Louis N. Irwin

A sulfur-based survival strategy for putative phototrophic life in the venusian atmosphere.

Several observations indicate that the cloud deck of the venusian atmosphere may provide a plausible refuge for microbial life. Having originated in a hot proto-ocean or been brought in by meteorites from Earth (or Mars), early life on Venus could have adapted to a dry, acidic atmospheric niche as the warming planet lost its oceans. The greatest obstacle for the survival of any organism in this niche may be high doses of ultraviolet (UV) radiation. Here we make the argument that such an organism may utilize sulfur allotropes present in the venusian atmosphere, particularly S(8), as a UV sunscreen, as an energy-converting pigment, or as a means for converting UV light to lower frequencies that can be used for photosynthesis. Thus, life could exist today in the clouds of Venus.

The prospect of alien life in exotic forms on other worlds

The nature of life on Earth provides a singular example of carbon-based, water-borne, photosynthesis-driven biology. Within our understanding of chemistry and the physical laws governing the universe, however, lies the possibility that alien life could be based on different chemistries, solvents, and energy sources from the one example provided by Terran biology. In this paper, we review some of these possibilities. Silanes may be used as functional analogs to carbon molecules in environments very different from Earth; solvents other than water may be compatible for life-supporting processes, especially in cold environments, and a variety of energy sources may be utilized, some of which have no Terran analog. We provide a detailed discussion of two possible habitats for alien life which are generally not considered as such: the lower cloud level of the Venusian atmosphere and Titan’s surface environment.

A Two-Tiered Approach to Assessing the Habitability of Exoplanets

In the next few years, the number of catalogued exoplanets will be counted in the thousands. This will vastly expand the number of potentially habitable worlds and lead to a systematic assessment of their astrobiological potential. Here, we suggest a two-tiered classification scheme of exoplanet habitability. The first tier consists of an Earth Similarity Index (ESI), which allows worlds to be screened with regard to their similarity to Earth, the only known inhabited planet at this time. The ESI is based on data available or potentially available for most exoplanets such as mass, radius, and temperature. For the second tier of the classification scheme we propose a Planetary Habitability Index (PHI) based on the presence of a stable substrate, available energy, appropriate chemistry, and the potential for holding a liquid solvent. The PHI has been designed to minimize the biased search for life as we know it and to take into account life that might exist under more exotic conditions. As such, the PHI requires more detailed knowledge than is available for any exoplanet at this time. However, future missions such as the Terrestrial Planet Finder will collect this information and advance the PHI. Both indices are formulated in a way that enables their values to be updated as technology and our knowledge about habitable planets, moons, and life advances. Applying the proposed metrics to bodies within our Solar System for comparison reveals two planets in the Gliese 581 system, GJ 581 c and d, with an ESI comparable to that of Mars and a PHI between that of Europa and Enceladus.

Gene expression following traumatic brain injury in humans : analysis by microarray

Global changes in gene expression were analyzed in pericontusional tissue taken during surgery from 4 patients with traumatic brain injury (TBI), in cerebral infarction tissue from a patient with vasculitis and in normal brain tissue resected during craniotomy for meningioma. Of approximately 1,200 genes showing some level of expression by cDNA microarray hybridization, 104 ( approximately 8%) showed differential expression in traumatized tissue. Genes controlling transcriptional regulation, intermediary and energy metabolism, signal transduction, and intercellular adhesion and recognition were differentially affected most often. Four genes previously shown to be associated with TBI (c-Fos, Jun B, HSP70, and Zif/268) were all found to be up-regulated in at least one TBI patient. Thus, the robust response to TBI of several immediate early genes is confirmed, and a longer list of candidate genes from other functional categories is suggested for further studies aimed at understanding the molecular and cellular consequences of TBI.

Energy cycling and hypothetical organisms in Europa's ocean.

While Europa has emerged as a leading candidate for harboring extraterrestrial life, the apparent lack of a source of free energy for sustaining living systems has been argued. In this theoretical analysis, we have quantified the amount of energy that could in principle be obtained from chemical cycling, heat, osmotic gradients, kinetic motion, magnetic fields, and gravity in Europas subsurface ocean. Using reasonable assumptions based on known organisms on Earth, our calculations suggest that chemical oxidation-reduction cycles in Europas subsurface ocean could support life. Osmotic and thermal gradients, as well as the kinetic energy of convection currents, also represent plausible alternative sources of energy for living systems at Europa. Organisms thriving on these gradients could interact with each other to form the complex energy cycling necessary for establishing a stable ecosystem.

Gene expression in the hippocampus of behaviorally stimulated rats: analysis by DNA microarray

Gene expression in the hippocampus of rats exposed to a brief vigorous swimming task was analyzed by DNA microarray hybridization against 5184 known DNA sequences. Each of 12 rats consistently expressed 17% of the genes probed on the microarrays. Transcripts from genes for energy metabolism, development and differentiation, and gene regulation were expressed in the hippocampus to the highest degree relative to their availability on the microarray. The number of genes that were differentially expressed in behaviorally stimulated compared to undisturbed rats was estimated at 2.7% of all expressed genes. Behavioral effects were relatively greater on expression of genes for control of the cell cycle and apoptosis, development and differentiation, protein processing and gene regulation. The magnitude of differential expression due to behavioral stimulation was lower than that generally reported for developmental processes and disease states. Thus the impact of acute behavioral stimulation on steady-state levels of gene expression was small, but (with four replicates per condition) detectable at a statistically significant level. The effects of behavioral stimulation on transcription may thus involve changes in the expression of a relatively small number of genes to a low but reproducible degree.

Assessing the Plausibility of Life on Other Worlds

As the field of astrobiology matures and search strategies for life on other worlds are developed, the need to analyze in a systematic way the plausibility for life on other planetary systems becomes increasingly apparent. We propose the adoption of a simple plausibility of life (POL) rating system based on specific criteria. Category I applies to any body shown to have conditions essentially equivalent to those on Earth. Category II applies to bodies for which there is evidence of liquid water and sources of energy and where organic compounds have been detected or can reasonably be inferred (Mars, Europa). Category III applies to worlds where conditions are physically extreme but possibly capable of supporting exotic forms of life unknown on Earth (Titan, Triton). Category IV applies to bodies that could have seen the origin of life prior to the development of conditions so harsh as to make its perseverance at present unlikely but conceivable in isolated habitats (Venus, Io). Category V would be reserved for sites where conditions are so unfavorable for life by any reasonable definition that its origin or persistence there cannot be rated a realistic probability (the Sun, gas giant planets). The proposed system is intended to be generic. It assumes that life is based on polymeric chemistry occurring in a liquid medium with uptake and degradation of energy from the environment. Without any additional specific assumptions about the nature of life, the POL system is universally applicable.

Reassessing the Possibility of Life on Venus: Proposal for an Astrobiology Mission

With their similar size, chemical composition, and distance from the Sun, Venus and Earth may have shared a similar early history. Though surface conditions on Venus are now too extreme for life as we know it, it likely had abundant water and favorable conditions for life when the Sun was fainter early in the Solar System. Given the persistence of life under stabilizing selection in static environments, it is possible that life could exist in restricted environmental niches, where it may have retreated after conditions on the surface became untenable. High-pressure subsurface habitats with water in the supercritical liquid state could be a potential refugium, as could be the zone of dense cloud cover where thermoacidophilic life might have retreated. Technology based on the Stardust Mission to collect comet particles could readily be adapted for a pass through the appropriate cloud layer for sample collection and return to Earth.

Scenarios for the evolution of life on Mars

Received 10 March 2005; revised 2 August 2005; accepted 7 September 2005; published 22 November 2005. [1] As the environmental histories of Earth and Mars have diverged drastically after the first few hundred million years, so would the history of any life on them. While Earth has had liquid water on its surface for billions of years, Mars most likely had long dry and cold environments interspersed with warmer and wetter periods. Life thrived on Earth but may have been severely restricted on Mars. There it could be present today in liquid water in or beneath ice sheets or glaciers, in subterranean aqueous reservoirs, especially in regions of elevated heat flow, or in protected habitats such as lava tubes, caves, or cracks and fissures. The potential for life is enhanced in regions where elevated heat flow may occur, such as in parts of the Tharsis and Elysium volcanic provinces. Possible organisms would be chemoautotrophic psychrophiles adapted to a nutrient-poor environment or photoautotrophic life in selected near-surface habitats. Alternatively, life may have evolved alternating cycles between active and dormant forms, in which case microbes could be present in dormant forms close to the surface and in active forms in protected environments. Periodic liquid water on Mars could have provided opportunities for biologic activity, as well as evolutionary progress, at the surface during the short-lived climatic perturbations. Ancient organisms from any of these environments may also have left a detectable fossil record.

Locating potential biosignatures on Europa from surface geology observations.

We evaluated the astrobiological potential of the major classes of geologic units on Europa with respect to possible biosignatures preservation on the basis of surface geology observations. These observations are independent of any formational model and therefore provide an objective, though preliminary, evaluation. The assessment criteria include high mobility of material, surface concentration of non-ice components, relative youth, textural roughness, and environmental stability. Our review determined that, as feature classes, low-albedo smooth plains, smooth bands, and chaos hold the highest potential, primarily because of their relative young age, the emplacement of low-viscosity material, and indications of material exchange with the subsurface. Some lineaments and impact craters may be promising sites for closer study despite the comparatively lower astrobiological potential of their classes. This assessment will be expanded by multidisciplinary examination of the potential for habitability of specific features.