Zaki, A. S.; Edgett, K. S.; Pajola, M.; Kite, E.; Davis, J. M.; Mangold, N.; Madof, A. S.; Lucchetti, A.; Grindrod, P.; Hughes, C. M.; Sangwan, K.; Thomas, N.; Schuster, M.; Gupta, S.; Cremonese, G.; Castelltort, S. (2023). Prolonged Record of Hydroclimatic Changes at Antoniadi Crater, Mars. Journal of geophysical research: Planets, 128(7) American Geophysical Union 10.1029/2022JE007606
|
Text
JGR_Planets_-_2023_-_Zaki_-_Prolonged_Record_of_Hydroclimatic_Changes_at_Antoniadi_Crater__Mars.pdf - Published Version Available under License Creative Commons: Attribution (CC-BY). Download (18MB) | Preview |
The first billion years of Martian geologic history consisted of surface environments and landscapes dramatically different from those seen today, with flowing liquid water sculpting river channels and ponding to form bodies of water. However, the hydro-climatic context, the frequency, and the duration under which these systems existed remain uncertain. Addressing these fundamental questions may improve our understanding of early Mars climate. Here, we reconstruct a long-lived archive consisting of an array of fluvial systems inside the Antoniadi crater––one of the largest lake basins on Mars (9.58 × 104 km2). We found that the fluvial activity occurred throughout four major intermittent active intervals during the Late Noachian to Early Amazonian (∼3.7 to >2.4 Ga). This resulted in at least two major lakes, which formed during periods of markedly increased surface runoff production. The record of these four riverine phases is preserved in fluvial ridges, valley networks, back-stepping or down-stepping fan-shaped landforms, and terrace-like formations within an outlet canyon. These morphologies point to lake-controlled base-level fluctuations suggestive of episodic precipitation-fed surface runoff punctuated by intermittent catastrophic floods that were capable of breaching crater-lake rims and incising outlet canyons. Fluvial-deposit thickness, junction angles of channels, and lake morphometry suggest that riverine systems lasted at least 103–106 years and episodically occurred under primarily arid and semi-arid climates. These findings place new regional constraints on the fluvial frequency, longevity, and climatic regime of one of the largest Martian lakes, thereby bolstering the hypothesis that episodic warming likely punctuated the planet's early history
Item Type: |
Journal Article (Original Article) |
---|---|
Division/Institute: |
08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences 08 Faculty of Science > Physics Institute 08 Faculty of Science > Physics Institute > NCCR PlanetS |
UniBE Contributor: |
Thomas, Nicolas |
Subjects: |
500 Science > 520 Astronomy 600 Technology > 620 Engineering 500 Science 500 Science > 530 Physics |
ISSN: |
2169-9097 |
Publisher: |
American Geophysical Union |
Language: |
English |
Submitter: |
Agnès Véronique Schär Vuillemin |
Date Deposited: |
04 Apr 2024 11:53 |
Last Modified: |
04 Apr 2024 11:53 |
Publisher DOI: |
10.1029/2022JE007606 |
Uncontrolled Keywords: |
Mars, Martian surface, geological processes, Early Mars climate, hydroclimate, fluvial processes |
BORIS DOI: |
10.48350/194798 |
URI: |
https://boris.unibe.ch/id/eprint/194798 |