Organic Geochemistry Gordon Conference 1984; Marilyn 3rd row 2nd from left |
As a new staff member, it was exciting
to move into my own dedicated laboratory space. The original Geophysical
Laboratory on Upton Street in Washington, DC, was built in 1908, had 18-inch
walls and big hallways. Director Yoder assigned me a laboratory to share with
retiring staff scientist, Gordon Davis. Davis’ career focused on radiogenic
dating of rocks. His laboratory was primarily a preparatory, “semi-clean” lab
where he purified lead and other radiogenic isotopes for dating. For about a
year, we “shared” the space with my culturing equipment on benches in the clean
lab. It was an arrangement that would never really work, because I did not have
full control over my lab space. Only many years later did I realize that this
arrangement put the start of my career at a moderate disadvantage. Fortunately
for me, after one year Gordon fully retired and I was able to renovate the
laboratory, move in two isotope mass spectrometers, and build my first original
vacuum line.
After investigating hydrogen isotopes
for several years, my interests turned to oxygen in organic matter with an
experimental plan similar to what I had carried out for hydrogen isotopes. The
analysis of organic oxygen was, at this time, limited to carbohydrates. The
Caltech group was analyzing cellulose in plants and tree rings. John Hayes and
his student Kim Wedeking at Indiana University were revising a method,
originally described by Rittenberg and Ponticorvo (1956), for analyzing
proteins and kerogens, compounds with N, S, and other elements. Tom Hoering and
I followed their work closely. Their method, published only in Kim Wedeking’s
dissertation, was based on a reaction with mercuric chloride (HgCl2) to form a mixture of carbon monoxide (CO) and carbon dioxide (CO2). Tom Hoering and I were working on a similar method. Organic matter
was heated in an evacuated sealed tube with HgCl2 at 500°C. Products included
both CO and CO2, with HCl and other impurities that were
separated by gas chromatography (Hoering and Estep, 1981). CO was converted to
CO2 by disproportionation in a high-voltage discharge apparatus where
excess carbon is plated out on platinum electrodes. The method was never
robust, and as a byproduct of the high-voltage discharge in the reaction
chamber, NO2 was formed from N2 in organic matter. Multiple analyses of biological samples introduced
NO2 unwittingly into the flight
tube of our homemade IRMS. NO2 is
notoriously sticky on metal surfaces. Eventually the IRMS would not pump down.
A real disaster resulted in which Tom Hoering removed the flight tube, took it
out on the lawn of the Geophysical Laboratory, and sandblasted it. In the environment
of the Geophysical Lab, where everyone seemed to have research successes all
the time, I felt deflated, maybe an “imposter”, but I immediately moved on to
other projects.
The analysis of oxygen isotopes in
organic matter was my first failed project, but I learned a lot during the
process. The most important lesson was learning to deal with failure. A
scientist’s life is filled with a certain amount of rejection: manuscripts,
proposals, ideas. Only rarely does one get affirmation and accolades. Learning
to not give up, but to keep searching for the next promising idea, is key to a
successful long-term career. For example, the vacuum line I designed was my
first. Parts of it were constructed using Swagelock fittings for water-cooling
lines. When the water was first turned on, the line dripped at every connection
because I did not know how to assemble a Swagelock fitting properly. As Tom
noted: “You have these in ass-backward.” In this system, I learned preparative
gas chromatography, a skill needed for later work on oxygen isotopes in
molecular O2 and even later for continuous flow gas
chromatography-combustion-IRMS (GC-C-IRMS).
Fortunately, I had the ability to shift
my emphasis to two other major projects: the biogeochemistry of extremophiles living
in hot springs and stable isotope biogeochemistry of nitrogen. On the way to
attending a Plant Physiology conference in eastern Washington state in 1980, I
made a trip through Yellowstone National Park armed with a newly purchased book
authored by Thomas Brock entitled Thermophilic microorganisms and life at
high temperatures (1978). The juxtaposition of my earlier work with
microalgal cultures and isotope fractionation in comparison to naturally
growing algal and bacterial mats struck me as the perfect analogous system with
which to study Precambrian stromatolites. I devoured Brock’s book and was
determined to set my sights on carrying out an ambitious field-based study in
summer of 1981 in Yellowstone.
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