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Ancient northern ocean on Mars evidenced by in situ observations of marine sedimentary rocks

Peer-Reviewed Publication

Science China Press

Topographic map of the northern hemisphere of Mars showing extent of former northern ocean.

image: Topographic map of the northern hemisphere of Mars showing previously proposed shorelines. The red star denotes the location of the landing site of the Zhurong rover, ~282 km to the north of the Deuteronilus shorelines. The data are color-coded MOLA elevation over MOLA shaded relief centered at the North Pole with the Lambert azimuthal equal-area projection. view more 

Credit: ©Science China Press

An international research team led by Professor Long Xiao from the School of Earth Sciences of China University of Geosciences (Wuhan) discovered the presence of marine sedimentary rocks on the surface of Mars for the first time by comprehensively analyzing the scientific data obtained by the multispectral camera (MSCam) carried by the Zhurong rover. The relevant research results were published in the journal "National Science Review" under the title "Evidence for Marine Sedimentary Rocks in Utopia Planitia: Zhurong Rover Observations.”

Currently Mars is cold and dry, lacking water and traces of life, but the Martian environment billions of years ago may have been very different. Past studies have proven that there was a large amount of liquid water on Mars in the early days, and the paleo-ocean hypothesis was proposed through landform analysis of satellite images and numerical simulation. It is proposed that the paleo-ocean area in the northern lowlands (Multimedia Material 1) formed a special marine sedimentary geological unit, called the Vasitas Borealis Formation (VBF), but lacks the support of in situ data. Therefore, whether there was an ocean in the northern plain of Mars has been the focus of controversy for decades.

In 2021, the "Zhurong" rover carried by China’s Tianwen-1 Mars mission successfully landed on the southern edge of the Utopia Plain in the eastern part of the northern plain of Mars. Part of the mission was to search for any possible evidence for or against the existence of an ancient ocean on Mars, which possibly may have hosted early life.

Since landing, the Zhurong has been heading south towards potential coastline areas, observing the exposed Vasitas Borealis Formation along the way. Zhurong traveled about 1921 meters (Multimedia Material 2), and used different imaging and analysis systems to conduct detailed in-situ observations of outcrops and surface rocks. The navigation and terrain cameras have obtained 106 sets of panoramic images, which recorded in detail "the surface morphology and structural characteristics of many rocks near the route of the Zhurong rover.

The research team examined the photos sent back by the Mars rover's on-board camera and found that the exposed rocks developed bedding structures, which are significantly different from the common volcanic rocks on the surface of Mars, and also different from the bedding structures formed by aeolian sand deposition. The structures indicated bidirectional flow characteristics consistent with low-energy tidal currents in Earth's littoral-shallow marine environment.

Based on the rock images obtained by MSCam, the research team analyzed in detail the surface structure of the rocks in the inspection area of the Zhurong rover. Since the observed rocks are all located in the Zhurong inspection area, the research team named the geological unit it represents the Zhurong Member. During the study, the research team found that the rocks in the section typically retain local lens-shaped cross-bedding fabrics, mainly composed of a variety of small-scale cross-bedding, accompanied by a small amount of lens-shaped flaser bedding and sedimentary structures of small channel structures (Multimedia Material 3).

Among them, the layers that make up the cross-bedding overlap and tilt in two opposite directions, indicating a bidirectional paleocurrent environment. In addition, since the thickness and grain size of the strata have large differences in different directions, it indicates that there are differences in the intensity of paleocurrents in the two directions. This bidirectional water flow pattern is usually formed by the fluid action with periodic flow direction changes, which is not common in eolian and fluvial environments, but is common in the littoral-shallow sea environment of Earth. Compared with Earth, Mars has only two small satellites, which makes its surface have a low-energy tidal system, and only small-scale bedding structures can be formed in this tidal environment. In addition, the bedforms and sedimentary structures identified in the study have evidence supporting aqueous flow rather than eolian deposition.

The team’s observational results of the Zhurong member rocks in this study are the first direct in situ evidence detected to support the existence of ancient oceans in the northern plains of Mars. The location of the landing site of Zhurong indicates that the observed sedimentary structures may have formed during the regression of the northern plain paleo-ocean (Multimedia Material 4).

The sedimentary structures found in the Vasitas Borealis Formation provide new insights into the early history of Mars. The in-depth exploration by Zhurong in this area and future sample return will deepen our understanding of the habitability of Mars and the preservation of microbial life traces.

The joint research team of this research work comes from 13 co-authors from universities in China and USA. Professors Long Xiao and Jun Huang from China University of Geosciences (Wuhan) are the co-first authors of the paper. Professors Long Xiao and Timothy Kusky from China University of Geosciences (Wuhan) ·are the co-corresponding authors of the paper.



See the article:

Evidence for Marine Sedimentary Rocks in Utopia Planitia: Zhurong Rover Observations

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