: 20 scientists 95 D-Index: 9 scientists 96 D-Index: 10 scientists 97 D-Index: 15 scientists 98 D-Index: 13 scientists 99 D-Index: 3 scientists 100 D-Index: 13 scientists 101 D-Index: 3 scientists 102 D-Index: 9 scientists 103 D-Index: 4 scientists 104 D-Index: 6 scientists 105 D-Index: 6 scientists 106+ D-Index: 98 scientists
30 D-Index 106+

This scientist: 112 D-Index — 99th percentile

99% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 106 D-Index or more.

Research.com Recognitions

  • 2026 - Research.com Earth Science in United States Leader Award
  • 2025 - Research.com Earth Science in United States Leader Award
  • 2008 - Fellow of the American Association for the Advancement of Science (AAAS)
  • 2006 - Fellow of American Geophysical Union (AGU)
  • 2002 - Fellow of the American Academy of Arts and Sciences

Overview

Harry Y. McSween is affiliated with the University of Tennessee at Knoxville in the United States. Their research primarily spans the fields of Physics and Astronomy, with a strong focus on Astronomy and Astrophysics, Nuclear and High Energy Physics, Atmospheric Science, Geophysics, and Ecology.

Their scholarly work concentrates on topics including Astro and Planetary Science, Planetary Science and Exploration, Stellar, planetary, and galactic studies, Geology and Paleoclimatology Research, Astronomical and nuclear sciences, Space Science and Extraterrestrial Life, and Isotope Analysis in Ecology.

McSween has published extensively in the following venues:

  • Abstracts with programs - Geological Society of America
  • Meteoritics and Planetary Science
  • Proceedings of the National Academy of Sciences
  • Journal of Geophysical Research Planets
  • Geochimica et Cosmochimica Acta

Frequent co-authors collaborating with McSween include:

  • G. R. Huss
  • Nick Dygert
  • J. E. Moersch
  • Jialong Ren
  • Marc A. Hesse

Recent publications by McSween include:

  • "Perspectives on Mars Sample Return: A critical resource for planetary science and exploration," 2025, Proceedings of the National Academy of Sciences
  • "On the Diversity and Formation Modes of Martian Minerals," 2023, Journal of Geophysical Research Planets
  • "Extensive and ancient feldspathic crust detected across north Hellas rim, Mars: Possible implications for primary crust formation," 2022, Geology
  • "Thermochemical evolution of the acapulcoite-lodranite parent body: Evidence for fragmentation-disrupted partial differentiation," 2022, Meteoritics and Planetary Science
  • "Evidence for early fragmentation-reassembly of ordinary chondrite (H, L, and LL) parent bodies from REE-in-two-pyroxene thermometry," 2020, Geochimica et Cosmochimica Acta

McSween has received recognition through several fellowships, including:

  • Fellow of the American Association for the Advancement of Science (AAAS), 2008
  • Fellow of American Geophysical Union (AGU), 2006
  • Fellow of the American Academy of Arts and Sciences, 2002

Best Publications

  • In situ evidence for an ancient aqueous environment at Meridiani Planum, Mars.

    Steven W. Squyres;John P. Grotzinger;Raymond E. Arvidson;James F. Bell

  • The Thermal Emission Imaging System (THEMIS) for the Mars 2001 Odyssey mission

    Philip R. Christensen;Bruce M. Jakosky;Hugh H. Kieffer;Michael C. Malin

  • Meteorites and the early solar system II

    Dante S. Lauretta;Harry Y. McSween

  • What we have learned about Mars from SNC meteorites

    Harry Y. Mcsween

  • Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills

    R. E. Arvidson;S. W. Squyres;R. C. Anderson;J. F. Bell

  • The chemical composition of Martian soil and rocks returned by the mobile alpha proton x-ray spectrometer : Preliminary results from the x-ray mode

    R. Rieder;T. Economou;H. Wänke;A. Turkevich

  • The Opportunity Rover's Athena science investigation at Meridiani Planum, Mars.

    S. W. Squyres;R. E. Arvidson;J.F. Bell;J. Brückner

  • Provenance and diagenesis of the evaporite-bearing Burns formation, Meridiani Planum, Mars

    S.M. McLennan;J.F. Bell;W. M. Calvin;P. R. Christensen

  • Dawn at Vesta: Testing the Protoplanetary Paradigm

    C. T. Russell;C. A. Raymond;A. Coradini;H. Y. McSween

  • Elemental Composition of the Martian Crust

    Harry Y. McSween;G. Jeffrey Taylor;Michael B. Wyatt

  • The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars

    Steven W. Squyres;Raymond E. Arvidson;James F. Bell;J. Bruckner

  • SNC meteorites: Clues to Martian petrologic evolution?

    Harry Y. McSween

  • Mineralogy at Meridiani Planum from the Mini-TES Experiment on the Opportunity Rover.

    Philip Christensen;M. B. Wyatt;T. D. Glotch;A. D. Rogers

  • Petrology and origin of the shergottite meteorites

    Edward Stolper;Harry Y. McSween

  • An integrated view of the chemistry and mineralogy of martian soils

    Albert S. Yen;Ralf Gellert;Christian Schröder;Richard V. Morris

  • Chemistry and mineralogy of outcrops at Meridiani Planum

    Benton C. Clark;R. V. Morris;S. M. McLennan;R. Gellert

  • Morphology and Composition of the Surface of Mars: Mars Odyssey THEMIS Results

    Philip R. Christensen;Joshua L. Bandfield;James F. Bell;Noel Gorelick

  • Correlated alteration effects in CM carbonaceous chondrites

    Lauren B. Browning;Lauren B. Browning;Harry Y. McSween;Michael E. Zolensky

  • Are carbonaceous chondrites primitive or processed? A review

    Harry Y. McSween

  • Alteration in CM carbonaceous chondrites inferred from modal and chemical variations in matrix

    Harry Y. McSween

Frequent Co-Authors

Ralf Jaumann
Ralf Jaumann Freie Universität Berlin
Thomas H. Prettyman
Thomas H. Prettyman Planetary Science Institute
M. C. De Sanctis
M. C. De Sanctis National Institute for Astrophysics
Christopher T. Russell
Christopher T. Russell University of California, Los Angeles
Andreas Nathues
Andreas Nathues Max Planck Society
Michael J. Toplis
Michael J. Toplis Paul Sabatier University
Federico Tosi
Federico Tosi National Institute for Astrophysics
Scott M. McLennan
Scott M. McLennan Stony Brook University
Carle M. Pieters
Carle M. Pieters Brown University
Philip R. Christensen
Philip R. Christensen Arizona State University

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