Characterization of a Hot-Spring Bacterium Resembling Heliothrix oregonensis

An Honors Thesis Written in 1989 for Bev Pierson, University of Puget Sound

 

Reformatted for On-Line Presentation, March 2005 by S. Boomer – Click HERE for pdf.

Some old graphs & images replaced as fading has occurred or current software does not open them.

 

INTRODUCTION

 

Extreme temperature  [45-60°C] microbial communities such as those thriving in hot springs in Yellowstone National Park are hypothesized to be modern analogues to the most ancient forms of life on earth.  Evidence of stromatolites resembling modern mats exists from at least 3.6 billion years ago [Schopf and Packer, 1987].  Petrographic thin sections from stromatolites reveal filamentous bacteria resembling extant phototrophic species such as cyanobacteria and Chloroflexus [Walter, 1983]. Micropaleontologists consequently hypothesize that ancient bacteria were also phototrophic [Walter, 1983].  Current research of thermal mat systems, therefore, inquires to discover and identify new filamentous mat-forming bacteria that may be relatives of the most ancient forms of life on earth.

 

 

Stromatolite, micrographs of stromatolites (A-C), and living filamentous bacteria (C).

Images provided to me as slides for thesis presentation (Pierson).

 

Such modern mat communities are often composed of two types of organisms that form distinct laminations.  The top layer of these mat systems is generally composed of oxygenic, photoautotrophic cyanobacteria.  Beneath this lies a layer of anoxygenic, photoheterotrophic Chloroflexus [Castenholz, 1984].  Incident light striking the mat surface is filtered through the mat such that the quality of light penetrating each layer of the mat differs.  At each layer, the phototrophic organisms consume those wavelengths absorbed by their pigment-protein complexes.  In this way, the light-absorbing properties of the bacteria within the layers of the mat are believed to correlate with their positions in the mat [Castenholz, 1984].

 

Another extant species of filamentous, phototrophic bacterium considered a possible analogue to stromatolitic bacteria is Heliothrix oregonensis [Pierson, et al., 1984, 1985].  This bacterium constructs unusual mats found only in hot springs at the Warm Springs Indian Reservation, Oregon.   The spring had a temperature of 45°C and a pH of 8.2   Inversions of the typical hot spring mats, these mats are composed of a top layer of H. oregonensis and a lower layer of cyanobacteria.  H. oregonensis  glides to form conspicuous orange puffs on the surface of the mat when it grows in full sunlight.  When grown in lower intensities of light, the organism turns deep red.  The organism has a septate and filamentous structure.  Its intracellular matrix contains poly-ß-hydroxybutyrate (PHB) granules but no other membranous structures.  This organism is photoheterotrophic, possessing bacteriochlorophyll a (Bchl a) as its major light-harvesting pigment.  The in vivo  absorption maxima for the pigment protein complex are at 795 and 865 nm.  In 1987, the organism was successfully cultured in co-culture with  a non-phototrophic bacterium   [Pierson et al., 1984, 1985].

 

 

Left:  Heliothrix mats at Warm Springs Indian Reservation, Oregon (image by Pierson).

Right:  Heliothrix mat turns red after low light (image by Pierson).

 

A second, unidentified, extant bacterium was reported by D'Amelio et al.  [1987].  This organism is a filamentous purple sulfur bacterium that possesses an extensive intracellular structure of lamellae.  The bacterium was observed in mats found in hypersaline (65 - 128 ppt) ponds in Guerrero Negro, Baja California Sur, Mexico and in Solar Lake, Sinai, Egypt. The unidentified bacterium was observed to either use reduced species of sulfur in a photoautotrophic mode or grow photoheterotrophically using organic carbon excreted by coinhabiting cyanobacteria. 

 

 

Left:  Rabbit Creek spouter and mat at Yellowstone (image by Pierson).

Right:  Published Rabbit Creek core (Castenholz, 1984).

 

Dr. Richard Castenholz first observed an unusual filamentous organism in a thick hot spring mat sustained by a six-inch spouting geyser near Rabbit Creek in Yellowstone National Park [Castenholz, 1984].  Like the typical Yellowstone hot spring mat, this Rabbit Creek Mat is composed of a top layer of cyanobacteria and an underlayer of Chloroflexus.   Deep within the mat, however, is a red layer of bacteria that strikingly resembled H. oregonensis grown in low light intensity.   When cores were removed from the mat and examined in full solar light, orange conglomerates puffed from the red layer.  These orange puffs strikingly resembled H. oregonensis grown in full light intensity.  Initial observations by Castenholz [1984] established that the red layer organism was filamentous and contained Bchl a as its photosynthetic pigment.  Preliminary experiments by Hocson [1986] showed that the organism was photoheterotrophic.  Further investigations by Pierson [unpublished] revealed that the absorption maxima for the Bchl a protein complexes were near 915 and 804 nm.  The objectives of this study were to characterize this organism in its habitat, to study its ultrastructure, and to isolate it in pure culture with the ultimate purpose of establishing whether or not the red layer organism was related to H. oregonensis  or the purple sulfur bacterium. 

 

MATERIALS AND METHODS

 

Field Observations

Field measurements were made in late June, 1988.  Temperatures were measured using a YSI Model 42SC Tele-Thermometer.  pH was measured using Colorphast indicator strips (6.5 - 10.0  pH range) and a battery-operated pH meter.  Spectral irradiance within the mat was measured using a Li-Cor LI-1800 portable spectroradiometer connected to a fiber optic probe that was inserted into the mat.  Measurements were taken at 1 mm depth intervals while the mat was exposed to natural solar radiation.

 

 

Li-Cor spectroradiometer and schematic diagram of its set-up, click to enlarge (images by Boomer)

 

Light Microscopy

Light microscopy was carried out using a Zeiss 16 light microscope.  This microscope was equipped with a Zeiss Mercury arc lamp with BG 12 and BG 38 filters to induce fluorescence from Bchl a in living filaments.  In combination with a Wratten 88A barrier filter, an MTI video camera permitted the visualization of infrared fluorescence on a Lenco PMM-925 monitor. Oil immersion light microscopy was utilized in conjunction with the Gram stain to characterize the cell wall structure of the bacterium. 

 

Pigment Analysis

Methanol extraction was carried out on mat suspensions for thirty minutes over ice and in the dark.  In vivo extracts were carried out using suspensions of homogenized mat in Tris-Sodium-Magnesium buffer (pH 8.0).  These were sonicated using a Branson 200 sonifier cell disruptor [Pierson  et al., 1987].   Spectra from both extracts were recorded using a Varian Cary 2300 spectrophotometer.   Methanol extract spectra were run from 350 to 850 nm.  In vivo extract spectra were run from 350 to 1100 nm. 

 

Electron Microscopy  

Fixation of samples for transmission electron microscopy was carried out according to procedures by D'Amelio (personal correspondence) and adapted by Kaake (personal correspondence).  Primary fixation was done in situ using 2.5% EM grade glutaraldehyde and spring water.   Samples were refrigerated until further processing.  Two fifteen-minute buffer rinses in 0.2 M sodium cacodylate (pH 7.4) were then carried out.  Secondary fixation was in 1% osmium tetroxide buffered in 0.1 M sodium cacodylate (pH 7.4) for two hours.   Samples were dehydrated via an ethanolic dehydration series (50%, 70%, 90% 100% X3).  Each step lasted fifteen minutes and was carried out under a vacuum of approximately 5 lb/square inch.  Following dehydration, samples were prepared for resin infiltration and encapsulation by passing them through three propylene oxide transfers (once through 50:50 propylene oxide/ethanol, and twice through 100% propylene oxide, under a vacuum of 5 lb/square inch).  Samples were embedded in Spurr's resin/propylene oxide, polymerized for twelve hours at 60° C, sectioned on a Sorvall MT 5000 ultramicrotome, collected on mesh copper grids.  Following post-staining in uranyl acetate and lead citrate, samples were viewed on a Zeiss EM 109 electron microscope.

 

 

Action spectrum uptake experiment and schematic diagram of its set-up, click to enlarge (images by Boomer).

 

Photosynthetic Activity

Photosynthetic activity was determined by measuring the uptake of [14C]-acetate.  Uniformly labeled [14C]-acetate (specific activity, 56 mCi/mmol) was obtained from Amersham/Searle Corp.  Experiments were carried out with freshly collected filaments suspended in spring water.  Suspended cells were incubated in 2-ml screw-cap vials containing 10-4 M 3-(3,4-di-chlorophenyl)-1,1-dimethylurea (DCMU) and 0.01uCi/ml [14C]-acetate.  DCMU was added to inhibit oxygenic photosynthesis by the cyanobacteria.  All incubations were carried out for 60-90 minutes under in situ temperatures (39-42°C) and were halted with the addition of 0.1 ml formalin.  Vials were refrigerated until further processing in the laboratory.  To measure the effects of different conditions on acetate uptake, vials were incubated on their sides in petri plates. Covers were blackened except for a central window and fitted over the plates so that the only radiation illuminating the samples was that which entered through the window.  Over this window, filters were placed according to the tested variables.

 

 

Left:  Setting up uptake experiments (image by Boomer).

Right:  Light intensity/IR uptake experiment (image by Boomer).

 

To measure the effect of wavelength of acetate uptake (action spectrum), interference filters [ESCO products, Inc.] were placed over the window above the incubation vials. Filters with wavelength maxima of 640, 670, 710, 740, 790, 840, 910, 950, 1020, 1060 nm were used. The filters were placed at the base of 15 cm chimneys that were used to collimate the light from the sun.   To measure the effect of light intensity, vials were incubated under varying thickness of neutral density filters of vinyl film (Universal Plastics, Portland, Ore.).  The absorbance of the film as a function of wavelength was nearly uniform from 400 to 100 nm.  Attenuated radiation intensities were measured using a Li-Cor LI-185B radiometer.   Acetate uptake was measured at 100%, 75%, 50%, 25%, and 0% of full solar radiation at the surface of the mat.  To measure the effects of near infrared radiation, Wratten 88A barrier filters sandwiched between two plates of glass were combined with varying thickness of neutral density filters.  Acetate uptake was measured at near infrared intensities of  100%, 80%, 60%, 20% and 0%.

 

 

Oxic/anoxic uptake experiment and schematic diagram of its set-up, click to enlarge (images by Boomer).

 

Acetate uptake was also measured in the presence or absence of oxygen.  To measure acetate uptake under oxic conditions, 4.0 ml vials were fitted with rubber serum caps and a steady stream of compressed air was passed through the cell suspension during the incubation period.  The air was introduced through a syringe needle extending to the bottom of the cell suspension.  A second syringe needle permitted to escape of gas from the headspace so as to prevent pressure from building up in the vial.  To create an anoxic environment, a similar apparatus to above system was used;  In this case, argon was passed through the incurrent syringe during the course of the incubation.  All incubation vials were placed in an opaque dish and covered with neutral density nylon so that incubation was carried out with approximately 50% full solar radiation.

 

In the laboratory, all acetate uptake experiment samples were processed by the following procedures:  Settled filaments were resuspended and a known volume was withdrawn and vacuum filtered (Gelman membrane filter, pore size 0.22 um) so that cells were retained on the paper.  Cells were immediately washed with approximately 3 ml of 0.10 M unlabelled sodium acetate followed by 2 mls of glass distilled water to ensure that the only radioactivity on the paper was that taken up by the cells during the course of the experiment.  Samples were dried overnight in uncapped scintillation vials (Wheaton Wheaton 180 scintillation vials, 20 ml).  10 ml of scintillation fluid (Biofluor, NEN Research Products, Dupont) were then added to the dried cells in each vial.  Samples were counted using a scintillation counter (Beckman, LS 3133T) to obtain raw counts per minute. 

 

Culture

No previous attempts to culture this organism have been reported. Agar plates were prepared using a standard YED-medium containing sodium bicarbonate, glycylglycine buffer, yeast extract, and DCMU.  The first parameter examined and varied was carbon source: acetate, glucose, glycolate, casamino acids, bicarbonate and yeast extract.  Filaments grown on these media were observed for three successive days unless growth proceeded.  Each day, a sample of the inoculated filaments was aseptically removed from the agar and examined using fluorescence microscopy to evaluate the presence of Bchl a.  This property, combined with observing the color and quality of the filaments, was used to estimate the survival and possible growth of the filaments on each type of medium used.   Using the optimal carbon source, the pH was then varied: 6.0, 7.0, 8.0, 8.5, 9.0, 9.5, 10.0.  Growth was evaluated using the previously described criteria.  Using the optimal carbon source and pH determined previously, the third parameter, temperature, was examined.  The following temperatures were used:  14°, 25°, 35°, 45°, and 55° C.  Growth was evaluated using the previously described criteria.  Combining all optimal parameters, culturing was attempted using different conditions of light and oxygen.  Conditions tested included full solar light measuring 450 watts/m2 (45-50% of the solar radiation measured in Yellowstone), dark, near infrared radiation only, each in the presence and absence of oxygen. Growth was evaluated using the previously described criteria.  See Culture Appendix for additional information.

 

RESULTS

 

Field Observations                                                                               

The Rabbit Creek Spouter mat is maintained by its hot-spring source through the constant splashing which erupts from the geyser.  The mat forms a thick, gelatinous mass, approximately 1.5 m by 0.6 m, which curves a third of the way around the geyser source.  The water splashing from the spouter is approximately 85° C. The internal mat temperature is 40°C.  The spring water has a pH of 8.1. The red layer is located at a depth between 6.5 mm and 8.5 mm from the surface of the mat. 

 

 

 

Left:  Rabbit Creek mat, June 1988 (image by Boomer).

Right:  Spectrum of full solar radiation available on mat surface, click to enlarge (team data, 1988).

 

Analysis of the light throughout the Rabbit Creek mat demonstrated which layers attenuated which wavelengths of light.  The image above shows that spectrum of solar radiation available upon the surface of the mat.  The images below (team data, 1988) show the spectrum of the light available just above the red layer (left) and directly beneath the red layer (right).    The former (left) demonstrates that the green layer attenuates most wavelengths between 400-700 nm.  The latter (right) demonstrates that the red layer attenuates specific wavelengths at 804 and 910 nm.   Click on each to enlarge.

 

  

 

When cores were removed from the mat and examined in full solar light, orange conglomerates of filaments puffed from the red layer to the surface of the mat.  This phenomenon occurred at daytime temperatures of approximately 30°C within fifteen minutes of exposure to full solar radiation.  Samples placed immediately in cold, dark environments were not observed to puff. 

 

    

 

Left: Rabbit Creek mat puffs orange after exposure to light (image by Pierson).

Right:  Rabbit Creek filaments, light microscopy (image by Boomer).

 

Light Microscopy

Phase contrast microscopy demonstrated the red layer bacterium to be filamentous and septate.  Granular spots (inferred to be PHB) were observed inside the cells.  The lengths of filaments were in the millimeter range.  When exposed to intense blue radiation from the mercury ultraviolet lamp, filamental Bchl a fluoresced in the infrared region.  Gram staining demonstrated the organism to be gram negative.

 

Electron Microscopy

Filaments comprising the red layer and orange puffs were identical in structure.   Cytoplasmic PHB-granules and stacked membrane systems existed throughout both cells.  The dimensions of individual cells were 1 um by 8 um.  A multilaminate wall composed of three distinct layers was 0.03 um.

 

 

Left: electron micrograph of Rabbit Creek red layer filament (image by Boomer).

Right: electron micrograph of Rabbit Creek orange puff filament (image by Boomer).

 

Pigment Analysis

A single absorption maximum for Bchl a from the methanol extract existed at 770 nm. In vivo absorption maxima for the Bchl a-protein complex were at 804 and 912 nm.  The presence of large amounts of carotenoids (responsible for the orange and red color) was indicated by broad maxima at 475 nm in methanol and 475 nm in vivo.    

 

Photosynthetic Activity

Carbon uptake data from acetate uptake experiments were plotted as disintegrations per minute (dpm).  Dpm was calculated from counts per minute by correcting for the efficiency of the scintillation counter.  The action spectrum [left image below] revealed that maximal carbon uptake occurred between 790 nm and 800 nm and at 910 nm.  Variation of light intensity [middle image below], revealed maximal uptake at fifty percent light intensity.  Infrared intensity experiments [right image below] demonstrated high levels of uptake at both high and low intensities.  Finally, oxic/anoxic uptake analysis demonstrated the organism's similar uptake of carbon in the presence or absence of oxygen [data not shown]. 

 

      

 

Culture

Optimal growth was obtained using yeast extract as a carbon source, a temperature of 45°C temperature, and a pH of 8.5 in 50% intensity solar light.  Cultures were observed to fluoresce maximally and maintain strong orange color under these conditions.  The presence or absence of oxygen did not appear to affect growth.   The organism was shown to persist on media containing sodium acetate and glycolate as carbon sources.  Bicarbonate, the autotrophic carbon source, was the least successful.  The organism tolerated temperatures between 35° and 45° C.  Temperatures below 25°C and above 50°C proved immediately detrimental to the filaments.  The organism tolerated pH's over the range of 8.0 and 9.5.  The organism did not tolerate pH's below 7.  Attempts to culture the organism in the absence of light proved entirely unsuccessful.  The organism tolerated near infrared radiation.  In either the presence or absence of light, culture growth was the same under both oxic and anoxic conditions.

 

DISCUSSION

 

In this study, an unidentified bacterium resembling the known bacterium Heliothrix oregonensis and an unknown purple sulfur bacterium was characterized.  Although several features of this unknown bacterium are similar to those of the aforementioned bacteria, it is currently impossible to determine any relatedness.  The red layer organism was observed to form mats at a site known as Rabbit Creek Spouter in Yellowstone National Park.  This organism occupied a deep position in the mat and formed a stark red lamination below superior layers of cyanobacteria and Chloroflexus.

 

Morphology

All organisms were observed to be septate filaments in which the individual cells measured approximately 1 x 7 um.  Internal poly-ß-hydroxybutyrate (PHB) granules were evident inside the cells of all organisms.  All bacteria stained Gram negative.   The red layer organism was strikingly similar to the unidentified purple sulfur bacterium [D'Amelio  et al., 1987] in their possessions of a complex cytoplasmic lamellar system.  This feature contrasted with H. oregonensis that possesses no internal structures.

 

Pigmentation

The major light-harvesting pigment of the red layer organism is of Bchl a (methanol extract).  The pigment/protein complex absorbed at 804 and 912 nm in vivo.  Carotenoids absorbed at 450 nm in both methanol and in vivo.  H. oregonensis also possessed Bchl a  as its light-harvesting pigment but its pigment/protein complex exhibits absorbance maxima at 795 and 865 nm. [Pierson, et al.  1984].  The dissimilarity between the two specific pigment/protein absorbance maxima suggests that these two bacteria are evolutionarily distinct at the species level.  No such comparisons can be drawn with respect to the unidentified purple bacterium as no pigment data is currently available on this organism. 

 

Habitat

Positioned in a distinct layer 4-8 mm beneath the surface of the mat, the habitat of the red Yellowstone bacterium bore both similarities and contrasts to that of H. oregonensis and that of the unidentified purple sulfur bacterium.  H. oregonensis occupies a distinct surface layer wherease the purple sulfur bacterium coinhabits a nondistinct layer with the cyanobacterium, Microcoleus chthonoplastes.  The temperatures, acidities, and salinities of the habitats of the red layer organism and H. oregonensis are similar.  This contrasts with the hypersaline (6 - 13%) pond environments of the purple sulfur bacterium.  This mat exhibits large diurnal fluctuations in temperature and pH. The observed levels of oxygen deep within the Rabbit Creek mat were extremely low [R.W. Castenholz, personal communication].  Contrarily, H. oregonensis was exposed to saturated levels of oxygen.  The oxygen levels of the purple sulfur bacterium were observed to fluxuate in steep gradients (D'Amelio et al. 1987).  The specific presence of sulfur in this mat contrasted with its absence in the hot spring mats. The radiation penetrating to the red layer of the Yellowstone mat composed primarily of wavelengths in the 700 - 940 nm region.  These features contrasted with the surface position and bright orange color of the Heliothrix mat [Pierson  et al., 1984].  At this superficial level, Heliothrix was exposed to saturated levels of oxygen in addition to the full spectrum of solar radiation.  The Yellowstone organism's orange puffs in full illumination bore resemblance to  the orange layer of the Oregon mat.  Likewise, the Heliothrix mat's color changed to a deep red in low levels of illumination resembled the color of the deep red layer in the Yellowstone mat.  All organisms were observed to glide.

 

Reflecting the different habitats of the three organisms, the metabolisms of each organism were observed to vary.  The red layer organism was shown to be photoheterotrophic (Hocson, 1987).  In this study, the photosynthetic metabolism, as a function of carbon uptake, was maximal at wavelenths of 790 and 910 nm, reflecting both the radiation absorbed by this layer in the mat and the cell's photosynthetic pigment/protein absorbance maxima. Uptake was also maximal in low levels of light intensity (60% full solar radiation or less).  The organism was shown to be aerotolerant by virtue of similar carbon uptake in both the presence and absence of oxygen.   H. oregonensis was described as an aerotolerant photoheterotroph (Pierson et al., 1984, 1985).  The purple sulfur bacterium was observed to undergo marked changes in its metabolism in response to its fluxuating environment.  During the morning, when sulfide was present in the photic zone of the mat, the bacterium exhibited photoautotrophic metabolism with sulfide as the electron donor.  As the day progressed, the photic zone was observed to become highly oxygenated at which point the purple bacteria either used oxidized species of sulfur such as elemental sulfur and thiosulate in the photoautotrophic mode or used organic carbon excreted by cohabiting cyanobacteria in the photoheterotrophic mode.  The organism, then, possesses a metabolic mode similar, if not divergent, from that of the red layer organism and H. oregonensis.

 

Of the three compared organisms, only H. oregonensis has been successfully co-cultured with an aerobic chemoheterotroph in a medium containing glucose and casamino acids (Pierson, 1985).  No attempts to culture the purple sulfur bacterium have been reported to date.  Attempts to culture the red layer organism, though unsuccessful, have demonstrated persistence on a medium reflecting its natural habitat:  optimal conditions include 45°C, pH 8.5, yeast extract carbon source, and low intensity radiation.

 

At this time, it is impossible to conclude the relationship of the three organisms.  Based on dissimilar absorbance maxima of the pigment protein complexes between the red layer organism and H. oregonensis, it is hypothesized that these two organisms are distinct.  It is difficult to make any assertions concerning the purple sulfur bacterium based on currently available data. 

 

Immediate future work should concentrate specifically on the culturing of the red layer organism.  Ultimately the technique of ribosomal RNA sequencing should be employed to determine the evolutionary relatedness of the three organisms.  Additional analysis of the low-light intensity red H. oregonensis should be undertaken with an emphasis on examining ultrastructure of the organism using electron microscopy and pigment/protein absorbance maxima as a function of exposure to light;  that is, does H. oregonensis develop a lamellar complex and undergo a shift of pigment-protein absorbance in response to low levels of light intensity.  Finally, infrared uptake analysis should be re-examined to clarify ambiguities observed in this report. 

Additional Data From 1988 Grant Report

Given that I received funding over the summer of 1988, I wrote up a separate fieldwork report for the Murdock Foundation.  Although most of these data were included in my final thesis, one important dataset was not:  the examination of other Yellowstone areas for Heliothrix-like organisms.  I am adding it now because it is the molecular analysis of these - and more - sites that has become the focus of my current work (particularly given that the fires of 1988 - one month after I did this my thesis work - indirectly killed the Rabbit Creek mat).  Six additional sites were examined for the presence of red layers.  Specifically, cores were removed and, if a macroscopic red layer was visible, assessed for pigment content (in vivo and methanol).  Six different sites were shown to contain potential red layer organisms:  Bev's Sink (Mammoth), Imperial Geyser Pool (near Midway), Spray Geyser (near Midway), Fairy Geyser (near Lower), Hillside (near Upper), and Octopus Spring (near Lower).  The Hillside sample was provided to be by the Castenholz team.  A summary of collected data (in some cases partial) is shown below:

 

Site

Mat pH

Mat Temperature

Methanol A-max's

In vivo A-max's

Imperial Geyser Pool Edge

8.2

63-66

771, 665

877, 795

Spray Geyser

9.0

43-47

769, 667

893, 799

Fairy Geyser (3 subsites)

7.2-4

Not done

770-3, 666-670

891-912, 805-807

Bev's Sink

Not done

Not done

666

865, 795

Hillside

Not done

Not done

771, 669

889, 799

Octopus Spring

Not done

Not done

770, 668

908, 806

 

 

Left: Spray Geyser, prospective red layer community (image by Boomer).

Right:  Bev's Sink/Mammoth, prospective red layer community (image by Boomer).

 

 

Left: Imperial Geyser Pool (image by Boomer).

Right:  Pierson and Castenholz teams at Fairy Geyser (image by Castenholz).

 

ACKNOWLEDGEMENTS

 

There are numerous individuals who supported, contributed to, or assisted with this thesis project;  I with to thank and recognize these outstanding individuals for their contributions:  First, I laud Dr. Beverly Pierson, my thesis director, for her expertise, her inspiration, and her guidance.  Her primary assistance with field research, with experimental design, and with public and written presentations of my work have been phenomenal.  Second, I thank Scott Sheffield, my advisor and departmental reader, for his primary expertise using the electron microscope.  More importantly, though, I heartily praise him for encouraging me very early to think about and develop research skills, introducing me to this project in the process of teaching me the skills associated with electron microscopy (i.e. stamina and patience).  Third, I wish to thank Dr. Jay Mueller, my extra-departmental reader who intently, thoughtfully, and patiently assisted in the writing and rewriting (and rewriting) of my thesis.  His attentive interest in and support of my work has been extraordinary over the past year.

 

Aside from thesis director and readers, a substantial number of individuals partook in various activities in support of my work.  The most outstanding group was involved in field activities - running samples through timed experiments, hiking, measuring, recording, etc.  Among them, I thank Judith Frederick (research assistant to Bev Pierson) for her training skills in basic lab and field procedures.  I also wish to praise Dr. Richard Castenholz and his crew of graduate students - visiting or otherwise - whose dedicated presence and labor was exemplary.  Of these students, I wish to thank Diane Holmstrom whose assistance, constructive criticism, and friendship in and out of the field has been extraordinary [RETROSPECTIVE COMMENT - Diane was my best friend through college and remains one of my best friends today;  after college, she began a doctoral degree with Dick but left the program because of a serious family emergency]. In addition to Diane, members of my family and several friends were engaged in the re-working of my presentation.  I also was to single out Russ Kaake, whose primary work with electron microscopy on this organism allowed me to continue a fascinating project.  I commend the Honors Program for praising my work in the form of the Best Honors Thesis Presentation Award;  the wonderful experience of this presentation and the honorary value of this award has been one of the most rewarding events of all my work at the University.

 

Finally, my work has been funded by several sources.  First, I thank the Murdock Foundation and the University Murdock Committee who approved this funding.  Second, I thank the Phi Sigma Biological Honor Society who honored my work through a Slater Research Award.  Finally, I wish to recognize the National Science Foundation and NASA whose support of Dr. Pierson has allowed her to continue such gratifying work with students in the field.  The support of all these organizations has made my work all the more fulfilling and outstanding. 

 

    

Best Friends to this day - Diane in Yellowstone 1988

Left:  en route to Fairy;  Middle:  near West Thumb/Potts Basin;  Right:  Fairy Falls lunch stop. 

 

 

Left: Pierson and Castenholz teams, camp cookout (image by Castenholz).

Right:  Judith/Bev working with the Li-Cor spectroradiometer, Octopus Spring (image by Boomer).

 

 

Left: Sarah and Scott Sheffield, University of Puget Sound, 1989 graduation (image by my dad).

Right:  Jay Mueller and Sarah, Anderson Pass (Olympic National Park), 1991 (image by passerby).

 

WORKS CITED

 

Castenholz, Richard W., "Composition of Hot Spring Microbial Mats:  A Summary," Microbial Mats: Stromatolites, Alan R. Liss, Inc., New York, N.Y., 1984, 101 - 119.

 

D'Amelio, E. D., "Association of a new type of gliding, filamentous, purple phototrohpic bacterium inside bundles of Microcoleus chthonoplastes in hypersaline cyanobacterial mats," Archives of Microbiology, 147 (1987):  213 - 220.

 

Pierson, et al., " Heliothrix oregonensis, gen. nov., sp. nov., sp. nov., a phototrophic filamentous gliding bacterium containing bacterichlorophyll a," "Archives of Microbiology," 142 (1985):  164 - 167.

 

Pierson, et al., " Physiological Ecology of a Gliding Bacterium Containing Bacteriochlorophyll a, " Applied and Environmental Microbiology," 47 (1984):  576 - 584.

 

J. William Schopf and Bonnie M. Packer, "Early Archean (3.3- Billion to 3.5-Billion-Year-Old) Microfossils from Warrawoona Group, Australia, "Science," 237 (1987) : 70 - 73.

 

Walter, Malcolm R., "Archean Stromatolites:  Evidence of Earth's Earliest Benthos," from Earth's Earliest Biosphere - Its Origin and Evolution, Ed. J.W. Schopf, Princeton UP, Princeton, NJ, 1983.