Chlorophyll
as a Photoreceptor
Green plants are the only living things
that can make their own food. They do this using a process called
photosynthesis, which means "making things with light." During the
process of photosynthesis, the energy from the sun is turned into
chemical energy. The chemical energy is used to join carbon dioxide
and water. In the process, sugar and oxygen are created. This process
takes place mainly in the leaves of the plant. Leaves contain a
substance called
chlorophyll that traps the sun's energy. The chlorophyll is a
bright green color, which explains why plants are green.
Chlorophyll is the molecule that traps this 'most elusive of all
powers' - and is called a photoreceptor. It is found in the
chloroplasts of green plants, and is what makes green plants, green.
The basic structure of a chlorophyll molecule is a porphyrin ring,
co-ordinated to a central atom. This is very similar in structure to
the heme group found in
hemoglobin, except that in heme the central atom is iron,
whereas in chlorophyll it is magnesium.

There are actually 2 types of
chlorophyll, named a and b. They differ only slightly,
in the composition of a sidechain (in a it is -CH3,
in b it is CHO). Both of these two chlorophylls are very
effective photoreceptors because they contain a network of
alternating single and double bonds, and the orbitals can delocalise
stabilising the structure. Such delocalised polyenes have very strong
absorption bands in the visible regions of the spectrum, allowing the
plant to absorb the energy from sunlight.

The different sidegroups in the 2
chlorophylls 'tune' the absorption spectrum to slightly different
wavelengths, so that light that is not significantly absorbed by
chlorophyll a, at, say, 460nm, will instead be captured by
chlorophyll b, which absorbs strongly at that wavelength. Thus
these two kinds of chlorophyll complement each other in absorbing
sunlight. Plants can obtain all their energy requirements from the
blue and red parts of the spectrum, however, there is still a large
spectral region, between 500-600nm, where very little light is
absorbed. This light is in the green
region of the spectrum, and since it is reflected, this is the reason
plants appear green. Chlorophyll absorbs so strongly that it can mask
other less intense colours. Some of these more delicate colours (from
molecules such as carotene and quercetin) are revealed when the
chlorophyll molecule decays in the Autumn, and the woodlands turn
red, orange, and golden brown. Chlorophyll can also be damaged when
vegetation is cooked, since the central Mg atom is replaced by
hydrogen ions. This affects the energy levels within the molecule,
causing its absorbance spectrum to alter. Thus cooked leaves change
colour - often becoming a paler, insipid yellowy green.
|
As the
chlorophyll in leaves decays in the autumn, the green colour fades
and is replaced by the oranges and reds of carotenoids.
|
Chlorophyll in Plants
The
chlorophyll molecule is the active part that absorbs the sunlight,
but just as with hemoglobin, in order to do its job (synthesising
carbohydrates) it needs to be attached to the backbone of a very
complicated protein. This protein may look haphazard in design, but
it has exactly the correct structure to orient the chlorophyll
molecules in the optimal position to enable them to react with nearby
CO2 and H2O molecules in a very efficient
manner. Several chlorophyll molecules are lurking inside this
bacterial photoreceptor protein (right).
References:
- Introduction to Organic Chemistry, Streitweiser and
Heathcock (MacMillan, New York, 1981).
- Biochemistry, L. Stryer (W.H. Freeman and Co, San
Francisco, 1975).
THE PHOTOSYNTHETIC PROCESS
In: "Concepts in
Photobiology: Photosynthesis and Photomorphogenesis", Edited by GS
Singhal, G Renger, SK Sopory, K-D Irrgang and Govindjee, Narosa
Publishers/New Delhi; and Kluwer Academic/Dordrecht, pp. 11-51.
John Whitmarsh
Photosynthesis Research Unit, Agricultural Research Service/USDA
Department of Plant Biology and Center of Biophysics and
Computational Biology,
University of Illinois at Urbana-Champaign
Govindjee
Department of Plant Biology and Center of Biophysics and
Computational Biology
University of Illinois at Urbana-Champaign
Summary
The primary source of energy for nearly all life is the Sun. The
energy in sunlight is introduced into the biosphere by a process
known as photosynthesis, which occurs in plants, algae and some types
of bacteria. Photosynthesis can be defined as the physico-chemical
process by which photosynthetic organisms use light energy to drive
the synthesis of organic compounds. The photosynthetic process
depends on a set of complex protein molecules that are located in and
around a highly organized membrane. Through a series of energy
transducing reactions, the photosynthetic machinery transforms light
energy into a stable form that can last for hundreds of millions of
years. This introductory chapter focuses on the structure of the
photosynthetic machinery and the reactions essential for transforming
light energy into chemical energy.
Table of Contents
3.1 Oxygenic Photosynthetic Organisms
3.2 Anoxygenic Photosynthetic Organisms
5.1 Chloroplasts - Structure and Organization
5.2 Light Absorption - The Antenna System
5.3 Primary Photochemistry - Photosystem II and
Photosystem I Reaction Centers
5.4 Electron Transport
5.5 Creation of a Proton Electrochemical Potential
5.6 Synthesis of ATP by the ATP-Synthase Enzyme
5.7 Synthesis of Carbohydrates
5.8 Photosynthetic Quantum Yields, Energy Conversion
Efficiency and Productivity
5.9 Oxygenic Photosynthesis in Algae
5.10 Oxygenic Photosynthesis in Bacteria
6.1 Purple Bacteria
6.2 Green Sulfur Bacteria
6.3 Green Gliding Bacteria
6.4 Heliobacteria
Photosynthesis is the physico-chemical process by
which plants, algae and photosynthetic bacteria use light energy to
drive the synthesis of organic compounds. In plants, algae and
certain types of bacteria, the photosynthetic process results in the
release of molecular oxygen and the removal of carbon dioxide from
the atmosphere that is used to synthesize carbohydrates (oxygenic
photosynthesis). Other types of bacteria use light energy to create
organic compounds but do not produce oxygen (anoxygenic
photosynthesis). Photosynthesis provides the energy and reduced
carbon required for the survival of virtually all life on our planet,
as well as the molecular oxygen necessary for the survival of oxygen
consuming organisms1 . In addition, the fossil fuels currently being
burned to provide energy for human activity were produced by ancient
photosynthetic organisms. Although photosynthesis occurs in cells or
organelles that are typically only a few microns across, the process
has a profound impact on the earth's atmosphere and climate. Each
year more than 10% of the total atmospheric carbon dioxide is reduced
to carbohydrate by photosynthetic organisms. Most, if not all, of the
reduced carbon is returned to the atmosphere as carbon dioxide by
microbial, plant and animal metabolism, and by biomass combustion. In
turn, the performance of photosynthetic organisms depends on the
earth's atmosphere and climate. Over the next century, the large
increase in the amount of atmospheric carbon dioxide created by human
activity is certain to have a profound impact on the performance and
competition of photosynthetic organisms. Knowledge of the physico-chemical
process of photosynthesis is essential for understanding the
relationship between living organisms and the atmosphere and the
balance of life on earth. Several books on photosynthesis are
available for the uninitiated (Hall and Rao, 1994; Lawlor, 1993; and
Walker, 1992) or advanced student (Govindjee, 1982; Amesz, 1987;
Briggs, 1989; Barber, 1992; Scheer, 1991; Bryant, 1994; Blankenship
et al. 1995; Amesz and Hoff, 1996, Baker, 1996; and Ort and Yocum,
1996). Taiz and Zeiger (1991) place the photosynthetic process in the
context of over all plant physiology, and Cramer and Knaff (1991)
describe the bioenergetic foundation of photosynthesis.
The overall equation for photosynthesis is deceptively
simple. In fact, a complex set of physical and chemical reactions
must occur in a coordinated manner for the synthesis of
carbohydrates. To produce a sugar molecule such as sucrose, plants
require nearly 30 distinct proteins that work within a complicated
membrane structure. Research into the mechanism of photosynthesis
centers on understanding the structure of the photosynthetic
components and the molecular processes that use radiant energy to
drive carbohydrate synthesis. The research involves several
disciplines, including physics, biophysics, chemistry, structural
biology, biochemistry, molecular biology and physiology, and serves
as an outstanding example of the success of multidisciplinary
research. As such, photosynthesis presents a special challenge in
understanding several interrelated molecular processes.
In the 1770s Joseph Priestley, an English chemist and
clergyman, performed experiments showing that plants release a type
of air that allows combustion. He demonstrated this by burning a
candle in a closed vessel until the flame went out. He placed a sprig
of mint in the chamber and after several days showed that the candle
could burn again. Although Priestley did not know about molecular
oxygen, his work showed that plants release oxygen into the
atmosphere. It is noteworthy that over 200 years later, investigating
the mechanism by which plants produce oxygen is one of the most
active areas of photosynthetic research. Building on the work of
Priestley, Jan Ingenhousz, a Dutch physician, demonstrated that
sunlight was necessary for photosynthesis and that only the green
parts of plants could release oxygen. During this period Jean
Senebier, a Swiss botanist and naturalist, discovered that CO2 is
required for photosynthetic growth and Nicolas- Théodore de Saussure,
a Swiss chemist and plant physiologist, showed that water is
required. It was not until 1845 that Julius Robert von Mayer, a
German physician and physicist, proposed that photosynthetic
organisms convert light energy into chemical free energy. An
interesting time line of the history of photosynthesis has been
presented by Huzisige and Ke (1993).
By the middle of the nineteenth century
the key features of plant photosynthesis were known, namely, that
plants could use light energy to make carbohydrates from CO2 and
water. The empirical equation representing the net reaction of
photosynthesis for oxygen evolving organisms is :
CO2 + 2H2O + Light Energy ______>
[CH2O] + O2 + H2O, (1) where [CH2O]
represents a carbohydrate (e.g., glucose, a six-carbon sugar). The
synthesis of carbohydrate from carbon and water requires a large
input of light energy. The standard free energy for the reduction of
one mole of CO2 to the level of glucose is +478 kJ/mol. Because
glucose, a six carbon sugar, is often an intermediate product of
photosynthesis, the net equation of photosynthesis is frequently
written as :
6CO2 + 12H2O + Light Energy _____>
C6H12O6 + 6O2 + 6H2O. (2) The standard free energy
for the synthesis of glucose is +2,870 kJ/mol.
Not surprisingly, early scientists
studying photosynthesis concluded that the O2 released by plants came
from CO2, which was thought to be split by light energy. In the 1930s
comparison of bacterial and plant photosynthesis lead Cornelis van
Niel to propose the general equation of photosynthesis that applies
to plants, algae and photosynthetic bacteria (discussed by Wraight,
1982). Van Niel was aware that some photosynthetic bacteria could use
hydrogen sulfide (H2S) instead of water for photosynthesis and that
these organisms released sulfur instead of oxygen. Van Niel, among
others, concluded that photosynthesis depends on electron donation
and acceptor reactions and that the O2 released during photosynthesis
comes from the oxidation of water. Van Niel's generalized equation is
:
CO2 + 2H2A + Light Energy _____> [CH2O]
+ 2A + H2O. (3) In oxygenic photosynthesis, 2A is
O2, whereas in anoxygenic photosynthesis, which occurs in some
photosynthetic bacteria, the electron donor can be an inorganic
hydrogen donor, such as H2S (in which case A is elemental sulfur) or
an organic hydrogen donor such as succinate (in which case, A is
fumarate). Experimental evidence that molecular oxygen came from
water was provided by Hill and Scarisbrick (1940) who demonstrated
oxygen evolution in the absence of CO2 in illuminated chloroplasts
and by Ruben et al. (1941) who used 18O enriched water.
The biochemical conversion of CO2 to carbohydrate is a
reduction reaction that involves the rearrangement of covalent bonds
between carbon, hydrogen and oxygen. The energy for the reduction of
carbon is provided by energy rich molecules that are produced by the
light driven electron transfer reactions. Carbon reduction can occur
in the dark and involves a series of biochemical reactions that were
elucidated by Melvin Calvin, Andrew Benson and James Bassham in the
late 1940s and 1950s. Using the radioisotope 14C, most of the
intermediate steps that result in the production of carbohydrate were
identified. Calvin was awarded the Nobel Prize for Chemistry in 1961
for this work (see Calvin, 1989).
In 1954 Daniel Arnon and coworkers discovered that
plants, and A. Frenkel discovered that photosynthetic bacteria, use
light energy to produce ATP, an organic molecule that serves as an
energy source for many biochemical reactions (discussed by Frenkel,
1995). During the same period L.N.M. Duysens showed that the primary
photochemical reaction of photosynthesis is an oxidation/reduction
reaction that occurs in a protein complex (the reaction center). Over
the next few years the work of several groups, including those of
Robert Emerson, Bessel Kok, L.N.M. Duysens, Robert Hill and Horst
Witt, combined to prove that plants, algae and cyanobacteria require
two reaction centers, photosystem II and photosystem I, operating in
series (Duysens, 1989; Witt, 1991).
In 1961 Peter Mitchell suggested that cells can store
energy by creating an electric field or a proton gradient across a
membrane. Mitchell's proposal that energy is stored as an
electrochemical gradient across a vesicular membrane opened the door
for understanding energy transformation by membrane systems. He was
awarded the Nobel Prize in Chemistry in 1978 for his theory of
chemiosmotic energy transduction (Mitchell, 1961).
Most of the proteins required for the conversion of
light energy and electron transfer reactions of photosynthesis are
located in membranes. Despite decades of work, efforts to determine
the structure of membrane bound proteins had little success. This
changed in the 1980s when Johann Deisenhofer, Hartmut Michel, Robert
Huber and co-workers determined the structure of the reaction center
of the purple bacterium Rhodospeudomonas viridis. (Deisenhofer et
al., 1984, 1985; Deisenhofer and Michel, 1993). They were awarded the
Nobel Prize for Chemistry in 1988 for their work, which has provided
insight into the relationship between structure and function in
membrane-bound proteins .
A key element in photosynthetic energy conversion is
electron transfer within and between protein complexes and simple
organic molecules. The electron transfer reactions are rapid (as fast
as a few picoseconds) and highly specific. Much of our current
understanding of the physical principles that guide electron transfer
is based on the pioneering work of Rudolph A. Marcus (Marcus and
Sutin, 1985), who received the Nobel Prize in Chemistry in 1992 for
his contributions to the theory of electron transfer reaction in
chemical systems.
All life can be divided into three domains, Archaea,
Bacteria and Eucarya, which originated from a common ancestor (Woese
et al., 1990). Historically, the term photosynthesis has been applied
to organisms that depend on chlorophyll (or bacteriochlorophyll) for
the conversion of light energy into chemical free energy (Gest ,
1993). These include organisms in the domains Bacteria
(photosynthetic bacteria) and Eucarya (algae and higher plants). The
most primitive domain, Archaea, includes organisms known as
halobacteria, that convert light energy into chemical free energy.
However, the mechanism by which halobacteria convert light is
fundamentally different from that of higher organisms because there
is no oxidation/reduction chemistry and halobacteria cannot use CO2
as their carbon source. Consequently some biologists do not consider
halobacteria as photosynthetic (Gest 1993). This chapter will follow
the historical definition of photosynthesis and omit halobacteria.
3.1 Oxygenic Photosynthetic
Organisms
The photosynthetic process in all plants and algae as well as
in certain types of photosynthetic bacteria involves the reduction of
CO2 to carbohydrate and removal of electrons from H20, which results
in the release of O2. In this process, known as oxygenic
photosynthesis, water is oxidized by the photosystem II reaction
center, a multisubunit protein located in the photosynthetic
membrane. Years of research have shown that the structure and
function of photosystem II is similar in plants, algae and certain
bacteria, so that knowledge gained in one species can be applied to
others. This homology is a common feature of proteins that perform
the same reaction in different species. This homology at the
molecular level is important because there are estimated to be
300,000-500,000 species of plants. If different species had evolved
diverse mechanisms for oxidizing water, research aimed at a general
understanding of photosynthetic water oxidation would be hopeless.
3.2 Anoxygenic Photosynthetic
Organisms
Some photosynthetic bacteria can use light energy to extract
electrons from molecules other than water. These organisms are of
ancient origin, presumed to have evolved before oxygenic
photosynthetic organisms. Anoxygenic photosynthetic organisms occur
in the domain Bacteria and have representatives in four phyla -
Purple Bacteria, Green Sulfur Bacteria, Green Gliding Bacteria, and
Gram Positive Bacteria.
The energy that drives photosynthesis originates in
the center of the sun, where mass is converted to heat by the fusion
of hydrogen. Over time, the heat energy reaches the sun's surface,
where some of it is converted to light by black body radiation that
reaches the earth. A small fraction of the visible light incident on
the earth is absorbed by plants. Through a series of energy
transducing reactions, photosynthetic organisms are able to transform
light energy into chemical free energy in a stable form that can last
for hundreds of millions of years (e.g., fossil fuels). A simplified
scheme describing how energy is transformed in the photosynthetic
process is presented in this section. The focus is on the structural
and functional features essential for the energy transforming
reactions. For clarity, mechanistic and structural details are
omitted. A more highly resolved description of oxygenic and
anoxygenic photosynthesis is given in the remaining sections.
The photosynthetic process in plants and algae occurs
in small organelles known as chloroplasts that are located inside
cells. The more primitive photosynthetic organisms, for example
oxygenic cyanobacteria, prochlorophytes and anoxygenic photosynthetic
bacteria, lack organelles. The photosynthetic reactions are
traditionally divided into two stages - the "light reactions," which
consist of electron and proton transfer reactions and the "dark
reactions," which consist of the biosynthesis of carbohydrates from
CO2. The light reactions occur in a complex membrane system (the
photosynthetic membrane) that is made up of protein complexes,
electron carriers, and lipid molecules. The photosynthetic membrane
is surrounded by water and can be thought of as a two-dimensional
surface that defines a closed space, with an inner and outer water
phase. A molecule or ion must pass through the photosynthetic
membrane to go from the inner space to the outer space. The protein
complexes embedded in the photosynthetic membrane have a unique
orientation with respect to the inner and outer phase. The
asymmetrical arrangement of the protein complexes allows some of the
energy released during electron transport to create an
electrochemical gradient of protons across the photosynthetic
membrane.
Photosynthetic electron transport consists of a series
of individual electron transfer steps from one electron carrier to
another. The electron carriers are metal ion complexes and aromatic
groups. The metal ion complexes and most of the aromatic groups are
bound within proteins. Most of the proteins involved in
photosynthetic electron transport are composed of numerous
polypeptide chains that lace through the membrane, providing a
scaffolding for metal ions and aromatic groups. An electron enters a
protein complex at a specific site, is transferred within the protein
from one carrier to another, and exits the protein at a different
site. The protein controls the pathway of electrons between the
carriers by determining the location and environment of the metal ion
complexes and aromatic groups. By setting the distance between
electron carriers and controlling the electronic environment
surrounding a metal ion complex or aromatic group, the protein
controls pairwise electron transfer reactions. Between proteins,
electron transfer is controlled by distance and free energy, as for
intraprotein transfer, and by the probability that the two proteins
are in close contact. Protein association is controlled by a number
of factors, including the structure of the two proteins, their
surface electrical and chemical properties and the probability that
they collide with one another. Not all electron carriers are bound to
proteins. The reduced forms of plastoquinone or ubiquinone and
nicotinamide adenine dinucleotide phosphate (NADPH) or NADH act as
mobile electron carriers operating between protein complexes. For
electron transfer to occur, these small molecules must bind to
special pockets in the proteins known as binding sites. The binding
sites are highly specific and are a critical factor in controlling
the rate and pathway of electron transfer.
The light reactions convert energy into several forms
(Fig.
1). The first step is the conversion of a photon to an excited
electronic state of an antenna pigment molecule located in the
antenna system. The antenna system consists of hundreds of pigment
molecules (mainly chlorophyll or bacteriochlorophyll and carotenoids)
that are anchored to proteins within the photosynthetic membrane and
serve a specialized protein complex known as a reaction center. The
electronic excited state is transferred over the antenna molecules as
an exciton. Some excitons are converted back into photons and emitted
as fluorescence, some are converted to heat, and some are trapped by
a reaction center protein. (For a discussion of the use of
fluorescence as a probe of photosynthesis, see e.g., Govindjee et
al., 1986 and Krause and Weis, 1991.) Excitons trapped by a reaction
center provide the energy for the primary photochemical reaction of
photosynthesis - the transfer of an electron from a donor molecule to
an acceptor molecule. Both the donor and acceptor molecules are
attached to the reaction center protein complex. Once primary charge
separation occurs, the subsequent electron transfer reactions are
energetically downhill.
In oxygenic photosynthetic organisms (see section 5), two different
reaction centers, known as photosystem II and photosystem I, work
concurrently but in series. In the light photosystem II feeds
electrons to photosystem I. The electrons are transferred from
photosystem II to the photosystem I by intermediate carriers. The net
reaction is the transfer of electrons from a water molecule to NADP+,
producing the reduced form, NADPH. In the photosynthetic process,
much of the energy initially provided by light energy is stored as
redox free energy (a form of chemical free energy) in NADPH, to be
used later in the reduction of carbon. In addition, the electron
transfer reactions concentrate protons inside the membrane vesicle
and create an electric field across the photosynthetic membrane. In
this process the electron transfer reactions convert redox free
energy into an electrochemical potential of protons. The energy
stored in the proton electrochemical potential is used by a membrane
bound protein complex (ATP-Synthase) to covalently attach a phosphate
group to adenosine diphosphate (ADP), forming adenosine triphosphate
(ATP). Protons pass through the ATP-Synthase protein complex that
transforms electrochemical free energy into a type of chemical free
energy known as phosphate group-transfer potential (or a high-energy
phosphate bond) (Klotz, 1967). The energy stored in ATP can be
transferred to another molecule by transferring the phosphate group.
The net effect of the light reactions is to convert radiant energy
into redox free energy in the form of NADPH and phosphate
group-transfer energy in the form of ATP. In the light reactions, the
transfer of a single electron from water to NADP+ involves about 30
metal ions and 7 aromatic groups. The metal ions include 19 Fe, 5 Mg,
4 Mn, and 1 Cu. The aromatics include quinones, pheophytin, NADPH,
tyrosine and a flavoprotein. The NADPH and ATP formed by the light
reactions provide the energy for the dark reactions of
photosynthesis, known as the Calvin cycle or the photosynthetic
carbon reduction cycle. The reduction of atmospheric CO2 to
carbohydrate occurs in the aqueous phase of the chloroplast and
involves a series of enzymatic reactions. The first step is catalyzed
by the protein Rubisco (D-ribulose 1,5-bisphosphate carboxylase/oxygenase),
which attaches CO2 to a five-carbon compound. The reaction produces
two molecules of a three-carbon compound. Subsequent biochemical
reactions involve several enzymes that reduce carbon by hydrogen
transfer and rearrange the carbon compounds to synthesize
carbohydrates. The carbon reduction cycle involves the transfer and
rearrangement of chemical bond energy.
In anoxygenic photosynthetic organisms (see section 6) water is not
used as the electron donor. Electron flow is cyclic and is driven by
a single photosystem, producing a proton electrochemical gradient
that is used to provide energy for the reduction of NAD+ by an
external H-atom or e-donor (e.g., H2S or an organic acid) in a
process known as "reverse electron flow". Fixation of CO2 occurs via
different pathways in different organisms.
5.1 Chloroplasts - Structure and
Organization
In plants the photosynthetic process occurs inside
chloroplasts, which are organelles found in certain cells.
Chloroplasts provide the energy and reduced carbon needed for plant
growth and development, while the plant provides the chloroplast with
CO2, water, nitrogen, organic molecules and minerals necessary for
the chloroplast biogenesis. Most chloroplasts are located in
specialized leaf cells, which often contain 50 or more chloroplasts
per cell. Each chloroplast is defined by an inner and an outer
envelope membrane and is shaped like a meniscus convex lens that is
5-10 microns in diameter (Fig.
2), although many different shapes and sizes can be found in
plants. For details of chloroplast structure, see Staehlin (1986).
The inner envelope membrane acts as a barrier, controlling the flux
of organic and charged molecules in and out of the chloroplast. Water
passes freely through the envelope membranes, as do other small
neutral molecules like CO2 and O2. There is evidence that
chloroplasts were once free living bacteria that invaded a
non-photosynthetic cell long ago. They have retained some of the DNA
necessary for their assembly, but much of the DNA necessary for their
biosynthesis is located in the cell nucleus. This enables a cell to
control the biosynthesis of chloroplasts within its domain.
Inside the chloroplast is a complicated membrane system, known as
the photosynthetic membrane (or thylakoid membrane), that contains
most of the proteins required for the light reactions. The proteins
required for the fixation and reduction of CO2 are located outside
the photosynthetic membrane in the surrounding aqueous phase. The
photosynthetic membrane is composed mainly of glycerol lipids and
protein. The glycerol lipids are a family of molecules characterized
by a polar head group that is hydrophilic and two fatty acid side
chains that are hydrophobic. In membranes, the lipid molecules
arrange themselves in a bilayer, with the polar head toward the water
phase and the fatty acid chains aligned inside the membrane forming a
hydrophobic core (Fig.
3). The photosynthetic membrane is vesicular, defining a closed
space with an outer water space (stromal phase) and an inner water
space (lumen). The organization of the photosynthetic membrane can be
described as groups of stacked membranes (like stacks of pita or
chapati bread with the inner pocket representing the inner aqueous
space), interconnected by non-stacked membranes that protrude from
the edges of the stacks (Fig.
2). Experiments indicate that the inner aqueous space of the
photosynthetic membrane is likely continuous inside of the
chloroplast. It is not known why the photosynthetic membrane forms
such a convoluted structure. To understand the energetics of
photosynthesis the complicated structure can be ignored and the
photosynthetic membrane can be viewed as a simple vesicle.
5.2 Light Absorption - The
Antenna System
Plant photosynthesis is driven primarily by visible light
(wavelengths from 400 to 700 nm) that is absorbed by pigment
molecules (mainly chlorophyll a and b and carotenoids). The chemical
structure of chlorophyll a molecule is shown in
Fig. 4.
In chlorophyll b, CH3 in ring II is replaced by CHO group. Plants
appear green because of chlorophyll, which is so plentiful that
regions of the earth appear green from space. The absorption spectrum
of chloroplast chlorophyll a and b and carotenoids along with the
action spectrum of photosynthesis of a chloroplast is shown in
Fig. 5.
Light is collected by 200-300 pigment molecules that are bound to
light- harvesting protein complexes located in the photosynthetic
membrane. The light-harvesting complexes surround the reaction
centers that serve as an antenna. The three-dimensional structure of
the light-harvesting complex (Kühlbrandt et al., 1994) shows that the
protein determines the position and orientation of the antenna
pigments. Photosynthesis is initiated by the absorption of a photon
by an antenna molecule, which occurs in about a femtosecond (10-15 s)
and causes a transition from the electronic ground state to an
excited state. Within 10-13 s the excited state decays by vibrational
relaxation to the first excited singlet state. The fate of the
excited state energy is guided by the structure of the protein.
Because of the proximity of other antenna molecules with the same or
similar energy states, the excited state energy has a high
probability of being transferred by resonance energy transfer to a
near neighbor. Exciton energy transfer between antenna molecules is
due to the interaction of the transition dipole moment of the
molecules. The probability of transfer is dependent on the distance
between the transition dipoles of the donor and acceptor molecules
(1/R6), the relative orientation of the transition dipoles, and the
overlap of the emission spectrum of the donor molecule with the
absorption spectrum of the acceptor molecule (see van Grondelle and
Amesz, 1986). Photosynthetic antenna systems are very efficient at
this transfer process. Under optimum conditions over 90% of the
absorbed quanta are transferred within a few hundred picoseconds from
the antenna system to the reaction center which acts as a trap for
the exciton. A simple model of the antenna and its reaction center is
shown in
Fig. 6.
5.3 Primary Photochemistry -
Photosystem II and Photosystem I Reaction Centers
Photosystem II uses light energy to drive two chemical
reactions - the oxidation of water and the reduction of plastoquinone.
The photosystem II complex is composed of more than fifteen
polypeptides and at least nine different redox components
(chlorophyll, pheophytin, plastoquinone, tyrosine, Mn, Fe, cytochrome
b559, carotenoid and histidine) have been shown to undergo
light-induced electron transfer (Debus, 1992). However, only five of
these redox components are known to be involved in transferring
electrons from H2O to the plastoquinone pool - the water oxidizing
manganese cluster (Mn)4, the amino acid tyrosine, the reaction center
chlorophyll (P680), pheophytin, and the plastoquinone molecules, QA
and QB. Of these essential redox components, tyrosine, P680,
pheophytin, QA and QB have been shown to be bound to two key
polypeptides that form the heterodimeric reaction center core of
photosystem II (D1 and D2). Recent work indicates that the D1 and D2
polypeptides also provide ligands for the (Mn)4 cluster. The
three-dimensional structure of photosystem II is not known. Our
knowledge of its structure is guided by the known structure of the
reaction center in purple bacteria and biochemical and spectroscopic
data.
Fig. 7
shows a schematic view of photosystem II that is consistent with
current data.
Photochemistry in photosystem II is initiated by charge separation
between P680 and pheophytin, creating P680+/Pheo-. Primary charge
separation takes about a few picoseconds (Fig.
8). Subsequent electron transfer steps have been designed through
evolution to prevent the primary charge separation from recombining.
This is accomplished by transferring the electron within 200
picoseconds from pheophytin to a plastoquinone molecule (QA) that is
permanently bound to photosystem II. Although plastoquinone normally
acts as a two-electron acceptor, it works as a one-electron acceptor
at the QA-site. The electron on QA- is then transferred to another
plastoquinone molecule that is loosely bound at the QB-site.
Plastoquinone at the QB-site differs from QA in that it works as a
two-electron acceptor, becoming fully reduced and protonated after
two photochemical turnovers of the reaction center. The full
reduction of plastoquinone requires the addition of two electrons and
two protons, i.e., the addition of two hydrogen atoms. The reduced
plastoquinone (Fig.
9) then debinds from the reaction center and diffuses into the
hydrophobic core of the membrane. After which, an oxidized
plastoquinone molecule finds its way to the QB-binding site and the
process is repeated. Because the QB-site is near the outer aqueous
phase, the protons added to plastoquinone during its reduction are
taken from the outside of the membrane.
Photosystem II is the only known protein complex that can oxidize
water, resulting in the release of O2 into the atmosphere. Despite
years of research, little is known about the molecular events that
lead to water oxidation. Energetically, water is a poor electron
donor. The oxidation- reduction midpoint potential (Em,7) of water is
+0.82 V (pH 7). In photosystem II this reaction is driven by the
oxidized reaction center, P680+ (the midpoint potential of P680/P680+
is estimated to be +1.2 V at pH 7). How electrons are transferred
from water to P680+ remains a mystery (Govindjee and Coleman, 1990).
It is known that P680+ oxidizes a tyrosine on the D1 protein and that
Mn plays a key role in water oxidation. Four Mn ions are present in
the water oxidizing complex. X-ray absorption spectroscopy shows that
Mn undergoes light-induced oxidation. Water oxidation requires two
molecules of water and involves four sequential turnovers of the
reaction center. This was shown by an experiment demonstrating that
oxygen release by photosystem II occurs with a four flash dependence
(Fig. 10;
Joliot et al., 1969; Joliot and Kok, 1975). Each photochemical
reaction creates an oxidant that removes one electron. The net
reaction results in the release of one O2 molecule, the deposition of
four protons into the inner water phase, and the transfer of four
electrons to the QB-site (producing two reduced plastoquinone
molecules) (reviewed by Renger, 1993; Klein et al., 1993; and
Lavergne and Junge , 1993).
Photosystem II reaction centers contain a number of redox
components with no known function. An example is cytochrome b559, a
heme protein, that is an essential component of all photosystem II
reaction centers (discussed by Whitmarsh and Pakrasi, 1996). If the
cytochrome is not present in the membrane, a stable PS II reaction
center cannot be formed. Although the structure and function of Cyt
b559 remain to be discovered, it is known that the cytochrome is not
involved in the primary enzymatic activity of PS II, which is the
transfer of electrons from water to plastoquinone. Why PS II reaction
centers contain redox components that are not involved in the primary
enzymatic reactions is a puzzling question. The answer may be found
in the unusual chemical reactions occurring in PS II and the fact
that the reaction center operates at a very high power level.
Photosystem II is an energy transforming enzyme that must switch
between various high energy states that involve the creation of the
powerful oxidants required for removing electrons from water and the
complex chemistry of plastoquinone reduction which is strongly
influenced by protons. In saturating light a single reaction center
can have an energy throughput of 600 eV/s (equivalent to 60,000 kW
per mole of PS II). Operating at such a high power level results in
damage to the reaction center. It may be that some of the "extra"
redox components in photosystem II may serve to protect the reaction
center.
Photosystem II has another perplexing feature. Many plants and
algae have been shown to have a significant number of photosystem II
reaction centers that do not contribute to photosynthetic electron
transport (e.g., Chylla and Whitmarsh, 1989). Why plants devote
resources for the synthesis of reaction centers that apparently do
not contribute to energy conversion is unknown (for reviews of
photosystem II heterogeneity see Ort and Whitmarsh, 1990; Guenther
and Melis, 1990; Govindjee, 1990; Melis, 1991; Whitmarsh et al.,
1996; Lavergne and Briantais, 1996)
The photosystem I complex catalyzes the oxidation of plastocyanin,
a small soluble Cu- protein, and the reduction of ferredoxin, a small
FeS protein (Fig.
11). Photosystem I is composed of a heterodimer of proteins that
act as ligands for most of the electron carriers (Krauss et al.,
1993). The reaction center is served by an antenna system that
consists of about two hundred chlorophyll molecules (mainly
chlorophyll a) and primary photochemistry is initiated by a
chlorophyll a dimer, P700. In contrast to photosystem II, many of the
antenna chlorophyll molecules in photosystem I are bound to the
reaction center proteins. Also, FeS centers serve as electron
carriers in photosystem I and, so far as is known, photosystem I
electron transfer is not coupled to proton translocation. Primary
charge separation occurs between a primary donor, P700, a chlorophyll
dimer, and a chlorophyll monomer (Ao). The subsequent electron
transfer events and rates are shown in
Fig. 12
(see Golbeck, 1994).
5.4 Electron Transport
Electron transport from water to NADP+ requires three membrane
bound protein complexes operating in series - photosystem II, the
cytochrome bf complex and photosystem I (Fig.
3). Electrons are transferred between these large protein
complexes by small mobile molecules (plastoquinone and plastocyanin
in plants). Because these small molecules carry electrons (or
hydrogen atoms) over relatively long distances, they play a unique
role in photosynthetic energy conversion. This is illustrated by
plastoquinone (PQ), which serves two key functions. Plastoquinone
transfers electrons from the photosystem II reaction center to the
cytochrome bf complex and carries protons across the photosynthetic
membrane (see Kallas, 1994). It does this by shuttling hydrogen atoms
across the membrane from photosystem II to the cytochrome bf complex.
Because plastoquinone is hydrophobic its movement is restricted to
the hydrophobic core of the photosynthetic membrane. Plastoquinone
operates by diffusing through the membrane until, due to random
collisions, it becomes bound to a specific site on the photosystem II
complex. The photosystem II reaction center reduces plastoquinone at
the QB-site by adding two electrons and two protons creating PQH2.
The reduced plastoquinone molecule debinds from photosystem II and
diffuses randomly in the photosynthetic membrane until it encounters
a specific binding site on the cytochrome bf complex. The cytochrome
bf complex is a membrane bound protein complex that contains four
electron carriers, three cytochromes and an FeS center. The crystal
structure has been solved for cytochrome f from turnip (Martinez et
al., 1994) and the FeS center from bovine heart mitochondria (Iwata
et al., 1996). In a complicated reaction sequence that is not fully
understood, the cytochrome bf complex removes the electrons from
reduced plastoquinone and facilitates the release of the protons into
the inner aqueous space. The electrons are eventually transferred to
the photosystem I reaction center. The protons released into the
inner aqueous space contribute to the proton chemical free energy
across the membrane.
Electron transfer from the cytochrome bf complex to photosystem I
is mediated by a small Cu-protein, plastocyanin (PC). Plastocyanin is
water soluble and operates in the inner water space of the
photosynthetic membrane. Electron transfer from photosystem I to NADP+
requires ferredoxin, a small FeS protein, and ferredoxin-NADP
oxidoreductase, a peripheral flavoprotein that operates on the outer
surface of the photosynthetic membrane. Ferredoxin and NADP+ are
water soluble and are found in the outer aqueous phase.
The pathway of electrons is largely determined by the energetics of
the reaction and the distance between the carriers. The electron
affinity of the carriers is represented in
Fig. 13
by their midpoint potentials, which show the free energy available
for electron transfer reactions under equilibrium conditions. (It
should be kept in mind that reaction conditions during photosynthesis
are not in equilibrium.) Subsequent to primary charge separation,
electron transport is energetically downhill (from a lower (more
negative) to a higher ( more positive) redox potential). It is the
downhill flow of electrons that provides free energy for the creation
of a proton chemical gradient.
Photosynthetic membranes effectively limit electron transport to
two dimensions. For mobile electron carriers, limiting diffusion to
two dimensions increases the number of random encounters (Whitmarsh,
1986). Furthermore, because plastocyanin is mobile, any one
cytochrome bf complex can interact with a number of photosystem I
complexes. The same is true for plastoquinone, which commonly
operates at a stoichiometry of about six molecules per photosystem II
complex.
5.5 Creation of a
Proton Electrochemical Potential
Electron transport creates the proton electrochemical
potential of the photosynthetic membrane by two types of reactions.
(1) The release of protons during the oxidation of water by
photosystem II and the translocation of protons from the outer
aqueous phase to the inner aqueous phase by the coupled reactions of
photosystem II and the cytochrome bf complex in reducing and
oxidizing plastoquinone on opposite sides of the membrane. This
creates a concentration difference of protons across the membranes (DpH
= pHin - pHout). (2) Primary charge separation at the reaction center
drives an electron across the photosynthetic membrane, which creates
an electric potential across the membrane (DY = Yin - Yout).
Together, these two forms of energy make up the proton
electrochemical potential across the photosynthetic membrane (DmH+)
which is related to the pH difference across the membrane and the
electrical potential difference across the membrane by the following
equation:
DmH+ = F DY - 2.3 RT DpH, (4)
where F is the Faraday constant, R is the gas constant,
and T the temperature in Kelvin. Although the value of DY across the
photosynthetic membrane in chloroplasts can be as large as 100 mV,
under normal conditions the proton gradient dominates. For example,
during photosynthesis the outer pH is typically near 8 and the inner
pH is typically near 6, giving a pH difference of 2 across the
membrane that is equivalent to 120 mV. Under these conditions the free
energy for proton transfer from the inner to the outer aqueous phase
is -12 kJ/mol of protons.
5.6 Synthesis of
ATP by the ATP Synthase Enzyme
The conversion of proton electrochemical energy into chemical
free energy is accomplished by a single protein complex known as ATP
synthase. This enzyme catalyzes a phosphorylation reaction, which is
the formation of ATP by the addition of inorganic phosphate (Pi) to
ADP
ADP-3 + Pi-2 + H+ _____> ATP-4 + H2O.
(5) The reaction is energetically uphill (DG = +32
kJ/mol) and is driven by proton transfer through the ATP synthase
protein. The ATP Synthase complex is composed of two major subunits,
CF0 and CF1 (Fig.
14). The CF0 subunit spans the photosynthetic membrane and forms
a proton channel through the membrane. The CF1 subunit is attached to
the top of the CF0 on the outside of the membrane and is located in
the aqueous space. CF1 is composed of several different protein
subunits, referred to as a, b, g, d and e. The top portion of the CF1
subunit is composed of three ab-dimers that contain the catalytic
sites for ATP synthesis. A recent major breakthrough has been the
elucidation of the structure of ATPase of beef heart mitochondria by
Abrahams et al. (1994). The molecular processes that couple proton
transfer through the protein to the chemical addition of phosphate to
ADP are poorly understood. It is known that phosphorylation can be
driven by a pH gradient, a transmembrane electric field, or a
combination of the two. Experiments indicate that three protons must
pass through the ATP synthase complex for the synthesis of one
molecule of ATP. However, the protons are not involved in the
chemistry of adding phosphate to ADP. Paul Boyer and coworkers have
proposed an alternating binding site mechanism for ATP synthesis
(Boyer, 1993). One model based on their proposal is that there are
three catalytic sites on each CF1 that cycle among three different
states (Fig.
15). The states differ in their affinity for ADP, Pi and ATP. At
any one time, each site is in a different state. This model is
supported by the structure of ATPase elucidated by Abrahams et al.
(1994). Initially, one catalytic site on CF1 binds one ADP and one
inorganic phosphate molecule relatively loosely. Due to a
conformational change of the protein, the site becomes a tight
binding site, that stabilizes ATP. Next, proton transfer induces an
alteration in protein conformation that causes the site to release
the ATP molecule into the aqueous phase. In this model, the energy
from the proton electrochemical gradient is used to lower the
affinity of the site for ATP, allowing its release to the water
phase. The three sites on CF1 act cooperatively, i.e., the
conformational states of the sites are linked. It has been proposed
that protons affect the conformational change by driving the rotation
of the top part (the three ab-dimers) of CF1. Such a rotating model
has recently been supported by recording of a rotation of the gamma
subunit relative to the alpha-beta subunits by Sabbert et al. (1996).
This revolving site mechanism would require rates as high as 100
revolutions per second. It is worth noting that flagella that propel
some bacteria are driven by a proton pump and can rotate at 60
revolutions per second.
5.7 Synthesis of Carbohydrates
All plants and algae remove CO2 from the environment and
reduce it to carbohydrate by the Calvin cycle. The process is a
sequence of biochemical reactions that reduce carbon and rearrange
bonds to produce carbohydrate from CO2 molecules. The first step is
the addition of CO2 to a five-carbon compound (ribulose
1,5-bisphosphate) (Fig.
16). The six-carbon compound is split, giving two molecules of a
three-carbon compound (3-phosphoglycerate). This key reaction is
catalyzed by Rubisco, a large water soluble protein complex. The
3-dimensional structure has been determined by X-ray analysis for
Rubisco isolated from tobacco (Schreuder et al. 1993) from a
cyanobacterium (Synechococcus) (Newman and Gutteridge, 1993) and from
a purple bacterium (Rhodospirillum rubrum) (Schneider et al. 1990).
The carboxylation reaction is energetically downhill. The main energy
input in the Calvin cycle is the phosphorylation by ATP and
subsequent reduction by NADPH of the initial three-carbon compound
forming a three-carbon sugar, triosephosphate. Some of the
triosephosphate is exported from the chloroplast and provides the
building block for synthesizing more complex molecules. In a process
known as regeneration, the Calvin cycle uses some of the
triosephosphate molecules to synthesize the energy rich ribulose
1,5-bisphosphate needed for the initial carboxylation reaction. This
reaction requires the input of energy in the form of one ATP.
Overall, thirteen enzymes are required to catalyze the reactions in
the Calvin cycle. The energy conversion efficiency of the Calvin
cycle is approximately 90%. The reactions do not involve energy
transduction, but rather the rearrangement of chemical energy. Each
molecule of CO2 reduced to a sugar [CH2O]n requires 2 molecules of
NADPH and 3 molecules of ATP.
Rubisco is a bifunctional enzyme that, in addition to binding CO2
to ribulose bisphosphate, can also bind O2. This oxygenation reaction
produces the 3-phosphoglycerate that is used in the Calvin cycle and
a two-carbon compound (2-phosphoglycolate) that is not useful for the
plant. In response, a complicated set of reactions (known as
photorespiration) are initiated that serve to recover reduced carbon
and to remove phosphoglycolate. The Rubisco oxygenation reaction
appears to serve no useful purpose for the plant. Some plants have
evolved specialized structures and biochemical pathways that
concentrate CO2 near Rubisco. These pathways (C4 and CAM), serve to
decrease the fraction of oxygenation reactions (see Chapter this
volume on carbon reduction).
5.8 Photosynthetic Quantum Yield
and Energy Conversion Efficiency
The theoretical minimum quantum requirement for photosynthesis
is 8 quanta for each molecule of oxygen evolved (four quanta required
by photosystem II and four by photosystem I). Measurements in algal
cells and leaves under optimal conditions (e.g., low light) give
quantum requirements of 8-10 photons per oxygen molecule released
(see Emerson, 1958). These quantum yield measurements show that the
quantum yields of photosystem II and photosystem I reaction centers
under optimal conditions are near 100%. These values can be used to
calculate the theoretical energy conversion efficiency of
photosynthesis (free energy stored as carbohydrate/light energy
absorbed). If 8 red quanta are absorbed (8 mol of red photons are
equivalent to 1,400 kJ) for each CO2 molecule reduced (480 kJ/mol),
the theoretical maximum energy efficiency for carbon reduction is
34%. Under optimal conditions, plants can achieve energy conversion
efficiencies within 90% of the theoretical maximum. However, under
normal growing conditions the actual performance of the plant is far
below these theoretical values. The factors that conspire to lower
the quantum yield of photosynthesis include limitations imposed by
biochemical reactions in the plant and environmental conditions that
limit photosynthetic performance. One of the most efficient crop
plants is sugar cane, which has been shown to store up to 1% of the
incident visible radiation over a period of one year. However, most
crops are less productive. The annual conversion efficiency of corn,
wheat, rice, potatoes, and soybeans typically ranges from 0.1% to
0.4% (Odum, 1971).
5.9 Oxygenic Photosynthesis in
Algae
Algae are photosynthetic eukaryotic organisms that, like
plants, evolve O2 and reduce CO2. They represent a diverse group that
include the dinoflagellates, the euglenoids, yellow-green algae,
golden-brown algae, diatoms, red algae, brown algae, and green algae.
The photosynthetic apparatus and biochemical pathways of carbon
reduction of algae are similar to plants. Photosynthesis occurs in
chloroplasts that contain photosystems II and I, the cytochrome bf
complex, the Calvin cycle enzymes and pigment-protein complexes
containing chlorophyll a, and other antenna pigments (e.g.,
chlorophyll b in green algae, chlorophyll c and fucaxanthol in brown
algae and diatoms, and phycobilins in red algae). Green algae are
thought to be the ancestral group from which land plants evolved (see
Douglas, 1994). Algae are abundant and widespread on the earth,
living mainly in fresh and sea water. Some algae live as single
celled organisms, while others form multicellular organisms some of
which can grow quite large, like kelp and seaweed. Phytoplankton in
the ocean is made up of algae and oxygenic photosynthetic bacteria.
Most photosynthesis in the ocean is due to phytoplankton, which is an
important source of food for marine life.
5.10 Oxygenic Photosynthesis in
Bacteria
Cyanobacteria are photosynthetic prokaryotic organisms that
evolve O2 (Bryant, 1994). Fossil evidence indicates that
cyanobacteria existed over 3 billion years ago and it is thought that
they were the first oxygen evolving organisms on earth (Wilmotte,
1994). Cyanobacteria are presumed to have evolved in water in an
atmosphere that lacked O2. Initially, the O2 released by
cyanobacteria reacted with ferrous iron in the oceans and was not
released into the atmosphere. Geological evidence indicates that the
ferrous Fe was depleted around 2 billion years ago, and earth's
atmosphere became aerobic. The release of O2 into the atmosphere by
cyanobacteria has had a profound affect on the evolution of life.
The photosynthetic apparatus of cyanobacteria is
similar to that of chloroplasts. The main difference is in the
antenna system. Cyanobacteria depend on chlorophyll a and specialized
protein complexes (phycobilisomes) to gather light energy (Sidler,
1994). They do not contain chlorophyll b. As in chloroplasts, the
chlorophyll a is located in membrane bound proteins. The
phycobilisomes are bound to the outer side of the photosynthetic
membrane and act to funnel exciton energy to the photosystem II
reaction center. They are composed of phycobiliproteins, protein
subunits that contain covalently attached open ring structures known
as bilins that are the light absorbing pigments. Primary
photochemistry, electron transport, phosphorylation and carbon
reduction occur much as they do in chloroplasts. Cyanobacteria have a
simpler genetic system than plants and algae that enable them to be
easily modified genetically. Because of this cyanobacteria have been
used as a model to understand photosynthesis in plants. By
genetically altering photosynthetic proteins, researchers can
investigate the relationship between molecular structure and
mechanism (Barry et al., 1994).
Over the past three decades several types of oxygenic
bacteria known as prochlorophytes (or oxychlorobacteria) have been
discovered that have light harvesting protein complexes that contain
chlorophyll a and b, but do not contain phycobilisomes (Palenik and
Haselkorn 1992, Urbach et al., 1992; Matthijs et al., 1994). Because
prochlorophytes have Chlorophyll a/b light harvesting proteins like
chloroplasts, they are being investigated as models for plant
photosynthesis.
Anoxygenic photosynthetic bacteria differ from
oxygenic organisms in that each species has only one type of reaction
center (Blankenship et al., 1995). In some photosynthetic bacteria
the reaction center is similar to photosystem II and in others it is
similar to photosystem I. However, neither of these two types of
bacterial reaction center is capable of extracting electrons from
water, so they do not evolve O2. Many species can only survive in
environments that have a low concentration of O2. To provide
electrons for the reduction of CO2, anoxygenic photosynthetic
bacteria must oxidize inorganic or organic molecules available in
their environment. For example, the purple bacterium Rhodobacter
sphaeroides can use succinate to reduce NAD+ by a membrane-linked
reverse electron transfer that is driven by a transmembrane
electrochemical potential. Although many photosynthetic bacteria
depend on Rubisco and the Calvin cycle for the reduction of CO2, some
are able to fix atmospheric CO2 by other biochemical pathways.
Despite these differences, the general principles of
energy transduction are the same in anoxygenic and oxygenic
photosynthesis. Anoxygenic photosynthetic bacteria depend on
bacteriochlorophyll, a family of molecules that are similar to the
chlorophyll, that absorb strongly in the infrared between 700 and
1000 nm. The antenna system consists of bacteriochlorophyll and
carotenoids that serve a reaction center where primary charge
separation occurs. The electron carriers include quinone (e.g.,
ubiquinone, menaquinone) and the cytochrome bc complex, which is
similar to the cytochrome bf complex of oxygenic photosynthetic
apparatus. As in oxygenic photosynthesis, electron transfer is
coupled to the generation of an electrochemical potential that drives
phosphorylation by ATP synthase and the energy required for the
reduction of CO2 is provided by and ATP and NADH, a molecule similar
to NADPH.
6.1 Purple Bacteria
There are two divisions of photosynthetic purple bacteria, the
non-sulfur purple bacteria (e.g., Rhodobacter sphaeroides and
Rhodospeudomonas viridis) and the sulfur purple bacteria (e.g.,
Chromatium vinosum) (Blankenship et al., 1995). Non-sulfur purple
bacteria typically use an organic electron donor, such as succinate
or malate, but they can also use hydrogen gas. The sulfur bacteria
use an inorganic sulfur compound, such as hydrogen sulfide as the
electron donor. The only pathway for carbon fixation by purple
bacteria is the Calvin cycle. Sulfur purple bacteria must fix CO2 to
live, whereas non-sulfur purple bacteria can grow aerobically in the
dark by respiration on an organic carbon source.
The determination of the three-dimensional structures
of the reaction center of the non- sulfur purple bacteria,
Rhodopseudomonas viridis and Rhodobacter sphaeroides, has provided an
unprecedented opportunity to understand the structure and function of
photosynthetic reaction centers (Deisenhofer et al., 1984, 1985;
Feher et al., 1989; Lancaster et al., 1995). The positions of the
electron transfer components in the reaction center of Rhodobacter
sphaeroides are shown in
Fig. 17
(Norris and van Brakel, 1986), and those of the three protein
subunits L, M, and H, in
Fig. 18.
The reaction center contains four bacteriochlorophyll and two
bacteriopheophytin molecules. Two of the bacteriochlorophyll
molecules form the primary donor (P870). At present, there is
controversy over whether a bacteriochlorophyll molecule is an
intermediate in electron transfer from the P870 to bacteriopheophytin.
However, there is agreement that the remaining steps involve two
quinone molecules (QA and QB) and that two turnovers of the reaction
center results in the release of reduced quinone (QH2) into the
photosynthetic membrane. Although there is a non-heme Fe between the
two quinone molecules, there is convincing evidence that this Fe is
not involved directly in transferring an electron from QA to QB.
Because the primary donor (P870), bacteriopheophytin and quinone
acceptors of the purple bacterial reaction center are similar to the
photosystem II reaction center, the bacterial reaction center is used
as guide to understand the structure and function of photosystem II.
Light driven electron transfer is cyclic in Rhodobacter sphaeroides
and other purple bacteria (Fig.
19). The reaction center produces reduced quinone, which is
oxidized by the cytochrome bc complex. Electrons from the cytochrome
bc complex are transferred to a soluble electron carrier, cytochrome
c2, which reduces the oxidized primary donor P870+. The product of
the light driven electron transfer reactions is ATP. The electrons
for the reduction of carbon are extracted from an organic donor, such
as succinate or malate or from hydrogen gas, but not by the reaction
center. The energy needed to reduce NAD+ is provided by light driven
cyclic electron transport in the form of ATP. The energy
transformation pathway is complicated. Succinate is oxidized by a
membrane bound enzyme (succinate dehydrogenase) that transfers the
electrons to quinone, which is the source of electrons for the
reduction of NAD+. However, electron transfer from reduced quinone to
NAD+ is energetically uphill. By a mechanism that is poorly
understood, a membrane bound enzyme is able to use energy stored in
the proton electrochemical potential to drive electrons from reduced
quinone to NAD+.
6.2 Green Sulfur Bacteria
Green sulfur bacteria (e.g., Chlorobium thiosulfatophilum and
Chlorobium vibrioforme) can use sulfur compounds as the electron
donor as well as organic hydrogen donors (Blankenship et al., 1995).
As shown in Fig. 19 the reaction center of green sulfur bacteria is
similar to the photosystem I reaction center of oxygenic organisms (Feiler
and Hauska, 1995). The FeS centers in the reaction center can reduce
NAD+ (or NADP+) by ferredoxin and the ferredoxin-NAD(P)+
oxidoreductase enzyme, therefore green sulfur bacteria are not
necessarily dependent on reverse electron flow for carbon reduction.
The antenna system of the green sulfur bacteria is composed of
bacteriochlorophyll and carotenoids and is contained in complexes
known as a chlorosomes that are attached to the surface of the
photosynthetic membrane. This antenna arrangement is similar to the
phycobilisomes of cyanobacteria. Green sulfur bacteria can fix CO2
without Rubisco. It has been proposed that they accomplish this by
using the respiratory chain that normally oxidizes carbon (known as
the Krebs cycle), resulting in the release of CO2. With the input of
energy this process can be run in the reverse direction, resulting
the uptake and reduction of CO2.
6.3 Green Gliding Bacteria
Green gliding bacteria (e.g., Chloroflexus aurantiacus), also
known as green filamentous bacteria, can grow photosynthetically
under anaerobic conditions or in the dark by respiration under
aerobic conditions. Like the green sulfur bacteria, green gliding
bacteria harvest light using chlorosomes. The green gliding bacteria
appear to have reaction centers similar to those of the purple
bacteria (Fig. 19), but there are several notable differences. For
example, instead of two monomer bacteriochlorophyll molecules, C.
aurantiacus has one bacteriochlorophyll and one bacteriopheophytin
and the metal between the two quinones is Mn rather than Fe (Feick et
al., 1995). C. aurantiacus appears to fix CO2 by a scheme that does
not involve the Calvin cycle or the reverse Krebs cycle (Ivanovsky et
al., 1993).
6.4 Heliobacteria
Heliobacteria (e.g., Heliobacterium chlorum and Heliobacillus
mobilis) are in the phylum Gram Positive Bacteria that are strict
anaerobes. Although the heliobacterial reaction center is similar to
photosystem I in that it can reduce NAD+ (or NADP+), it contains a
different type of chlorophyll known as bacteriochlorophyll g (Amesz,
1995).
The three-dimensional structure of the reaction center
of Rhodopseudomonas viridis and Rhodobacter sphaeroides reveals the
distances between the electron donors and acceptors (Deisenhofer et
al. 1984,1985; Norris and van Brakel, 1986; Feher et al. 1989) and
has had an important influence on biophysical and molecular genetics
studies designed to identify the factors that control the rate of
electron transfer within proteins. There is currently a controversy
concerning the importance of specific amino acid composition of the
protein on the rate of intraprotein electron transfer. In part, the
disagreement centers on whether the protein between the donor and
acceptor molecules can be treated as a uniform material, or whether
the specific amino acid composition of the protein significantly
alters the rate. For example, it has been proposed that aromatic
amino acids may provide a particular pathway that facilitates
electron transfer between a donor and acceptor pair. This is the case
in the photosystem II reaction center, where a tyrosine residue on
one of the reaction center core proteins ( precisely, Tyr 161 on the
D1 protein) donates an electron to the primary donor chlorophyll,
P680+. However, in other cases, replacement of an aromatic by another
non-aromatic residue has resulted in relatively minor changes in the
rate of electron transfer. L. Dutton and coworkers (Moser et al.,
1992) have analyzed electron transfer reactions in biological and
chemical systems in terms of electron tunneling theory developed by
R. Marcus and others (DeVault, 1984). Dutton and coworkers argue that
protein provides a uniform electronic barrier to electron tunneling
and a uniform nuclear characteristic frequency. They suggest that the
specific amino acid residues between an electron transfer pair is
generally of less importance than the distance in determining the
rate of pairwise electron transfer. In their view, protein controls
the rate of electron transfer mainly through the distance between the
donor and acceptor molecules, the free energy, and the reorganization
energy of the reaction. The importance of distance is demonstrated by
electron transfer data from biological and synthetic systems showing
that the dependence of the electron transport rate on the edge to
edge distance is exponential over 12-orders of magnitude when the
free energy is optimized (Moser et al., 1992). Increasing the
distance between two carriers by 1.7 Å slows the rate of electron
transfer 10-fold. The extent to which this view is generally
applicable for intraprotein transfer remains to be established
(Williams, 1992). One of the challenges in understanding pairwise
electron transfer rates from first principles is illustrated by the
reaction centers of Rhodopsuedobacter sphaeroides in which the redox
components are arranged along two-fold axis of symmetry that extends
from the primary donor (P870) to the non heme Fe. Despite the fact
that the reaction center presents two spatially similar pathways for
electron transfer from P870 to quinone, nearly all electrons are
transferred down the right-arm of the reaction center as shown in
Fig. 17. The same is true for the reaction center of Rhodopseudomonas
viridis, in which it is estimated that electron transfer down the
left-arm is less than 1:100 (Kellogg et al., 1989). The challenge to
theorists is to explain the surprisingly high probability that
electron flow goes down the right-arm. Since the distances are
similar, it has been suggested that electron transfer down the
left-arm is less probable due to an endothermic free energy change
(Parson et al., 1990) or to an unfavorable rearrangement energy for
the reaction (Moser et al., 1992).
The amount of CO2 removed from the atmosphere each
year by oxygenic photosynthetic organisms is massive. It is estimated
that photosynthetic organisms remove 100 x 1015 grams of carbon
(C)/year (Houghton and Woodwell, 1990). This is equivalent to 4 x
1018 kJ of free energy stored in reduced carbon, which is roughly
0.1% of the incident visible radiant energy incident on the
earth/year. Each year the photosynthetically reduced carbon is
oxidized, either by living organisms for their survival, or by
combustion. The result is that more CO2 is released into the
atmosphere from the biota than is taken up by photosynthesis. The
amount of carbon released by the biota is estimated to be 1-2 x 1015
grams of carbon/year. Added to this is carbon released by the burning
of fossil fuels, which amounts to 5 x 1015 grams of carbon/year. The
oceans mitigate this increase by acting as a sink for atmospheric
CO2. It is estimated that the oceans remove about 2 x 1015 grams of
carbon/year from the atmosphere. This carbon is eventually stored on
the ocean floor. Although these estimates of sources and sinks are
uncertain, the net global CO2 concentration is increasing. Direct
measurements show that each year the atmospheric carbon content is
currently increasing by about 3 x 1015 grams. Over the past two
hundred years, CO2 in the atmosphere has increased from about 280
parts per million (ppm) to its current level of 360 ppm. Based on
predicted fossil fuel use and land management, it is estimated that
the amount of CO2 in the atmosphere will reach 700 ppm within the
next century. The consequences of this rapid change in our atmosphere
are unknown. Because CO2 acts as a greenhouse gas, some climate
models predict that the temperature of the earth's atmosphere may
increase by 2-8°reeC. Such a large temperature increase would lead
to significant changes in rainfall patterns. Little is known about
the impact of such drastic atmospheric and climatic changes on plant
communities and crops. Current research is directed at understanding
the interaction between global climate change and photosynthetic
organisms.
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Fig. 1
Photosynthesis is shown as a series of reactions that transform
energy from one form to another. The different forms of energy are
shown in boxes and the direction of energy transformation is shown by
the arrows. The energy-transforming reaction is shown by italics in
the arrows. The site at which the energy is stored is shown in
capital letters outside the boxes. The primary photochemical
reaction, charge separation, is shown in the oval. Details of these
reactions are given in the text.
Fig. 2
A. An electron micrograph of a plant chloroplast (Micrograph by A.D.
Greenwood, courtesy of J. Barber). The chloroplast is about 6 Å long.
Inside the chloroplast is the photosynthetic membrane, which is
organized into stacked and unstacked regions. It is not known why the
photosynthetic membrane forms such a complicated architecture. The
stacked regions are linked by unstacked membranes. B. A model of the
chloroplast (Ort, 1994) showing the photosynthetic membrane.
Fig. 3
Model of the photosynthetic membrane of plants showing the electron
transport components and the ATP Synthase enzyme (cross sectional
view). The complete membrane forms a vesicle. The pathways of
electrons are shown by solid arrows. The membrane bound electron
transport protein complexes involved in transferring electrons are
the photosystem II and I reaction centers (PSII and PSI) and the
cytochrome bf complex (Cyt bf). Abbreviations: Tyr, a specific
tyrosine on the D1 protein ; P680 and P700, the reaction center
chlorophyll of photosystem II and photosystem I, respectively; Pheo,
pheophytin; QA, and QB bound plastoquinones; PQH2, reduced
plastoquinone; Cyt bL and Cyt bH, different forms of b-type
cytochromes; FeS, iron-sulfur centers; Cyt f, cytochome f; PC,
plastocyanin; A0, chlorophyll; A1, phylloquinone; FX, FA and FB, iron
sulfur centers; Fd, ferredoxin; FNR, ferredoxin/NADP+ oxidoreductase;
NADPH, nicotinomide adenine dinucleotide phosphate (reduced form);
ADP, adenosine diphosphate; ATP, adenosine triphosphate; Pi,
inorganic phosphate; H+, protons; DY, the light-induced electrical
potential across the membrane. In this diagram, plastoquinone
(PQ,PQH2) and plastocyanin (PC) are shown with feet to indicate that
they are mobile. The light- harvesting protein complexes are not
shown. Details are given in the text.
Fig. 4
Chemical structure of chlorophyll a molecule.
Fig. 5
TOP: Estimated absorption spectra of chlorophyll a , chlorophyll b
and carotenoids in chloroplasts. BOTTOM: Action spectrum of
photosynthesis (oxygen evolution/incident photon) shows peaks at
wavelengths where chlorophylls a and b have absorption peaks, proving
that light absorbed by these pigments leads to photosynthesis
(unpublished data).
Fig. 6
A simplified scheme showing light absorption in antenna pigments
followed by excitation energy transfer to a reaction center
chlorophyll. The antenna and reaction center chlorophyll molecules
are physically located in different proteins. Primary photochemistry
(electron transfer from the primary electron donor to the primary
electron acceptor) takes place in the reaction center.
Fig. 7
Schematic drawing of photosystem II. Photosystem II is composed of
numerous polypeptides, but only two of them, D1 and D2, bind the
electron carriers involved in transferring electrons from YZ to
plastoquinone. Abbreviations: YZ, tyrosine; P680, reaction center
chlorophyll (primary electron donor); Pheo, pheophytin; QA and QB,
bound plastoquinone; PQH2, reduced plastoquinone, Cyt b559, b-type
cytochrome. Details are given in the text.
Fig. 8
Photosystem II electron transport pathways and rates. The vertical
axis shows the midpoint potential of the electron carriers. The heavy
vertical arrow show light absorption. P680* is the electronically
excited state of P680. The abbreviations are given in the legend of
figs. 3.
Fig. 9
Structure of plastoquinone (reduced form), an aromatic molecule that
carries electrons and protons in photosynthetic electron transport.
Fig.
10 Yield of oxygen from photosynthetic membranes exposed to a
series of brief flashes as a function of flash number. The maximum
oxygen yield exhibits a four-flash periodicity. The yield is highest
after the third flash and peaks again four flashes later. The four
flash dependence of the amplitude gradually decreases as the number
of flashes increases due to misses and double hits. The occurrence of
the peaks every 4th flash is due to the chemistry of water oxidation
(4 electrons must be removed from two water molecules to yield one
oxygen molecule) and the machinery of photosystem II (each reaction
center works independently, binding two water molecules and releasing
one molecule of oxygen every four flashes). Water oxidizing machinery
works as a cyclic process that supplies electrons to the oxidized
primary donor, P680+. After one flash of light, P680+ is formed, and
an electron is transferred via the tyrosine Yz from a manganese
complex (4 Mn atoms). After a second flash, this process is repeated
and a second oxidation occurs at the Mn complex; after a third flash,
a third oxidation occurs; and after a fourth flash, a fourth
oxidation occurs, i.e., the Mn complex accumulates 4 positive (+)
charges. This enables the Mn complex to oxidize 2 H2O, release
molecular oxygen and 4 protons (H+s). This is the process known as
the oxygen clock.
Fig.
11 Schematic drawing of photosystem I. Photosystem I is composed
of numerous polypeptides, but only three of them bind the electron
carriers. Abbreviations: PC, plastocyanin; P700, reaction center
chlorophyll (primary electron donor); A0, chlorophyll, A1,
phylloquinone; FeS, FeS centers; Fd, ferredoxin. Details are given in
the text.
Fig.
12 Photosystem I electron transport pathways and rates. The
vertical axis shows the midpoint potential of the electron carriers.
Abbreviations are given in the legend of fig. 11( FA and FB are
equivalent names for FeSA and FeSB).
Fig.
13 The electron transport pathway of plants (oxygenic
photosynthesis). Abbreviations are given the legend of fig. 3.
Details are given in the text.
Fig.
14 Schematic drawing of the ATP synthase enzyme embedded in the
membrane. Proton transfer through the ATP Synthase provides the
energy for the creation of ATP from ADP and Pi. Abbreviations are
given in the legend of fig. 3. Details are given in the text.
Fig.
15 The ATP synthase consists of a membrane portion and an water
exposed portion (see Fig. 14). The water exposed portion, which looks
like a door knob, has five subunits ( 1g,1d, 1e ). The combine as ab
pairs. The catalytic sites of the enzyme are on the b-subunits. The g
subunit sort of connects the exposed part to the membrane part (Fo).
The diagram shows a model of the top of the ATP synthase according to
Boyer (1993). In this model, there are three alternate binding sites.
At one site ADP and Pi bind; at another site ADP and Pi produce bound
ATP; and at the third site bound ATP is released. In this model, most
energy is used to release bound ATP. Each of the three sites perform
all three steps, but at different times. Thus, the activity rotates
on the a/b pairs. The energy of the proton gradient is converted, in
this model, to conformational energy of the g protein that rotates
and transfers the energy to the a/b pairs for the simultaneous
binding of ADP and Pi and the release of ATP. (Evidence for such a
scheme has been found by Abrahams et al. (1994) in beef-heart
mitochondria and by Sabbert et al. (1996) in chloroplasts.)
Fig.
16 An abbreviated scheme showing reduction of carbon dioxide by
the Calvin Cycle. The first step is carboxylation, in which Ribulose
1,5-bisphosphate carboxylase/oxygenase (Rubisco) catalyzes the
addition of CO2 to the five-carbon compound, ribulose
1,5-bisphosphate, which is subsequently split into two molecules of
the three-carbon compound, 3-phosphoglycerate. Next are reduction and
phosphorylation reactions that form the carbohydrate, triose
phosphate. Some of the triose phosphate molecules are used to form
the products of photosynthesis, sucrose and starch, while the rest is
used to regenerate ribulose 1,5-bisphosphate needed for the
continuation of the cycle. Details are given in the text.
Fig.
17 Relative positions of the chromophores of the reaction center
of Rhodobacter sphaeroides (from Norris and van Brakel, 1986).
Abbreviations: P870, reaction center bacteriochlorophyll (primary
electron donor); BChl, bacteriochlorophyll; B Pheo,
bacteriopheophytin, QA and QB, bound ubiquinones. Fe is non-heme
iron. Diagram shows center to center distances and times for electron
transfers. Details are given in the text.
Fig.
18 Structure of the bacterial reaction center by H. Michel, J.
Deisenhofer and R. Huber and co-workers. It contains three proteins:
"H (shown in black) "L" (shown as dotted)" and "M" (shown as hatched
bars). Both "L" and "M" have 5 helices each (labeled LA, LB, etc.)
and "H" is shown on the very top of the molecule -- it has one helix
(HA) that goes through the membrane. P is photoactive dimer of
bacteriochlorophyll; B is monomeric bacteriochlorophyll; H is
bacteriopheophytin - like bacteriochlorophyll, but without Mg2+; QA
and QB are quinone molecules. Diagram courtesy of Colin Wraight.
Fig.
19 Comparison of electron transport pathways in oxygenic and
anoxygenic organisms (from Blankenship, 1992). Abbreviations: Cyt
bc1, cytochrome bc complex; P840, reaction center bacteriochlorophyll;
other abbreviations are given in the legend of figs. 3 and 17. 1 Some
organisms derive their energy from electron donating inorganic
molecules such as hydrogen gas or sulfur compounds and are not
dependent on current or past photosynthesis for their survival.
Examples include the bacterium Methanobacterium thermoautotrophicum,
which grows in sewage sludge living on hydrogen gas and carbon
dioxide and the bacterium Methanocococcus jannaschii, which grows in
the ocean near hot vents.
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