Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model

We present a pre-fracture incrementally non-linear elastic–hydric model to constrain the models of formation of giant (spacing of 20–300 m) desiccation cracks on Earth, and possibly intermediate sized (80 to 350 m) polygonal networks of cracks located in many impact craters on Mars which have been i...

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Published in:Earth and Planetary Science Letters
Main Authors: El-Maarry, Mohamed Ramy, Kodikara, J., Wijessoriya, S., Markiewicz, W.J., Thomas, N.
Format: Article in Journal/Newspaper
Language:unknown
Published: Elsevier 2012
Subjects:
Online Access:https://eprints.bbk.ac.uk/id/eprint/24708/
https://doi.org/10.1016/j.epsl.2012.01.016
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spelling ftbirkbeckcoll:oai:eprints.bbk.ac.uk.oai2:24708 2023-05-15T17:58:05+02:00 Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model El-Maarry, Mohamed Ramy Kodikara, J. Wijessoriya, S. Markiewicz, W.J. Thomas, N. 2012-03-15 https://eprints.bbk.ac.uk/id/eprint/24708/ https://doi.org/10.1016/j.epsl.2012.01.016 unknown Elsevier El-Maarry, Mohamed Ramy and Kodikara, J. and Wijessoriya, S. and Markiewicz, W.J. and Thomas, N. (2012) Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model. Earth and Planetary Science Letters 323-32 , pp. 19-26. ISSN 0012-821X. Earth and Planetary Sciences Article PeerReviewed 2012 ftbirkbeckcoll https://doi.org/10.1016/j.epsl.2012.01.016 2022-01-09T09:03:48Z We present a pre-fracture incrementally non-linear elastic–hydric model to constrain the models of formation of giant (spacing of 20–300 m) desiccation cracks on Earth, and possibly intermediate sized (80 to 350 m) polygonal networks of cracks located in many impact craters on Mars which have been interpreted to form by desiccation as opposed to thermal contraction (El Maarry et al., 2010). The results of the model show that tensile stresses rise monotonically with desiccation. However, in soils with diffusivities below 10− 4 m2/s, it is not possible to generate high enough stresses to cause fracturing. On the other hand, intermediate values between 10− 2 and 10− 4 m2/s create optimum conditions for the formation of cracks at the time scales suggested for the formation of giant desiccation polygons on Earth. Our model clearly shows that for typical diffusivity values of clayey soils with a considerable amount of smectites enough stress can build up to stimulate cracking of various spatial scales. These results corroborate earlier assumptions that giant desiccation polygons on Earth occur through lowering of the water table rather than surface evaporation. Extending the model to Mars shows that soils would crack within similar diffusivity limits but in slightly longer periods of time owing to the lower gravity. Finally, a model for formation of desiccation cracks on Mars is presented that shows that two main conditions need to be fulfilled for desiccation cracks to occur under current martian climatic conditions, namely, that the thermal and soil diffusivity conditions 1) allow for the formation of an unsaturated zone with a considerable thickness while at the same time 2) limiting the growth of the permafrost downward which would disrupt the cracking process. Article in Journal/Newspaper permafrost BIROn - Birkbeck Institutional Research Online (Birkbeck University of London) Earth and Planetary Science Letters 323-324 19 26
institution Open Polar
collection BIROn - Birkbeck Institutional Research Online (Birkbeck University of London)
op_collection_id ftbirkbeckcoll
language unknown
topic Earth and Planetary Sciences
spellingShingle Earth and Planetary Sciences
El-Maarry, Mohamed Ramy
Kodikara, J.
Wijessoriya, S.
Markiewicz, W.J.
Thomas, N.
Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
topic_facet Earth and Planetary Sciences
description We present a pre-fracture incrementally non-linear elastic–hydric model to constrain the models of formation of giant (spacing of 20–300 m) desiccation cracks on Earth, and possibly intermediate sized (80 to 350 m) polygonal networks of cracks located in many impact craters on Mars which have been interpreted to form by desiccation as opposed to thermal contraction (El Maarry et al., 2010). The results of the model show that tensile stresses rise monotonically with desiccation. However, in soils with diffusivities below 10− 4 m2/s, it is not possible to generate high enough stresses to cause fracturing. On the other hand, intermediate values between 10− 2 and 10− 4 m2/s create optimum conditions for the formation of cracks at the time scales suggested for the formation of giant desiccation polygons on Earth. Our model clearly shows that for typical diffusivity values of clayey soils with a considerable amount of smectites enough stress can build up to stimulate cracking of various spatial scales. These results corroborate earlier assumptions that giant desiccation polygons on Earth occur through lowering of the water table rather than surface evaporation. Extending the model to Mars shows that soils would crack within similar diffusivity limits but in slightly longer periods of time owing to the lower gravity. Finally, a model for formation of desiccation cracks on Mars is presented that shows that two main conditions need to be fulfilled for desiccation cracks to occur under current martian climatic conditions, namely, that the thermal and soil diffusivity conditions 1) allow for the formation of an unsaturated zone with a considerable thickness while at the same time 2) limiting the growth of the permafrost downward which would disrupt the cracking process.
format Article in Journal/Newspaper
author El-Maarry, Mohamed Ramy
Kodikara, J.
Wijessoriya, S.
Markiewicz, W.J.
Thomas, N.
author_facet El-Maarry, Mohamed Ramy
Kodikara, J.
Wijessoriya, S.
Markiewicz, W.J.
Thomas, N.
author_sort El-Maarry, Mohamed Ramy
title Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
title_short Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
title_full Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
title_fullStr Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
title_full_unstemmed Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model
title_sort desiccation mechanism for formation of giant polygons on earth and intermediate-sized polygons on mars: results from a pre-fracture model
publisher Elsevier
publishDate 2012
url https://eprints.bbk.ac.uk/id/eprint/24708/
https://doi.org/10.1016/j.epsl.2012.01.016
genre permafrost
genre_facet permafrost
op_relation El-Maarry, Mohamed Ramy and Kodikara, J. and Wijessoriya, S. and Markiewicz, W.J. and Thomas, N. (2012) Desiccation mechanism for formation of giant polygons on Earth and intermediate-sized polygons on Mars: results from a pre-fracture model. Earth and Planetary Science Letters 323-32 , pp. 19-26. ISSN 0012-821X.
op_doi https://doi.org/10.1016/j.epsl.2012.01.016
container_title Earth and Planetary Science Letters
container_volume 323-324
container_start_page 19
op_container_end_page 26
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