Journal of the American Chemical Society
ARTICLE
Greenland,35 where they may have arisen from evaporite basins
of the sort needed for the cycles proposed here. Borate
minerals are also associated with stromatolites in the Barberton
greenstone belt in South Africa, where they seem almost
certain to have arisen from evaporites.18 While some have
questioned whether the early Earth was sufficiently differen-
tiated to have allowed borate concentration in the geosphere,36
borate is enriched in the residual melt of any igneous species,
from which borates are easily weathered, allowing them to be
concentrated in the hydrosphere even if they are not concen-
trated in the lithosphere. This makes it difficult to argue against
borate-rich evaporates in any early Earth scenario that includes
dry land.
Molybdate presents more of a challenge to the prebiotic
chemist, as it is oxidized relative to the redox state of early
Earth, as presently modeled (MoO2 þ H2O þ 2Fe3þ f MoO3 þ
2Hþ þ 2Fe2þ = þ236 mV). However, a “planetary redox
potential” is unlikely to be relevant to the existence of such
minerals. Emerging models for early Earth suggest that con-
tinents and their associated subduction zones were present as
early as 4.4ꢀ4.5 Ga.37 These would have generated felsic
magmas that would have included minerals that are more
oxidized than the terran surface as a whole, including sulfate,
borate, and molybdate (S. J. Mojzsis, personal communication).
These results highlight the potential of minerals to provide
simultaneously both the desired reactivity and the desired
nonreactivity within a “prebiotic soup”. Further, they offer a
“vestigiality” explanation for why pent(ul)oses, including ribose,
are found in genetic material. With excess HCHO, pentoses are
the first species that can be formed by a cycle with excess HCHO
that have available a hemiacetal form that can be bound and
stabilized by borate. Once stabilized, they react no further to give
hexoses, heptoses, and higher sugars, even with excess HCHO.
While aldotetroses can form cyclic ligands that are extremely
stable in borate, they are not accessible by the pathway where
HCHO is in excess, and therefore they are not formed.
Further, this work illustrates how fluctuating conditions might
support transformations of prebiotic organic molecules, includ-
ing changes in pH or the relative amounts of stabilizing mineral
species and organic species needing stabilization. For example,
for those concerned that it might be difficult to release ribose
from its borate complex,38 simply lowering the pH through
buffering from atmospheric CO2 can do this. At pH 7, ribose is
released from borate to nearly neutral conditions, where it is
quite stable against enolization and aldol reactions that lead to
the destruction of carbonyl compounds at high pH. There, ribose
is available to be phosphorylated by prebiotic mechanisms
developed in other laboratories.39
As a final word, although the work here is driven by the “RNA-
first” hypothesis for the origin of life, the cycles described here
share some of the features proposed for cycles hypothesized for
“metabolism-first” models.40 Although “genetics-first” and “me-
tabolism-first” models for the origin of life are currently being
presented as adversaries,41 no logic compels them to be. It is
nearly certain that chemical processes that might be likened to
metabolism occurred on Earth before genetics was established in
its macromolecular form. These processes may have provided the
components of whatever genetic system did first emerge. While it
is difficult to know whether borate-moderated formaldehyde-
fixation cycles meet criteria required by advocates of a “metabo-
lism-first” scenario, Figure 2 represents a metabolic cycle resem-
bling those found in contemporary terran life.
’ EXPERIMENTAL SECTION
General Methods. 13C-labeled carbohydrates (arabinitol, arabinose,
lyxose, ribose, xylose, ribulose, xylulose, glycolaldehyde, glyceraldehydes)
were obtained from Omicron Bio. H13CHO and labeled paraformalde-
hyde were obtained from Cambridge Isotopes. All other reagents were
obtained from Sigma-Aldrich and were used without purification. Flash
column chromatography was carried out using Merck 9385 silica gel 60
(230ꢀ400 mesh). NMR spectroscopy was carried out on a Varian
Mercury 300 NMR spectrometer.
Typical Procedure for Dinitrophenylhydrazone Forma-
tion and Analysis by HPLC. A mixture of dihydroxyacetone (0.18 g,
2 mmol) and formaldehyde (0.18 g, 6 mmol) in borate buffer (1100 mM
carbonate and 278 mM borate, made by dissolving 4.68 g of Na2CO3 and
0.688 g of H3BO3 in 40 mL of H2O) was stirred at 60ꢀ65 ꢀC for 2 days
under an Ar atmosphere.
To 20 μL of the above reaction mixture were added 300 μL of TFA
solution (2% TFA in MeOH, v/v) and 200 μL of 2,4-dinitrophenylhy-
drazine solution (1.5% DNP in dimethoxyethane, w/v). The mixture
was heated at 65 ꢀC for 90 min and then cooled to room temperature,
and 400 μL of acetone was added. After evaporation to dryness, the
residue was treated with 400 μL of 5% triethylamine in methanol and
evaporated. This residue was dissolved in 80 μL of 1,2-dimethoxyethane
and treated with 500 μL of water, and the resultant suspension was
centrifuged (10 000 rpm, 2 min). The aliquot was injected into the
HPLC (column, Waters Nova-Pak HR C18 6 μm, 60 Å, 7.8 ꢁ 300 mm
Prep Column; eluents, A = 0.02% TFA in water, B = CH3CN, gradient
from 15 to 25% B in 60 min, flow rate 1 mL/min). The peaks of the
DNPꢀsugar derivatives eluted were detected by their absorbance at
360 nm.
Typical Procedure for Acetate Derivatization. A mixture of
dihydroxyacetone (0.18 g, 2 mmol) and formaldehyde (0.18 g, 6 mmol)
in borate buffer was heated to 60ꢀ65 ꢀC for 2 days under Ar atmo-
sphere. After cooling to room temperature, the mixture was neutralized
by acidic resin (Dowex), filtered, and lyophilized. The resulting solid was
dissolved in methanol (20 mL), evaporated on a rotary evaporator
(repeated three times), and further dried under high vacuum to give a
reddish brown solid. It was then treated with acetic anhydride (3 mL),
DMAP (50 mg), and pyridine (20 mL) and stirred at room temperature
for 24 h. It was evaporated and separated by silica gel column
chromatography (EtOAc:Hex = 1:2 to 2:1) to give 11 crude fractions.
1
After evaporation, each fraction was weighed and characterized by H
NMR. The identity of the each fraction was confirmed by comparison
with the authentic material.
Typical Procedure for Acetonide Derivatization. A mixture
ofdihydroxyacetone (0.18 g, 2 mmol) and formaldehyde(0.18g, 6 mmol)
in borate buffer was heated to 60ꢀ65 ꢀC for 2 days under Ar atmo-
sphere. After cooling to room temperature, the mixture was neutralized
by acidic resin (Dowex), filtered, and lyophilized. The resulting solid was
dissolved in methanol (20 mL), evaporated on a rotary evaporator
(repeated three times), and further dried under high vacuum to give a
reddish brown solid. It was then treated with acetone (50 mL) and
sulfuric acid (1 mL) and stirred at room temperature for 1.5 h. It was
neutralized by sodium bicarbonate and evaporated and separated by
silica gel column chromatography (EtOAc:Hex = 1:2 to 2:1) to give five
crude fractions. After evaporation, each fraction was weighed and
characterized by 1H NMR. The identity of the each fraction was
confirmed by comparison with the authentic material.
’ ASSOCIATED CONTENT
S
Supporting Information. Relative stability of pent-
b
(ul)oses (Tables S1 and S2 and Figure S3), consumption of
formaldehyde in formose reaction (Figure S1), and synthetic
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dx.doi.org/10.1021/ja201769f |J. Am. Chem. Soc. 2011, 133, 9457–9468