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MarsSat: assured communication with Mars.

The author developed the MarsSat concept during the 1990s. For this task, he designed a class of orbits to solve the problem of communicating with crews on Mars when the planet is in solar conjunction as seen from Earth, a planetary configuration that occurs near the midpoint of a conjunction class mission to Mars. This type of orbit minimizes the distance between Mars and the communications satellite; thus, minimizing the size, weight, and power requirements, while providing a simultaneous line-of-sight to both Earth and Mars. The MarsSat orbits are solar orbits that have the same period as Mars, but are inclined a few degrees out of the plane of the Mars orbit and also differ in eccentricity from the orbit of Mars. These differences cause a spacecraft in this orbit to rise North of Mars, then fall behind Mars, then drop South of Mars, and then pull ahead of Mars, by some desired distance in each case-typically about 20 million kilometers-in order to maintain an angular separation of a couple of degrees as seen from a point in the orbit of Earth on the opposite side of the Sun. A satellite in this type of orbit would relay communications between Earth and Mars during the period of up to several weeks, when direct communication is blocked by the Sun. These orbits are far superior for this purpose when compared to stationing a satellite at one of the Sun-Mars equilateral Lagrangian points, L(4) or L(5), for two reasons. First, L(4) and L(5) are 228 million kilometers from Mars, about 10 times the distance of a spacecraft in one of the MarsSat orbits, and by virtue of the inverse-square law, all other things being equal, the signal strength received at L(4) or L(5) would be one percent of the signal strength received by a spacecraft in one of the MarsSat orbits. Thus, a relay satellite stationed at L(4) or L(5) would have to be that much more powerful to receive data at the same rate, with concomitant increases in spacecraft size and weight. Second, a number of Martian Trojan asteroids have been discovered at the Sun-Mars L(4) and L(5) points, and there are probably countless smaller objects that have collected in these regions that pose a significant threat to any spacecraft located there.

Journal Article↗

Survival of endospores of Bacillus subtilis on spacecraft surfaces under simulated martian environments: implications for the forward contamination of Mars.

Experiments were conducted in a Mars simulation chamber (MSC) to characterize the survival of endospores of Bacillus subtilis under high UV irradiation and simulated martian conditions. The MSC was used to create Mars surface environments in which pressure (8.5 mb), temperature (-80, -40, -10, or +23 degrees C), gas composition (Earth-normal N2/O2 mix, pure N2, pure CO2, or a Mars gas mix), and UV-VIS-NIR fluence rates (200-1200 nm) were maintained within tight limits. The Mars gas mix was composed of CO2 (95.3%), N2 (2.7%), Ar (1.7%), O2 (0.2%), and water vapor (0.03%). Experiments were conducted to measure the effects of pressure, gas composition, and temperature alone or in combination with Mars-normal UV-VIS-NIR light environments. Endospores of B. subtilis, were deposited on aluminum coupons as monolayers in which the average density applied to coupons was 2.47 x 10(6) bacteria per sample. Populations of B. subtilis placed on aluminum coupons and subjected to an Earth-normal temperature (23 degrees C), pressure (1013 mb), and gas mix (normal N2/O2 ratio) but illuminated with a Mars-normal UV-VIS-NIR spectrum were reduced by over 99.9% after 30 sec exposure to Mars-normal UV fluence rates. However, it required at least 15 min of Mars-normal UV exposure to reduce bacterial populations on aluminum coupons to non-recoverable levels. These results were duplicated when bacteria were exposed to Mars-normal environments of temperature (-10 degrees C), pressure (8.5 mb), gas composition (pure CO2), and UV fluence rates. In other experiments, results indicated that the gas composition of the atmosphere and the temperature of the bacterial monolayers at the time of Mars UV exposure had no effects on the survival of bacterial endospores. But Mars-normal pressures (8.5 mb) were found to reduce survival by approximately 20-35% compared to Earth-normal pressures (1013 mb). The primary implications of these results are (a) that greater than 99.9% of bacterial populations on sun-exposed surfaces of spacecraft are likely to be inactivated within a few tens of seconds to a few minutes on the surface of Mars, and (b) that within a single Mars day under clear-sky conditions bacterial populations on sun-exposed surfaces of spacecraft will be sterilized. Furthermore, these results suggest that the high UV fluence rates on the martian surface can be an important resource in minimizing the forward contamination of Mars.

Atmospheric Pressure↗

Molecular adsorbent recirculating system (MARS).

INTRODUCTION: Molecular adsorbent recirculating system (MARS) for albumin liver dialysis has been used as a bridge to liver transplantation in patients with fulminant hepatic failure (FHF). This review examines the available data on its clinical use, its technical aspects and present gaps in knowledge. METHODS: Peer-reviewed journals and monographs on the subject were covered. RESULTS: FHF is associated with elevation in various substances including bilirubin, ammonia, lactate, free fatty acids and aromatic amino acids. Some of these toxic metabolites, such as ammonia and bilirubin, are believed to be central to the clinical manifestations of hepatic encephalopathy and acute renal failure. MARS ameliorates both biochemical and clinical manifestations of FHF by removing both water-soluble and protein-bound toxins. Among the benefits of MARS is the attenuation of severe cerebral oedema and raised intracranial pressure found in FHF, possibly through reduction in high concentrations of these toxins. Although MARS has been shown to be useful in FHF, its clinical efficacy in subfulminant hepatic failure and less severe forms of acute liver failure (ALF) remains uncertain. The current literature also suggests that it may be beneficial to treat cases of acute-on-chronic liver failure (AoCLF). Deranged systemic chemistries can be similarly ameliorated, but the impact of MARS on the natural history of AoCLF remains uncertain. The difficulty lies in being able to accurately quantify residual liver function and variability in the course of acute intercurrent events. The broader question is whether MARS can favourably change the natural history of ALF and FHF. For this, large multi-centre, randomised controlled trials are needed. Furthermore, it is also uncertain how hepatic excretory-assist devices, such as MARS, compare with bio-artificial liver-assist devices which have both synthetic and excretory hepatic functions in ALF treatment in intensive care unit patients. Nevertheless, MARS has proven to be a valuable homeostatic tool that may be useful in restoring the biochemical and clinical status quo in much the same way that continuous veno-venous haemofiltration and mechanical ventilation provide temporary artificial organ support while these organs are in distress. This is the evolving concept of multi-organ support therapy. Other major unresolved issues with MARS include the timing of initiation of albumin liver dialysis, the clinical and/or biochemical parameters to base this decision on, the intensity of MARS therapy (continuous versus intermittent) and the saturation capacity of the system for different metabolites in intermittent MARS. CONCLUSIONS: MARS is an effective and, thus far, safe homeostatic tool in treating FHF. More studies are needed to delineate its role as a homeostatic tool in less severe forms of ALF, including that which occurs in multi-organ failure and in AoCLF. Other studies need to focus on the optimal timing of initiation of and intensity of MARS albumin liver dialysis. The larger issue is to compare MARS with bio-assist liver devices in treating the whole spectrum of ALF.

Albumins↗

[Isolation and functional analysis of tobacco MARs].

Two new MAR segments (M14 and M17) were cloned from tobacco genome. Both of the sequences contained several typical consensus sequences of MARs, which were different from the original MAR sequence, such as 90%AT-box, A-box, T-box, the base unpairing regions (BUR), autonomously replicating sequences (ARS), the consensus sequence for topoisomerase II, MAR recognition sequence (MRS), origin of replication (ORI), curved DNA motifs and ATATTT et al. To investigate the effects of these two sequences on gene expression in transgenic plants, 3 plant expression vectors were constructed with uidA gene coding beta-glucuronidase (GUS) which were flanked on one side and on both sides by the MARs we obtained. These plant expression vectors with one or two MARs were transformed into tobaccos via Agrobacterium-mediated transformation method, with the plant expression vector pCAMBIA2301 without MAR and wild type tobacco as controls. GUS histochemical staining results showed that the uidA gene expressed stably in transgenic tobaccos. Quantitative detection of GUS activity showed that the MARs could increase GUS expression levels in vivo in contrast to the controls, wherever they were flanked on one side or both sides of uidA gene. The vector ligated with MARs in the same direction on both sides of uidA could increase the GUS expression level much better than both vectors which just ligated with single MARs on one side. The former one increased the average GUS activity for 3.14 folds, but 1.56 and 2.43 folds for the latter two vectors with single MARs respectively contrasting to the pCAMBIA2301 control. But the expression differences among individual transformants were still obvious. Therefore, it was concluded that the DNA sequences we obtained in this experiment were two novel MARs and could enhance gene expression in vivo. In the meanwhile, although the numbers of the MARs typical motifs in M14 were more than in M17, especially the 90% AT box which had been considered to be the highest correlative motif with binding strength in vitro, the enhancement of gene expression was lower yet, which implied no correlation between improvement of gene expression and binding strength between MARs and nuclear matrix in vitro.

Cloning, Molecular↗

marA locus causes decreased expression of OmpF porin in multiple-antibiotic-resistant (Mar) mutants of Escherichia coli.

Mar (multiple antibiotic resistant) mutants of Escherichia coli express chromosomally mediated resistance to a variety of structurally unrelated hydrophilic and hydrophobic antibiotics. Insertion of transposon Tn5 into the marA locus at min 34.05 on the chromosome completely reverses the Mar phenotype (A. M. George and S. B. Levy, J. Bacteriol. 155:531-540, 1983). We found that among changes in the outer membrane of Mar mutants, porin OmpF was greatly reduced, although Mar mutants were more resistant than cells lacking only OmpF. Transduction of the marA region from a Mar strain, but not a wild-type strain, led to loss of OmpF. P1 transduction of marA::Tn5 into a Mar mutant partially restored OmpF levels. Therefore, OmpF reduction required a mutation in the marA region. Mar mutants of an ompF-lacZ operon fusion strain expressed 50 to 75% of the beta-galactosidase activity of the isogenic non-Mar parental strain, while Mar mutants of a protein fusion strain expressed less than 10% of the enzyme activity in the non-Mar strain. These changes were completely reversed by insertion of marA::Tn5. The responsiveness of OmpF-LacZ to osmolarity and temperature changes was similar in Mar and wild-type strains. Although some transcriptional control may have been present, OmpF reduction appeared to occur primarily by a posttranscriptional mechanism. The steady-state levels of ompF mRNA were twofold lower and the mRNA was five times less stable in the Mar mutant than in the wild-type strain. Expression of micF, which lowers ompF mRNA levels, was elevated in Mar strains, as revealed by a micF-lacZ fusion. Studies with strains deleted for the micF locus showed that the marA-dependent reduction of OmpF required an intact micF locus. Our findings suggest that the marA locus directly or indirectly increases micF expression, causing a posttranscriptional decrease in ompF mRNA and reduced amounts of OmpF.

Bacterial Outer Membrane Proteins↗

The matrix attachment regions (MARs) associated with the Heat Shock Cognate 80 gene ( HSC80) of tomato represent specific regulatory elements.

Matrix Attachment Regions (MARs) flank certain plant genes and appear in certain cases to be necessary for their proper regulation. For example, we previously demonstrated that the MARs and introns from the Heat Shock Cognate 80 gene of tomato (HSC80) are necessary for efficient expression of HSC80-based transgenes. MARs may exert their effect by anchoring the ends of a chromatin loop to the nuclear matrix, thereby establishing an independent chromatin domain. Alternatively, MARs may facilitate interactions between activating complexes and DNA. In the first case, MARs should enhance the expression of most genes, while in the latter case, their action might be gene-specific. We addressed this problem by testing whether the HSC80 MARs affected the regulation of an unrelated transgene. We constructed a chimeric transgene composed of the Arabidopsis ADENINE PHOSPHORIBOSYLTRANSFERASE (APT) promoter fused to the maize gene Lc, which encodes a regulator of anthocyanin synthesis, and compared the expression of Lc in Arabidopsis transparent testa glabra (ttg) mutants (which lack anthocyanin pigments) transformed with transgene constructs incorporating the MARs or control DNA fragments that do not bind to the nuclear matrix. Quantitative RT-PCR analysis was used to compare Lc expression in the different transgenic lines. Whether the APT-Lc transgene was flanked by the HSC80 MARs or a control fragment had no effect on expression, while the use of a different MAR, the ARS1 MAR from yeast, significantly decreased expression (P=0.03). Comparison of single-copy and multicopy T-DNA insertions indicated that neither the HSC80 MARs nor the ARS1 MAR could protect the APT-Lc transgene from the negative effect of the integration of multiple copies. In conclusion, this work supports a model in which different regulatory elements within the HSC80 locus interact with the nuclear matrix to induce transcriptional competence.

Adenine Phosphoribosyltransferase↗

Matrix attachment regions (MARs) enhance transformation frequencies and reduce variance of transgene expression in barley.

Nuclear matrix attachment regions (MARs) are defined as genomic DNA sequences, located at the physical boundaries of chromatin loops. They are suggested to play a role in the cis unfolding and folding of the chromatin fibre associated with the regulation of gene transcription. Inclusion of MARs in transgene cassettes enhances their expression and reduces position-effect variations in the transgenic host. The present study is the first to investigate the influence of MAR sequences on transformation frequencies and transgene expression in barley, which is highly relevant to the future improvement of this crop by biotechnology. Two plant MAR sequences were tested both for their ability to bind to the nuclear matrix of barley leaf nuclei and to regulate the expression of a reporter gene in transgenic barley. Competitive in vitro MAR binding assays with the 520 bp P1-MAR from soybean and the 516 bp TBS-MAR from petunia revealed that only the P1-MAR had specific binding affinity for barley nuclear matrices. The barley transformation frequency with the uidA reporter gene was increased 2-fold when the gene was flanked with either the P1-MAR or TBS-MAR, while the gene copy number was strongly reduced. The presence of P1-MAR sequences increased the mean activity and reduced the variance in expression of a co-integrated reporter gene in barley consistent with the proposed model of MAR activity.

Cells, Cultured↗

In vitro comparison of the molecular adsorbent recirculation system (MARS) and single-pass albumin dialysis (SPAD).

The detoxification capacities of single-pass albumin dialysis (SPAD), the molecular adsorbents recirculation system, (MARS) and continuous veno-venous hemodiafiltration (CVVHDF) were compared in vitro. In each experiment 4,100 mL of toxin-loaded human plasma was processed for 6.5 hours. MARS treatment (n = 6) was undertaken in combination with CVVHDF. For SPAD (n = 6) and CVVHDF (n = 6) a high-flux hollow fiber hemodiafilter (identical to the MARS filter) was used. Levels of ammonia, urea, creatinine, bilirubin, and bile acids were determined. Concentrations before and after application of detoxification procedures were expressed as differences and were compared using the Kruskal-Wallis test. Post hoc comparisons for pairs of groups were adjusted according to Bonferroni-Holm. Time, group, and interaction effects were tested using the nonparametric ANOVA model for repeated measurements. SPAD and CVVHDF induced a significantly greater reduction of ammonia levels than MARS. No significant differences were found among SPAD, MARS, and CVVHDF with respect to other water-soluble substances. SPAD induced a significantly greater reduction in bilirubin levels than MARS. Reductions in bile acid levels were similar for SPAD and MARS. When operating MARS in continuous veno-venous hemodialysis mode, as recommended by the manufacturer, no significant differences in the removal of bilirubin, bile acids, urea, and creatinine were found. However, MARS in continuous veno-venous hemodialysis mode was significantly less efficient in removing ammonia than MARS in CVVHDF mode. In conclusion, the detoxification capacity of SPAD is similar to or even greater than that of MARS.

Hemodialysis Solutions↗

Economic evaluation of the artificial liver support system MARS in patients with acute-on-chronic liver failure.

BACKGROUND: Acute-on-chronic liver failure (ACLF) is a life threatening acute decompensation of a pre-existing chronic liver disease. The artificial liver support system MARS is a new emerging therapeutic option possible to be implemented in routine care of these patients. The medical efficacy of MARS has been demonstrated in first clinical studies, but economic aspects have so far not been investigated. Objective of this study was to estimate the cost-effectiveness of MARS. METHODS: In a clinical cohort trial with a prospective follow-up of 3 years 33 ACLF-patients treated with MARS were compared to 46 controls. Survival, health-related quality of life as well as direct medical costs for in- and outpatient treatment from a health care system perspective were determined. Based on the differences in outcome and indirect costs the cost-effectiveness of MARS expressed as incremental costs per life year gained and incremental costs per QALY gained was estimated. RESULTS: The average initial intervention costs for MARS were 14600 EUR per patient treated. Direct medical costs over 3 years follow up were overall 40000 EUR per patient treated with MARS respectively 12700 EUR in controls. The 3 year survival rate after MARS was 52% compared to 17% in controls. Kaplan-Meier analysis of cumulated survival probability showed a highly significant difference in favour of MARS. Incremental costs per life-year gained were 31400 EUR; incremental costs per QALY gained were 47200 EUR. CONCLUSION: The results after 3 years follow-up of the first economic evaluation study of MARS based on empirical patient data are presented. Although high initial treatment costs for MARS occur the significantly better survival seen in this study led to reasonable costs per live year gained. Further randomized controlled trials investigating the medical efficacy and the cost-effectiveness are recommended.

Journal Article↗

Characterization of randomly-obtained matrix attachment regions (MARs) from higher plants.

Matrix attachment regions (MARs) can be operationally defined as DNA fragments that bind to the nuclear matrix. We have created a library of randomly obtained MARs from tobacco (Nicotiana tobacum) by cloning DNA fragments that co-isolate with nuclear matrixes prepared by a method involving lithium diiodosalicylate. The interactions of several of the cloned MARs with nuclear matrixes were tested by an in vitro binding assay in which genomic DNA was used as competitor. Based on this assay, the MARs were classified as strong, medium, and weak binders. Examples of each of the binding classes were further studied by in vitro binding using self- and cross-competition. Estimates of dissociation constants for several MARs ranged from 6 to 11 nM and correlated inversely with binding strength. The number of binding sites per matrix for several MARs ranged from 4 x 10(5) to 9 x 10(5) and correlated directly with binding strength. We conclude that binding strength, as we have measured it, is a function of both numbers of binding sites and affinity for the sites. The tobacco MARs were sequenced and analyzed for overall AT content, for distribution of AT-rich regions, and for the abundance of several MAR-related motifs. Previously identified MAR motifs correlate to various degrees with binding strength. Notably, the Drosophila topoisomerase II motif does not correlate with binding strength of the tobacco MARs. A newly identified motif, the "90%AT Box," correlates better with binding strength than any of the previously identified motifs we investigated.

Base Sequence↗

A short synthetic MAR positively affects transgene expression in rice and Arabidopsis.

Matrix Attachment Regions (MARs) are DNA elements that are thought to influence gene expression by anchoring active chromatin domains to the nuclear matrix. When flanking a construct in transgenic plants, MARs could be useful for enhancing transgene expression. Naturally occurring MARs have a number of sequence features and DNA elements in common, and using different subsets of these sequence elements, three independent synthetic MARs were created. Although short, these MARs were able to bind nuclear scaffold preparations with an affinity equal to or greater than naturally occurring plant MARs. One synthetic MAR was extensively tested for its effect on transgene expression, using different MAR orientations, plant promoters, transformation methods and plant species. This MAR was able to increase average transgene expression and produced integration patterns of lower complexity. These data show the potential of making well defined synthetic MARs and using them to improve transgene expression.

Journal Article↗

A MAR-like antibody in a DCWe/DCWe person.

BACKGROUND: MAR (RH51), a high-incidence antigen in the Rh blood group system, is absent from RBCs with a double dose of CW or CX or a single dose each of CW and CX antigens, as well as from rare Rh phenotypes including D- - and Rh(null). The MAR antigen is associated with the presence of Ala36 and Gln41 on the RhCe protein. The original example of anti-MAR, described in 1994, was made by a DCWe/DCXe woman. It was possible that the antibody directed against a high-incidence antigen in the Rh system made by a DCXe/DCXe woman (CM) in 1983 was anti-MAR. CASE REPORT: A 52-year-old, multiply transfused, white woman (CJ) with pre-existing anti-c, -E, and -Jk(a) presented for preoperative work-up for her fifth open heart procedure. The strength of the reaction of her RBCs with anti-CW suggested a double dose of CW antigen. Her serum, which unexpectedly was strongly reactive with c-, E-, Jk(a-) RBCs by PEG indirect antiglobulin test, was incubated with E-c-, Jk(a-) RBCs, and an eluate was prepared. This eluate reacted 3+ with E-c-, Jk(a-) RBCs but did not react with Rh(null) (n = 5), - - (3), DCW- (2), Dc- (1), or DCWe/DCWe (1) RBCs. Two related DCXe/DCXe and two unrelated DCWe/DCXe RBC samples were weakly agglutinated. The patient's RBCs were negative with the original anti-MAR but reacted as strongly as the positive control RBCs with the antibody made by the DCXe/DCXe person. CONCLUSION: This is the first example of a MAR-like antibody made by a DCWe/DCWe woman. The specificity cannot be called anti-MAR, because some MAR-negative samples react, albeit weakly. The original anti-MAR, made by a DCWe/DCXe woman, did not react with DCWe/DCWe, DCWe/DCXe, or DCXe/DCXe RBCs. It is apparent that the specificity of "anti-MAR" differs slightly, depending on the CW/CX status of the antibody maker.

Antibody Specificity↗

Antigenic variation (mar mutations) in herpes simplex virus glycoprotein B can induce temperature-dependent alterations in gB processing and virus production.

Monoclonal antibody-resistant (mar) mutants altered in the antigenic structure of glycoprotein B (gB) of herpes simplex virus type 1, strain KOS-321, were selected by neutralization with each of six independently derived gB-specific monoclonal antibodies. Analysis of the reactivity patterns of these mar mutants with a panel of 16 virus-neutralizing monoclonal antibodies identified at least five nonoverlapping epitopes on this antigen, designated groups I through V. Multiple mar mutations were also introduced into the gB structural gene by recombination and sequential antibody selection to produce a set of mar mutants with double, triple, and quadruple epitope alterations. Group II (B2) and group III (B4) antibodies were used to select the corresponding mutants, mar B2.1 and mar B4.1, which in addition to carrying the mar phenotype were temperature sensitive (ts) for processing of the major partially glycosylated precursor of gB, pgB (Mr = 107,000), to mature gB (Mr = 126,000) and showed reduced levels of gB on the cell surface at high temperature (39 degrees C). These mutants were not, however, ts for production of infectious progeny. A recombinant virus, mar B2/4.1, carrying both of these alterations was ts for virus production and failed to produce and transport any detectable mature gB to the cell surface at 39 degrees C. Rather, pgB accumulated in the infected cell. Revertants of the ts phenotype, isolated from virus plaques at 39 degrees C, regained the B2 but not the B4 epitope and were phenotypically indistinguishable from the mar B4.1 parent. Finally, it was shown that group II (B5) and group III (B4) antibodies failed to immunoprecipitate pgB (39 degrees C) produced by ts gB mutants of herpes simplex virus type 1 which were not selected with monoclonal antibodies. Taken together, our findings indicate that (i) mar mutations can alter antigenic as well as other functional domains of gB, namely, the domain(s) involved in processing and infectivity, and (ii) group II and group III epitopes lie within an essential functional domain of gB which is a target for ts gB mutations.

Antibodies, Monoclonal↗

Reflectance and Mossbauer spectroscopy of ferrihydrite-montmorillonite assemblages as Mars soil analog materials.

Spectroscopic analyses show that Fe(3+)-doped smectites prepared in the laboratory exhibit important similarities to the soils on Mars. Ferrihydrite has been identified as the interlayer ferric component in Fe(3+)-doped smectites by a low quadrupole splitting and magnetic field strength of approximately 48 tesla in Mossbauer spectra measured at 4.2 K, as well as a crystal field transition at 0.92 micrometer. Ferrihydrite in these smectites explains features in the visible-near infrared region that resemble the energies and band strengths of features in reflectance spectra observed for several bright regions on Mars. Clay silicates have met resistance in the past as Mars soil analogs because terrestrial clay silicates exhibit prominent hydrous spectral features at 1.4, 1.9, and 2.2 micrometers; and these are observed weakly, if at all, in reflectance spectra of Mars. However, several mechanisms can weaken or compress these features, including desiccation under low-humidity conditions. The hydration properties of the interlayer cations also effect band strengths, such that a ferrihydrite-bearing smectite in the Martian environment would exhibit a 1.9 micrometers H2O absorption that is even weaker than the 2.2 micrometers structural OH absorption. Mixing experiments demonstrate that infrared spectral features of clays can be significantly suppressed and that the reflectance can be significantly darkened by mixing with only a few percent of a strongly absorbing opaque material. Therefore, the absolute reflectance of a soil on Mars may be disproportionately sensitive to a minor component. For this reason, the shape and position of spectral features and the chemical composition of potential analogs are of utmost importance in assessing the composition of the soil on Mars. Given the remarkable similarity between visible-infrared reflectance spectra of soils in bright regions on Mars and Fe(3+)-doped montmorillonites, coupled with recent observations of smectites in SNC meteorites and a weak 2.2 micrometers absorption in some Mars soils, ferrihydrite-bearing smectites warrant serious consideration as a Mars soil analog.

Aluminum Silicates↗

The biological terraforming of Mars: planetary ecosynthesis as ecological succession on a global scale.

Mars is bitterly cold and dry, but robotic spacecraft have returned abundant data that indicate Mars once had a much warmer and wetter climate in the past. These data, the basis of the search for past or present life on Mars, suggest the possibility of returning Mars to its previous climate by global engineering techniques. Greenhouse gases, such as perfluorocarbons, appear to be the best method for warming Mars and increasing its atmospheric density so that liquid water becomes stable. The process of making Mars habitable for terrestrial organisms is called terraforming or planetary ecosynthesis. The process of introducing terrestrial ecosystems to Mars can be compared with a descent down a high mountain. Each drop in elevation results in a warmer, wetter climate and more diverse biological community. Beginning with a polar desert, the sequence of ecosystems passes through tundra, boreal forest, and temperate ecosystems where moisture determines the presence of desert, grassland, or forest. This model suggests a sequence for the introduction of ecosystems to Mars and the communities to search for potential colonizing species for Mars.

Ecosystem↗

Searching for signatures of life on Mars: an Fe-isotope perspective.

Recent spacecraft and lander missions to Mars have reinforced previous interpretations that Mars was a wet and warm planet in the geological past. The role of liquid water in shaping many of the surface features on Mars has long been recognized. Since the presence of liquid water is essential for survival of life, conditions on early Mars might have been more favourable for the emergence and evolution of life. Until a sample return mission to Mars, one of the ways of studying the past environmental conditions on Mars is through chemical and isotopic studies of Martian meteorites. Over 35 individual meteorite samples, believed to have originated on Mars, are now available for lab-based studies. Fe is a key element that is present in both primary and secondary minerals in the Martian meteorites. Fe-isotope ratios can be fractionated by low-temperature processes which includes biological activity. Experimental investigations of Fe reduction and oxidation by bacteria have produced large fractionation in Fe-isotope ratios. Hence, it is considered likely that if there is/were any form of life present on Mars then it might be possible to detect its signature by Fe-isotope studies of Martian meteorites. In the present study, we have analysed a number of Martian meteorites for their bulk-Fe-isotope composition. In addition, a set of terrestrial analogue material has also been analysed to compare the results and draw inferences. So far, our studies have not found any measurable Fe-isotopic fractionation in bulk Martian meteorites that can be ascribed to any low-temperature process operative on Mars.

Biological Evolution↗

HIV-1 integration sites are flanked by potential MARs that alone can act as promoters.

Matrix attachment regions (MARs) are cis regulatory elements that modulate gene expression in a tissue and cell stage specific manner. Recent reports show that viral integration within the genome takes place at nonrandom active genes. We have checked for the presence of MARs in the vicinity of the reported 524 HIV-1 integration sites. Our studies show that in 92.5% cases, MARs flank the integration sites. Similarly, for adeno-associated virus, two potential MARs were present next to the integration site on the human chromosome. Earlier we have shown that short MAR sequences present upstream of HIV-1 LTR promote processive transcription at a distance. Here, using a well-studied IgH-MAR and another potential MAR from p53 promoter, we demonstrate that MARs alone can act as promoters. Thus, we propose that MAR elements near the HIV-1 integration sites can act as potential promoters, which may facilitate proviral integration and transcription.

Chromosome Mapping↗

Treatment of refractory cholestatic pruritus with molecular adsorbent recirculating system (MARS).

UNLABELLED: Pruritus is a common complication of cholestatic liver diseases or liver graft dysfunction. Current medical therapies lack efficacy. The molecular adsorbent recirculating system (MARS) represents an interesting therapeutic option. Our objective was to report our experience in the management of four patients with intractable pruritus with MARS. PATIENTS AND METHODS: The MARS treatment cycle included three consecutive treatments, each of 8 hours duration. The four patients with intractable pruritus who were treated had primary biliary cirrhosis/autoimmune hepatitis overlap syndrome (n = 1), ductopenic allograft rejection (n = 2), or posttransplant cholestatic HCV recurrence (n = 1). Intensity of pruritus was documented 24 hours before as well as 24 hours, 7 and 30 days after MARS therapy, and at the end of follow-up. We measured complete blood cell counts, glucose, BUN, creatinine, sodium, potassium, AST, ALT, GGT, alkaline phosphatase, bilirubin, prothrombin activity, and activated partial thromboplastin time. RESULTS: MARS therapy was well tolerated. Patient 1 experienced temporal relief of pruritus, but needed another MARS cycle because of relapse. Patient 2 experienced partial and temporary relief of pruritus, was listed for retransplantation, and received a liver graft 2 months later. Patient 3 showed a dramatic reduction in the degree of pruritus with MARS. Pruritus in patient 4 decreased promptly with MARS therapy and conversion of immunosuppression to tacrolimus, thereby avoiding retransplantation. CONCLUSION: MARS therapy is a promising, safe therapeutic option to treat refractory pruritus caused by cholestatic liver disorders.

Adult↗