Ether in the observed concentrations spontaneously, constitutes a potential DUV Raman biosignature, the apparent sensitivity from the cellular spectrum to tertiary structure gives direct proof of largerscale structure and complexity that cannot exist in abiotic systems, strengthening the interpretation of biogenicity. It seems that, from a spectral perspective, the cell is certainly more than the sum of its components. Deep UV Raman spectroscopy has been chosen as an instrument on the Mars 2020 rover in part as a result of its sensitivity and specificity for the detection of aromatic organic molecules (Beegle et al., 2015). We do not predict here the distinct aromatic organics that might be detected on Mars nor do we attempt to approximate the mineral matrix in which they may be preserved. Rather we demonstrate the significance of molecular complexity towards the interpretation of DUV Raman Fluorescein-DBCO Epigenetic Reader Domain spectra of aromatic organic molecules fundamental to terrestrial life. The mechanisms that led towards the structural organization of pre-biotic organic compounds into N-Acetyl-L-tryptophan Metabolic Enzyme/Protease complicated assemblages conferring the functions of power transduction, replication, and facts storage are at the moment unknown. It can be argued that the emergence of particularly structured functional complexity gave rise to molecular assemblages capable of preforming the functions that we associate with life. At a standard level, these processes harness absolutely free power to predictably and systematically create particular outcomes that devoid of facilitation or catalysis by living systems wouldn’t be predicted to happen. A defining characteristic of life should be to make low probability outcomes reflected in characteristic enrichments of specific organic molecules (e.g., McKay, 2004; Des Marais et al., 2008; Des Marais, 2013; Mustard et al., 2013). One example is Fischer-Tropsch-Type synthesis is hypothesized to account for amino acids in carbonaceous chondrites top to a thermodynamically driven distribution characterized by a lower in abundance with escalating carbon chain length (Donnelly and Satterfield, 1989) as recorded inside the organic inventory of amino acids in extraterrestrial samples (e.g., Pizzarello et al., 2006) whereas biogenic processes enrich thermodynamically expensive, structurally complex, molecules including C17 31 alkanes and aromatic rings (Lovelock, 1965; Scalanand Smith, 1970; Amend and Shock, 1998; Kuhn et al., 2010). Biosignatures reflect the persistence of these low probability outcomes, recording the mechanisms of energy capture and transduction into the unlikely emergence of complexity. It’s established that just identifying aromatic molecules will not constitute proof of life. We show that molecular complexity is considerable and the DUV Raman spectra of those molecules may be made use of to define a threshold for aromatic organic molecules uniquely connected with life. The premise of astrobiology relies around the assumption that the activity of living organisms will lead to the formation of geochemical, molecular, andor structural patterns which can be each recognizable and distinguishable in the atmosphere in which they formed and that their presence is statistically unachievable within a purely abiotic technique (Cady et al., 2003; Des Marais et al., 2008; Summons et al., 2008; Mustard et al., 2013). Whilst it’s not anticipated that life beyond Earth would necessarily be comprised of your same subset of organic molecules, specificity and patterns indicative of biological complexity is believed to be a.