Sergio Duran
Knickpoints in Martian channels indicate past ocean levels
Duran, Sergio; Coulthard, Tom J.; Baynes, Edwin R.C.
Authors
Abstract
On Mars, the presence of extensive networks of sinuous valleys and large channels provides evidence for a wetter and warmer environment where liquid water was more abundant than it is at present. We undertook an analysis of all major channel systems on Mars and detected sharp changes in elevation along the river long profiles associated with steep headwall theatre-like valleys and terraces left downstream by channel incision. These breaks in channel longitudinal slope, headwalls and terraces exhibit a striking resemblance with terrestrial fluvial features, commonly termed 'knickpoints'. On Earth, such knickpoints can be formed by more resistant bedrock or where changes in channel base-level have initiated erosion that migrates upstream (such as tectonic uplift or sea level change). We observed common elevations of Martian knickpoints in eleven separate channel systems draining into the Martian Northern lowlands. Numerical modeling showed that the common elevations of some of these knickpoints were not random. As the knickpoints are spread across the planet, we suggest that these Martian knickpoints were formed in response to a common base level or ocean level rather than local lithology. Thus, they potentially represent a record of past ocean levels and channel activity on Mars.
Citation
Duran, S., Coulthard, T. J., & Baynes, E. R. (2019). Knickpoints in Martian channels indicate past ocean levels. Scientific reports, 9(1), Article 15153. https://doi.org/10.1038/s41598-019-51574-2
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 23, 2019 |
Online Publication Date | Oct 22, 2019 |
Publication Date | Oct 22, 2019 |
Deposit Date | Oct 22, 2019 |
Publicly Available Date | Oct 23, 2019 |
Journal | Scientific reports |
Print ISSN | 2045-2322 |
Publisher | Nature Publishing Group |
Peer Reviewed | Peer Reviewed |
Volume | 9 |
Issue | 1 |
Article Number | 15153 |
DOI | https://doi.org/10.1038/s41598-019-51574-2 |
Keywords | Geomorphology; Hydrology; Inner planets |
Public URL | https://hull-repository.worktribe.com/output/2976581 |
Publisher URL | https://www.nature.com/articles/s41598-019-51574-2 |
Contract Date | Oct 22, 2019 |
Files
Published article
(1.5 Mb)
PDF
Copyright Statement
This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
You might also like
Learning histories, participatory methods and creative engagement for climate resilience
(2023)
Journal Article
Historic Spatial Patterns of Storm-Driven Compound Events in UK Estuaries
(2022)
Journal Article
Sensitivity of Estuaries to Compound Flooding
(2021)
Journal Article
Downloadable Citations
About Repository@Hull
Administrator e-mail: repository@hull.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search