Statistical characterization of PIXL trace element detection limits

Christian, John R.; VanBommel, Scott J.; Elam, William T.; Ganly, Brianna; Hurowitz, Joel A.; Heirwegh, Christopher M.; Allwood, Abigail C.; Clark, Benton C.; Kizovski, Tanya V.; Knight, Abigail L.

doi:10.1016/j.actaastro.2023.08.032

Cited by 4 publications

(1 citation statement)

References 33 publications

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“…As a proof-of-concept, we applied our model to the average elemental abundance composition from Mars regolith samples as determined by Perseverance's Planetary Instrument for X-ray Lithochemistry (PIXL; Christian et al, 2023) (Table 4). Our model computes a 73.5% probability that the OC abundance is low ([OC] < 2.5 wt% TOC), a 17.8% probability that it is moderately abundant in OC (2.5 wt% < [OC] < 10.0 wt%), and an 8.2% probability that OC is high in abundance (10.0 wt% < [OC]).…”

Section: Application Of a Pre-trained Model To Mars Datamentioning

confidence: 99%

Leveraging Machine Learning Approaches to Predict Organic Carbon Abundance in Mars‐Analog Hypersaline Lake Sediments

Nichols,

Pontefract,

Masterson

et al. 2024

Journal of Geophysical Research: Machine Learning and Computati

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Modern advancements in laboratory and instrumental techniques in astrobiology have improved our life detection capabilities on both Earth and beyond. These advancements have also increased the complexity of data often resulting in data sets that are characterized by complex and non‐linear relationships. Machine learning methods are underutilized in astrobiology; however, these methods are extremely effective at revealing structure and patterns in complex data sets when paired with the right algorithms. Here, we employ a series of classification and regression algorithms to predict the abundance of organic carbon (OC) from X‐ray fluorescence (XRF) heavy element (>Mg) data in dynamic Mars‐analog hypersaline lake sediments. More specifically, we constructed models using the random forest, k‐nearest neighbors (KNN), support vector machine, and logistic regression algorithms. Overall, our trained models showed good performance with predicting the abundance of OC, with accuracies from 80% to 94%. Machine learning approaches such as classification and regression algorithms offer insight into complex data while providing agnostic insights, ultimately creating a more efficient search for OC. We applied our trained model on XRF data from Martian soil using rover‐based (PIXL) and orbital (Odyssey) data sets to produce probability predictions of OC abundance. Our predictions show a high probability that OC abundance is low which is comparable to OC data from recently landed missions. These results highlight the potential for predictive machine learning models to be trained on data from analog environments on Earth and then applied to extraterrestrial targets, ultimately, improving life detection efforts.

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Section: Application Of a Pre-trained Model To Mars Datamentioning

confidence: 99%