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Chapter 2 Chemistry Comes Alive Part A Shilla Chakrabarty, Ph.D. Copyright © 2010 Pearson Education, Inc. Matter And Energy Matter is anything that has mass and occupies space States of matter: 1. Solid - definite shape and volume 2. Liquid - definite volume, changeable shape 3. Gas - changeable shape and volume Energy is the capacity to do work or put matter into motion Types of energy: • Kinetic - energy in action • Potential - stored (inactive) energy Copyright © 2010 Pearson Education, Inc. Forms of Energy and Energy Conversions Forms Of Energy • Chemical energy — stored in bonds of chemical substances • Electrical energy — results from movement of charged particles • Mechanical energy — directly involved in moving matter • Radiant or electromagnetic energy —exhibits wavelike properties (i.e., visible light, ultraviolet light, and X-rays) Energy Conversions • Energy may be converted from one form to another • Conversion is inefficient because some energy is “lost” as heat Copyright © 2010 Pearson Education, Inc. Composition of Matter • All matter is composed of elements • Elements cannot be broken down by ordinary chemical means • Each element has unique physical and chemical properties: Physical properties are detectable with our senses, or are measurable Chemical properties determine how atoms interact (bond) with one another • Of the 92 naturally occurring elements, only 25 are essential for living organisms • Atoms are the unique building blocks for each element Copyright © 2010 Pearson Education, Inc. Major Elements Lesser Elements Trace Elements Copyright © 2010 Pearson Education, Inc. Properties Of An Element Depend On The Structure Of Its Atoms Each element consists of unique atoms. An atom is the smallest unit of matter that still retains the properties of an element. composed of even smaller parts, called subatomic particles. Neutrons and protons: packed together to form a dense core, the Atomic Nucleus, at the center of an atom. Neutrons: No charge; mass = 1 atomic mass unit (amu) Protons: Positive charge; mass = 1 amu Electrons: Form a cloud around the nucleus; equal in number to protons in an atom Negative charge, negligible mass (1/2000th that of protons and neutrons) Copyright © 2010 Pearson Education, Inc. Models of the Atom Orbital model: current model used by chemists • Depicts probable regions of greatest electron density (an electron cloud) • Useful for predicting chemical behavior of atoms Planetary model — oversimplified, outdated model • Incorrectly depicts fixed circular electron paths • Useful mostly for illustrations Copyright © 2010 Pearson Education, Inc. Nucleus Nucleus Helium atom Helium atom 2 protons (p+) 2 neutrons (n0) 2 electrons (e–) 2 protons (p+) 2 neutrons (n0) 2 electrons (e–) (a) Planetary model Proton Copyright © 2010 Pearson Education, Inc. Neutron (b) Orbital model Electron Electron cloud Figure 2.1 Atomic Number and Atomic Mass • Atoms of the various elements differ in number of subatomic particles • Atomic number: Number of protons in the nucleus of an atom. Written as a subscript before the symbol for the element (example, 2He). • Atoms generally have equal numbers of protons and electrons - no net charge. • Mass number: Is the sum of protons and neutrons in the nucleus of an atom Written as a superscript before an element’s symbol (example, 4He). Copyright © 2010 Pearson Education, Inc. Identifying Elements Proton Neutron Electron Atoms of different elements contain different numbers of subatomic particles Hydrogen (H) (1p+; 0n0; 1e–) Copyright © 2010 Pearson Education, Inc. Helium (He) (2p+; 2n0; 2e–) Lithium (Li) (3p+; 4n0; 3e–) Figure 2.2 Isotopes Of Elements All atoms of an element have the same number of protons (atomic number) but may differ in number of neutrons Proton Neutron Electron Isotopes are two atoms of an element that differ in number of neutrons. In nature, an element occurs as a mixture of isotopes. Hydrogen (1H) (1p+; 0n0; 1e–) Copyright © 2010 Pearson Education, Inc. Deuterium (2H) (1p+; 1n0; 1e–) Tritium (3H) (1p+; 2n0; 1e–) Radioisotopes And Their Applications • Radioactive isotopes • Decay spontaneously, giving off particles and energy Example: 14C is a radioactive isotope. In its decay, a neutron is converted to a proton and an electron. This converts 14C to 14N, changing the identity of that atom. • Cause damage to living tissues Example: Radon from Uranium decay causes Lung Cancer. • Can be detected by scanners • Some applications of radioactive isotopes in biological research: Dating fossils Tracing atoms through metabolic processes Diagnosing and treating medical conditions Copyright © 2010 Pearson Education, Inc. Molecules, Compounds and Mixtures • Most atoms combine chemically with other atoms to form molecules and compounds Molecule — two or more atoms bonded together (e.g., H2 or C6H12O6) Compound — two or more different kinds of atoms bonded together (e.g., C6H12O6) • Most matter exists as mixtures Mixtures — Two or more components physically intermixed Three types of mixtures Solutions Colloids Suspensions Copyright © 2010 Pearson Education, Inc. Solutions Homogeneous mixtures Usually transparent, e.g., atmospheric air or seawater Solvent: Present in greatest amount, usually a liquid Solute(s): Present in smaller amounts Concentration of solutions is expressed as: • Percent, or parts per 100 parts • Milligrams per deciliter (mg/dl) • Molarity, or moles per liter (M) 1 mole = the atomic weight of an element or molecular weight (sum of atomic weights) of a compound in grams 1 mole of any substance contains 6.02 1023 molecules (Avogadro’s number) Copyright © 2010 Pearson Education, Inc. Colloids and Suspensions Colloids (emulsions) • Are heterogeneous translucent mixtures, e.g., cytosol • Are large solute particles that do not settle out • Undergo sol-gel transformations Suspensions: • Heterogeneous mixtures, e.g., blood • Large visible solutes tend to settle out Copyright © 2010 Pearson Education, Inc. Solution Colloid Suspension Solute particles are very tiny, do not settle out or scatter light. Solute particles are larger than in a solution and scatter light; do not settle out. Solute particles are very large, settle out, and may scatter light. Solute particles Solute particles Solute particles Example Example Example Mineral water Gelatin Blood Copyright © 2010 Pearson Education, Inc. Figure 2.4 Mixtures vs. Compounds • Mixtures • No chemical bonding between components • Can be separated physically, such as by straining or filtering • Heterogeneous or homogeneous • Compounds • Can be separated only by breaking bonds • All are homogeneous Copyright © 2010 Pearson Education, Inc. Chemically Inert and Chemically Reactive Elements • Electrons occupy up to seven electron shells (energy levels) around nucleus • Octet rule: Except for the first shell which is full with two electrons, atoms interact in a manner to have eight electrons in their outermost energy level (valence shell) • Chemically Inert Elements Stable and unreactive Outermost energy level fully occupied or contains eight electrons • Chemically Reactive Elements Outermost energy level not fully occupied by electrons Tend to gain, lose, or share electrons (form bonds) with other atoms to achieve stability Copyright © 2010 Pearson Education, Inc. (a) Chemically inert elements Outermost energy level (valence shell) complete 8e 2e Helium (He) (2p+; 2n0; 2e–) Copyright © 2010 Pearson Education, Inc. 2e Neon (Ne) (10p+; 10n0; 10e–) Figure 2.5a (b) Chemically reactive elements Outermost energy level (valence shell) incomplete 1e Hydrogen (H) (1p+; 0n0; 1e–) 6e 2e Oxygen (O) (8p+; 8n0; 8e–) Copyright © 2010 Pearson Education, Inc. 4e 2e Carbon (C) (6p+; 6n0; 6e–) 1e 8e 2e Sodium (Na) (11p+; 12n0; 11e–) Figure 2.5b Chemical Bonds Types of Chemical Bonds • Ionic • Covalent • Hydrogen Copyright © 2010 Pearson Education, Inc. Ionic Bonds • Ions are formed by transfer of valence shell electrons between atoms • Anions (– charge) have gained one or more electrons • Cations (+ charge) have lost one or more electrons • Attraction of opposite charges results in an ionic bond • Ionic compounds form crystals instead of individual molecules (Example: NaCl or Sodium chloride) Copyright © 2010 Pearson Education, Inc. Ionic Bond Between Sodium And Chlorine Sodium atom (Na) (11p+; 12n0; 11e–) Chlorine atom (Cl) (17p+; 18n0; 17e–) + – Sodium ion (Na+) Chloride ion (Cl–) Sodium chloride (NaCl) (a) Sodium gains stability by losing one electron, and chlorine becomes stable by gaining one electron. Copyright © 2010 Pearson Education, Inc. (b) After electron transfer, the oppositely charged ions formed attract each other. Figure 2.6a-b Salt Crystals CI– Na+ (c) Large numbers of Na+ and Cl– ions associate to form salt (NaCl) crystals. Copyright © 2010 Pearson Education, Inc. Figure 2.6c Covalent Bonds • Formed by sharing of two or more valence shell electrons • Allows each atom to fill its valence shell at least part of the time Reacting atoms Resulting molecules + Hydrogen atoms or Carbon atom Molecule of methane gas (CH4) (a) Formation of four single covalent bonds: Structural formula shows single bonds. Carbon shares four electron pairs with four hydrogen atoms. Copyright © 2010 Pearson Education, Inc. Double Covalent Bonds Reacting atoms Resulting molecules + Oxygen atom or Oxygen atom Molecule of oxygen gas (O2) Structural formula shows double bond. (b) Formation of a double covalent bond: Two oxygen atoms share two electron pairs. Copyright © 2010 Pearson Education, Inc. Figure 2.7b Triple Covalent Bonds Reacting atoms Resulting molecules + Nitrogen atom or Nitrogen atom Molecule of nitrogen gas (N2) Structural formula shows triple bond. (c) Formation of a triple covalent bond: Two nitrogen atoms share three electron pairs. Figure 2.7c Copyright © 2010 Pearson Education, Inc. Non-polar Covalent Bonds • Sharing of electrons may be equal or unequal • Atoms with six or seven valence shell electrons are electronegative, e.g., oxygen • Atoms with one or two valence shell electrons are electropositive, e.g., sodium Equal sharing of electrons produces electrically balanced nonpolar molecules Example: CO2 Copyright © 2010 Pearson Education, Inc. Polar Covalent Bonds Unequal sharing by atoms with different electronattracting abilities produces polar molecules Example: Water Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. Figure 2.9 Hydrogen Bonds • A hydrogen bond forms when a hydrogen atom covalently bonded to one electronegative atom is also attracted to another electronegative atom In living cells, the electronegative partners of hydrogen are usually oxygen or nitrogen atoms • Hydrogen bonds are common between dipoles such as water • Hydrogen bonds also act as intramolecular bonds, holding a large molecule in a threedimensional shape Copyright © 2010 Pearson Education, Inc. Hydrogen Bonding Between Water Molecules + – Hydrogen bond (indicated by dotted line) + + – – – + + + – (a) The slightly positive ends (+) of the water molecules become aligned with the slightly negative ends (–) of other water molecules. Copyright © 2010 Pearson Education, Inc. Figure 2.10a (b) A water strider can walk on a pond because of the high surface tension of water, a result of the combined strength of its hydrogen bonds. Copyright © 2010 Pearson Education, Inc. Figure 2.10b Chemical Reactions • Occur when chemical bonds are formed, rearranged, or broken • Represented as chemical equations • Chemical equations contain: Molecular formula for each reactant and product Relative amounts of reactants and products, which should balance Examples: H + H H2 (hydrogen gas) 4H + C CH4 (methane) (reactants) Copyright © 2010 Pearson Education, Inc. (product) Patterns of Chemical Reactions (a) Synthesis reactions • Synthesis (combination) reactions • Decomposition reactions • Exchange reactions Synthesis Reactions • A + B AB • Always involve bond formation • Anabolic Smaller particles are bonded together to form larger, more complex molecules. Example Amino acids are joined together to form a protein molecule. Amino acid molecules Protein molecule Figure 2.11a Copyright © 2010 Pearson Education, Inc. Decomposition Reactions • AB A + B • Reverse synthesis reactions • Involve breaking of bonds • Catabolic (b) Decomposition reactions Bonds are broken in larger molecules, resulting in smaller, less complex molecules. Example Glycogen is broken down to release glucose units. Glycogen Glucose molecules Copyright © 2010 Pearson Education, Inc. Figure 2.11b Exchange Reactions (c) Exchange reactions • AB + C AC + B • Also called displacement reactions • Bonds are both made and broken Bonds are both made and broken (also called displacement reactions). Example ATP transfers its terminal phosphate group to glucose to form glucose-phosphate. + Glucose Adenosine triphosphate (ATP) + Glucose Adenosine diphosphate (ADP) phosphate Copyright © 2010 Pearson Education, Inc. Oxidation-Reduction (Redox) Reactions • Decomposition reactions: Reactions in which fuel is broken down for energy • Also called exchange reactions because electrons are exchanged or shared differently • Electron donors lose electrons and are oxidized • Electron acceptors receive electrons and become reduced Copyright © 2010 Pearson Education, Inc. Chemical Reactions All chemical reactions are either exergonic or endergonic • Exergonic reactions — release energy Catabolic reactions • Endergonic reactions — products contain more potential energy than did reactants Anabolic reactions Copyright © 2010 Pearson Education, Inc. Chemical Reactions • All chemical reactions are theoretically reversible A + B AB AB A + B • Chemical equilibrium occurs if neither a forward nor reverse reaction is dominant • Many biological reactions are essentially irreversible due to Energy requirements Removal of products Copyright © 2010 Pearson Education, Inc. Rate of Chemical Reactions • Rate of a chemical reaction is influenced by: • temperature rate • particle size rate • concentration of reactant rate • Catalysts: rate without being chemically changed Enzymes are biological catalysts Copyright © 2010 Pearson Education, Inc.