Martian environment and life]

Five conditions for life to arise are discussed with referring to early Martian environment. The key to determine whether any life form appeared on Mars is found to be the early Martian carbon dioxide atmospheric pressure and then the temperature. The importance to determine the heat flow is indicated. The items to be measured for future Martian exploration are listed. The surface materials, which has been poorly understood, are emphasized for further exploration. Two strategies for search for life on Mars, "step by step" strategy and quick strategy, are suggested.     

Pros and cons for Martian life: scientific debate on ALH84001]

Scientific debate related to possible martian life is summarized in this article. Even there is no firm conclusion yet to convince the existence of life on Mars, intensive studies on the meteorite ALH84001 have invoked many valuable findings.     

Magnetite biomineralization and ancient life on Mars

Certain chemical and mineral features of the Martian meteorite ALH84001 were reported in 1996 to be probable evidence of ancient life on Mars. In spite of new observations and interpretations, the question of ancient life on Mars remains unresolved. Putative biogenic, nanometer magnetite has now become a leading focus in the debate.     

Martian channels and the search for extraterrestrial life

Summary The origin of the channels on Mars has been a subject of intense interest since they were first recognized on early Mariner 9 images (Driscoll, 1972; Masursky, 1973). Their presence on the planet, and their striking resemblance to terrestrial flood channels related to glacial outbursts or to dendritic river systems has suggested to most investigators (Baker, 1974, 1977; Nummedal, 1978; Carr, 1979; Masursky et al., 1977) that they were formed by running water. Because life as we know it is dependent on water, the discovery by the Mariner cameras, of watercut channels and volcanoes as a source for water, and water ice in the residual north polar cap by Viking, has reaffirmed the choice of Mars as the best target for the search for extraterrestrial life.     

New insights into ancient seasonal life timers

Organisms must adapt to seasonal changes in the environment and time their physiology accordingly. In vertebrates, the annual change in photoperiod is often critical for entraining the neuroendocrine pathways, which drive seasonal metabolic and reproductive cycles. These cycles depend on thyroid hormone (TH), reflecting its ancestral role in metabolic control. Recent studies reveal that - in mammals and birds - TH effects are mediated by the hypothalamus. Photoperiodic manipulations alter hypothalamic TH availability by regulating the expression of TH deiodinases (DIO). In non-mammalian vertebrates, light acts through extraretinal, 'deep brain' photoreceptors, and the eyes are not involved in seasonal photoperiodic responses. In mammals, extraretinal photoreceptors have been lost, and the nocturnal melatonin signal generated from the pineal gland has been co-opted to provide the photoperiodic message. Pineal function is phased to the light-dark cycle by retinal input, and photoperiodic changes in melatonin secretion control neuroendocrine pathway function. New evidence indicates that these comparatively divergent photosensensory mechanisms re-converge in the pars tuberalis of the pituitary, lying beneath the hypothalamus. In all vertebrates studied, the pars tuberalis secretes thyrotrophin in a light- or melatonin-sensitive manner, to act on neighbouring hypothalamic DIO expressing cells. Hence, an ancient and fundamentally conserved brain thyroid signalling system governs seasonal biology in vertebrates.     

100 kGy gamma-affected microbial communities within the ancient Arctic permafrost under simulated Martian conditions

Extremophiles - This research aimed to investigate the viability and biodiversity of microbial communities within ancient Arctic permafrost after exposure to a gamma-radiation dose of...     

The origin of life: RNA and protein co-evolution on the ancient Earth

How life emerged from simple non-life chemicals on the ancient Earth is one of the greatest mysteries in biology. The gene expression system of extant life is based on the interdependence between multiple molecular species (DNA, RNA, and proteins). While DNA is mainly used as genetic material and proteins as functional molecules in modern biology, RNA serves as both genetic material and enzymes (ribozymes). Thus, the evolution of life may have begun with the birth of a ribozyme that replicated itself (the RNA world hypothesis), and proteins and DNA joined later. However, the complete self-replication of ribozymes from monomeric substrates has not yet been demonstrated experimentally, due to their limited activity and stability. In contrast, peptides are more chemically stable and are considered to have existed on the ancient Earth, leading to the hypothesis of RNA–peptide co-evolution from the very beginning. Our group and collaborators recently demonstrated that (1) peptides with both hydrophobic and cationic moieties (e.g., KKVVVVVV) form β-amyloid aggregates that adsorb RNA and enhance RNA synthesis by an artificial RNA polymerase ribozyme and (2) a simple peptide with only seven amino acid types (especially rich in valine and lysine) can fold into the ancient β-barrel conserved in various enzymes, including the core of cellular RNA polymerases. These findings, together with recent reports from other groups, suggest that simple prebiotic peptides could have supported the ancient RNA-based replication system, gradually folded into RNA-binding proteins, and eventually evolved into complex proteins like RNA polymerase.     

Protoporphyrin ix as a possible ancient photosensitizer: Spectral and photochemical studies

Due to the potential special position of protoporphyrin IX in the evolution of photosynthesis, the absorption and fluorescence characteristics of this pigment and its complexes with human serum albumin (HSA) and basic proteinoid have been studied in parallel with their photochemical activity. The most significant change in the absorption spectrum of PP IX was the appearance of a new maximum at 455 (or 461) nm in the presence of HSA or proteinoid respectively. Some changes in the physicochemical properties of PP IX in different microenvironments have been detected by changes in fluorescence emission and excitation spectra (intensity, quantum yields, position of maxima). The increase of fluorescence quantum yield resulting from the formation of PP IX complexes with HSA or proteinoid correlates with the increase of their photochemical activity. Results obtained are discussed from the point of view of the early evolution of the photosynthetic apparatus.     

A major clade of prokaryotes with ancient adaptations to life on land

Evolutionary trees of prokaryotes usually define the known classes and phyla but less often agree on the relationships among those groups. This has been attributed to the effects of horizontal gene transfer, biases in sequence change, and large evolutionary distances. Furthermore, higher level clades of prokaryote phyla rarely are supported by information from ecology and cell biology. Nonetheless, common patterns are beginning to emerge as larger numbers of species are analyzed with sophisticated methods. Here, we show how combined evidence from phylogenetic, cytological, and environmental data support the existence of an evolutionary group that appears to have had a common ancestor on land early in Earth's history and includes two-thirds of known prokaryote species. Members of this terrestrial clade (Terrabacteria), which includes Cyanobacteria, the gram-positive phyla (Actinobacteria and Firmicutes), and two phyla with cell walls that differ structurally from typical gram-positive and gram-negative phyla (Chloroflexi and Deinococcus-Thermus), possess important adaptations such as resistance to environmental hazards (e.g., desiccation, ultraviolet radiation, and high salinity) and oxygenic photosynthesis. Moreover, the unique properties of the cell wall in gram-positive taxa, which likely evolved in response to terrestrial conditions, have contributed toward pathogenicity in many species. These results now leave open the possibility that terrestrial adaptations may have played a larger role in prokaryote evolution than currently understood.     

High-temperature deep-subsurface microbial communities as a possible equivalent of ancient ecosystems

Microbiological, molecular biological, and radioisotopic studies suggest that active and complex microbial communities exist in the deep layers of the subsurface biosphere. This review discusses only one group of such communities, i.e., those developing at high (above 60°C temperatures). Oil wells, subsurface water reservoirs (e.g., the Great Artesian Basin in Australia), deep mines (in South Africa), and high-temperature horizons below the seafloor in the areas of underwater volcanic activity contain the best-studied high-temperature subsurface ecosystems. These microbial communities differ considerably from one another in biodiversity, initial energy substrate, and major microbiological processes. However, before they can be considered as equivalents of the Earth’s primordial ecosystems, it is necessary to demonstrate that they are energetically independent of the modern biosphere.     

Perchlorate and halophilic prokaryotes: implications for possible halophilic life on Mars

In view of the finding of perchlorate among the salts detected by the Phoenix Lander on Mars, we investigated the relationships of halophilic heterotrophic microorganisms (archaea of the family Halobacteriaceae and the bacterium Halomonas elongata) toward perchlorate. All strains tested grew well in NaCl-based media containing 0.4 M perchlorate, but at the highest perchlorate concentrations, tested cells were swollen or distorted. Some species (Haloferax mediterranei, Haloferax denitrificans, Haloferax gibbonsii, Haloarcula marismortui, Haloarcula vallismortis) could use perchlorate as an electron acceptor for anaerobic growth. Although perchlorate is highly oxidizing, its presence at a concentration of 0.2 M for up to 2 weeks did not negatively affect the ability of a yeast extract-based medium to support growth of the archaeon Halobacterium salinarum. These findings show that presence of perchlorate among the salts on Mars does not preclude the possibility of halophilic life. If indeed the liquid brines that may exist on Mars are inhabited by salt-requiring or salt-tolerant microorganisms similar to the halophiles on Earth, presence of perchlorate may even be stimulatory when it can serve as an electron acceptor for respiratory activity in the anaerobic Martian environment.     

The biogenicity of modern terrestrial roll-up structures and its significance for ancient life on land

Roll-up structures (Roll-ups) are sedimentary structures formed by the desiccation-mediated curling of a surface, cohesive layer into a subcylindrical, coiled shape. Their origin in terrestrial environments has been attributed to the shrinking effect of argillaceous components, while microbes are thought to be the curling agent in intertidal marine settings. Roll-ups also exist in terrestrial environments and the rock record, but their genesis is unclear. Proving a biogenic origin of terrestrial roll-ups would make them excellent biosignatures to track ancient life on land. In this study, we tested the biogenicity of modern roll-ups from arid terrestrial environments, showing that, regardless of their geographic location and textural properties, they invariably contained large and distinct cyanobacterial populations compared to adjacent, non-rolled surface soil. Cyanobacterial populations inhabiting these roll-ups were genetically diverse, but consistently dominated by filamentous, non-heterocystous forms. We could also recreate roll-ups artificially by desiccating clay and organic polysaccharide slurries on sandy substrates, and show that clay roll-ups were less prone to re-form after wetting-and-drying cycles and less resistant to erosion than organically bound or naturally occurring ones. All this evidence suggests that fossil roll-ups found in ancient terrestrial deposits are biogenic features.     

Mitochondrial sequence variation in ancient horses from the Carpathian Basin and possible modern relatives

Movements of human populations leave their traces in the genetic makeup of the areas affected; the same applies to the horses that move with their owners This study is concerned with the mitochondrial control region genotypes of 31 archaeological horse remains, excavated from pre-conquest Avar and post-conquest Hungarian burial sites in the Carpathian Basin dating from the sixth to the tenth century. To investigate relationships to other ancient and recent breeds, modern Hucul and Akhal Teke samples were also collected, and mtDNA control region (CR) sequences from 76 breeds representing 921 individual specimens were combined with our sequence data. Phylogenetic relationships among horse mtDNA CR haplotypes were estimated using both genetic distance and the non-dichotomous network method. Both methods indicated a separation between horses of the Avars and the Hungarians. Our results show that the ethnic changes induced by the Hungarian Conquest were accompanied by a corresponding change in the stables of the Carpathian Basin.     

Solar radiation incident on the Martian surface

Summary Calculations indicate that the maximum daily solar radiation reaching the Martian surface is about 325 cal/cm² during southern hemisphere summer at latitude of about 40°S. In the ultraviolet region of the spectrum, the radiation reaching the surface at wavelengths greater than 2800 Å is within 10% of the radiation incident on the atmosphere. There is significant extinction of radiation in the spectral region near 2500 Å in mid and high latitudes due to absorption of radiation by ozone; radiation reaching the surface may be reduced to one one-thousandth of that incident on the atmosphere during winter. Virtually no radiation of wavelengths less than 1900 Å reaches the surface because of absorption by the large column abundance of carbon dioxide. Daily and latitudinal distributions of radiation are presented for wavelengths of 3000, 2500 and 2000 Å.