cenki-tok-2020-crustal-roots-in-stable-continents

[benedictecenki]

-> submitter ORCID (or name)

https://orcid.org/0000-0001-7649-4498

-> slug

cenki-tok-2020-crustal-roots-in-stable-continents

-> license

CC-BY-4.0

-> alternative license URL

No response

-> model category

model published in study

-> model status

completed

-> associated publication DOI

https://doi.org/10.1130/G47301.1

-> model creators

0000-0001-7649-4498
0000-0002-1767-8593
0000-0001-6773-0807

-> title

No response

-> description

Away from tectonically active regions, the continental crust has an average thickness of 40 ± 1 km. Yet, it shows a remarkable variability from 25 to 65 km, comparable to that of the most tectonically active regions. Here, we consider the problem of the formation and preservation of anomalous deep crustal roots in stable intracontinental regions. Using two- dimensional thermomechanical experiments, we show that the interplay between partial melting, the formation of garnet-pyroxene-bearing rocks, and their strain rate–dependent retrogression result in the preservation of thick and strong crustal roots. We argue that it is the partitioning into narrow regions of strain, retrogression, and weakening coupled into a positive feedback loop that explains why strong high-grade crustal roots remain largely immune to gravitational stresses and are able to persist over hundreds of millions of years.

-> abstract

No response

-> scientific keywords

No response

-> funder

https://ror.org/02wbb9367, 793978

-> model embargo?

No response

-> include model code ?

• yes

-> model code/inputs DOI

https://github.com/underworld-community/cenki-tok-et-al-crustal-roots-in-stable-continents

-> model code/inputs notes

No response

-> include model output data?

• yes

-> data creators

No response

-> model output data DOI

No response

-> model output data notes

No response

-> model output data size

No response

-> software framework DOI/URI

Underworld 2 version 2.8.5

-> software framework source repository

No response

-> name of primary software framework (e.g. Underworld, ASPECT, Badlands, OpenFOAM)

Underworld 2

-> software framework authors

No response

-> software & algorithm keywords

Python, Finite Element

-> computer URI/DOI

No response

-> add landing page image and caption

Fast modeling results (1.8 cm.y-1 extension speed) at an average strain rate of 3e-15 s-1 and 25 % extension. Colors are the same as in Fig 2. Model a. Only partial melting is allowed (garnet-pyroxene isograde and retrogression into amphibolite are removed). Model b. Partial melting, crystallization of garnet-pyroxene assemblages and retrogression are allowed. The temperature for the transformation of the continental crust into garnet-pyroxene rich rocks is 777 °C (see text for explanation). The reference temperatures for the solidus of the continental crust and the garnet-pyroxene rich crust are 650 °C and 790 °C, respectively. Model c. Same as model b but the temperature for the continental crust solidus is increased to 720 °C. Model d. Zoom on model b illustrating the velocity field (black arrows) when the boundary condition mimicking extension is removed (after 2 Myr of gravity forces operating) showing that the partially molten crust flows while garnet-pyroxene rich rocks do not.

-> add an animation (if relevant)

-> add a graphic abstract figure (if relevant)

Fast modeling results (1.8 cm.y-1 extension speed) at an average strain rate of 3e-15 s-1 and 25 % extension. Colors are the same as in Fig 2. Model a. Only partial melting is allowed (garnet-pyroxene isograde and retrogression into amphibolite are removed). Model b. Partial melting, crystallization of garnet-pyroxene assemblages and retrogression are allowed. The temperature for the transformation of the continental crust into garnet-pyroxene rich rocks is 777 °C (see text for explanation). The reference temperatures for the solidus of the continental crust and the garnet-pyroxene rich crust are 650 °C and 790 °C, respectively. Model c. Same as model b but the temperature for the continental crust solidus is increased to 720 °C. Model d. Zoom on model b illustrating the velocity field (black arrows) when the boundary condition mimicking extension is removed (after 2 Myr of gravity forces operating) showing that the partially molten crust flows while garnet-pyroxene rich rocks do not.

-> add a model setup figure (if relevant)

Model geometry, initial conditions as well as geotherm, viscosity and density profiles. A weak prismatic region dipping 45° simulates a detachment fault in upper crust. The circles pattern superimposed on the continental crust represents the finite strain ellipses.

-> add a description of your model setup

Our 2D thermo-mechanical experiments consider a 360 km wide orogenic plateau with a 70 km thick crust (i.e. the thickness of the Tibetan plateau, Nabelek et al., 2009) above 40 km of mantle (Fig.2). A layer of air-like material with low-viscosity and low-density is imposed on top of the crust to accommodate the development of surface topography. The plateau is experiencing extensional deformation as the crust returns to a normal thermo-mechanical state. Extensional velocity boundary conditions are imposed on both vertical walls of the model. We have tested slow (0.18 cm.y-1) and fast (1.8 cm.y-1) velocities, delivering a strain rate averaged over the length of the model of 3e-16 s-1 and 3e-15 s-1 respectively. Horizontal boundaries of the model are free slips. The thermal properties of the material combined with constant basal heat flow and constant top temperature deliver an initial steady-state geotherm leading to a Moho temperature of ca. 900 °C (Fig. 2). We select from the literature plausible visco-plastic parameters (Suppl Data) so the mechanical behavior of the modeled lithosphere depends on temperature, strain rate, deviatoric stress and accumulated strain. Details of modeling procedures, rheological and thermal parameters as well as the input python script are available in GSA Data Repository*.
In order to explore the interplay between partial melting, the formation of stronger garnet-pyroxene bearing rocks and their retrogression into weaker amphibolite facies rocks we parameterize three first-order metamorphic phase transitions. The first phase change simulates partial melting and its feedback on density, viscosity and temperature (Rey et al., 2009, Suppl Data). A second phase change with feedback on density and viscosity occurs at T = 1050 K to simulate prograde amphibolite to garnet-pyroxene rock reaction (Philpotts and Ague, 2009). Finally, a third phase change with feedback on density and viscosity accounts for the retrogression of garnet-pyroxene bearing rocks back into amphibolite facies rocks. This third phase change occurs at T = 1050 K as well and for a strain rate ≥ 10-14 s-1. Our model implicitly assume that water is available. Therefore, retrogression is contingent upon strain rate, which simulates the metastability of dry high-grade rocks during exhumation. This strain rate threshold is in the range of expected strain rates measured in orogenic shear zones (Sassier et al., 2009; Boutonnet et al., 2013; Faregeng and Biggs, 2018). Rock solidus depends on their fertility and availability of fluid. Hence, we have tested different solidus for the continental crust and the garnet-pyroxene-bearing rocks (Suppl Data) in the range commonly accepted for these rock types. For the continental crust we have tested a solidus representative of fertile metapelites with a melting temperature at room pressure of 923 K (Fig. 3a, b; White et al., 2001), and a solidus representative of less fertile rocks with a melting temperature at room pressure of 993 K (Fig. 3c; Rey and Müller, 2010). For the dry garnet-pyroxene-bearing crust, we use a melting temperature at room pressure of 1063 K representative of refractory granulites (Cenki-Tok et al., 2016). We use Underworld, a well-tested open source finite element code, to solve the equations of conservation of momentum, mass and energy for an incompressible fluid on a Cartesian Eulerian mesh (Moresi et al., 2007; Beucher et al., 2019).

Please provide any feedback on the model submission process?

No response

[m-te-bot]

Model Report

Thank you for submitting.

Using Github actions, we have regenerated a report summarising information about your model

• Please check the report below, including the Errors and Warnings section

• You can update any information, by editing the markdown file at the top of the issue

• these edits will trigger the report will be regenerated

• once you are satisfied with the results, please add a review requested Review requested label

Parsed data

Section 1: Summary of your model

Model Submitter:

Bénédicte Cenki-Tok or Cenki (0000-0001-7649-4498)

Model Creator(s):

• Bénédicte Cenki-Tok or Cenki (0000-0001-7649-4498)
• Patrice Rey (0000-0002-1767-8593)
• Diane Arcay (0000-0001-6773-0807)

Model slug:

cenki-tok-2020-crustal-roots-in-stable-continents-1

(this will be the name of the model repository when created)

Model name:

Strain and retrogression partitioning explain long-term stability of crustal roots in stable continents

License:

Creative Commons Attribution 4.0 International

Model Category:

• model published in study

Model Status:

• completed

Associated Publication title:

Strain and retrogression partitioning explain long-term stability of crustal roots in stable continents

Short description:

Away from tectonically active regions, the continental crust has an average thickness of 40 ± 1 km. Yet, it shows a remarkable variability from 25 to 65 km, comparable to that of the most tectonically active regions. Here, we consider the problem of the formation and preservation of anomalous deep crustal roots in stable intracontinental regions. Using two- dimensional thermomechanical experiments, we show that the interplay between partial melting, the formation of garnet-pyroxene-bearing rocks, and their strain rate–dependent retrogression result in the preservation of thick and strong crustal roots. We argue that it is the partitioning into narrow regions of strain, retrogression, and weakening coupled into a positive feedback loop that explains why strong high-grade crustal roots remain largely immune to gravitational stresses and are able to persist over hundreds of millions of years.

Abstract:

Away from tectonically active regions, the continental crust has an average thickness of 40 ± 1 km. Yet, it shows a remarkable variability from 25 to 65 km, comparable to that of the most tectonically active regions. Here, we consider the problem of the formation and preservation of anomalous deep crustal roots in stable intracontinental regions. Using two-dimensional thermomechanical experiments, we show that the interplay between partial melting, the formation of garnet-pyroxene-bearing rocks, and their strain rate–dependent retrogression result in the preservation of thick and strong crustal roots. We argue that it is the partitioning into narrow regions of strain, retrogression, and weakening coupled into a positive feedback loop that explains why strong high-grade crustal roots remain largely immune to gravitational stresses and are able to persist over hundreds of millions of years.

Funder(s):

• European Regions Research and Innovation Network (https://ror.org/02wbb9367)

Section 2: your model code, output data

No embargo on model contents requested

Include model code:

True

Model code existing URL/DOI:

https://github.com/underworld-community/cenki-tok-et-al-crustal-roots-in-stable-continents

Include model output data:

True

Section 3: software framework and compute details

Software Framework DOI/URL:

Found software: [Underworld 2](Underworld 2 version 2.8.5)

Name of primary software framework:

Underworld 2

Software & algorithm keywords:

• Python
• Finite Element

Section 4: web material (for mate.science)

Landing page image:

Filename: 459D1B30-8E88-4E84-81CE-3201350F335A.jpg
Caption: Fast modeling results (1.8 cm.y-1 extension speed) at an average strain rate of 3e-15 s-1 and 25 % extension. Colors are the same as in Fig 2. Model a. Only partial melting is allowed (garnet-pyroxene isograde and retrogression into amphibolite are removed). Model b. Partial melting, crystallization of garnet-pyroxene assemblages and retrogression are allowed. The temperature for the transformation of the continental crust into garnet-pyroxene rich rocks is 777 °C (see text for explanation). The reference temperatures for the solidus of the continental crust and the garnet-pyroxene rich crust are 650 °C and 790 °C, respectively. Model c. Same as model b but the temperature for the continental crust solidus is increased to 720 °C. Model d. Zoom on model b illustrating the velocity field (black arrows) when the boundary condition mimicking extension is removed (after 2 Myr of gravity forces operating) showing that the partially molten crust flows while garnet-pyroxene rich rocks do not.

Animation:

Filename: GeolMov.gif
Caption:

Graphic abstract:

Filename: 459D1B30-8E88-4E84-81CE-3201350F335A.jpg
Caption: Fast modeling results (1.8 cm.y-1 extension speed) at an average strain rate of 3e-15 s-1 and 25 % extension. Colors are the same as in Fig 2. Model a. Only partial melting is allowed (garnet-pyroxene isograde and retrogression into amphibolite are removed). Model b. Partial melting, crystallization of garnet-pyroxene assemblages and retrogression are allowed. The temperature for the transformation of the continental crust into garnet-pyroxene rich rocks is 777 °C (see text for explanation). The reference temperatures for the solidus of the continental crust and the garnet-pyroxene rich crust are 650 °C and 790 °C, respectively. Model c. Same as model b but the temperature for the continental crust solidus is increased to 720 °C. Model d. Zoom on model b illustrating the velocity field (black arrows) when the boundary condition mimicking extension is removed (after 2 Myr of gravity forces operating) showing that the partially molten crust flows while garnet-pyroxene rich rocks do not.

Model setup figure:

Filename: 5F6DD5CC-DF90-4860-8E76-6AA35305A50B.png
Caption: Model geometry, initial conditions as well as geotherm, viscosity and density profiles. A weak prismatic region dipping 45° simulates a detachment fault in upper crust. The circles pattern superimposed on the continental crust represents the finite strain ellipses.
Description: Our 2D thermo-mechanical experiments consider a 360 km wide orogenic plateau with a 70 km thick crust (i.e. the thickness of the Tibetan plateau, Nabelek et al., 2009) above 40 km of mantle (Fig.2). A layer of air-like material with low-viscosity and low-density is imposed on top of the crust to accommodate the development of surface topography. The plateau is experiencing extensional deformation as the crust returns to a normal thermo-mechanical state. Extensional velocity boundary conditions are imposed on both vertical walls of the model. We have tested slow (0.18 cm.y-1) and fast (1.8 cm.y-1) velocities, delivering a strain rate averaged over the length of the model of 3e-16 s-1 and 3e-15 s-1 respectively. Horizontal boundaries of the model are free slips. The thermal properties of the material combined with constant basal heat flow and constant top temperature deliver an initial steady-state geotherm leading to a Moho temperature of ca. 900 °C (Fig. 2). We select from the literature plausible visco-plastic parameters (Suppl Data) so the mechanical behavior of the modeled lithosphere depends on temperature, strain rate, deviatoric stress and accumulated strain. Details of modeling procedures, rheological and thermal parameters as well as the input python script are available in GSA Data Repository*.
In order to explore the interplay between partial melting, the formation of stronger garnet-pyroxene bearing rocks and their retrogression into weaker amphibolite facies rocks we parameterize three first-order metamorphic phase transitions. The first phase change simulates partial melting and its feedback on density, viscosity and temperature (Rey et al., 2009, Suppl Data). A second phase change with feedback on density and viscosity occurs at T = 1050 K to simulate prograde amphibolite to garnet-pyroxene rock reaction (Philpotts and Ague, 2009). Finally, a third phase change with feedback on density and viscosity accounts for the retrogression of garnet-pyroxene bearing rocks back into amphibolite facies rocks. This third phase change occurs at T = 1050 K as well and for a strain rate ≥ 10-14 s-1. Our model implicitly assume that water is available. Therefore, retrogression is contingent upon strain rate, which simulates the metastability of dry high-grade rocks during exhumation. This strain rate threshold is in the range of expected strain rates measured in orogenic shear zones (Sassier et al., 2009; Boutonnet et al., 2013; Faregeng and Biggs, 2018). Rock solidus depends on their fertility and availability of fluid. Hence, we have tested different solidus for the continental crust and the garnet-pyroxene-bearing rocks (Suppl Data) in the range commonly accepted for these rock types. For the continental crust we have tested a solidus representative of fertile metapelites with a melting temperature at room pressure of 923 K (Fig. 3a, b; White et al., 2001), and a solidus representative of less fertile rocks with a melting temperature at room pressure of 993 K (Fig. 3c; Rey and Müller, 2010). For the dry garnet-pyroxene-bearing crust, we use a melting temperature at room pressure of 1063 K representative of refractory granulites (Cenki-Tok et al., 2016). We use Underworld, a well-tested open source finite element code, to solve the equations of conservation of momentum, mass and energy for an incompressible fluid on a Cartesian Eulerian mesh (Moresi et al., 2007; Beucher et al., 2019).

Errors and Warnings

Associated Publication
Error fetching metadata with application/ld+json from https://api.crossref.org/works/https://doi.org/10.1130/G47301.1: 406 Client Error: Not Acceptable for url: https://api.crossref.org/works/https://doi.org/10.1130/G47301.1
Software Framework DOI/URI
Error fetching metadata with application/ld+json from https://doi.org/No valid DOI found in the input string.: 404 Client Error: Not Found for url: https://www.doi.org/No%20valid%20DOI%20found%20in%20the%20input%20string.
Error fetching metadata with application/json from https://doi.org/No valid DOI found in the input string.: 404 Client Error: Not Found for url: https://www.doi.org/No%20valid%20DOI%20found%20in%20the%20input%20string.
Failed to fetch metadata with any content type or URL.
Error: unable to parse software metadata.
Software Repository
Warning: no repository URL provided.
Software framework authors
Error: no authors found
Submitter
ORCID metadata record succesfully extracted in json-ld format

Model creators
ORCID metadata record succesfully extracted in json-ld format
ORCID metadata record succesfully extracted in json-ld format
ORCID metadata record succesfully extracted in json-ld format
Model Repository Slug
Warning: slug should be in the format familyname-year-keyword

Warning: Model repo cannot be created with proposed slug cenki-tok-2020-crustal-roots-in-stable-continents.
Either propose a new slug or repo will be created with name cenki-tok-2020-crustal-roots-in-stable-continents-1.

Scientific keywords
Warning: No keywords given
Could not parse Embargo date. Check format is
Model code/inputs notes
Warning: No notes provided.
Model creators
Error: no data creators found
Model output DOI
Warning: No DOI/URI provided.
Model data notes
Warning: No notes provided.
Model data size
Warning: No notes provided.
Invalid size stringComputer URI/DOI
Warning: No URI/DOI provided.
Animation
Error: No caption found for image.

Next steps

• once the model_reviewers team has approved the model, we will create a repository for your model

[m-te-bot]

Review Requested

A review of this submission has been requested from @ModelAtlasofTheEarth/model_reviewers

[m-te-bot]

Workflow Failure ❌

Unfortunately, the workflow to create the model repo has failed. View the logs here for more information:

🔗 Workflow logs

You may need to delete the following repo that was created via this workflow run since the run was not fully successful: ModelAtlasofTheEarth/cenki-tok-2020-crustal-roots-in-stable-continents

[m-te-bot]

Workflow Failure ❌

Unfortunately, the workflow to create the model repo has failed. View the logs here for more information:

🔗 Workflow logs

You may need to delete the following repo that was created via this workflow run since the run was not fully successful: ModelAtlasofTheEarth/cenki-tok-2020-crustal-roots-in-stable-continents

[m-te-bot]

Workflow Failure ❌

Unfortunately, the workflow to create the model repo has failed. View the logs here for more information:

🔗 Workflow logs

You may need to delete the following repo that was created via this workflow run since the run was not fully successful: ModelAtlasofTheEarth/cenki-tok-2020-crustal-roots-in-stable-continents

[m-te-bot]

Model repository created at https://github.com/ModelAtlasofTheEarth/cenki-tok-2020-crustal-roots-in-stable-continents

[m-te-bot]

Model repository created at https://github.com/ModelAtlasofTheEarth/cenki-tok-2020-crustal-roots-in-stable-continents