Selene R Islas1, Mayra Cuéllar-Cruz2. 1. Instituto de Ciencias Aplicadas y Tecnología, Universidad Nacional Autónoma de México, Circuito Exterior S/N, Ciudad Universitaria, Ciudad de México 04510, México. 2. Departamento de Biología, División de Ciencias Naturales y Exactas, Campus Guanajuato, Universidad de Guanajuato, Noria Alta S/N, Col. Noria Alta, C.P. 36050 Guanajuato, Guanajuato, México.
Abstract
The Precambrian era is called the first stage of the Earth history and is considered the longest stage in the geological time scale. Despite its duration, several of its environmental and chemical characteristics are still being studied. It is an era of special relevance not only for its duration but also because it is when a set of conditions gave rise to the first organism. This pioneer organism has been proposed to have been formed by a mineral and an organic part. A chemical element suggested to have been part of the structure of this cell is iron. However, what special characteristic does iron have with respect to other chemical elements to be proposed as part of this first cell? To answer this and other questions, it is indispensable to have a model that will allow extrapolating the first chemical structures of the pioneer organism formed in the Precambrian. In this context, for several decades, in vitro structures chemically formed by silica-carbonates have been synthetized, called biomorphs, because they could emulate living organisms and might resemble primitive organisms. It has been inferred that because biomorphs form structures with characteristic morphologies, they could resemble the microfossils found in the cherts of the Precambrian. Aiming at providing some insight on how iron contributed to the formation of the chemical structures of the primitive organism, we evaluated how iron contributes to the morphology and chemical-crystalline structure during the synthesis of these compounds under different conditions found in the primitive atmosphere. Experimentally, synthesis of biomorphs was performed at four different atmospheric conditions including UV light, nonionizing microwave radiation (NIR-mw), water steam (WS), and CO2 in the presence of Fe2+, Fe3+, and Fe2+/Fe3+, obtaining 48 different conditions. The produced biomorphs were observed under scanning electron microscopy (SEM). Afterward, their chemical composition and crystalline structure were analyzed through Raman and IR spectroscopy.
The Precambrian era is called the first stage of the Earth history and is considered the longest stage in the geological time scale. Despite its duration, several of its environmental and chemical characteristics are still being studied. It is an era of special relevance not only for its duration but also because it is when a set of conditions gave rise to the first organism. This pioneer organism has been proposed to have been formed by a mineral and an organic part. A chemical element suggested to have been part of the structure of this cell is iron. However, what special characteristic does iron have with respect to other chemical elements to be proposed as part of this first cell? To answer this and other questions, it is indispensable to have a model that will allow extrapolating the first chemical structures of the pioneer organism formed in the Precambrian. In this context, for several decades, in vitro structures chemically formed by silica-carbonates have been synthetized, called biomorphs, because they could emulate living organisms and might resemble primitive organisms. It has been inferred that because biomorphs form structures with characteristic morphologies, they could resemble the microfossils found in the cherts of the Precambrian. Aiming at providing some insight on how iron contributed to the formation of the chemical structures of the primitive organism, we evaluated how iron contributes to the morphology and chemical-crystalline structure during the synthesis of these compounds under different conditions found in the primitive atmosphere. Experimentally, synthesis of biomorphs was performed at four different atmospheric conditions including UV light, nonionizing microwave radiation (NIR-mw), water steam (WS), and CO2 in the presence of Fe2+, Fe3+, and Fe2+/Fe3+, obtaining 48 different conditions. The produced biomorphs were observed under scanning electron microscopy (SEM). Afterward, their chemical composition and crystalline structure were analyzed through Raman and IR spectroscopy.
The
Precambrian era is the most extensive geological era because
it goes from the creation of Earth until the Cambrian explosion. During
this time, relevant events happened related to the creation of the
Earth, including the first chemical reactions that gave origin to
the primitive organism and, consequently, to life. Evidence of life
in the Precambrian has been reported in geological sediments of different
ages of that era.[1−3] It has been documented that Precambrian sediments
contain organic and inorganic compounds coming from microfossils and
minerals found in that epoch, a fact that will allow understanding
the origin and evolution of life on Earth.[2,4,5] Stromatolites are laminated or stratified
structures formed by sediments and minerals from which microfossils
and organic compounds originated by the degradation of other fossils
that existed in the Precambrian era.[2,6−9] Among the organic compounds that have been identified in the different
materials that constitute the Precambrian sediments, such as microfossils,
stromatolites, and cherts (biogenic cherts are formed by radiolarians,
diatoms, and sponge spicules), are lipids, aliphatic hydrocarbons,
isoprenoid alkanes, fatty acids, ethers, ketones, carbon isotopic
ratios, porphyrins, and amino acids.[1,6,10−12] Primitive minerals existing in
the Precambrian era were formed by chemical elements like nitrogen,
oxygen, sodium, silicon, calcium, iron, potassium, titanium, and magnesium.[13,14] In this way, it is well documented that the origin of life proceeded
from minerals and clayish sediments. Hence, in the Precambrian era,
the first organism has been suggested to have been formed by a mineral
and an organic superstructure,[15] where
the mineral part was constituted by Fe, Ni, S, H2O, CO,
and OH, whereas the organic superstructure was composed of CO, CO2, COS, NH3, H2S, N2, H2, and HCN.[15] When analyzing the
chemical composition proposed for the pioneer organism, one of the
arising questions is: What is the explanation for the chemical composition
of the first organism to be formed by iron (Fe) and not calcium (Ca)?
One explanation is that the oxidation of Fe during meteorization and
diagenesis requires a lower exchange of redox equivalents with respect
to the biological mechanisms mediated by Ca and S.[16] The second explanation is that it is possible that in the
atmospheric conditions of the Precambrian era, the iron oxides contained
in the sediments were formed as rocks, which favored that the first
organism is formed in this type of rocks.[17,18] The third explanation is based on the Precambrian lutites formed
by pyrite crystals (FeS2); this information indicates that
Fe2+ and sulfide ions were abundant in the seas of that
era, which gave rise to the formation of lutites. Interestingly, as
a step before the formation of pyrite crystals, the sulfide iron had
been produced by the first sulfate-reducing bacteria. This datum is
possibly the most direct evidence that iron was the main ion in the
pioneer organism that allowed it to perform the first biological reactions.
Therefore, iron is one of the chemical elements that has played a
pivotal role in the origin and evolution of the different forms of
life. The iron existing in the Precambrian, in a reducing atmosphere
and being part of the first organism, became pyrite (FeS2) with O2-producing hematite (Fe2O3) and gypsum (CaSO4.2H2O) once the environment
changed to an oxidizing atmosphere. Hematite (Fe3+) played
a relevant role in the early stage of the oxidizing atmosphere because
it precipitated from the upper part of oceans due to its lower solubility
compared with Fe2+.[17] Although
it has been proposed that iron was part of the pioneer organism, it
is fundamental to know the structure adopted by that first cell in
the presence of iron in the atmospheric conditions prevailing in the
Precambrian era. To answer this and other questions, it is indispensable
to have a model that will allow extrapolating the first chemical structures
of the pioneer organism formed in the Precambrian. In this context,
for several decades, in vitro structures chemically formed by silica-carbonates
have been synthetized, called biomorphs, because they could emulate
living organisms and might resemble primitive organisms.[19−26] Because biomorphs form structures with characteristic morphologies,
they could resemble the microfossils found in the cherts of the Precambrian.[20] Their resemblance to the Precambrian microfossils
is so evident that a detailed research using strict comparisons of
these biomorphs with archaic microfossils could indicate that life
did not generate in this geological era but, rather, that it is more
recent. Actually, what has been dated are silica biomorphs that formed
according to the chemical and physical conditions prevailing in that
geological era, and their inclusion in sedimentary rocks is nothing
else than a simple common biomineralization process.[27] Experimentally, it has been demonstrated that minerals,
including clays (clays are very abundant orthosilicates in many parts
of the Earth, planets, and satellites in space and could have played
an important role in the chemical stereoselectivity of the biological
macromolecules that participated in the chemical origin of life),
participated in the concentration, alignment, and polymerization of
the first biomolecules, giving rise to the first organism in the Precambrian
era.[28,29] Another characteristic of these compounds
is that the adopted morphology could go from emulating organisms to
a spherical morphology or no morphology at all.[24,25] Due to these unique characteristics, the silica-carbonate compounds
are a good study model to evaluate the different morphologies that
could have been adopted by the first organisms in the primitive era
of the Earth. Aiming to understand how iron participated in the formation
of the first chemical structures of the primitive organisms, we assessed
how iron contributes to the morphology and chemical–crystalline
structure during the synthesis of these biomorphs in different conditions
prevailing in the primitive atmosphere.
Results
and Discussion
Water Steam Together with
UV Light Are the
Atmospheric Conditions that Allow Obtaining Biomorphs Emulating Complex
Life Form Groupings
To determine the influence of iron on
the morphology of the biomorph during its synthesis and to know whether
the crystalline structure is modified in the presence of iron in either
oxidation number (Fe2+, Fe3+) with different
anions (Cl–, SO42–),
as well as in both oxidation states (FeO, Fe2O3), we evaluated the formation of barium silica-carbonates in the
presence of the five compounds, FeCl2·4H2O, FeCl3·6H2O, FeSO4·7H2O, Fe2(SO4)3·H2O, and FeO·Fe2O3, in four different atmospheric
conditions. It was decided to perform the synthesis of biomorphs on
glass or on silicon wafers to assess whether the composition of the
support material affects the morphology of the formed biomorph because,
chemically, glass is mainly formed by SiO2 (silica), B2O3, and P2O5 oxides, whereas
the silicon wafer is formed by crystalline silicon. To emulate the
Precambrian conditions where these conditions have been reported in
comparison to the current atmosphere,[30,31] experiments
were performed under different conditions, including UV light, nonionizing
microwave radiation (NIR-mw), water steam (WS), and CO2, obtaining a total of 48 different conditions (Figure ). Once synthetized, biomorphs
were observed through SEM. As seen in Figure , the control silica-carbonates obtained
in standard conditions of temperature, pressure, and CO2 (STP) depict a morphology of leaves and helices on both glass and
silicon wafers (Figure A), which correspond to characteristic morphologies of the biomorphs
previously reported.[19−26]
Figure 1
Morphologies
obtained of the barium biomorphs synthetized under
the following atmospheric conditions and the mixture of different
ion composition: (A) control, (B) Fe2+/Cl–, (C) Fe3+/Cl–, (D) Fe2+/(SO4)2–, (E) Fe3+/(SO4)2–, and (F) Fe2+/Fe3+. Standard
conditions (STP); UV/NIR-mw/CO2atm; UV/NIR-mw/WS/CO2atm; 15% UV/NIR-mw/CO2. UV, ultraviolet light;
NIR-mw, nonionizing microwave radiation; WS, water steam; CO2atm, CO2 from the environment; 15% CO2, 15%
CO2 stream.
Morphologies
obtained of the barium biomorphs synthetized under
the following atmospheric conditions and the mixture of different
ion composition: (A) control, (B) Fe2+/Cl–, (C) Fe3+/Cl–, (D) Fe2+/(SO4)2–, (E) Fe3+/(SO4)2–, and (F) Fe2+/Fe3+. Standard
conditions (STP); UV/NIR-mw/CO2atm; UV/NIR-mw/WS/CO2atm; 15% UV/NIR-mw/CO2. UV, ultraviolet light;
NIR-mw, nonionizing microwave radiation; WS, water steam; CO2atm, CO2 from the environment; 15% CO2, 15%
CO2 stream.The combination exposed
to UV and NIR-mw revealed a morphology
emulating different shells with leaves and stems on both support materials
(Figure A). We chose
to work with two types of nonionizing radiations, short waves of UV
light, and long waves of microwaves (mw),[32] because solar radiation emits both types of radiations and it is
the energy source needed for the existence of life on Earth; the origin
of the first biomolecule (RNA), the emergence of the primitive organism,
the evolution and perpetuation of life, and ensuring the continuity
of the different species are all tied to sunlight. The sun emits gamma,
X, and UV (visible and infrared) rays of which we receive, on the
terrestrial surface, part of the UV light, visible, and near-infrared.
UV light is divided in three types: UVC (100–280 nm), UVB (280–315
nm), and UVA (315–400 nm); however, the ozone layer allows
only a minimal amount of UVA and UVB to reach the Earth.[33] Both UVA and UVB directly affect chemical molecules
because they can generate free radicals, making the molecules very
reactive and altering the global chemical reaction. Notwithstanding,
the amount of midday radiation received by the terrestrial atmosphere
is of 95% UVA.[34,35] The change in morphology of the
sample exposed to UV/NIR-mw, compared to the nonexposed sample (Figure A), could be because
the UV light generated photoionization of the molecules contained
in the reaction mixture, changing the structural arrangement of the
biomorphs. This result agrees with other works that have shown that
UV light modifies the structure of molecules. Oparin was one of the
pioneering researchers suggesting that the UV radiation could have
favored the chemical reaction to generate the first molecules.[36,37] Urey and Miller showed that, starting with a primitive mixture in
conditions emulating the atmosphere of the Precambrian era, amino
acids and organic chemical compounds can be obtained.[38,39] In a more recent work, it was shown that the photolysis of 5-substituted
hydantoin by UV light leads to obtain amino acids and imidazolidinedione.[40] In more complex organisms, like plants, these
have adapted to high radiations of this UVB light; thus, their branches,
stems, and internodes are shorter compared to plants not exposed to
high radiation.[41−44] The diminution in the size of their organs is due to UVB affecting
different biomolecules and, hence, modifying the metabolic processes.
These works reveal that UV light has exerted a fundamental role not
only in the chemical origin of life but also in the origin and modification
of the different morphologies adopted by organisms.To analyze
whether a change in the chemical and crystalline structure
occurred in the barium biomorphs synthetized with or without UV/NIR-mw,
Raman and FTIR techniques were used. These methods were chosen because
Raman is a high-resolution method that provides, in a few seconds,
chemical and structural information of any organic and inorganic compound,
allowing for the identification of the polymorphs.[45] FTIR is a powerful technique that provides information
on the structure and molecular concentration of each compound.[46,47] Bands of 139, 304, 521, 691, 972, and 1059 cm–1 were identified in the Raman spectra corresponding to the control
samples synthetized on glass or on the silicon wafer (Figure Aii).
Figure 2
Identification of the
crystalline base of the BaCO3 biomorphs
through Raman spectroscopy and FTIR. (A) Control sample. (B) Sample
synthetized with UV light. (i) SEM, optical, and confocal images.
(ii) Raman spectra. (iii) FTIR spectra. The BaCO3 biomorphs
show a witherite crystalline structure.
Identification of the
crystalline base of the BaCO3 biomorphs
through Raman spectroscopy and FTIR. (A) Control sample. (B) Sample
synthetized with UV light. (i) SEM, optical, and confocal images.
(ii) Raman spectra. (iii) FTIR spectra. The BaCO3 biomorphs
show a witherite crystalline structure.These vibrations correspond to BaCO3(I) in its aragonite-type
crystalline structure, called witherite, which belongs to the orthorhombic
space group.[48,49] Regarding the samples of barium
biomorphs synthetized under UV/NIR-mw, the characteristic bands reported
for the silica-carbonate biomorph were found in its witherite crystalline
structure just as found in the control sample (Figure Bii). When analyzing the microstructure of
the barium silica-carbonate crystals with FTIR, the spectra of the
samples in STP conditions showed peaks at 691, 783, 855, 1074, 1418,
and 3318 cm–1 (Figure Aiii). The biomorphs obtained with exposure
to UV/NIR-mw showed peaks at 691, 786, 855, 1069, and 1421 cm–1 (Figure Biii). In both conditions, the peaks correspond to those reported
for BaCO3 crystals.[50] It is
well documented that the peaks at 855, 783, and 691 cm–1 are found in the in-plane and out-of-plane bending of CO32–.[50] The IR bands at
1418 cm–1 correspond to the asymmetric stretching
mode of the C–O bond, and the peak at 1074 cm–1 corresponds to the symmetric C–O stretching vibration.[50] These data reveal that the chemical composition
and the chemical structure are not modified by the presence of UV
light (Figure ) in
contrast to the morphology, which is modified as previously described
(Figure A).Another biomorph synthesis condition to be evaluated was the morphology
and crystalline structure in the presence of water steam. The aim
of studying biomorph synthesis in two or more conditions that predominated
in the Precambrian era was to know if there is a predominating atmospheric
factor. In this third condition, biomorphs were obtained under UV/NIR-mw
and water steam (UV/NIR-mw/WS) conditions. WS was chosen because there
is controversy in this aspect; some authors have interpreted that
the silicon isotopes found in the cherts imply seawater temperatures
from 60 to 80 °C,[51] whereas other
research groups have argued that the hyperthermophilic microorganisms
that dwell at temperatures of 110 °C, as well as those organisms
that inhabit the Earth at other temperatures, do not indicate an origin
of life at these temperatures.[52,53] In addition, some authors
consider that in the Precambrian era, the WS favored the formation
of primeval oceans, in which the start of life is postulated to have
occurred in volcanic vents at least 3.2 Ga, where the first chemical
reactions were generated.[54] Barium biomorphs
obtained in UV/NIR-mw/WS condition in glass and silicon wafers presented
a morphology of leaves, stems, and flowers (Figure A). Interestingly, in these conditions, the
formation of leaves, stems, and flowers had an unusual growth not
reported previously because clusters were observed (Figure A). Magnification of the clusters
at 500× (Figure B) revealed a complex network. A higher magnification at 3000×
revealed that these clusters emulate foliage due to the dense network
of leaves, stems, and flowers that were synthetized (Figure C).
Figure 3
Micrographs of silica-BaCO3 biomorphs synthetized in
the presence of UV/NIR-mw/WS. (A) Clusters of the silica-BaCO3 crystals observed at a magnification of 100×. (B) Magnification
of clusters at 500×. (C) Magnification of a part of the clusters
at 3000×, revealing clusters that emulate foliage due to the
dense network of leaves, stems, and flowers that were synthetized.
The double-direction arrows show the similitude in the morphology
of the silica–barium carbonate biomorphs obtained by synthesis
with the foliage of nature.
Micrographs of silica-BaCO3 biomorphs synthetized in
the presence of UV/NIR-mw/WS. (A) Clusters of the silica-BaCO3 crystals observed at a magnification of 100×. (B) Magnification
of clusters at 500×. (C) Magnification of a part of the clusters
at 3000×, revealing clusters that emulate foliage due to the
dense network of leaves, stems, and flowers that were synthetized.
The double-direction arrows show the similitude in the morphology
of the silica–barium carbonate biomorphs obtained by synthesis
with the foliage of nature.Other works have shown that the morphology of the biomorphs synthetized
at high temperature varies—for example, at 45 °C, biomorphs
emulate flowers and twisted ribbons; at 60 °C, leaves and filamentous
clusters have been observed; and at 70 °C, star-shaped clusters
have been observed.[55] However, the crystalline
clusters that we obtained in the presence of UV/NIR-mw/WS have not
been observed (Figure ). A possible explanation for the dense network that emulates the
foliage in nature is that the water steam favored the BaCO3 chemical groups to grow in both length and width when the crystals
became intertwined, as shown by the growth of the BaCO3 crystals obtained under a controlled hydrothermal growth.As a whole, these results show that by the presence of these two
atmospheric conditions in the Precambrian era (UV and WS), it was
chemically possible for more complex structures to be formed from
few chemical elements. This could evidence that organisms like plants
adopted this morphology since the primitive era, and has been modified
along the years. In this way, some chemical elements have been incorporated
until the plants acquired the functions and chemical composition as
we know them nowadays. This hypothesis is based on reports through
protein sequencing analyses that before plants, 1000 Ma ago, a bacterial
flora of cyanobacteria existed, which are algae that emulated the
morphology of plants and took volcanic chemical elements in the water
as source of food and energy.[56] Later on,
terrestrial plants appeared at 700 Ma together with green algae and
the first fungi, contributing to the change from a reducing atmosphere
to an oxidizing one, allowing in this way the origin of multicellular
organisms in the Precambrian era.[57] Our
data and the reports of other research teams foster the hypothesis
that the first bacterial cells had their origin at hydrothermal vents
because, as observed, the WS favored importantly the formation of
barium biomorphs in dense clusters that emulate the morphology of
foliage (Figure ).
The Raman analysis of the barium biomorphs synthetized in these two
atmospheric conditions, either on glass or silicon wafer, showed bands
at 139, 225, 519, 693, 1058, and 1353 cm–1 (Figure A). These bands correspond
to BaCO3 in its witherite polymorph. Additionally, results
of FTIR showed peaks at 691, 763, 786, 855, 891, 944, 1069, and 1421
cm–1 (Figure B). In both conditions, the peaks correspond to those reported
for BaCO3 crystals.[50] These
results are relevant because they show that the crystalline structure
of the BaCO3 biomorph is conserved in either atmospheric
condition; however, the morphology and growth of the crystals are
changed depending on the atmospheric condition to which they are subjected
during the synthesis.
Figure 4
Analysis of biomorphs synthetized under UV/NIR-mw/WS/CO2 atmosphere. Identification of the crystalline phase of the
biomorphs
by (A) Raman and (B) FTIR spectroscopy.
Analysis of biomorphs synthetized under UV/NIR-mw/WS/CO2 atmosphere. Identification of the crystalline phase of the
biomorphs
by (A) Raman and (B) FTIR spectroscopy.This is perhaps the most plausible explanation as to why most organisms
from unicellular to multicellular are formed by the same chemical
elements but with different morphologies as a result of the atmospheric
conditions in Earth.The fourth condition considered was to
assess the influence of
carbon dioxide (CO2) on the morphology and crystalline
structure of the barium biomorphs. CO2 has been reported
by some authors as one of the dominant gases in the Precambrian era,[58,59] whereas other authors have indicated that CO2 cannot
remain in the atmosphere for a long time.[60−62] It is converted
through a chemical reaction that yields calcium carbonate (CaCO3) and silicon oxide (SiO2); this process enables
the dissolution of CaCO3 from rocks. Through this set of
reactions, the CO2 in the atmosphere and soil, during the
early era of the Earth, diminished its concentration.[63] In addition, it has been reported that light, together
with CO2, has played a fundamental role in the chemical
origin of life as demonstrated by the early experiments of Oparin,
Urey, and Miller in which they emulated the conditions of the Precambrian
environment, obtaining organic compounds.[36−39] From those experiments up to
now, it has been demonstrated that UV light produces photodissociation
of CO2-yielding O2.[64] This is evidence revealing that the high energy of the UV light
was able to produce O2 in the reducing atmosphere prevailing
in the Precambrian era, which would favor the hypothesis that the
CO2 concentration in the atmosphere could not have been
high because, on one side, O2 would be formed with the
UV light and, on the other side, CaCO3 and silicon oxide
(SiO2) would be formed as postulated by diverse research
teams.[36−39,63] To assess the effect of a high
CO2 concentration in the presence of UV light on the morphology
of barium biomorphs, we synthetized biomorphs in the presence of UV
light and under a current of 15% CO2 (UV/NIR-mw/CO2 15%) (Figure A). As shown in Figure A, the barium biomorphs obtained in these atmospheric conditions
presented a morphology of spheres. The spherulitic morphology in biomorphs
has been found in other synthesis conditions.[24,25] Although this morphology could be reminiscient of the morphology
of the first bacteria, at a high CO2 concentration, the
morphologies that resemble life forms would not be possible. This
event suggests that the presence of O2 in the first photosynthetic
bacteria and in the photolysis of CO2 modified the environmental
atmosphere and favored the synthesis of other morphologies that, in
conjunction, gave rise to the diverse chemical structures constituting
the terrestrial organisms.The Raman spectrum of the spheres
obtained in the presence of UV/NIR-mw/CO2 15% showed bands
at 96, 139, 155, 225, 692, and 1059 cm–1 (Figure S1A). These bands
correspond to BaCO3 in its witherite polymorph. FTIR results
showed peaks at 692, 777, 855, 892, 1059, 1417, and 2452 cm–1 (Figure S1B). In both conditions, peaks
correspond to those reported for BaCO3 crystals.[50] As observed with the different environmental
factors that emulate the atmosphere existing in the Precambrian era,
the origin of the diverse morphologies that reminisce terrestrial
organisms (leaves, flowers, stems, helices, and ribbons, among others)
were probably formed mostly at lower CO2 concentrations,
with water steam being probably one of the determining atmospheric
factors for the obtainment of morphologies emulating different forms
of life. These data agree with the hypothesis of some research groups,
suggesting that CO2 cannot remain in the atmosphere for
a long time.[60−62]
Versatility of the Oxidation
Potential of
Fe2+/Fe3+ Enables the Formation of Diverse Morphologies
of Complex Chemical Composition
It has been suggested that
iron has been part of the chemical composition of the pioneer organism.[15] However, one of the questions that still remain
without any answer is: Why is it proposed that this first organism
was formed by iron (Fe) and not by calcium (Ca) or another chemical
element? In order to elucidate this question, we performed the synthesis
of biomorphs in the previously described atmospheric conditions (Figure A) in the presence
of Fe2+2Cl– or Fe3+3Cl–. We chose to work with both iron oxidation states
to know whether the morphology of biomorphs changes or is conserved
depending on the oxidation number of iron. The latter is based on
the report that in the iron cycle, in nature, most of the reduced
iron is part of sedimentary rocks, whereas ferrous Fe is oxidized
by weathering.[16] After performing the synthesis
of biomorphs in the four atmospheric conditions (STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm, or UV/NIR-mw/CO2 15%) in the presence of Fe2+or Fe3+ and observing
the samples through SEM to know the formed morphology, surprisingly,
we found that the synthesis of biomorphs had not been accomplished
(Figure B,C). Notwithstanding,
with Fe2+ in the STP and UV/NIR-mw/WS/CO2 atm
conditions, some biomorphs in the form of spherulite-like structures
were scarcely identified (Figure B). Identification of the chemical composition and
the crystalline structure of these biomorphs through both Raman and
FTIR in both conditions revealed that they correspond to BaCO3 in the witherite polymorph (data not shown). Based on these
results, the next question arose: Does iron inhibit the synthesis
of biomorphs, or is the chloride ion responsible for the unfavorable
chemical reaction and, hence, the synthesis of biomorphs is not accomplished?
To answer these two questions, we decided to use FeSO4 and
Fe2(SO4)3, where the anion is the
sulfate ion SO42–. After performing the
synthesis, when visualizing the samples through SEM, we found that
in the four tested atmospheric conditions, as well as in the presence
of Fe2+ or Fe3+, the morphology of the biomorphs
was in the shape of stars (Figure D,E), except for the UV/NIR-mw/CO2atm with
Fe3+condition where no synthesis of biomorphs was accomplished
(Figure E). This result
reveals that Fe3+ in the presence of UV light and CO2 at low concentration is not a favorable condition for the
synthesis of biomorphs. The latter is possible because iron, being
in an oxidized state and in these atmospheric conditions, is insoluble
and behaves as a weak acid as observed in other conditions,[65] indicating that water steam or a higher concentration
of CO2 is required for the Fe3+ to be available
for the formation of biomorphs. Once the morphology of biomorphs in
the presence of Fe2+ or Fe3+ had been observed
(Figure A), Raman
and FTIR were applied to know the chemical composition and crystalline
structure. Samples in the presence of Fe2+, in the Raman
analysis, showed peaks at 100, 458, 621, 988, and 2514 cm–1 (Figure B). These
peaks correspond to a mixture of BaCO3, FeCO3, and FeO according to the Raman spectra reported for these compounds.[48,49,66−69] The FTIR spectrum showed bands
at 761, 891, 1030, and 1435 cm–1, which corroborated
that the stars’ morphology obtained in all conditions in the
presence of Fe2+ corresponds to BaCO3, FeCO3, and FeO (Figure C).[50,70]
Figure 5
Representative image of the biomorphs
obtained in the presence
of Fe2+ in the four atmospheric conditions analyzed in
this study: STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm, or UV/NIR-mw/CO2 15%. (A) SEM, optical, and
confocal images. (B, C) Identification of the crystalline phase of
the biomorphs through (B) Raman and (C) FTIR spectroscopy.
Representative image of the biomorphs
obtained in the presence
of Fe2+ in the four atmospheric conditions analyzed in
this study: STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm, or UV/NIR-mw/CO2 15%. (A) SEM, optical, and
confocal images. (B, C) Identification of the crystalline phase of
the biomorphs through (B) Raman and (C) FTIR spectroscopy.For the biomorphs synthetized in the presence of Fe3+, the Raman spectrum identified peaks at 103, 448, 519, 980, 1604,
and 2075 cm–1 (Figure A). These bands correspond to BaCO3, Fe2O3, and Fe2(CO3)3.[48,49,66−69] The FTIR spectrum identified the characteristic peaks revealed by
Raman spectroscopy (Figure B).[50,70]
Figure 6
Representative image of the biomorphs
obtained in the presence
of Fe3+ (SEM, optical, and confocal images), in the four
analyzed atmospheric conditions: STP, UV/NIR-mw/CO2atm,
UV/NIR-mw/WS/CO2 atm, or UV/NIR-mw/CO2 15%.
Identification of the crystalline phase of biomorphs through (A) Raman
and (B) FTIR spectroscopy.
Representative image of the biomorphs
obtained in the presence
of Fe3+ (SEM, optical, and confocal images), in the four
analyzed atmospheric conditions: STP, UV/NIR-mw/CO2atm,
UV/NIR-mw/WS/CO2 atm, or UV/NIR-mw/CO2 15%.
Identification of the crystalline phase of biomorphs through (A) Raman
and (B) FTIR spectroscopy.The star morphology obtained with iron in either oxidation state
led us to question whether placing both ions (Fe2+, Fe3+) in the reaction mixture would conserve the same star morphology
or it would be susceptible to be changed. To respond to this query,
we included the Fe2+ and Fe3+ ions in the reaction
mixture at an equimolar concentration, and this mixture was exposed
to each one of the four assessed atmospheric conditions (STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm, or UV/NIR-mw/CO2 15%). Biomorphs synthetized in standard atmospheric conditions (STP)
presented a morphology of flowers and arrangements (Figure F), whereas biomorphs obtained
under UV/NIR-mw/CO2atm conditions showed morphologies of
leaves and spheres formed by leaves (Figure F). Biomorphs produced with UV/NIR-mw/WS/CO2atm presented a morphology of stems and leaves (Figure F), with the same density as
that observed without Fe (Figure A). Finally, the morphology of the biomorph treated
with UV/NIR-mw/CO2 15% was of spheres (Figure F). Once we found that iron
must count upon the two oxidation numbers to enable the formation
of different morphologies (Figure A), we analyzed the chemical composition of the biomorphs
to determine whether barium had been displaced by iron or it was still
conserved in the structure. Once the morphology of the biomorphs in
the presence of both iron cations had been observed, we proceeded
to know their chemical composition. Raman spectroscopy revealed peaks
at 98, 143, 226, 522, 691, 1061, 1358, 1495, 1788, 1848, 2042, 2124,
and 2788 cm–1 (Figure B).
Figure 7
Representative images of the biomorphs obtained
in the presence
of the Fe2+/Fe3+mixture with the four analyzed
atmospheric conditions: STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm or UV/NIR-mw/CO2 15%. (A) Identification of
the crystalline phase of biomorphs by (B) Raman and (C) FTIR spectroscopy.
Representative images of the biomorphs obtained
in the presence
of the Fe2+/Fe3+mixture with the four analyzed
atmospheric conditions: STP, UV/NIR-mw/CO2atm, UV/NIR-mw/WS/CO2atm or UV/NIR-mw/CO2 15%. (A) Identification of
the crystalline phase of biomorphs by (B) Raman and (C) FTIR spectroscopy.With these peaks, we identified that the structures
were formed
by BaCO3, δ-FeOOH, Fe3+O(OH), α-Fe2OH, FeCO3, and Fe2(CO3)3.[48,49,66−69] The FTIR spectrum identified the peaks confirming the compounds
by Raman (Figure C).[50,70] In contrast to the morphologies obtained in the control samples
(Figure A), morphologies
produced with Fe2+/Fe3+ are more chemically
complex (Figures –7). The versatility depicted by Fe with respect to
another chemical element, like barium, is extraordinary because, although
the obtained morphologies emulate organisms with barium (Figure A), they possess
only one single chemical element (Figures –4 and Figure S1); with Fe2+/Fe3+, morphologies of organisms are also obtained but with a complex
chemical composition (Figures –7).As a whole, these
results are of special interest because, as shown,
when iron is found with the chloride ion (Cl–),
the chemical reaction cannot take place (Figure B,C), whereas in the presence of another
anion like sulfate (SO42–), the chemical
reaction is favored toward a single morphology. This morphology that
emulates a starfish or star-shaped bacteria like those of the Stella genus[71] could be one of
the first morphologies possibly adopted by the pioneering organisms
in the Precambrian era, since its chemical composition is reduced
to iron carbonate and iron oxide (Figures and 6). For bacteria
of the Stella genus, it is known that their habitat
is fresh and residual waters and they live at low nutrient concentrations
in the soil.[71] This information, in conjunction
with our results, could be indicative that, indeed, as postulated
by Wächtershäuser in 2006, the first organism must have
been formed by iron.[15] Hence, the next
question is: how was it possible that from the primitive organism,
other morphologies arose and with them, other organisms? As shown,
when the two iron ions (Fe2+, Fe3+) are present,
morphologies that emulate higher organisms, like plants, are obtained
(Figures F and 7A). The fact that iron can be oxidized or reduced,
going from an oxidized state to a reduced one and vice versa in the
environment as has occurred since the Precambrian era[16,72] favored the emergence of other morphologies and with them, other
organisms with a higher number of chemical compounds from the primitive
organisms (Figure B,C). This hypothesis agrees with the current knowledge on iron in
organisms. Thus, from the biological point of view, the potential
of the Fe2+/Fe3+ oxidation/reduction makes iron
extremely versatile when it is incorporated as an electron carrier.[73] In humans, iron exerts vital functions as it
is part of numerous enzymes[74] and proteins,
like transferrins, lactoferrins, and ferritins. Ferritins are found
in animals, vegetables, and microorganisms.[75−77] Hemoglobin
is another protein where Fe plays a fundamental role, as it allows
capturing oxygen molecules keeping the human body oxygenated. Also,
Fe is essential to produce energy and protect cells against free radicals
and bacteria-producing free radicals as part of the immune response.
It has also been described that in certain physiological processes,
like those occurring in enterocytes of the gastric lumen and the proximal
duodenum, Fe is oxidized or reduced, respectively.[78,79] In microorganisms, Fe is extremely necessary for their vital functions;
they have developed siderophores, which are molecules secreted by
them in deficient conditions to sequester iron from their surroundings.[80,81] Plants also need Fe for their functions; it avoids chlorosis, participates
in their oxygenation or respiration, and helps form chlorophyll. Plants
benefit mainly from the Fe available in the soil through microbial
siderophores.[82−84] As explained, iron is essential for the vital functions
of any terrestrial organism from bacteria to higher organisms; this
is probably because since the formation of the first cell in the Precambrian
era, it played a preponderant role in the origin, maintenance, and
evolution of life.
Conclusions
The
chemical origin of life is the conjunction of multifactorial
events, both atmospheric and chemical, that allowed for the synthesis
of the first biomolecules, which jointly favored the origin of the
pioneer organism. This pioneer organism has been proposed to be formed
by the chemical compounds most abundant in the Precambrian era, like
iron (found in minerals like hematite). Our data suggest that apparently,
iron, from the first organism until nowadays, has played a fundamental
role in the evolution of terrestrial living beings because iron fosters
the formation of several morphologies with a more complex chemical
composition. The latter could have favored the evolution of the pioneer
organism to more complex life forms. To the best of our knowledge,
this is the first work where, from a model like the biomorphs, the
participation of iron is evaluated in the morphology and chemical
composition that the pioneering organism might have had. This work
aims at contributing to the long path that still has to be discovered
regarding the chemical origin of life.
Experimental
Section
Synthesis of Biomorphs with Iron under Different
Atmospheric Conditions
The biomorphs were obtained by the
gas diffusion method.[85] Synthesis was performed
on glass or silicon squares of 1 mm thickness. Synthesis of biomorphs
was performed with both substrates to assess whether the morphology
changes or is retained on an ordered substrate (as is the case of
the silicon disk that is crystalline) with respect to another that
is not ordered (like glass, where the atoms are randomly arranged).
The used glass or silicon square had a size of 5 mm in length and
5 mm in width. The glass or silicon square was placed in a crystallization
cell, where 1000 ppm of sodium metasilicate and 20 mM barium chloride
(BaCl2) were added; this mixture was aliquoted in equal
volumes, and each aliquot was supplemented with one of the following
compounds: FeCl2.4H2O, FeCl3.6H2O, FeSO4.7H2O, Fe2(SO4)3.H2O, mixed oxide (FeO.Fe2O3 or Fe3O4), at a concentration
of 20 mM. The pH of the mixture was adjusted to 11.0 with sodium hydroxide.
All reagents were from Sigma-Aldrich (St. Louis, MO, USA). Biomorphs
were synthetized in the following conditions: (1) standard conditions
of temperature, pressure, and CO2 (STP); (2) UV radiation
at 325 nm (UV) during 10 min, followed by nonionizing microwave radiation
(NIR-mw) during 5 min; (3) UV/10 min, followed by NIR-mw/5 min, water
steam (WS) during 15 min, under an atmospheric CO2 current;
and (4) UV/10 min, followed by NIR-mw/5 min, WS/15 min, under a constant
CO2 current at 15 or 5% at 37 °C. In each of the four
conditions, the synthesis of biomorphs was performed in 24 h. Experiments
were made in triplicate.
Characterization of Biomorphs
Biomorphs
were observed through scanning electron microscopy (SEM) and analyzed
through Raman microspectroscopy and Fourier transform infrared (FTIR)
microspectroscopy.
Scanning Electron Microscopy
Biomorphs
were observed by means of SEM microphotographs in a TESCAN microscope
(Brno, Czech Republic) model VEGA3 SB with a secondary electron detector
(SE) from 10 to 20 kV in high vacuum conditions (work distance of
10 mm).
Raman Microspectroscopy
Raman spectrum
measurements were recorded with a WITec Alpha300 R (WITec GmbH, Ulm,
Germany) using a 672 lines/mm grating and 532 nm laser light excitation
originated from a Nd:YVO4 green laser. The incident laser beam with
a power of 14.4 mW was focused by 20, 50, and 100× objectives
(Zeiss, Germany) with 0.4, 0.75, and 0.9 NA, respectively. Punctual
Raman spectra were obtained with 0.5 s of integration time and 10
accumulations, and the Raman map was obtained using 0.01 s of integration
time. The data processing and analysis were performed with WITec Project
Version 5.1 software.
Fourier Transform Infrared
Spectroscopy
(FTIR)
Fourier transform infrared spectroscopy (FTIR) analysis
was made in a Nicolet iS50R Thermo Scientific (Waltham, MA, USA) spectrometer
equipped with an attenuated total reflectance (ATR) diamond crystal
accessory (Smart-iTX). Spectra acquisitions were collected with 32
scans with 4 cm–1 of spectral resolution in the
range of 525 to 3600 cm–1. Additionally, the iron
salts were used to form KBr pellets for FT-IR spectrum measurements
on the same spectrophotometer in the transmittance mode. The data
processing and analysis were performed with OriginPro version 2021
software.