Abstract
Mercury, a planet with a lithosphere that forms a single tectonic plate, is replete with tectonic structures interpreted to be the result of planetary cooling and contraction. However, the amount of global contraction inferred from spacecraft images has been far lower than that predicted by models of the thermal evolution of the planet’s interior. Here we present a synthesis of the global contraction of Mercury from orbital observations acquired by the MESSENGER spacecraft. We show that Mercury’s global contraction has been accommodated by a substantially greater number and variety of structures than previously recognized, including long belts of ridges and scarps where the crust has been folded and faulted. The tectonic features on Mercury are consistent with models for large-scale deformation proposed for a globally contracting Earth—now obsolete—that pre-date plate tectonics theory. We find that Mercury has contracted radially by as much as 7 km, well in excess of the 0.8–3 km previously reported from photogeology and resolving the discrepancy with thermal models. Our findings provide a key constraint for studies of Mercury’s thermal history, bulk silicate abundances of heat-producing elements, mantle convection and the structure of its large metallic core.
This is a preview of subscription content, access via your institution
Relevant articles
Open Access articles citing this article.
-
Surface Exospheric Interactions
Space Science Reviews Open Access 23 January 2023
-
The Fe-FeSi phase diagram at Mercury’s core conditions
Nature Communications Open Access 19 January 2022
-
BepiColombo - Mission Overview and Science Goals
Space Science Reviews Open Access 08 December 2021
Access options
Subscribe to this journal
Receive 12 print issues and online access
$259.00 per year
only $21.58 per issue
Rent or buy this article
Prices vary by article type
from$1.95
to$39.95
Prices may be subject to local taxes which are calculated during checkout



References
De Beaumont, E. L. Faits pour servir a l’histoire des montagnes de l’Oisans. Mém. Soc. d’Hist. Natur. Paris 5, 1–32 (1829).
Dana, J. D. On some results of the Earth’s contraction from cooling, including a discussion of the origin of mountains and the nature of the Earth’s interior. Am. J. Sci. 5, 423–443 (1873).
Wilson, J. T. Hypothesis of Earth’s behaviour. Nature 198, 925–929 (1963).
Dutton, C. E. A criticism of the contractional hypothesis. Am. J. Sci. 8, 113–123 (1874).
Strom, R. G., Trask, J. J. & Guest, J. E. Tectonism and volcanism on Mercury. J. Geophys. Res. 80, 2478–2507 (1975).
Melosh, H. J. & McKinnon, W. B. in Mercury (eds Vilas, F., Chapman, C. R. & Matthews, M. S.) The tectonics of Mercury. 374–400 (Univ. Arizona Press, 1988).
Hauck, S. A. II, Dombard, A. J., Phillips, R. J. & Solomon, S. C. Internal and tectonic evolution of Mercury. Earth Planet. Sci. Lett. 222, 713–728 (2004).
Watters, T. R., Robinson, M. S. & Cook, A. C. Topography of lobate scarps on Mercury: New constraints on the planet’s contraction. Geology 26, 991–994 (1998).
Watters, T. R. et al. The tectonics of Mercury: The view after MESSENGER’s first flyby. Earth Planet. Sci. Lett. 285, 283–296 (2009).
Marchi, S. et al. Global resurfacing of Mercury 4.0–4.1 billion years ago by heavy bombardment and volcanism. Nature 499, 59–61 (2013).
Watters, T. R. & Nimmo, F. in Planetary Tectonics (eds Watters, T. R. & Schultz, R. A.) The tectonics of Mercury. 15–80 (Cambridge Univ. Press, (2010).
Di Achille, G. et al. Mercury’s radius change estimates revisited using MESSENGER data. Icarus 221, 456–460 (2012).
Solomon, S. C. The relationship between crustal tectonics and internal evolution in the Moon and Mercury. Phys. Earth. Plan. Inter. 15, 135–145 (1977).
Schubert, G., Ross, M. N., Stevenson, D. J. & Spohn, T. in Mercury (eds Vilas, F., Chapman, C. R. & Matthews, M. S.) Mercury’s thermal history and the generation of its magnetic field. 429–460 (Univ. Arizona Press, 1988).
Dombard, A. J. & Hauck II, S. A Despinning plus global contraction and the orientation of lobate scarps on Mercury: Predictions for MESSENGER. Icarus 198, 274–276 (2008).
Stille, H. Über Alter und Art der Phasen variszischer Gebirgsbildung. Nachr. k. Ges. Will. Göttingen, Math.-Phys. Kl., Jg. 218–224 (1920).
Zuber, M. T. et al. Topography of the northern hemisphere of Mercury from MESSENGER laser altimetry. Science 336, 217–220 (2012).
Denevi, B. W. et al. The distribution and origin of smooth plains on Mercury. J. Geophys. Res. Planets 118, 891–907 (2013).
Trask, N. J. & Guest, J. E. Preliminary geologic terrain map of Mercury. J. Geophys. Res. 80, 2461–2477 (1975).
Head, J. W. et al. Flood volcanism in the northern high latitudes of Mercury revealed by MESSENGER. Science 333, 1853–1856 (2011).
Melosh, H. J. & Dzurisin, D. Mercurian global tectonics: A consequence of tidal despinning?. Icarus 35, 227–236 (1978).
Poblet, J. & Lisle, R. J. Kinematic evolution and styles of fold-and-thrust belts. Geol. Soc. Lond. Spec. Pub. 349, 1–24 (2011).
Burke, K. C., Şengör, A. M. C. & Francis, P. W. Maxwell Montes in Ishtar—A collisional plateau on Venus?. Lunar Planet. Sci. 15, 104–105 (1984).
Thrust Tectonics (ed McClay, K. R.) (Chapman & Hall, 1992).
Roeder, D. American and Tethyan Fold-Thrust Belts (Gebrüder Borntraeger, (2009).
Rothery, D. A. & Massironi, M. Beagle Rupes—Evidence for a basal decollement of regional extent in Mercury’s lithosphere. Icarus 209, 256–261 (2010).
Watters, T. R. Elastic dislocation modeling of wrinkle ridges on Mars. Icarus 171, 284–294 (2004).
Weider, S. Z. et al. Chemical heterogeneity on Mercury’s surface revealed by the MESSENGER X-Ray Spectrometer. J. Geophys. Res. 117, E00L05 (2012).
Denevi, B. W. et al. The evolution of Mercury’s crust: A global perspective from MESSENGER. Science 324, 613–618 (2009).
Mueller, K. & Golombek, M. Compressional structures on Mars. Annu. Rev. Earth Planet. Sci. 32, 435–464 (2004).
Schultz, R. A. Localization of bedding plane slip and backthrust faults above blind thrust faults: Keys to wrinkle ridge structure. J. Geophys. Res. 105, 12035–12052 (2000).
Smith, D. E. et al. Gravity field and internal structure of Mercury from MESSENGER. Science 336, 214–217 (2012).
Suess, E. Das Antlitz der Erde, Vol. III.2 (Tempsky, Prag & Freytag, (1909).
Şengör, A. M. C., Natal’in, B. A. & Burtman, V. S. Evolution of the Altaid tectonic collage and Palaeozoic crustal growth in Eurasia. Nature 364, 299–307 (1993).
Trümpy, R. Geology of Switzerland, A Guide-book. A: An Outline of the Geology of Switzerland (Schweizerische Geologische Kommission, (1980).
Bois, C. et al. in Reflection Seismology: A Global Perspective (eds Barazangi, M. & Brown, L.) Deep seismic profiling of the crust in northern France: The ECORS Project. 21–29 (Am. Geophys. Un., 1986).
Hatcher, R. D. Jr in The Appalachian-Ouachita Orogen in the United States, The Geology of North America (eds Hatcher, R. D. Jr, Thomas, W. A. & Viele, G. W.) Tectonic synthesis of the US Appalachians. 511–535 (Geol. Soc. Am., 1989).
McDougall, J. W., Hussain, A. & Yeats, R. S. in Himalayan Tectonics (eds Treolar, P. J. & Searle, M. P.) 581–588 (Geol. Soc. Lond. Spec. Pub. 74, 1993).
Stille, H. Einführung in den Bau Amerikas (Gebrüder Borntraeger, (1940).
Roeder, D. Andean-age structure of Eastern Cordillera (Province of La Paz, Bolivia). Tectonics 7, 23–39 (1988).
Klimczak, C. et al. Insights into the subsurface structure of the Caloris Basin, Mercury, from assessments of mechanical layering and changes in long-wavelength topography. J. Geophys. Res. Planets 118, 2030–2044 (2013).
McAdoo, D. C. & Sandwell, D. T. Folding of oceanic lithosphere. J. Geophys. Res. 90, 8563–8569
King, S. D. Pattern of lobate scarps on Mercury’s surface reproduced by a model of mantle convection. Nature Geosci. 1, 229–232 (2008).
Michel, N. C. et al. Thermal evolution of Mercury as constrained by MESSENGER observations. J. Geophys. Res. Planets 117, 1033–1044 (2013).
Peplowski, P. N. et al. Radioactive elements on Mercury’s surface from MESSENGER: Implications for the planet’s formation and evolution. Science 333, 1850–1852 (2011).
Grott, M., Breuer, D. & Laneuville, M. Thermo-chemical evolution and global contraction of Mercury. Earth. Planet. Sci. Lett. 307, 135–146 (2011).
Barclay, T. et al. A sub-Mercury-sized exoplanet. Nature 494, 452–454 (2013).
Hawkins, S. E. III et al. The Mercury Dual Imaging System on the MESSENGER spacecraft. Space Sci. Rev. 131, 247–338 (2007).
Becker, K. J. et al. Global controlled mosaic of Mercury from MESSENGER orbital images. Lunar Planet. Sci. 43, abstr. 2654 (2012).
Clark, R. M. & Cox, S. J. D. A modern regression approach to determining fault displacement-length scaling relationships. J. Struct. Geol. 18, 147–152 (2010).
Acknowledgements
We thank C. M. Ernst and N. L. Chabot (The Johns Hopkins University Applied Physics Laboratory, JHU/APL) for the incidence angle maps shown in Supplementary Fig. 2b, c and H. J. Melosh (Purdue University) for his constructive advice during the preparation of this paper. We also thank W. B. McKinnon for comments that substantially improved this manuscript. The MESSENGER project is supported by the NASA Discovery Program under contracts NASW-00002 to the Carnegie Institution of Washington and NAS5–97271 to JHU/APL. This research has made use of NASA’s Astrophysics Data System and Planetary Data System.
Author information
Authors and Affiliations
Contributions
P.K.B. and C.K. led the study, carried out data analyses and documented the findings; P.K.B., C.K., A.M.C.S. and S.A.H. wrote the manuscript and P.K.B. prepared the figures. A.M.C.S. led the historical review of the description and interpretation of contractional landforms on Earth. S.C.S. and T.R.W. participated in scientific discussions. All authors contributed to the interpretation of results and to the finalization of the submitted manuscript.
Corresponding author
Ethics declarations
Competing interests
The authors declare no competing financial interests.
Supplementary information
Supplementary Information
Supplementary Information (PDF 13820 kb)
Rights and permissions
About this article
Cite this article
Byrne, P., Klimczak, C., Celâl Şengör, A. et al. Mercury’s global contraction much greater than earlier estimates. Nature Geosci 7, 301–307 (2014). https://doi.org/10.1038/ngeo2097
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1038/ngeo2097
This article is cited by
-
Surface Exospheric Interactions
Space Science Reviews (2023)
-
The Fe-FeSi phase diagram at Mercury’s core conditions
Nature Communications (2022)
-
A model of crust–mantle differentiation for the early Earth
Acta Geochimica (2022)
-
The case for landed Mercury science
Experimental Astronomy (2022)
-
A case for limited global contraction of Mercury
Communications Earth & Environment (2021)