SCYTONEMIN, A CYANOBACTERIAL SHEATH PIGMENT, PROTECTS AGAINST UVC RADIATION: IMPLICATIONS FOR EARLY PHOTOSYNTHETIC LIFE

During the Precambrian, ultraviolet (UV) radiation reaching the Earth's surface, including UVC wavelengths (190–280 nm), was considerably higher than present because of the lack of absorbing gases (e.g. O₂ and O₃) in the atmosphere. High UV flux would have been damaging to photosynthetic organisms exposed to solar radiation. Nevertheless, fossil evidence indicates that cyanobacteria-like ancestors may have evolved as early as 3.5 × 10⁹ yr ago, and were common in shallow marine habitats by 2.5 × 10⁹ years ago. Scytonemin, a cyanobacterial extracellular sheath pigment, strongly absorbs UVC radiation. Exposure to high-irradiance conditions caused cells to synthesize scytonemin and resulted in decreased UVC inhibition of photosynthetic carbon uptake. It was further demonstrated that scytonemin alone was sufficient for substantial protection against UVC damage. This represents the first experimental demonstration of biological protection against UVC radiation in cyanobacteria. These results suggest that scytonemin may have evolved during the Precambrian and allowed colonization of exposed, shallow-water and terrestrial habitats by cyanobacteria or their oxygenic ancestors.     

Photocatalytic antibacterial effects on TiO2-anatase upon UV-A and UV-A/VIS threshold irradiation

Photocatalysis mediated by the anatase modification of titanium dioxide (TiO₂) has shown antibacterial effects in medical applications. The aim of this study was to investigate the possibility of expanding the excitation wavelengths for photocatalytic antibacterial effects from ultraviolet (UV) into the visible light range. After deposition of salivary pellicle and adhesion of Streptococcus gordonii on anatase, different irradiation protocols were applied to induce photocatalysis: ultraviolet A (UV-A) > 320 nm; ultraviolet/visible (UV-A/VIS) light > 380 nm and > 390 nm; and VIS light 400–410 nm. A quartz crystal microbalance with dissipation (QCM-D) tests and microscopic examination were used to observe the photoinduced antibacterial effects. Salivary pellicle could be photocatalytically decomposed under all irradiation protocols. In contrast, effective photocatalytic attack of bacteria could be observed by UV-A as well as by UV-A/VIS at 380 nm < λ < 390 nm only. Wavelengths above 380 nm show promise for in situ therapeutic antifouling applications.     

Possible oxidant sources in the atmosphere and surface of Mars

Summary Photolysis of H₂O in the atmosphere near the surface is a copious source of OH, HO₂, and probably superoxides, some of which are likely to condense on the surface and migrate through the pores. The processes have been modeled in detail for their atmospheric interest. The models successfully account for the rarity of CO and O₂, the notable variability of ozone, and the escape flux of hydrogen. Though only qualitative estimates can be made of surface deposition rates and lifetimes, the suggested amounts are in the range inferred by Viking. The OH rapidly destroys any organic molecules that are present as vapors.Analogous reactions involving adsorbed water have been studied by Huguenin. These processes can be driven by the much larger photon fluxes at longer ultraviolet wavelengths. The suggested explanations, and many of the experiments, make it likely that peroxides, superoxides, and adsorbed OH are all present. Both kinds of process, and their combinations, seem in principle able to explain the absence of all organic molecules and the variety of observed oxidants. Since they operate planetwide, there is a strong suggestion that the observed conditions are typical. Oases of higher than average humidity may in fact be even more hostile than the average region, because water under Martian surface conditions is anything but benign.Laboratory simulation of the atmospheric processes must pay careful attention to scaling.Curiously, similar OH densities occur at the Earth's surface, The notable differences are food for thought, and ideas about the origin of life may be particularly affected.Based on an invited paper at the Second International Colloquium on Mars, Pasadena, January 15–18, 1979     

Non-crystallographic symmetry in the crystal dimer of wheat germ agglutinin

Three isomorphous heavy atom derivatives of wheat germ agglutinin crystals, KAu(CN)₂, K₂Pt(NH₃)₂(NO)₂ and mersalyl, have been examined at high resolution. Heavy atom sites were located from difference Patterson maps in three dimensions at 2.15 Å resolution for the gold and platinum derivatives and with less certainty in the centrosymmetric [010] projection for the mersalyl derivative. These sites are distributed in the crystallographic asymmetric unit such that one half of them can be related to the other half by a 180 ° rotation about an axis parallel to a, and an additional translation of about 6.35 Å along that axis. It is suggested that the two subunits of the wheat germ agglutinin dimer, which represent the asymmetric unit of the C2 unit cell, are related by the same symmetry axis, causing heterologous subunit contacts due to the 6.35 Å translation of one relative to the other subunit.     

Higher levels of organization in chromosomes.

On the basis of recent results a unified view of different aspects of the higher levels in the organization of chromatin in chromosomes is presented. Basic to these forms of organization is the arrangement of DNA in the complex with nucleosomes and recent studies suggest that at least some species of satellite DNA may maintain a fixed DNA sequence relationship to the phasing of nucleosomes. Special proteins such as the high-mobility group (HMG) proteins or other non-histone proteins could serve specific functions in the recognition of satellite DNA sequences.In the presence of histone H1 the 110 Å nucleosome fiber formed from the basic string of nucleosomes can be further condensed into a thicker 250–300 Å fiber formed by a solenoidal coiling of the 110 Å fiber with about 6–8 nucleosomes per turn and the available evidence suggests that these structures are found in mitotic chromosomes as well as other forms of inactive chromatin. A further level of coiling of the 250–300 Å solenoid has been suggested by our recent studies of disintegrated mitotic chromosomes consisting of a thin-walled tube with an outer diameter of 4000 Å referred to as the unit fiber. This structure would account for a factor of 1400 × contraction of DNA in mitotic chromosomes which in their intact state are only 5-fold more contracted. The recently described “scaffold” proteins could be responsible for this final coiling of the unit fibers in intact chromosomes.Meiotic chromosomes are generally less contracted than mitotic chromosomes. An extreme example of this are lampbrush chromosomes that apart from the axial segments which might contain some structural proteins appear to consist of naked DNA arranged in lateral loops. In the later stages of meiosis more condensed structures arise as exemplified by the synaptonemal complex during the pachytene stage in many organisms. The characteristic features of this structure are interpreted to suggest that the structure consists of lateral components containing two parallel 110 Å nucleosome fibers each representing the axial segments of two sister chromatids. From these paired regions loops protrude laterally in a manner which closely resembles the less condensed lampbrush chromosomes. The implication of this structure in the process of crossingover is discussed.Less is known about the organization of chromatin in interphase nuclei, but structures analogous to the loop-like structures in meiotic chromosomes are suggested on the basis of the isolation of supercoiled DNA loops constrained by RNA-DNA and protein-DNA interactions. The position of these loops is suggested to be fixed by specific repeated DNA sequences that could be associated with specific tenacious non-histone or HMG proteins.     

Design,synthesis and photocytotoxicity of upconversion nanoparticles: Potential applications for near‐infrared photodynamic and photothermal therapy

Photodynamic therapy (PDT) and photothermal therapy (PTT) are emerging modalities for the treatment of tumors and nonmalignant conditions, based on the use of photosensitizers to generate singlet oxygen or heat, respectively, upon light (laser) irradiation. They have potential advantages over conventional treatments, being minimally invasive with precise spatial‐temporal selectivity and reduced side effects. However, most clinically employed PDT agents are activated at visible (vis) wavelengths for which the tissue penetration and, hence, effective treatment depth are compromised. In addition, the lipophilicity of near‐infrared (NIR) photothermal agents limits their use and efficiency. To achieve combined PDT/PTT effects, both excitation wavelengths need to be tuned into the NIR spectral window of biological tissues. This paper reports the synthesis of neodymium‐doped upconversion nanoparticles (NaYF₄:Yb,Er,Nd@NaYF₄:Nd) that convert 800 nm light into vis wavelengths, which can then activate conventional photosensitizers on the nanoparticle surface for PDT. Covalently bonded IR‐780 dyes can readily be activated by 800 nm laser irradiation. The PEGylated nanoplatform exhibited a narrow size distribution, good stability and efficient generation of singlet oxygen under laser irradiation. The in vitro photocytotoxicity of this engineered nanoplatform as either a PDT or PTT agent in HeLa cells is demonstrated, while fluorescence microscopy in nanoplatform‐incubated cells highlights its potential for bioimaging.     

Structure of human serum lipoproteins in solution. II. Small-angle x-ray scattering study of HDL and LDL.

Two human serum lipoprotein particles, HDL₃ and LDL, were studied in solution in solvents of variable density (NaBr in water) by small-angle X-ray scattering using a position-sensitive proportional counter. The data were analysed using the theoretical approach outlined in the accompanying paper (Luzzati et al., 1976). The structures of the particles were found to be independent of the salt concentration of the solution (i.e. the particles are impenetrable to NaBr). Density heterogeneities are negligible and size and shape heterogeneities appear to be small.The particle structures could be quantitatively described in terms of a set of parameters and of a few one-dimensional functions. The parameters are the volume, radius of gyration and surface area of the shape functions; the second moment and square average of the electron density contrast at buoyancy; the electron density level, volume, radius of gyration and surface area of the hydrocarbon and polar regions. The one-dimensional functions are: the distribution of chords, the spherical average of the shape function and of the electron density at buoyancy, and the fraction of each spherical shell occupied by the hydrocarbon and polar regions. These parameters and functions are internally consistent and agree with the chemical data confirming the assumptions made in their derivation.The results are compatible with the shape of the particle being compact and quasi-spherical although with deeply convoluted surfaces. They also indicate that the outer layers of the particles are occupied by the proteins and the polar groups of phospholipids and free cholesterol, and the cores by neutral lipids. The maximum diameters of the particles are 130Å and 280Å for HDL₃ and LDL, respectively, while the hydrocarbon cores have diameters of 80Å and 230Å, respectively. The solvent is considered to penetrate to 25Å from the center of the HDL₃ particle with a minimum solvation at a radius of 45Å. In the case of LDL, the solvent penetrates to 55Å from the center of the particle. The lipids in the cores of the particles, particularly the cholesterol esters, appear to display a micelle-like organization with the steroid nuclei segregated in regions distinct from those occupied by the hydrocarbon chains.Although the data are consistent with several aspects of previously proposed models, they indicate that the structures of the HDL₃ and LDL particles are more complex than previously believed.     

Chemical and structural status of copper associated with oxygenic and anoxygenic phototrophs and heterotrophs: possible evolutionary consequences

Copper adsorption on the surface and intracellular uptake inside the cells of four representative taxons of soil and aquatic micro‐organisms: aerobic rhizospheric heterotrophs (Pseudomonas aureofaciens), anoxygenic (Rhodovulum steppense) and oxygenic (cyanobacteria Gloeocapsa sp. and freshwater diatoms Navicula minima) phototrophs were studied in a wide range of pH, copper concentration, and time of exposure. Chemical status of adsorbed and assimilated Cu was investigated using in situ X‐ray absorption spectroscopy. In case of adsorbed copper, XANES spectra demonstrated significant fractions of Cu(I) likely in the form of tri‐coordinate complexes with O/N and/or S ligands. Upon short‐term reversible adsorption at all four studied micro‐organisms’ cell surface, Cu(II) is coordinated by 4.0 ± 0.5 planar oxygens at an average distance of 1.97 ± 0.02 Å, which is tentatively assigned to the carboxylate groups. The atomic environment of copper incorporated into diatoms and cyanobacteria during long‐term growth is similar to that of the adsorbed metal with slightly shorter distances to the first O/N neighbor (1.95 Å). In contrast to the common view of Cu status in phototrophic micro‐organisms, XAFS failed to detect sulfur in the nearest atomic environment of Cu assimilated by freshwater plankton (cyanobacteria) and periphyton (diatoms). The appearance of S in Cu 1st coordination shell at 2.27–2.32 Å was revealed only after long‐term interaction of Cu with anoxygenic phototrophs (and Cu uptake by soil heterotrophs), suggesting Cu scavenging in the form of sulfhydryl, histidine/carboxyl or a mixture of carboxylate and sulfhydryl complexes. These new structural constraints suggest that adsorbed Cu(II) is partially reduced to Cu(I) already at the cell surface, where as intracellular Cu uptake and storage occur in the form of both Cu(I)‐S linked proteins and Cu(II) carboxylates. Obtained results allow to better understand how, in the course of biological evolution, micro‐organisms elaborated various mechanisms of Cu uptake and storage, from passive adsorption and uptake to active, protein‐controlled surface reduction, and intracellular storage.     

Myelin P0-Glycoprotein: Predicted Structure and Interactions of Extracellular Domain

Protein zero (P₀), a transmembrane glycoprotein, accounts for over 50% of the total protein in PNS myelin. The extracellular domain of P₀ (P₀-ED) is similar to the immunoglobulin variable domain, carrying one acceptor sequence for N-linked glycosylation. The x-ray diffraction analysis of PNS myelin has demonstrated reversible transitions that depend on pH and ionic strength, resulting in three distinct structures characterized by widths of about 36 Å, 50 Å (native), and 90 Å between the extracellular surfaces of the membranes. In the current work, we considered the constraints imposed by these x-ray diffraction data on the orientation of P₀-ED, and we propose how this immunoglobulin-like domain could be accommodated in the variable widths of the extracellular space between myelin membranes. The modeling made use of the finding that β-strand predictions for P₀-ED are virtually superimposable with those of the V_H domain of the phosphocholine-binding immunoglobulin M603 of mouse, which has a similar number of residues as P₀-ED and a structure that has been solved crystallographically. The dimensions of P₀-ED from the space-filling model, developed using PC- based molecular modeling software, were found to be 44 Å× 25 Å× 23 Å. On the assumption that neither the shape nor the orientation of P₀-ED changes appreciably, then the different widths at the extracellular apposition would easily accommodate P₀-ED from apposed membranes if the molecules were oriented so that the β- strands were approximately perpendicular to the membrane surface. The apposed P₀-EDs would fully overlap at the closest apposition of the membranes, partially overlap in the native state, and align end to end in the incompletely swollen state. The P₀-ED regions analogous to the complementarity-determining regions of immunoglobulins can account for the recognition of P₀-ED from apposed membranes in the incompletely swollen state. Two of the faces of P₀-ED that show charge complementarity could account for the homophilic interactions of P₀-ED from apposed membranes in the native state. This association can be stabilized further by hydrophobic interactions. The N- linked nonasaccharide after energy minimization fit into a cavity, which was at the base of P₀-ED and which was lined with three positively charged residues. Thus, the carbohydrate may help to maintain the orientation of P₀ at the membrane surface. Our model shows how the single immunoglobulin-like domain of P₀ can account for distinct structural states of myelin membrane packing by homophilic interactions.     

The fascinating diatom frustule—can it play a role for attenuation of UV radiation?

Diatoms are ubiquitous organisms in aquatic environments and are estimated to be responsible for 20–25 % of the total global primary production. A unique feature of diatoms is the silica wall, called the frustule. The frustule is characterized by species-specific intricate nanopatterning in the same size range as wavelengths of visible and ultraviolet (UV) light. This has prompted research into the possible role of the frustule in mediating light for the diatoms’ photosynthesis as well as into possible photonic applications of the diatom frustule. One of the possible biological roles, as well as area of potential application, is UV protection. In this review, we explore the possible adaptive value of the silica frustule with focus on research on the effect of UV radiation on diatoms. We also explore the possible effect of the frustules on UV radiation, from a theoretical, biological, and applied perspective, including recent experimental data on UV transmission of diatom frustules.     

Importance of Biologically Active Aurora-like Ultraviolet Emission: Stochastic Irradiation of Earth and Mars by Flares and Explosions

Habitable planets will be subject to intense sources of ionizing radiation and fast particles from a variety of sources--from the host star to distant explosions--on a variety of timescales. Monte Carlo calculations of high-energy irradiation suggest that the surfaces of terrestrial-like planets with thick atmospheres (column densities greater than about 100 g cm(-2)) are well protected from directly incident X-rays and gamma-rays, but we find that sizeable fractions of incident ionizing radiation from astrophysical sources can be redistributed to biologically and chemically important ultraviolet wavelengths, a significant fraction of which can reach the surface. This redistribution is mediated by secondary electrons, resulting from Compton scattering and X-ray photoabsorption, the energies of which are low enough to excite and ionize atmospheric molecules and atoms, resulting in a rich aurora-like spectrum. We calculate the fraction of energy redistributed into biologically and chemically important wavelength regions for spectra characteristic of stellar flares and supernovae using a Monte-Carlo transport code and then estimate the fraction of this energy that is transmitted from the atmospheric altitudes of redistribution to the surface for a few illustrative cases. For atmospheric models corresponding to the Archean Earth, we assume no significant ultraviolet absorbers, only Rayleigh scattering, and find that the fraction of incident ionizing radiation that is received at the surface in the form of redistributed ultraviolet in the biologically relevant 200-320 nm region (UV-C and UV-B bands) can be up to 4%. On the present-day Earth with its ultraviolet ozone shield, this fraction is found to be 0.2%. Both values are many orders of magnitude higher than the fraction of direct ionizing radiation reaching the surface. This result implies that planetary organisms will be subject to mutationally significant, if intermittent, fluences of UV-B and harder radiation even in the presence of a narrow-band ultraviolet shield like ozone. We also calculate the surficial transmitted fraction of ionizing radiation and redistributed ultraviolet radiation for two illustrative evolving Mars atmospheres whose initial surface pressures were 1 bar. We discuss the frequency with which redistributed ultraviolet flux from parent star flares exceeds the parent star ultraviolet flux at the planetary surface. We find that the redistributed ultraviolet from parent star flares is probably a fairly rare intermittent event for habitable zone planets orbiting solar-type stars except when they are young, but should completely dominate the direct steady ultraviolet radiation from the parent star for planets orbiting all stars less massive than about 0.5 solar masses. Our results suggest that coding organisms on such planets (and on the early Earth) may evolve very differently than on contemporary Earth, with diversity and evolutionary rate controlled by a stochastically varying mutation rate and frequent hypermutation episodes.     

Absence of Binding Between the Human Transferrin Receptor and the Transferrin Complex of Biological Toxic Trace Element,Aluminum, Because of an Incomplete Open/Closed Form of the Complex

Human transferrin (Tf) very tightly binds two ferric ions to deliver iron to cells. Fe(III)₂Tf (Fe₂Tf) binds to the Tf receptor (TfR) at pH 7.4; however, iron-free Tf (apoTf) does not. Iron uptake is facilitated by endocytosis of the Fe₂Tf–TfR complex. Tf can also bind aluminum ions, which cause toxic effects and are associated with many diseases. Since Al(III)₂Tf (Al₂Tf) does not bind to TfR, the uptake of aluminum by the cells does not occur through a TfR-mediated pathway. We have studied the absence of binding between Al₂Tf and TfR by investigating the physicochemical characteristics of apoTf, Al₂Tf, Fe₂Tf, and TfR. The hydrodynamic radius of 38.8 Å for Al₂Tf obtained by dynamic light scattering was between that of 42.6 Å for apoTf and 37.2 Å for Fe₂Tf. The ζ potential of ?11.3 mV for Al₂Tf measured by capillary electrophoresis was close to ?11.2 mV for apoTf as compared to ?11.9 mV for Fe₂Tf, indicating that the Al₂Tf surface had a relatively scarce negative charge as the apoTf surface had. These results demonstrated that the structure of Al₂Tf was a trade-off between the closed and open forms of Fe₂Tf and apoTf, respectively. Consequently, it is suggested that Al₂Tf cannot form specific ionic interresidual interactions, such as those formed by Fe₂Tf, to bind to TfR, resulting in impossible complex formation between Al₂Tf and TfR.     

Structure and mechanism of action of riboflavin-binding protein: Small-angle X-ray scattering,sedimentation, and circular dichroism studies on the holo- and apoproteins

Riboflavin-binding protein, a transport protein occurring in egg whites, binds riboflavin tightly at pH values above 4.5 but releases it readily at pH values below 4.0. Structural aspects of this biologically important binding were studied by several methods. Analysis of sedimentation equilibrium data gave an average molecular weight of 32,500 ± 1000 for all forms of the protein and showed the absence of changes in quaternary structure when riboflavin was bound at neutral pH or released at pH 3.7. Sedimentation velocity showed no change in tertiary structure on binding at pH 7.0 but revealed a significant change in sedimentation constant at pH 3.7. While circular dichroism showed no appreciable change in secondary structure, it gave evidence of a marked change in the aromatic region at the lower pH. Small-angle X-ray scattering, going from the holoprotein at neutral pH to the apoprotein at low pH, showed a small but significant increase in radius of gyration (19.8 ± 0.2 vs 20.6 ± 0.1 Å) with slightly decreased anisotropy and with substantial increases in molecular volume (55,600 ± 530 vs 66,500 ± 240 ų), surface (11,840 ± 120 vs 13,470 ± 140 Å), and hydration (0.27 ± 0.01 vs 0.38 ± 0.01 g H₂O/g dry protein). Hydration values were obtained from small-angle X-ray scattering in two different ways for comparison with those calculated from sedimentation coefficients by way of frictional coefficients (derived from two different dimensionless ratios based independently on the structural small-angle X-ray scattering data). For either form of the protein, the surface calculated from an ellipsoidal model could account for only about 62% of the surface found experimentally. The excess surface was ascribed to topographic features of the molecule. Relative changes in this new parameter, together with the circular dichroism data and the known association of riboflavin binding with aromatic residues, suggested the opening of an aromatic-rich cleft concomitant with the release of riboflavin as a consequence of lowered pH.     

Gap junction structures: V. Structural chemistry inferred from X-ray diffraction measurements on sucrose accessibility and trypsin susceptibility

X-ray diffraction patterns have been recorded from partially oriented specimens of gap junctions isolated from mouse liver and suspended in sucrose solutions of different concentration and thus of different electron density. Analysis of these diffraction patterns has shown that sucrose is excluded from the 6-fold rotation axis of the junction lattice for a length of about 100 Å. This indicates that the aqueous channel of the junctions is in the closed, high resistance state in these preparations. Mapping of the sucrose-accessible space in the junction indicates that the cross-sectional area of the channel entrance on the cytoplasmic side of the membrane could be up to five times larger than the area of the transmembrane channel. Sucrose does not penetrate more than 20 Å into the membrane along the channel. Apparently the aqueous channel, 8 to 10 Å in radius for most of its length, is narrowed or blocked by a small feature about 50 Å from the center of the gap. Very close interactions exist between the gap junction protein and the lipid polar head groups on the cytoplasmic surface of the membrane. In this region, the protein intercalates between the polar head groups. These results suggest that the gap junction protein may have a functional two-domain structure. One domain, with a molecular weight of about 15,000, spans one bilayer and half of the gap and is contained largely within a radius of 25 Å from the 6-fold axis. The second domain is smaller and occupies the cytoplasmic surface of the gap junction membrane. Trypsin digestion removes about 4000 M_rmr from the cytoplasmic surface domain of the junction protein. Most of the material susceptible to trypsin digestion is located more than 28 å from the 6-fold axis.     

The eggs and half-eggs of Arbacia punctulata and the plutei,as photographed by ultraviolet,visible and infrared light

Normal and centrifuged eggs, the halves obtained by strong centrifugal force and the plutei of Arbacia have been photographed with visible, ultraviolet (1,537Å) and infrared (8,000–10,000Å) light. Differences in appearance with these different light sources are described and some of the photographs reproduced.     

An atomic model for the human septin hexamer by cryo-EM

In order to form functional filaments, human septins must assemble into hetero-oligomeric rod-like particles which polymerize end-to-end. The rules governing the assembly of these particles and the subsequent filaments are incompletely understood. Although crystallographic approaches have been successful in studying the separate components of the system, there has been difficulty in obtaining high resolution structures of the full particle. Here we report a first cryo-EM structure for a hexameric rod composed of human septins 2, 6 and 7 with a global resolution of ~3.6 Å and a local resolution of between ~3.0 Å and ~5.0 Å. By fitting the previously determined high-resolution crystal structures of the component subunits into the cryo-EM map, we are able to provide an essentially complete model for the particle. This exposes SEPT2 NC-interfaces at the termini of the hexamer and leaves internal cavities between the SEPT6-SEPT7 pairs. The floor of the cavity is formed by the two α₀ helices including their polybasic regions. These are locked into place between the two subunits by interactions made with the α₅ and α₆ helices of the neighbouring monomer together with its polyacidic region. The cavity may serve to provide space allowing the subunits to move with respect to one another. The elongated particle shows a tendency to bend at its centre where two copies of SEPT7 form a homodimeric G-interface. Such bending is almost certainly related to the ability of septin filaments to recognize and even induce membrane curvature.     

An instrument design for non-contact detection of biomolecules and minerals on Mars using fluorescence

We discuss fluorescence as a method to detect polycyclic aromatic hydrocarbons and other organic molecules, as well as minerals on the surface of Mars. We present an instrument design that is adapted from the ChemCam instrument which is currently on the Mars Science Lander Rover Curiosity and thus most of the primary components are currently flight qualified for Mars surface operations, significantly reducing development costs. The major change compared to ChemCam is the frequency multipliers of the 1064 nm laser to wavelengths suitable for fluorescence excitation (266 nm, 355 nm, and 532 nm). We present fluorescence spectrum for a variety of organics and minerals relevant to the surface of Mars. Preliminary results show minerals already known on Mars, such as perchlorate, fluoresce strongest when excited by 355 nm. Also we demonstrate that polycyclic aromatic hydrocarbons, such as those present in Martian meteorites, are highly fluorescent at wavelengths in the ultraviolet (266 nm, 355 nm), but not as much in the visible (532 nm). We conclude that fluorescence can be an important method for Mars applications and standoff detection of organics and minerals. The instrument approach described in this paper builds on existing hardware and offers high scientific return for minimal cost for future missions.     

X-Ray Analysis of New Crystal Forms of the Sweet Protein Thaumatin

Abstract

Thaumatin is a plant protein that in the mature form contains 8 disulfide bonds and 207 amino acids. Several forms of this protein occur naturally and each elicits an intense sweetness sensation when tasted in microgram quantities. The two major forms of thaumatin are easily separable by ion exchange chromatography. Crystals of the two proteins (designated here A and B) have been grown by vapor equilibration from solutions containing polyethylene glycol and examined by X-ray diffraction. The thaumatin A crystals are of space group P2₁2₁2₁ with a=44.3Å, b=63.7Åand c=72.7A. The crystals of thaumatin B are of space group C2 with a = 117.7Å, b=44.9Å, and c=38.0Å and β=94.0°. Both crystals diffract to well beyond 2.3Å and appear suitable for high resolution structure analysis. Four heavy atom derivatives of thaumatin B have been generated and diffraction data to 4Å resolution have been collected. This work is designed to provide a basis for studying the 3-dimensional structure of more than 100 genetically generated thaumatin derivatives, several of which show enhanced stability and improved taste characteristics.     

Crystallization of a scRIP—gelonin isolated from plant seeds Gelonium multiforum

Single crystals of the protein gelonin isolated from the seeds of Gelonium multiforum have been grown at room temperature by vapor diffusion method. The crystals are monclinic with a = 49.4 Å, b = 44.9 Å, c = 137.4 Å, and β = 98.3°. The space group is P2₁, with two molecules in the asymmetric unit which are related by a noncrystallographic 2-fold axis along ψ =13° and ? =88°. The crystals diffract X-rays to high resolution, making it possible to obtain an accurate structure of this single chain ribosome inactivating protein. © 1994 Wiley-Liss, Inc.