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The goals of NASA's Mars 2020 mission include searching for evidence of ancient life on Mars, studying the geology of Jezero crater, understanding Mars' current and past climate, and preparing for human exploration of Mars. During the mission's first science campaign, the Perseverance rover's SHERLOC deep UV Raman and fluorescence instrument collected microscale, two‐dimensional Raman and fluorescence images on 10 natural (unabraded) and abraded targets on two different Jezero crater floor units: Séítah and Máaz. We report SHERLOC Raman measurements collected during the Crater Floor Campaign and discuss their implications regarding the origin and history of Séítah and Máaz. The data support the conclusion that Séítah and Máaz are mineralogically distinct igneous units with complex aqueous alteration histories and suggest that the Jezero crater floor once hosted an environment capable of supporting microbial life and preserving evidence of that life, if it existed.

RNA-directed recombination can be used to catalyze a disproportionation reaction among small RNA substrates to create new combinations of sequences. But the accommodation of secondary and tertiary structural constraints in the substrates by recombinase ribozymes has not been explored. Here, we show that the Azoarcus group I intron can recombine oligoribonucleotides to construct class I ligase ribozymes, which are catalytically active upon synthesis. The substrate oligonucleotides, ranging in size from 58 to 104 nucleotides (nt), along with the 152-nt ligase ribozymes they reconstitute, can contain significant amounts of secondary structure. However, substrate recognition by the Azoarcus ribozyme depends on the existence of a single accessible CAU triplet for effective recombination. A biphasic temperature reaction profile was designed such that the sequential recombination/ligation events could take place in a thermocycler without human intervention. A temperaturedependent pH shift of the reaction buffer contributes to the success of the net reaction. When the substrate for the ligase ribozyme is introduced into the reaction mixture, as much as 11% can be observed being converted to product by the recombined ligase in the same reaction vessel. Recombination followed by ligation can also occur under isothermal conditions at 37 C. Tertiary structure formation of the ligase upon construction can provide some protection from cleavage by the Azoarcus ribozyme when compared to the constituent substrates. These data suggest that RNA-directed recombination can, in fact, articulate complex ribozymes, and that there are logical rules that can guide the optimal placement of the CAU recognition sequence.

The presence and distribution of preserved organic matter on the surface of Mars can provide key information about the Martian carbon cycle and the potential of the planet to host life throughout its history. Several types of organic molecules have been previously detected in Martian meteorites1 and at Gale crater, Mars2–4. Evaluating the diversity and detectability of organic matter elsewhere on Mars is important for understanding the extent and diversity of Martian surface processes and the potential availability of carbon sources1,5,6. Here we report the detection of Raman and fluorescence spectra consistent with several species of aromatic organic molecules in the Máaz and Séítah formations within the Crater Floor sequences of Jezero crater, Mars. We report specific fluorescence-mineral associations consistent with many classes of organic molecules occurring in different spatial patterns within these compositionally distinct formations, potentially indicating different fates of carbon across environments. Our findings suggest there may be a diversity of aromatic molecules prevalent on the Martian surface, and these materials persist despite exposure to surface conditions. These potential organic molecules are largely found within minerals linked to aqueous processes, indicating that these processes may have had a key role in organic synthesis, transport or preservation.

An RNA-DNA World could arise from an all-RNA system with the development of as few as three ribozymes-a DNA-dependent RNA polymerase, an RNA-dependent DNA polymerase, and a catalyst for the production of DNA nucleotides. A significant objection to DNA preceding proteins is that RNA has not been shown to catalyze the production of DNA. However, RNA- and DNAzymes have been recently discovered that catalyze chemical reactions capable of forming deoxyribose, such as mixed aldol condensation of 5'-glyceryl- and 3'-glycoaldehyde-terminated DNA strands. Thus, the only remaining obstacles to RNA-catalyzed in vitro DNA synthesis are alterations of substrate and template specificities of known ribozymes. The RNA-DNA World lessens genomic size constraints through a relaxed error threshold, affording the evolutionary time needed to develop protein synthesis. Separation of information from catalyst enables genotype and phenotype to be readily discriminated by absence or presence, respectively, of the 2'-OH. Novel ribozymes that arise through mutation can be preserved in DNA by reverse transcription, which makes them much more likely to be retained than in an RNA-genome milieu. The extra degree of separation between protein and mRNA, in terms of identifying and then retaining a useful enzyme, may have in fact necessitated storing information in DNA prior to the advent of translation.