The DOI matches its Crossref record; 38 of the 38 references it cites were found in a registry or an index.
Water contents of Earth-mass planets around M dwarfs
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“Particularly, Tian & Ida (2015) argued that Earth-mass planets with Earth-like water contents orbiting M-dwarfs have a 10-100 times reduced likelihood than around G dwarfs.”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida (2015)
In the citing paper
“It has also been pointed out that accreting planets, if formed, subsequently located in the CLI-HZ around stars cooler than K5 (including the full range of M-dwarfs) are most likely subjected to runaway greenhouse processes”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida 2015
In the citing paper
“and thus may lose substantial amounts of water initially delivered to them (Ramirez & Kaltenegger 2014; Luger & Barnes 2015; Tian & Ida 2015), thus emerging as (almost certainly) uninhabitable dry planets ('desert worlds').”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida 2015
Citations
Cites
MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA)
Paxton, B., Bildsten, L., Dotter, A., Herwig, F., Lesaffre, P., & Timmes, F. X. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/1/3 · Cited by 4,317
Modules for Experiments in Stellar Astrophysics (MESA)Preprint
Paxton, B. (2026) · doi:10.5281/zenodo.19685576 · Cited by 1,839
Hayashi, C. (1981) · Progress of Theoretical Physics Supplement · doi:10.1143/ptps.70.35 · Cited by 1,810
PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER
Howard, A. W., Marcy, G. W., Bryson, S. T., Jenkins, J. M., Rowe, J. F., Batalha, N. M., Borucki, W. J., Koch, D. G., Dunham, E. W., Gautier, T. N., et al. (2012) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/201/2/15 · Cited by 1,151
Tanaka, H., Takeuchi, T., & Ward, W. R. (2002) · The Astrophysical Journal · doi:10.1086/324713 · Cited by 1,041
Ribas, I., Guinan, E. F., Güdel, M., & Audard, M. (2005) · The Astrophysical Journal · doi:10.1086/427977 · Cited by 871
THE OCCURRENCE RATE OF SMALL PLANETS AROUND SMALL STARS
Dressing, C. D., & Charbonneau, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/95 · Cited by 749
HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: DEPENDENCE ON PLANETARY MASS
Kopparapu, R., Ramirez, R. M., Schottelkotte, J. C., Kasting, J. F., Domagal-Goldman, S. D., & Eymet, V. (2014) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/787/2/l29 · Cited by 659
Lopez, E. D., & Fortney, J. J. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/776/1/2 · Cited by 592
Energy exchange and water budget partitioning in a boreal minerogenic mire
Peichl, M., Sagerfors, J., Lindroth, A., Buffam, I. D., Grelle, A., Klemedtsson, L., Laudon, H., & Nilsson, M. B. (2012) · Journal of Geophysical Research Biogeosciences · doi:10.1029/2012jg002073 · Cited by 570
A torque formula for non-isothermal Type I planetary migration - II. Effects of diffusion
Paardekooper, S.-J., Baruteau, C., & Kley, W. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17442.x · Cited by 546
Planetary evaporation by UV and X-ray radiation: basic hydrodynamics
Owen, J. E., & Jackson, A. P. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21481.x · Cited by 438
Emergence of two types of terrestrial planet on solidification of magma ocean
Hamano, K., Abe, Y., & Genda, H. (2013) · Nature · doi:10.1038/nature12163 · Cited by 402
M Stars as Targets for Terrestrial Exoplanet Searches And Biosignature Detection
Scalo, J., Kaltenegger, L., Segura, A., Fridlund, M. C., Ribas, I., Kulikov, Y. N., Grenfell, J. L., Rauer, H., Odert, P., Leitzinger, M., et al. (2007) · Astrobiology · doi:10.1089/ast.2006.0125 · Cited by 397
Thermal evolution of an early magma ocean in interaction with the atmosphere
Lebrun, T., Massol, H., Chassefière, É., Davaille, A., Marcq, E., Sarda, P., Leblanc, F., & Brandeis, G. (2013) · Journal of Geophysical Research Planets · doi:10.1002/jgre.20068 · Cited by 288
The Pisa pre-main sequence tracks and isochrones
Tognelli, E., Moroni, P. G. P., & Degl’Innocenti, S. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913913 · Cited by 284
Ida, S., & Lin, D. N. C. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/1/810 · Cited by 231
Self-citationTOWARD A DETERMINISTIC MODEL OF PLANETARY FORMATION. VII. ECCENTRICITY DISTRIBUTION OF GAS GIANTS
Ida, S., Lin, D. N. C., & Nagasawa, M. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/775/1/42 · Cited by 207
Self-citationTognelli, E., Moroni, P. G. P., & Degl’Innocenti, S. (2011) · arXiv (Cornell University) · doi:10.48550/arxiv.1107.2318 · Cited by 165
Abbot, D. S., Cowan, N. B., & Ciesla, F. J. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/756/2/178 · Cited by 151
Observed Properties of Extrasolar Planets
Howard, A. (2013) · Science · doi:10.1126/science.1233545 · Cited by 144
Stellar Evolution in Early Phases of Gravitational Contraction
Hayashi, C. (1961) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/13.4.450 · Cited by 121
The escape of heavy atoms from the ionosphere of HD209458b. II. Interpretation of the observations
Koskinen, T., Yelle, R. V., Harris, M. J., & Lavvas, P. (2012) · Icarus · doi:10.1016/j.icarus.2012.09.026 · Cited by 99
The Upper Mesosphere and Lower Thermosphere: A Review of Experiment and Theory
Johnson, R. M., & Killeen, T. L. (1995) · Geophysical monograph · doi:10.1029/gm087 · Cited by 99
Atmospheric composition, chemistry, and clouds
Mills, F. P., Esposito, L. W., & Yung, Y. L. (2007) · Geophysical monograph · doi:10.1029/176gm06 · Cited by 95
THE IMPORTANCE OF DISK STRUCTURE IN STALLING TYPE I MIGRATION
Kretke, K. A., & Lin, D. N. C. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/755/1/74 · Cited by 91
WATER CYCLING BETWEEN OCEAN AND MANTLE: SUPER-EARTHS NEED NOT BE WATERWORLDS
Cowan, N. B., & Abbot, D. S. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/781/1/27 · Cited by 85
The upper mesosphere and lower thermosphere: A review of experiment and theory
RYCROFT, M. J. (1996) · Journal of Atmospheric and Terrestrial Physics · doi:10.1016/0021-9169(96)80446-6 · Cited by 72
Heating efficiencies in the thermosphere of venus reconsidered
Fox, J. L. (1988) · Planetary and Space Science · doi:10.1016/0032-0633(88)90144-4 · Cited by 64
Exploring Venus as a Terrestrial Planet
Esposito, L. W., STOFAN, E. R., & Cravens, T. E. (2007) · Geophysical monograph · doi:10.1029/gm176 · Cited by 61
ULTRAVIOLET OBSERVATIONS OF SUPER-CHANDRASEKHAR MASS TYPE Ia SUPERNOVA CANDIDATES WITHSWIFTUVOT
Brown, P. J., Kuin, N. P. M., Scalzo, R. A., Smitka, M. T., de Pasquale, M., Holland, S. T., Krisciunas, K., Milne, P., & Wang, L. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/787/1/29 · Cited by 59
Dohm, J. M., & Maruyama, S. (2014) · Geoscience Frontiers · doi:10.1016/j.gsf.2014.01.005 · Cited by 50
Impact of photo-evaporative mass loss on masses and radii of water-rich sub/super-Earths
Kurosaki, K., Ikoma, M., & Hori, Y. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201322258 · Cited by 27
Impact of photo-evaporative mass loss on masses and radii of water-rich sub/super-Earths
Kurosaki, K., Ikoma, M., & Hori, Y. (2014) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201322258/pdf · Cited by 27
NUMERICAL SIMULATIONS OF MULTIPLE SCATTERING OF THEf-MODE BY FLUX TUBES
Felipe, T., Crouch, A. D., & Birch, A. C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/775/1/74 · Cited by 18
Updated Pre-Main Sequence tracks at low metallicities for 0.1 ≤ M/M⊙ ≤ 1.5 ⋆Preprint
Criscienzo, M. D., & Ventura, P. (2012) · Cited by 13
Updated pre-main sequence tracks at low metallicities for 0.1 $\mathsf \le\ M/M _\odot\ \le 1.5$
Criscienzo, M. D., Ventura, P., & D'Antona, F. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200811174 · Cited by 12
Warm planets orbiting cool stars
Johnson, J. A. (2014) · Physics Today · doi:10.1063/pt.3.2309 · Cited by 7
Cited by
Sorted by citations
Temperate Earth-sized planets transiting a nearby ultracool dwarf star
Gillon, M., Jehin, E., Lederer, S. M., Delrez, L., de Wit, J., Burdanov, A., Grootel, V. V., Burgasser, A. J., Triaud, A. H. M. J., Opitom, C., et al. (2016) · Nature · doi:10.1038/nature17448 · Cited by 620
THE MUSCLES TREASURY SURVEY. I. MOTIVATION AND OVERVIEW*
France, K., Loyd, R. O. P., Youngblood, A., Brown, A., Schneider, P. C., Hawley, S. L., Froning, C. S., Linsky, J. L., Roberge, A., Buccino, A. P., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/820/2/89 · Cited by 430
Self-citationImpact of space weather on climate and habitability of terrestrial-type exoplanets
Airapetian, V. S., Barnes, R., Cohen, O., Collinson, G. A., Danchi, W. C., Dong, C., C, A. D. D. G., France, K., Garcia-Sage, K., Glocer, A., et al. (2019) · International Journal of Astrobiology · doi:10.1017/s1473550419000132 · Cited by 288
How to Characterize Habitable Worlds and Signs of Life
Kaltenegger, L. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122238 · Cited by 258
Large Interferometer For Exoplanets (LIFE)
Quanz, S. P., Ottiger, M., Fontanet, E., Kammerer, J., Menti, F., Dannert, F., Gheorghe, A., Absil, O., Airapetian, V., Alei, E., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202140366 · Cited by 218
Metadata
- Authors
- Tian, F., & Ida, S.
- Affiliations
- Tsinghua University (CN)
- Tokyo Institute of Technology (JP)
- Corresponding author
- Tian, Feng
- Venue
- Nature Geoscience
- Published
- 2015-02-16
- Volume
- 8
- Issue
- 3
- Pages
- 177-180
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W2035144479
- Cited by
- 162
- References
- 38
- Citations by year
- 2026: 4 · 2025: 7 · 2024: 11 · 2023: 7 · 2022: 16 · 2021: 16 · 2020: 19 · 2019: 24 · 2018: 22 · 2017: 10 · 2016: 11 · 2015: 14
- FWCI
- 10.81
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Keywords
- M dwarfs, habitable planets, moisture content, Earth-mass planets, water loss, hydrodynamic escape, planet population synthesis, ocean planets, habitability, G dwarfs
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review