World's Best Scientists 2026 revealed!
Tomokatsu Morota

Tomokatsu Morota

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Earth Science 44 4644 4274 114 105 276 8864

Tomokatsu Morota publications per year

The chart shows the history of publications by Tomokatsu Morota between 2003 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Tomokatsu Morota published across 23 years, from 2003 to 2025, averaging 13.6 papers a year. Output peaked at 36 publications in 2019. 8 of the 313 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 2003 to 2025. Vertical axis: number of publications, 0 to 36. Peak 36 publications in 2019. 2003: 2 publications 2004: 3 publications 2005: 1 publication 2006: 6 publications 2007: 3 publications 2008: 20 publications 2009: 13 publications 2010: 14 publications 2011: 16 publications 2012: 13 publications 2013: 4 publications 2014: 18 publications 2015: 16 publications 2016: 22 publications 2017: 14 publications 2018: 28 publications 2019: 36 publications 2020: 21 publications 2021: 23 publications 2022: 23 publications 2023: 9 publications 2024: 5 publications 2025: 3 publications
2003 2025

313 publications in total across all disciplines

View publications per year as a table
Tomokatsu Morota: publications per year, 2003 to 2025
Year Publications
2003 2
2004 3
2005 1
2006 6
2007 3
2008 20
2009 13
2010 14
2011 16
2012 13
2013 4
2014 18
2015 16
2016 22
2017 14
2018 28
2019 36
2020 21
2021 23
2022 23
2023 9
2024 5
2025 3
Total 313
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Tomokatsu Morota 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 Tomokatsu Morota sits on this spectrum.

No. of scientists
100 200 300 400 500
Bar chart with 58 bars. Horizontal axis: publications, 38–47 to 603+. Vertical axis: number of scientists, 0 to 557. Most scientists, 557, have 128–137 publications. The last bar groups every scientist with 603 publications or more. The highlighted bar, 268–277 publications, is where this scientist sits. 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
38–47 publications 603+

This scientist: 276 publications — 83rd percentile

83% of scientists in this discipline score the same or lower.

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

View publications distribution as a table
Number of Earth Science scientists by publication count, Research.com 2026 ranking edition. Based on 9,176 ranked scientists.
Publications Scientists This scientist
38–47 5
48–57 33
58–67 94
68–77 161
78–87 278
88–97 376
98–107 404
108–117 484
118–127 540
128–137 557
138–147 491
148–157 495
158–167 458
168–177 490
178–187 414
188–197 401
198–207 333
208–217 292
218–227 290
228–237 262
238–247 243
248–257 208
258–267 185
268–277 147 276
278–287 128
288–297 119
298–307 120
308–317 107
318–327 93
328–337 87
338–347 64
348–357 87
358–367 60
368–377 60
378–387 34
388–397 50
398–407 44
408–417 31
418–427 39
428–437 27
438–447 36
448–457 27
458–467 29
468–477 30
478–487 19
488–497 15
498–507 18
508–517 19
518–527 16
528–537 10
538–547 11
548–557 14
558–567 11
568–577 7
578–587 14
588–597 5
598–602 4
603+ 100
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Tomokatsu Morota 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 Tomokatsu Morota sits on this spectrum.

No. of scientists
100 200 300
Bar chart with 77 bars. Horizontal axis: D-Index, 30 to 106+. Vertical axis: number of scientists, 0 to 389. Most scientists, 389, have 36 D-Index. The last bar groups every scientist with 106 D-Index or more. The highlighted bar, 44 D-Index, is where this scientist sits. 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: 44 D-Index — 50th percentile

50% of scientists in this discipline score the same or lower.

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

View D-Index distribution as a table
Number of Earth Science scientists by D-index, Research.com 2026 ranking edition. Based on 9,176 ranked scientists.
D-Index Scientists This scientist
30 144
31 215
32 278
33 379
34 366
35 372
36 389
37 366
38 344
39 349
40 296
41 289
42 277
43 279
44 248 44
45 257
46 212
47 202
48 207
49 204
50 183
51 178
52 182
53 178
54 163
55 117
56 163
57 120
58 113
59 136
60 135
61 96
62 103
63 83
64 103
65 83
66 89
67 92
68 89
69 78
70 75
71 53
72 62
73 54
74 35
75 52
76 50
77 32
78 37
79 20
80 33
81 36
82 34
83 34
84 24
85 19
86 18
87 26
88 30
89 17
90 21
91 19
92 15
93 14
94 20
95 9
96 10
97 15
98 13
99 3
100 13
101 3
102 9
103 4
104 6
105 6
106+ 98
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Overview

Tomokatsu Morota is affiliated with Nagoya University in Japan and specializes in fields related to physics, astronomy, earth, and planetary sciences. Their research focuses primarily on astronomy and astrophysics, with significant contributions to atmospheric science, ecology, geophysics, and aerospace engineering.

The scientist has published extensively on topics including astro and planetary science, planetary science and exploration, geology and paleoclimatology research, isotope analysis in ecology, geological and geochemical analysis, stellar, planetary, and galactic studies, as well as space science and extraterrestrial life.

Morota's recent important papers include the following:

  • "Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu," 2021, Nature Astronomy
  • "An artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regime," 2020, Science
  • "Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites," 2022, Science
  • "Sample collection from asteroid (162173) Ryugu by Hayabusa2: Implications for surface evolution," 2020, Science
  • "Soluble organic molecules in samples of the carbonaceous asteroid (162173) Ryugu," 2023, Science

Frequent co-authors in Morota's research collaborations include:

  • Seiji Sugita
  • Eri Tatsumi
  • Naoya Sakatani
  • M. Matsuoka
  • Rie Honda

Morota has published across various venues, with the most frequent being:

  • Icarus
  • Science
  • Nature Astronomy
  • Earth Planets and Space
  • Journal of Geophysical Research Planets

The scientist's work contributes notably to understanding asteroid composition, surface evolution, and the geochemical and organic characteristics of returned samples from celestial bodies such as asteroid Ryugu, reflecting a multidisciplinary approach within planetary science and exploration.

Best Publications

  • Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pile

    S. Watanabe;S. Watanabe;M. Hirabayashi;N. Hirata;Na. Hirata

  • The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes

    S. Sugita;S. Sugita;R. Honda;T. Morota;S. Kameda

  • The global distribution of pure anorthosite on the Moon

    Makiko Ohtake;Tsuneo Matsunaga;Junichi Haruyama;Yasuhiro Yokota

  • Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples

    Unknown

  • The surface composition of asteroid 162173 Ryugu from Hayabusa2 near-infrared spectroscopy

    K. Kitazato;R. E. Milliken;T. Iwata;T. Iwata;M. Abe;M. Abe

  • Global lunar-surface mapping experiment using the Lunar Imager/Spectrometer on SELENE

    Junichi Haruyama;Tsuneo Matsunaga;Makiko Ohtake;Tomokatsu Morota

  • An artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regime

    M. Arakawa;T. Saiki;K. Wada;K. Ogawa;K. Ogawa

  • Possible mantle origin of olivine around lunar impact basins detected by SELENE

    Satoru Yamamoto;Ryosuke Nakamura;Tsuneo Matsunaga;Yoshiko Ogawa

  • Possible lunar lava tube skylight observed by SELENE cameras

    Junichi Haruyama;Kazuyuki Hioki;Motomaro Shirao;Tomokatsu Morota

  • On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective

    Unknown

  • Pebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to Earth

    Unknown

  • Long-Lived Volcanism on the Lunar Farside Revealed by SELENE Terrain Camera

    Junichi Haruyama;Makiko Ohtake;Tsuneo Matsunaga;Tomokatsu Morota

  • Sample collection from asteroid (162173) Ryugu by Hayabusa2: Implications for surface evolution

    T. Morota;T. Morota;S. Sugita;S. Sugita;Y. Cho;M. Kanamaru

  • Timing and characteristics of the latest mare eruption on the Moon

    Tomokatsu Morota;Junichi Haruyama;Makiko Ohtake;Tsuneo Matsunaga

  • Performance and scientific objectives of the SELENE (KAGUYA) Multiband Imager

    Makiko Ohtake;Junichi Haruyama;Tsuneo Matsunaga;Yasuhiro Yokota

  • Massive layer of pure anorthosite on the Moon

    S. Yamamoto;R. Nakamura;T. Matsunaga;Y. Ogawa

  • Boulder size and shape distributions on asteroid Ryugu

    Tatsuhiro Michikami;Chikatoshi Honda;Hideaki Miyamoto;Masatoshi Hirabayashi

  • Highly porous nature of a primitive asteroid revealed by thermal imaging

    Tatsuaki Okada;Tatsuaki Okada;Tetsuya Fukuhara;Satoshi Tanaka;Satoshi Tanaka;Satoshi Tanaka;Makoto Taguchi

  • Discoveries on the lithology of lunar crater central peaks by SELENE Spectral Profiler

    Tsuneo Matsunaga;Makiko Ohtake;Junichi Haruyama;Yoshiko Ogawa

  • Lunar photometric properties at wavelengths 0.5–1.6 μm acquired by SELENE Spectral Profiler and their dependency on local albedo and latitudinal zones

    Yasuhiro Yokota;Tsuneo Matsunaga;Makiko Ohtake;Junichi Haruyama

  • Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites

    R. Jaumann;R. Jaumann;N. Schmitz;T.-M. Ho;S. E. Schröder

  • Asymmetric crustal growth on the Moon indicated by primitive farside highland materials

    Makiko Ohtake;Hiroshi Takeda;Tsuneo Matsunaga;Yasuhiro Yokota

  • Lack of Exposed Ice Inside Lunar South Pole Shackleton Crater

    Junichi Haruyama;Makiko Ohtake;Tsuneo Matsunaga;Tomokatsu Morota

Frequent Co-Authors

Naru Hirata
Naru Hirata University of Aizu
Junichi Haruyama
Junichi Haruyama Japan Aerospace Exploration Agency
Tsuneo Matsunaga
Tsuneo Matsunaga National Institute for Environmental Studies
Yoshiaki Ishihara
Yoshiaki Ishihara Japan Aerospace Exploration Agency
Hideaki Miyamoto
Hideaki Miyamoto University of Tokyo
Takahiro Hiroi
Takahiro Hiroi Brown University
Tomoki Nakamura
Tomoki Nakamura Tohoku University
Sho Sasaki
Sho Sasaki Osaka University
Olivier S. Barnouin
Olivier S. Barnouin Johns Hopkins University Applied Physics Laboratory
Goro Komatsu
Goro Komatsu International Research School of Planetary Sciences

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