Lesson 2: The Chemistry of Life (Printer Friendly Format)


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Lesson 2: The Chemistry of Life

Introduction

 

The cell is considered the fundamental unit of life. Nothing smaller than the cell has all the properties of life. We are going to spend most of this lesson discussing macromolecules -- carbohydrates, proteins, fats, and nucleic acids. These are the molecules that make up all living organisms. To understand how they are made and how their structure relates to their function, we first have to understand some basic concepts of chemistry. Since some of you may not have taken any chemistry classes, our discussion of the topic will be fairly simple. For those who have taken some chemistry, consider this a good review.

Readings & Assignments

For this lesson, you will need to:
  • Read textbook Chapter 3, and Chapter 15 sections 15.1-15.2
  • Review the on-line material for Lesson 2
  • Submit questions and offer answers to the Lesson Two discussion forum in the Lesson Discussion Forums folder
  • Work on your Biology In Our Lives Essay #1 (Remember that topics need to be pre-approved by the instructor)
  • Please make sure that you have or are working on Securing a Suitable Exam Proctor and filling out a Proctor Information Form for your final exam

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Atoms

The reason that we cover chemistry in a biology course is because all life obeys chemical principles. We will start with the basic unit, the atom.  An element is the simplest form of matter and each element has a unique set of properties. An atom is the smallest component of an element that still has all of the properties of the element. An atom is to an element as a cell is to life. There are subatomic particles within an atom but if you look only at those particles you don't see all of the properties of the element that the atom belongs to. Similarly, a cell can be broken down into its components but those subcellular components don't have the properties of life. The following figure represents a helium atom. Helium exists as a gas; we use it to fill balloons, among other things.

A Helium Atom

Figure 2.1. A Helium Atom

In the center of an atom, is the nucleus, which is the core of the atom. The nucleus contains most of the mass of the atom. It is composed of positively charged subatomic particles, protons(+), and neutrally charged particles, neutrons. The nucleus is orbited by electrons which have a negative charge. Electrons contribute very little weight to an atom. In the text, the author uses the analogy that if you take all the electrons in your body compared to your body weight they would weigh less than your eye lashes. While electrons have very little mass, they are very important in chemical reactions. The configuration of the electrons determines how atoms interact with each other. Helium has two protons and two neutrons in the nucleus. It has two electrons orbiting the nucleus. Here the charge of the protons is balanced by the charge of the electrons. There are two positive charges for the protons and two negative charges for the electrons. Therefore, helium doesn't have any net charge- it is a neutral atom. Atoms can be seen using a scanning tunneling electronic microscope.

The atomic number, which is the number of protons that an atom has, identifies that atom as being a specific element.  For example, carbon atoms always have six protons so its atomic number is 6. The weight of an atom is the number of protons plus the number of neutrons because both subatomic particles have mass. Thus, carbon’s atomic weight is 12. Helium has an atomic number of two and an atomic weight of four because it has two protons and two neutrons. Chemists arrange the elements in a table by their atomic number and by their atomic weight.

The periodic table allows you to make predictions about how atoms should behave. This is important information if you're looking at the chemical properties of atoms. For example, if you look at the far right on the table, the column of elements, Helium (He), Neon (Ne), Argon (Ar), etc. are the noble gases. These are elements that exist as gases under normal conditions and they are very stable elements. While about 112 elements have been named, only 92 of these are naturally occurring elements; the others have been synthesized in the laboratory. Not all of these naturally-occurring elements are found in living organisms. Living organisms use a fairly small subset of all of the known elements, in particular carbon, hydrogen, oxygen, nitrogen, phosphorus and sulfur.

 

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Isotopes

Carbon is a very important atom for biological organisms, and we will talk about the chemical reasons for that. If you have ever watched Star Trek or other science fiction shows, you'll remember that they talk about carbon-based life forms. Life on Earth is considered to be carbon-based because the macromolecules that are the building blocks of life have a carbon "skeleton" to which other atoms attach. All carbon atoms have six protons. But different types of carbon have different numbers of neutrons. The element is defined by the number of protons but if there are different numbers of neutrons in the nucleus of that atom then you have a different isotope of that particular atom or element.

Carbon 12 is the most common form of carbon. It has six protons and six neutrons so it has an atomic weight of 12. Almost all of the carbon atoms in your body are Carbon 12. There is another form of carbon, Carbon 13, which is very rare. It is a stable form with six protons and seven neutrons. There also is a Carbon 14, which has six protons and eight neutrons. Carbon 14 occurs in very small quantities in the environment, with about one Carbon 14 atom for every trillion Carbon 12 atoms. All organisms have a little bit of Carbon 14 in their bodies. The carbon atoms in your body are constantly changing; you bring in food that has carbon atoms[,] which are then used to replace other carbon atoms in your body. Carbon 14 is incorporated into your body at about the same percent that it exists in nature. Chemically, these isotopes are identical in our body and they function the same way. The nucleus of Carbon 14 is not stable, however, and over time it breaks down or decays. When the nucleus is not stable we say that an isotope is radioactive. The rate of decay of a particular isotope is constant as are the particles that it decays into. We can use this information.
When an organism dies, incorporation of new carbon atoms stops. Death means that all of the carbon atoms that an organism has at that point are fixed, with the ratio of Carbon 12/Carbon 14 that exists in nature. As Carbon 14 decays over time, it is converted to an isotope of nitrogen, N14. This decay is the basis of Carbon 14 dating of fossils (Figure 3.7 in your text). We can measure the ratio of C12/C14 in the fossil and, knowing the rate of decay for C14, calculate its age; the smaller the ratio of C14, the older the specimen. We use radioactive decay of isotopes in a lot of different ways. Radioactivity has a bad public image because people associate radioactivity with mutation, but radioactive decay is a natural process.

There are many elements that have isotopes that are not stable. The decay of Carbon 14 does not release energy that can damage tissue, but there are some other radioactive decay processes that can cause tissue damage. Those isotopes release gamma rays or x rays, but even these can be used to benefit humans. Some are used in medicine. For example, if you have problems with your thyroid, the doctor may want to test thyroid function. Your thyroid uses the element iodine. The physician will give you a radioisotope of the element iodine. The half-life (the time that it takes for half of this radioactive form of iodine to decay) is very short. So physicians can measure the concentration of the element to see how well your thyroid is functioning. Radioisotopes are commonly used in scientific research. You can label DNA with a radioisotope of phosphorous and then visualize the DNA on a piece of film. You expose it to x-ray film because it releases energy when it decays. This allows you to determine the base composition of DNA in a process called DNA sequencing.

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Properties of Elements

Elements are the simplest form of matter. They are made up of only one kind of atom and each element has specific properties that are diagnostic of that element. For example, the element gold is a lustrous yellow metal that is solid under normal conditions. It has a very high melting point (1064°C.)  It is also soft and very malleable. In contrast, mercury, a silvery colored metal, is liquid at room temperature. Some elements readily combine with other elements while some like the noble gases (e.g. Neon) are inert. An element’s chemical properties are due to its electron configuration. It is the chemical properties, how the atoms of an element interact with other atoms that we are most interested in. We will discuss this more extensively in the Chemical Bonding section. We will not spend much more time on this except to mention that the properties of a molecule or compound are not the same as the properties of the atoms which make them up.

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Chemical Bonding

The process of the interaction between atoms is called bonding. There are several types of bonds depending upon the number of electrons in the atom. These different bonds are important in the structure and functioning of the various molecules. Because bonding depends upon the chemical properties of these atoms, it is important to look at the configuration of the electrons. Your text gives a good description of the position of electrons in an atom. If you think about the nucleus which consists of the protons and neutrons, being about the size of apple, the electrons would be about a mile away. They are like a "cloud" swarming around this atom. However, to represent them we draw them as orbitals. The first orbital can hold a maximum of two electrons. Each successive orbital can have eight electrons.  Figure 2.2 shows two elements, Helium and Neon. Helium has two electrons in its first orbital, while Neon has two electrons in its first orbital and eight electrons in the second orbital. These orbitals are full, carrying the maximum number of electrons for each level, which is why these gases are not chemically reactive. They do not form bonds with other atoms. Atoms that do not have a full outer orbital, however, will forms bonds in order to achieve that stable state.

The Configuration of Electrons in Helium and Neon

Figure 2.2. The Configuration of Electrons in Helium and Neon

We make this pictorial representation of electrons, but remember that electrons are never in the same position; they are constantly moving around the atom. Electrons have different energy states. If the electron is zipping around the atom and is fairly close to the nucleus, it's at a low energy level. The farther away the electron is from the nucleus, the more energy it is holding, so the higher the orbital, the more energy the electron has (see Figure 3.2 in your text). These orbitals and the energy in electrons, will be important when we talk about some of the cellular processes, such as photosynthesis. As I mentioned earlier, what we are most interested in is how individual atoms interact with each other and how atoms form molecules.

Molecules and Compounds

In Biology we usually don't talk about single elements, we talk about molecules and compounds. A compound is made up of atoms of two or more elements in a fixed ratio held together by chemical bonds. A molecule is the smallest unit of a compound. A molecule is to a compound as an atom is to an element. For instance, water is a compound composed of molecules of H2O, which means it has two hydrogen atoms and an oxygen atom. These atoms are bonded together in a specific way that gives water some unique properties. You can write the formula as H2O, or your can write it H-O-H, showing the position of the atoms relative to each other. As mentioned earlier, the physical characteristics of a compound are not necessarily the same as the physical properties of the elements which it is composed of. Using water as an example, we have hydrogen, which is a gas, and oxygen, which is a gas, making a liquid. Once these atoms are bonded together they exhibit different physical properties. While under what we call standard conditions, water is a liquid, we also all know that water can become a solid and water can become as well as a gas. Salt, NaCl, is another compound, composed of sodium (Na) and chloride (Cl) atoms. The molecules that comprise compounds are formed by chemical bonds between atoms. There are three types of chemical bonds that we will focus on, ionic bonds, covalent bonds and hydrogen bonds.

Ionic Bonds

Atoms are most stable when the have a complete outer electron shell. Because of this, atoms which have only one or two electrons in their outer orbital easily lose them to a atom which only needs one or two electrons to complete its outer orbital. The result is that each now has a full outer shell but they are left with a net electrical charge. Atoms which have an unequal number of protons and electrons are called ions. Ionic bonds then form between the ions due to the attraction of the opposite charges. For example, sodium chloride (NaCl) is formed through an ionic bond between a sodium ion and a chloride ion. In this process, Na loses the single electron in its outer orbital to Cl which had 7 electrons in its outer orbital. Na is now positively charged and Cl negatively charged. These opposite charges attract, holding the atoms together through electrostatic force (Figure 2.3).

Ionic Bonds - NaCl

Figure 2.3. Ionic Bonds - NaCl

Covalent Bonds

Covalent bonds form when electrons are shared between atoms. Essentially, this means that the electrons are orbiting around both of the atoms. This combining of orbitals results in a very strong and stable bond. The biological macromolecules that we are going to study are largely held together by covalent bonds. Water is an example of a molecule that is formed through covalent bonds. The oxygen atom has six electrons in its outer shell, so there is room for two more electrons before that shell is full. Each hydrogen atom has one electron in its electron shell and needs one more to be full (remember that the first orbital only holds two electrons). The two hydrogen atoms each share their electron with the oxygen atom (Figure 2.4), essentially filling the outer orbital of all three atoms. Carbon dioxide (CO2) is another example of a compound in which the atoms form molecules through covalent bonds. In this case, carbon needs four electrons and a double bond is formed between the carbon and each of the oxygen. In a double bond two electrons are shared between the two atoms.

Covalent Bonds - H2O

Figure 2.4. Covalent Bonds - H2O

Hydrogen Bonds

Another type of bond that is extremely important in biological systems is the hydrogen bond. These are very weak bonds that form between polar molecules. Polar molecules occur when one of the atoms in a covalent bond has a stronger attraction for the shared electron than the other. This usually involves an oxygen or nitrogen bonded with hydrogen. The result is that the electron spends more time around the larger atom giving that end of the molecule a partial negative charge and leaving the hydrogen atom with a partial positive charge. Hydrogen bonds then form between the slight negative end of one molecule and the slight positive end of another molecule. Hydrogen bonding is an important property of water as we’ll discuss next and in the structure and function of proteins and nucleic acids (DNA and RNA).

 

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Water

The one molecule that is considered to be essential to life is water. Water has a number of special properties that are key to its central importance for biological organisms. Most of these properties stem from the distribution of the electrons that oxygen and hydrogen share in the covalent bonds that form a water molecule. Oxygen is an electronegative atom. As we discussed above, it attracts electrons to it because oxygen has a larger positive charge (8 protons in the nucleus) when compared with the hydrogen atoms (one proton in the nucleus). Therefore, the electrons spend more time orbiting around the oxygen atom than the hydrogen atoms. Because of this, different parts of a water molecule have different charges, with the oxygen having a slightly more negative charge and the hydrogen a slightly more positive charge (Figure 2.5).

A Water Molecule

Figure 2.5. A Water Molecule

This difference in polarity means that water is a polar molecule. Hydrogen bonds join water molecules together, with the slightly positive hydrogen of one water molecule bonded to the slightly negative oxygen of anothr through weak electrostatic forces. It is this hydrogen bonding between water molecules that gives water many of its special properties.

Because of these bonds, water molecules tend to stick together, a property called cohesion. Surface tension is a consequence of this. Instead of spreading out flat on a surface, a drop of water will "bead-up". Some insects can use this property to allow them to walk on water. Figure 3.12 in you textbook shows a water strider pausing on top of the water.

Water also shows adhesion, which means that water molecules will also bond with other polar molecules. Capillary action, in which water can rise against gravity, is a result of adhesion. Plants are able to transport water from their roots to their leaves, sometimes over hundreds of feet, because water forms a column in the xylem, a type of plant vascular tissue, through adhesion with the cells of the xylem.

The difference in charge means that water can act as a polar solvent, so other molecules that are charged will dissolve in water. This is why salt dissolves when you pour it into a glass of water. The slightly positively charged hydrogen of the water molecules surround the negatively charged chloride ions (Cl-), while the slightly negatively charged oxygen of the water molecules surrounds the positively charged sodium ions (Na+), pulling them apart (Figure 2.6). Thus, the salt "dissolves". Molecules that will dissolve in water are called hydrophilic (water-loving) .

How NaCl dissolves in water.

Figure 2.6. How NaCl dissolves in water.
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Usually, as molecules go from a gas to a liquid and then to a solid, their density increases. However, solid water, or ice, is less dense than liquid water. This is a result of the hydrogen bonds between water molecules. As water freezes, the hydrogen bonds "set" the water molecules a certain distance apart, preventing them from moving closer together. Because the water molecules in ice are farther apart than they are in liquid water, ice is less dense and will float. This makes it possible for organisms that live in aquatic environments, primarily freshwater, to survive during the winter when the water freezes. They can live under the surface of the ice, where the temperature is around 4 degrees centigrade. If ice were more dense, the water would freeze from the bottom up.

Water also has a high heat capacity. A large amount of energy is required to disrupt the hydrogen bonds between water molecules and raise the temperature of water. This is important for organisms, which average about 70% water in their body composition, because it means that they are able to maintain a fairly constant temperature. Because of these hydrogen bonds, water also has a high temperature of vaporization. It takes a lot of energy to convert water from a liquid state to a gas. Many organisms take advantage of this by using evaporative cooling. When a dog pants, the evaporation of the water from its tongue disperses body heat, thus cooling the dog.

There are other properties of water that do not result directly from its polarity. Water is transparent. This means that light can penetrate it. This is important in aquatic ecosystems, because photosynthetic organisms require light energy. The region through which light can penetrate in a body of water is called the photic zone.

Water also is able to ionize, which means that the covalent bonds joining the oxygen and hydrogen break. This results in the formation of a hydrogen ion (H+) and a hydroxide ion (OH-). This is not common, as the covalent bonds joining the atoms are strong, but it does occur spontaneously. Approximately only one water molecule out of 550 million is ionized at any one moment. This corresponds to a concentration of H+ of 10-7 mole per liter in pure water. Therefore, pure water has a pH of 7.

Because the concentration of H+ and OH- are equal in pure water, pH7 is considered to be neutral. If the concentration of H+ in solution is higher, the solution is said to be acidic. Coffee (black) has a pH of 5, which means that the concentration of H+ is higher than the concentration of OH- ions. Because the pH scale is logarithmic, the coffee has a concentration of H+ 100 times higher than that of pure water. If there are more OH- in solution, then the solution is said to be basic. Bleach has a pH of about 12, which means that it has a concentration of OH- 100,000 times higher than pure water. As solutions become more acidic or more basic, they are more chemically reactive. Figure 3.14 in your textbook shows the pH scale.

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Forming Macromolecules

All organisms are composed of biological macromolecules. These are carbon-based compounds, which means that they have a fundamental structure composed of carbon atoms. Why carbon? Because carbon has only four electrons in its outer shell, it can form covalent bonds with four other atoms. Thus, it is able to form very stable bonds with other carbon molecules, enabling the formation of long carbon chains. Figure 2.7 shows methane,CH4, a simple carbon compound formed by these covalent bonds.

 

 

Methane

Figure 2.7. Methane

Biological macromolecules generally are polymers, (poly = many; mer = unit), formed by joining monomers, or single molecules, together in a long chain. They are formed by the process of polymerization. In this process, dehydration synthesis, or the removal of a water molecule, joins two monomers together (Figure 2.8). When cells produce polypeptides, chains of amino acids, during protein synthesis, the reaction that joins these amino acids together is a dehydration reaction (also called a condensation reaction).

Water molecules can be inserted between monomers to break down a polymer in a reaction called hydrolysis (Figure 2.8). This happens during digestion. For example, when you eat a cracker, enzymes in your mouth catalyze a chemical reaction, hydrolyzing the starch (a polymer) in the cracker and breaking it down into more simple sugars. This is why a cracker begins to taste sweet after you chew it.

 

Dehydration and Hydrolysis

Figure 2.8. Dehydration and Hydrolysis
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There are four major classes of biological macromolecules (Figure 2.9). The carbohydrates have two primary functions, to provide energy for cells and to provide structure.

Proteins play many roles in a cell, from enzymes which catalyze chemical reactions such as the amylase secreted by your salivary glands, to providing structure, the role of the keratin in your skin. Some proteins, such as insulin, function as hormones.

Lipids also have a diversity of functions, including energy storage as well as forming the primary structure of cell membranes.

Nucleic acids are information storage molecules, and play a role in converting this information into polypeptides.

These biological macromolecules can be very large. For example, the chemical formula of bovine growth hormone is C999H1529N263O299S7!

 

Biological Macromolecules

Figure 2.9. Biological Macromolecules
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Carbohydrates

Carbohydrates are molecules that have the chemical structure (CH2)n. The basic unit, or monomer, of a carbohydrate is a monosaccharide, or simple sugar (Figure 2.10). Glucose is a typical monosaccharide, with the chemical formula C6H12O6. Because of the hydroxyl (OH) groups, which have a slight positive charge on the hydrogen due to its covalent bond with the electronegative oxygen, glucose is water soluble.

The Structure of Glucose

Figure 2.10. The Structure of Glucose
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When two monosaccharides are joined together through dehydration synthesis, a dissacharide is formed (Figure 2.11). Maltose is composed of two glucose molecules.

Disaccharides

Figure 2.11. Disaccharides
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When many monomers are joined together a polysaccharide is formed. One of the two main functions of polysaccharides is energy storage. Energy is stored in the chemical bonds of the polysaccharides starch and glycogen, which are polymers of glucose molecules. Starch is the energy storage molecule of plants. Plants produce sugars through photosynthesis to meet their own energy needs. Any sugars that they do not immediately need are converted to starch for storage. When primary consumers eat plant material, they ingest starch, which is broken down through the process of digestion and the chemical bond energy released. We will learn more about this in lesson 4. Animals also store energy in the form of a carbohydrate, glycogen. However, glycogen is only used for short-term storage. In humans, glycogen is produced and broken down primarily in the liver.

Carbohydrates also have a structural role in some organisms. Plants use the polysaccharide cellulose as a major component of their cell walls. Cellulose also is a polymer of glucose monomers. However, the glucose molecules are bonded together differently, and the enzyme amylase, which can digest starch, cannot break the chemical bonds in cellulose. Therefore, in humans, cellulose acts as roughage, an important part of the diet that keeps material moving through the digestive system. It is not broken down during digestion. Animals that eat large amounts of plant material, such as cows and koalas, have organisms, bacteria and protists, living symbiotically in their digestive tract. These organisms do produce enzymes that can break the chemical bonds between glucose molecules in cellulose and allow the animal to obtain nutrition from that polysaccharide. The polysaccharide chitin also provides structure. It is a major component of the cell walls in fungi, and of the exoskeleton in arthropods.

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Proteins

Proteins have many diverse functions within organisms. See Table 3.4 in your textbook. Proteins are polymers of amino acids. Organisms use about 20 different amino acids to make proteins, and this means that the possible sequences of amino acids within proteins are almost infinite. There are structural proteins, such as the keratin that gives support to your skin or to a bird's feather.

Enzymes are proteins that catalyze chemical reactions within a cell, such as amylase which breaks starch into disaccharides and DNA polymerase which joins together DNA monomers. Some proteins transport substances across cell membranes, or through the body. For example, hemoglobin transports oxygen through your circulatory system.

There are even some proteins that function as hormones, including insulin, which regulates the level of glucose in your blood.

All proteins have the same basic structure. Amino acids are the monomers of proteins (Figure 2.12). They consist of a central carbon atom, which is bonded to a carboxyl group (COOH) at one end and an amino group (NHH) at the other. The carboxyl group allows the molecule to act as an acid, donating H+, while the amino group allows it to act like a base, accepting H+ ions.

The central carbon is covalently bonded to a side chain, the functional or “R group”. This R group is different for each of the 20 common amino acids and determines the property of the amino acids. R groups range from a single hydrogen atom to complex ring structures. Amino acids are joined together by dehydration synthesis to form a molecule called a polypeptide. When two amino acids are covalently bonded together, the bond is called a peptide bond, hence the name polypeptide (Figure 2.12).

 

Amino Acid Structure and Formation of the Peptide Bond

Figure 2.12. Amino Acid Structure and Formation of the Peptide Bond
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Most proteins do not function as a simple linear polypeptide chain.[, which is their primary structure]  In order to perform a specific task, they must be folded into a specific shape (Figure 2.13). There are four levels of protein structure. The first level, their primary structure, is the sequence of the amino acids.

Secondary structure is local folding [, usually through] which is held in place by hydrogen bonding of amino acids in close proximity to each other (Figure 2.13).
Levels of Protein Structure (1)

Figure 2.13. Levels of Protein Structure (1)
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Tertiary structure involves folding of the molecules across longer distances (Figure 2.14), often through disulfide bridges, which are bonds between two amino acids that contain a sulfur atom. These bridges occur in the proteins in hair. If you go the the hairdresser and get a permanent, the tertiary structure is denatured chemically. Sulfur atoms are released, resulting in the characteristic odor. The hair is then treated with other chemicals that reform the bonds when the hair is on rollers, giving it a different shape, curly versus straight.

Finally, quaternary structure is the association of multiple polypeptides (Figure 2.14). For example, the protein hemoglobin consists of four polypeptides joined together.

Levels of Protein Structure (2)

Figure 2.14. Levels of Protein Structure (2)
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There are special proteins called chaperone proteins which aid in the proper folding of the polypeptides into their final shape. Some assist in the folding of newly made proteins while others appear to refold proteins which are misfolded or have unfolded (denatured) due to increased temperatures.

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Lipids

Lipids have a number of different functions within cells. They are energy storage molecules, they are a major component of the plasma membrane, and they also function as hormones. So, how can lipids carry out these different functions? They are not polymers in the sense that we have discussed for proteins and carbohydrates. The fundamental structure of a lipid is comprised of fatty acids and a glycerol molecule. Fatty acids are a type of hydrocarbon, long chains of carbon atoms bonded to hydrogens. Because electrons usually are distributed evenly around these molecules, they are nonpolar, or hydrophobic (water-fearing), and therefore not water soluble. We will discuss the major groups of lipids and how this structure is modified to perform different functions.

Fats are used to store energy within their chemical bonds. They also serve as insulation in organisms that maintain a constant body temperature, such as mammals and birds. The building blocks of fats are triacylglycerol molecules. These molecules are composed of one glycerol and three fatty acids. The fatty acids are bonded to the glycerol molecule through three dehydration synthesis reactions, forming a triacylglycerol (Figure 2.15).

 

Formation of a Fat Molecule

Figure 2.15. Formation of a Fat Molecule
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Fatty acids determine the type of fat molecule, and can differ in the number of carbon atoms and the number of carbon to carbon double bonds. Steric acid is an example of a saturated fatty acid. It has no double bonds within its hydrocarbon chain; each carbon has the maximum number of hydrogens covalently bonded, it is “saturated”. Because of this, the chains lie flat (Figure 2.16). Saturated fats are usually solid at room temperature and usually come from animal sources.

Linoleic acid is an example of an unsaturated fatty acid. There are double bonds between some of the carbons within the hydrocarbon chain. These [some] carbons are not bound to the maximum number of hydrogens possible, or are unsaturated. Because of this, the chains tend to bend and flex (Figure 2.16). Therefore, unsaturated fats are usually liquid at room temperature. and These usually come from plant sources, such as corn, olives, and soybeans. Studies have shown that a diet high in saturated fats can raise the level of LDL cholesterol in the blood. Read "The Facts on Fats" on the Discovery Health Web site for more information on fats in the diet.

Fats are used for energy storage in both plants and animals. The average human has about 36 pounds of fat distributed throughout their body. Fat is also used for insulation. This is especially important in marine animals, because body heat is easily lost to the water (hypothermia). Therefore, mammals such as whales and dolphins have a thick layer of blubber, which insulates their bodies and greatly reduces heat loss.

 

Saturated and Unsaturated Fats

Figure 2.16. Saturated and Unsaturated Fats
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Phospholipids are the molecules that comprise the basic structure of all plasma membranes. We will go into much more detail about these membranes in lesson 3. In this lesson, we will concentrate on how the structure of these molecules leads to their function within the membrane.

Phospholipids have the same basic structures as triacylglycerols. However a phosphate group is present instead of the third fatty acid (Figure 2.17). This phosphate group has a negative charge. Because of this, the two ends of the molecule have different properties. The fatty acid end, with its long hydrocarbon tail, is nonpolar, and therefore insoluble in water. However, the end with the phosphate group is polar, therefore it is water soluble.

When these molecules interact to form a membrane, they form two layers, with the nonpolar fatty acid tails of each layer on the inside of the membrane and the polar phosphate groups on the outside. We will leave the discussion of the complexity of the membrane until lesson 3.

 

Phospholipid Structure

Figure 2.17. Phospholipid Structure
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Steroids are the group of lipids that includes many hormones. These molecules are secreted from glands that are part of the endocrine system and are used for long-range communication within the body. We will discuss the action of hormones when we cover human reproduction in lesson 10. Testosterone and estrogen are steroid hormones. These molecules generally have more complex ring structures, as shown in Figure 2.18.

Another type of steroid is cholesterol. Although excess levels of LDL cholesterol have been associated with coronary disease in human, this molecule is an integral part of the plasma membrane in most animal cells. Pigments are another important group of steroids. We will discuss the pigment chlorophyll in lesson 4.

 

Steroid Hormones

Figure 2.18. Steroid Hormones
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Nucleic Acids

The final group of biologial macromolecules are the nucleic acids, which function to store genetic information and to express that information in the production of polypeptides. The monomer of nucleic acids is the nucleotide. This monomer consists of three parts (Figure 2.19). The first is a five-carbon sugar molecule, either ribose or deoxyribose. The nucleic acid DNA has deoxyribose as its sugar, and the nucleic acid RNA has ribose (Figure 2.20). This sugar is joined to a phosphate group. These phosphates and sugars alternate to form the backbone of the nucleic acid. The third component, the nitrogenous base, is also bonded to the sugar, and is approximately perpedicular to the sugar/phosphate backbone. There are four types of nucleotides in DNA and RNA. Both include the nucleotides adenine (A), cytosine (C) and guanine (G). DNA includes the nucleotide thymine (T), which is replaced by uracil (U) in RNA (Figure 2.20).

The Structure of a Nucleotide

Figure 2.19. The Structure of a Nucleotide
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DNA and RNA Comparison

Figure 2.20. DNA and RNA Comparison
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RNA molecules are a single strand of nucleotides, whereas DNA is composed of two nucleotide strands that twist around each other. The structure of DNA is called a double helix (Figure 2.21). The two strands are held together by the hydrogren bonding of the nitrogenous bases. If you untwist the DNA and think of the sugar/phosphate backbone as the sides of the ladder, then the nitrogenous bases would be the rungs. The base adenine, which has a double ring structure, pairs with thymine, a single ring, while guanine, a double ring, pairs with cytosine, a single ring. This keeps the same spacing between the sides, thus insuring that the double helix has a constant width. We will discuss nucleic acids in much more detail in lesson 7.

 

 

 

 

Base-Pairing

Figure 2.21. Base-Pairing
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page 12 of 12

Origin of Life

The origin of life is one of the most interesting questions in biology. However, it also is one of the most difficult to address. There was no one there to witness the process, therefore we must deduce what happened through other means of inquiry. To address how life originated, we can perform experiments and examine organisms that live today. To address where this may have happened, we can examine existing organisms and perform experiments. Finally, to address when life first arose, we can look to the fossil record, as well as use the information from molecular clocks.

The universe formed about 10-15 billion years ago in a process known as The Big Bang. Earth formed 4.5 billion years ago. How do we know this date so precisely? There are no rocks on earth that are this old; the oldest rocks date to about 4 billion years ago (Figure 2.22). However, there are moon rocks, collected on manned missions to the moon, that have been dated to 4.5 billion years. Because it is assumed that the Earth and the moon formed at approximately the same time, these rocks provide information on the age of the Earth.

 

 

Clock of Biological Time

Figure 2.22. Clock of Biological Time
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A Single Origin of Life

At some point between 4 billion and 3.5 billion years ago, Earth was transformed from a non-living system to a living system. This time is constrained by the cooling of the Earth's crust. There was probably no constant surface water before about 4 billion years. The fossil record indicates that by 3.5 billion years there were prokaryotes on Earth. The evidence suggests that all life today had a single common ancestor, or a single origin. The most compelling argument for this is that all organisms use the same triplets of nucleotides to code for amino acids. This universality of the genetic code across all known organisms indicates a single common ancestor.

Early Conditions on Earth

The early Earth was very different from the planet we a familiar with. The surface would have been a chaotic place, with strong volcanic activity. Volcanoes today produce large amounts of water vapor and carbon dioxide, and it is assumed that the same would have been true early in Earth's history. Earth also would have experienced heavy bombardment by bolides, extraterrestrial objects such as asteroids and meteorites. While those impact craters are no longer apparent today, we only have to look at the surface of the moon to see evidence that bolide impacts were common in the early solar system. The atmosphere of early Earth also would have been very different. It would have been composed primarily of nitrogen, water vapor, carbon dioxide, with trace amounts of carbon monoxide, hydrogen and methane. Perhaps most importantly, there would have been little or no free oxygen. Therefore, the earliest forms of life were most likely anaerobic, that is they did not require oxygen for their cellular metabolism. Energy sources on the early earth would have been lightning, which is produced during volcanic eruptions, and sunlight. While the sun was weaker at that time, there was no protective ozone layer in the atmosphere; therefore more ultraviolet (UV) radiation would have struck Earth's surface.

The Miller-Urey Experiments

In 1953, Stanley Miller, then a graduate student, and Harold Urey, devised an experiment that would cast new light on the origin of life. They set up an apparatus that simulated the atmosphere of early Earth. They then applied energy, in the form of an electric spark, and collected the chemicals that resulted from this reaction. They were able to synthesize a number of organic molecules from inorganic components, including some amino acids. Their experiments have come under scrutiny in recent years because the "atmosphere" that they used was more H rich than the early Earth's atmosphere is now believed to be. But, if this experiment is run using a less reducing atmosphere, biological molecules or their precursors are synthesized. Formaldehyde (H2CO) is produced, and sugars can be derived from this molecule. Nucleotide bases can be synthesized from HCN, which is derived from methane. Finally, some molecules, such as phosphate, could come from the weathering of rock. But, it is clear that these experiments have shown that biotic compounds can be synthesized from abiotic compounds.

Where did life originate?

This question of where life originated is very difficult to address. Darwin spoke of a warm little pond as home for the first life forms. The support for this is that organic molecules can be synthesized from a simulated early atmosphere. It has been suggested that these compounds could rain down into pools, where further biochemical reactions would then occur. However, there are a number of arguments against this scenario. Remember, in our discussion of polymerization, that many of those reactions are a dehydration synthesis, with the loss of a water molecule.

Some biochemists argue that these reactions would have been unlikely to occur spontaneously in the water. Also, the surface of the early earth was most likely repeatedly sterilized by bolide impacts. As mentioned above, we can see impact craters on the surface of the moon. Some are very large. The Mare Imbrium crater was caused by a bolide about 70 miles in diameter.

Recently, some researchers have argued that life may have originated at deep-sea hydrothermal vents. Today, these vents house a diverse array of organisms whose ecosystem is based on chemosynthesis, rather than photosynthesis. Proponents of this theory point to DNA sequence information from organisms that live today. The data shows that many of the most divergent (oldest) lineages within the bacteria and archaea are thermophiles, species that live in very hot environments. However, this also could be the result of a selective event early in the history of life.

Finally, some researchers have suggested that earth was "seeded" by complex organic molecules from space. This theory is called panspermia. In 1969, a meteorite fell near Murchison, Australia. When that meteorite was examined, it was found to carry many organic chemicals, including amino acids, and in proportions similar to those generated by the Miller and Urey experiments. Most recently, it has been suggested that a Martian meteorite collected in Antarctica contains evidence that life existed on that planet. Obviously, this question will continue to be debated for many years to come.

How did the first macromolecules and cells form?

If polymerization in an aqueous environment does not seem likely, how did the first macromolecules form? It has been shown that polymers can be created in the laboratory without biological catalysts. In these experiments, dilute solutions of monomers, such as amino acids or nucleotides, are placed on a hot, mineral substrate, such as clay or sand. The water vaporizes and short polymers will form. It also has been shown that macromolecules will aggregate in solution. Microspheres, which are small droplets composed of protenoids (short polymers of amino acids), have been synthesized in the lab. These do show some properties of cells, including selective permeability.

How did early life transmit genetic information?

For many years, scientists were puzzled by a seeming paradox. DNA carries genetic information and the information is used to direct the synthesis of proteins within a cell. However, in order for this message to be transcribed from the DNA, or for the DNA to replicate, proteins are required. This leads to the question of which came first -- DNA or proteins?

In the 1980s, it was discovered that RNA, in addition to carrying genetic information, could, as "ribozymes", catalyze some basic reactions. This raised the possibility that perhaps the early earth was an RNA World, with RNA both carrying genetic information and catalyzing chemical reactions. This also is supported by the many functions of RNA within the cell; it is integral to all aspects of protein synthesis, including the formation of the peptide bond.

When did life originate?

The first prokaryotic fossils date to approximately 3.5 billion years ago. Many of these earliest fossils are microfossils, requiring a microscope to detect them. There are fossils of structures that look very much like present day stromatolites. These stromatolites are formed by mats of cyanobacteria, and are only found in very saline marine environments from which grazing animals are excluded. There are some chemical fossils dated to 3.8 billion years that suggest biological activity because they are enriched in the isotope of carbon, C12, that is used by living organisms. However, because there are relatively few rocks older than 3.5 billion years, fossils of the very earliest organisms may never be found. But, from the available evidence, it is likely that life originated and diversified within a 500 million year period; that earliest life was probably prokaryotic, and anaerobic. Aerobic respiration and the eukaryotic cell arose about 1 billion years later. In the next lesson, we turn our attention to cell structure, focusing on the eukaryotic cell. 

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