Samples collected by Perseverance

In its current stage, MASL contains analogues representative to samples collected by Perseverance during the first two campaigns of Mars2020: the Crater Floor and Delta Front. 

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The path taken by NASA’s Perseverance Mars rover during the first 1,100 sols (martian days) of its mission at Jezero crater, superimposed on a geologic map after Stack et al. (2020). Rover traverse and waypoints are shown with white line and dots, respectively. Sampling locations are marked with red crosses and labeled with the names. Labeled black boxes show approximate extent of each campaign. (Herd et al., 2024).

By Marine Ciocco & Agata Krzesińska
Published Nov. 13, 2024

Samples collected at the Jezero Crater Floor

The samples collected from the Crater Floor represent a suite of likely petrogenetically related igneous rocks emplaced as lava flows and intrusions mostly postdating the delta and displaying variable degrees of aqueous alteration (e.g., Udry et al., 2022; Simon et al., 2023). 

The intrusive samples link to Séítah formation, likely the oldest of the crater floor, and were sampled at the localities Brac and Issole. Based on texture and mineralogy, they represent olivine cumulate with poikilitic textures (Liu et al., 2022), with accessory augite and plagioclase. This formation also records carbonates and phyllosilicates, implying carbonation and salt precipitation during its history. 

The samples recovered at Brac are named Salette and Coulettes. The samples recovered at Issole are named Robine and Malay. The samples from Issole show less signs of alteration, but carbonates and hydrated sulfates are also present.

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Abrasion patches and Watson camera images of cores sampled from Séítah formation at a) Brac and b) Issole.

The second observed formation is Máaz, composed of lava flows and sampled at Rochette (Lower Máaz) and Sid (Upper Máaz). Cached rocks represent holocrystalline augite basalt (Farley et al., 2022), although the Lower and Upper Máaz differ in textures and in plagioclase crystal sizes. The first samples, recovered at Rochette are called Montdenier and Montagnac and are finer textured. The second set of samples, collected at the Sid locality, are called Atsah and Ha`ahoni and present larger scale crystals of plagioclase. Samples from Máaz additionally record aqueous activity: sulfates, perchlorates, silicates, carbonates and phosphates fill the voids in the Máaz formation rocks, although set of samples from Sid show less alteration.

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Abrasion patches and Watson camera images of cores sampled from Máaz formation at a) Rochette and b) Sid.

Samples collected from the Delta Front

Delta Front samples represent fluvial to deltaic sediments formed by the transport and deposition of materials from the Jezero watershed. The samples include fine-grained, sulfate- and carbonate-bearing mudstones (Benison et al., 2024; Stack et al., 2024) sampled at Amalik, Skinner Ridge and Wildcat Ridge. 

The samples Mageik and Shuyak, recovered at the Amalik site, appear to be mudstones with olivine framework. They contain salts such as sulfates and dolomite in cement, as well as silica. They are likely to derive from rocks compositionally similar to Seitah formation, but having undergone subaqueous alteration. The samples from the Amalik outcrop appear less oxidized than the rest of the Delta, richer in olivine and poorer in sulfates.

 

The samples from Skinner Ridge are Swift Run and Skyland. Those are sandstones which contain larger clasts (up to 2 mm in diameter) compared to mudstones from Amalik. Grain framework of rocks from sinner Ridge is dominated by detrital fragments. The fragments vary in composition, from mafic minerals to alteration products such as phyllosilicates. The matrix cementing those rocks is interpreted to be Fe,Mg-rich carbonate. These samples present evidence of alteration and oxidation.

 

Finally, the samples from Wildcat Ridge, Bearwallow and Hazeltop, are well sorted, layered and fine grained mudstones with weakly hydrated sulfate inclusions. They also contain small amounts of clay, hydrated silica, and possibly carbonates. These two samples tend to contain less inclusions than the other delta sediments.

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Abrasion patches and Watson camera images of cores sampled from sediments at the delta front. a) carbonate-cemented basaltic sediments from Amalik. b and c) carbonate-sulfate-cemented basaltic sediments from Skinner Ridge and Wildcat Ridge, respectively.

Additionally, one sample of loose regolith was cached at Hidden Harbor. The sample and its backup are named Atmo Mountain and Crosswind Lake. It appears as this regolith is a mix of sedimentary and igneous dust collected from an inactive mega ripple. In texture, it is a mix of coarse grains (<5 mm) and finer sand (~150 μm). The alteration of the different phases appears to be heterogeneous.

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Abrasion patch and Watson camera images of loose regolith cached from the delta front at the Hidden Harbor.

 

Tags: Mars Sample Return Analogue Sample Library, Mars Sample Return, Three Forks Depot, space mission
Published Nov. 13, 2024 12:58 PM - Last modified July 30, 2025 10:42 AM