目录

  • 1 Nomenclature
    • 1.1 Nomenclature
    • 1.2 Inorganic compounds
    • 1.3 Organic compounds
  • 2 Atom
    • 2.1 Basic Atomic Theory
    • 2.2 Evolution of Atomic Theory
    • 2.3 Atomic Structure and Symbolism
    • 2.4 Isotopes
    • 2.5 Early development of the periodic table of elements
    • 2.6 Organization of the elements
  • 3 Atoms: the quantum world
    • 3.1 Wave Nature of Light
    • 3.2 Quantized Energy and Photons
    • 3.3 the Bohr Model
    • 3.4 Wave Character of Matter
    • 3.5 Atomic Orbitals
    • 3.6 3D Representation of Orbitals
    • 3.7 Electron Spin
    • 3.8 Electron Configurations
  • 4 Molecular Shape and Structure
    • 4.1 VSEPR theory
    • 4.2 Hybridization
    • 4.3 sp3 hybridization
    • 4.4 sp2 hybridization
    • 4.5 sp hybridization
    • 4.6 Other hybridization
    • 4.7 Multiple Bonds
    • 4.8 Molecular Orbitals
    • 4.9 Second-Row Diatomic Molecules
  • 5 Fundamentals of Thermochemistry
    • 5.1 Systems, States and Processes
    • 5.2 Heat as a Mechanism to Transfer Energy
    • 5.3 Work as a Mechanism to Transfer Energy
    • 5.4 Heat Capacity and Calorimetry
    • 5.5 The First Law of Thermodynamics
    • 5.6 Heats of Reactions - ΔU and ΔH
    • 5.7 Indirect Determination of ΔH - Hess's Law
    • 5.8 Standard Enthalpies of Formation
  • 6 Principles of Thermodynamics
    • 6.1 The Nature of Spontaneous Processes
    • 6.2 Entropy and Spontaneity - A Molecular Statistical Interpretation
    • 6.3 Entropy Changes and Spontaneity
    • 6.4 Entropy Changes in Reversible Processes
    • 6.5 Quantum States, Microstates, and Energy Spreading
    • 6.6 The Third Law of Thermodynamics
    • 6.7 Gibbs Energy
  • 7 Chemical equilibrium
    • 7.1 Equilibrium
    • 7.2 Reversible and irreversible reaction
    • 7.3 Chemical equilirbium
    • 7.4 Chemical equilibrium constant, Kc
    • 7.5 Le Chatelier's principle
    • 7.6 RICE table
    • 7.7 Haber process
  • 8 Acid–Base Equilibria
    • 8.1 Classifications of Acids and Bases
    • 8.2 The Brønsted-Lowry Scheme
    • 8.3 Acid and Base Strength
    • 8.4 Buffer Solutions
    • 8.5 Acid-Base Titration Curves
    • 8.6 Polyprotic Acids
    • 8.7 Exact Treatment of Acid-Base Equilibria
    • 8.8 Organic Acids and Bases
  • 9 Kinetics
    • 9.1 Prelude to Kinetics
    • 9.2 Chemical Reaction Rates
    • 9.3 Factors Affecting Reaction Rates
    • 9.4 Rate Laws
    • 9.5 Integrated Rate Laws
    • 9.6 Collision Theory
    • 9.7 Reaction Mechanisms
    • 9.8 Catalysis
Atomic Structure and Symbolism



The development of modern atomic theory revealed much about the inner structure of atoms. It was learned that an atom contains a very small nucleus composed of positively charged protons and uncharged neutrons, surrounded by a much larger volume of space containing negatively charged electrons. The nucleus contains the majority of an atom’s mass because protons and neutrons are much heavier than electrons, whereas electrons occupy almost all of an atom’s volume. The diameter of an atom is on the order of 10−10 m, whereas the diameter of the nucleus is roughly 10−15 m—about 100,000 times smaller. For a perspective about their relative sizes, consider this: If the nucleus were the size of a blueberry, the atom would be about the size of a football stadium (Figure 1).


The diagram on the left shows a picture of an atom that is 10 to the negative tenth power meters in diameter. The nucleus is labeled at the center of the atom and is 10 to the negative fifteenth power meters. The central figure shows a photograph of an American football stadium. The figure on the right shows a photograph of a person with a handful of blueberries.
Figure 1: If an atom could be expanded to the size of a football stadium, the nucleus would be the size of a single blueberry. (credit middle: modification of work by “babyknight”/Wikimedia Commons; credit right: modification of work by Paxson Woelber).


Atoms—and the protons, neutrons, and electrons that compose them—are extremely small. For example, a carbon atom weighs less than 2 × 10−23 g, and an electron has a charge of less than 2  10−19 C (coulomb). When describing the properties of tiny objects such as atoms, we use appropriately small units of measure, such as the atomic mass unit (amu) and the fundamental unit of charge (e). The amu was originally defined based on hydrogen, the lightest element, then later in terms of oxygen. Since 1961, it has been defined with regard to the most abundant isotope of carbon, atoms of which are assigned masses of exactly 12 amu. (This isotope is known as “carbon-12” as will be discussed later in this module.) Thus, one amu is exactly1/12 of the mass of one carbon-12 atom: 1 amu = 1.6605  10−24 g. (The Dalton (Da) and the unified atomic mass unit (u) are alternative units that are equivalent to the amu.) The fundamental unit of charge (also called the elementary charge) equals the magnitude of the charge of an electron (e) with e = 1.602  10−19 C.

A proton has a mass of 1.0073 amu and a charge of 1+. A neutron is a slightly heavier particle with a mass 1.0087 amu and a charge of zero; as its name suggests, it is neutral. The electron has a charge of 1− and is a much lighter particle with a mass of about 0.00055 amu (it would take about 1800 electrons to equal the mass of one proton. The properties of these fundamental particles are summarized in Table 1. (An observant student might notice that the sum of an atom’s subatomic particles does not equal the atom’s actual mass: The total mass of six protons, six neutrons, and six electrons is 12.0993 amu, slightly larger than the 12.00 amu of an actual carbon-12 atom. This “missing” mass is known as the mass defect, and you will learn about it in the chapter on nuclear chemistry.)

Table 1: Properties of Subatomic Particles


The number of protons in the nucleus of an atom is its atomic number (Z). This is the defining trait of an element: Its value determines the identity of the atom. For example, any atom that contains six protons is the element carbon and has the atomic number 6, regardless of how many neutrons or electrons it may have. A neutral atom must contain the same number of positive and negative charges, so the number of protons equals the number of electrons. Therefore, the atomic number also indicates the number of electrons in an atom. The total number of protons and neutrons in an atom is called its mass number (A). The number of neutrons is therefore the difference between the mass number and the atomic number: A – Z = number of neutrons.

atomicnumber(Z)=numberofprotonsmassnumber(A)=numberofprotons+numberofneutronsAZ=numberofneutrons


Atoms are electrically neutral if they contain the same number of positively charged protons and negatively charged electrons. When the numbers of these subatomic particles are not equal, the atom is electrically charged and is called an ion. The charge of an atom is defined as follows:

Atomic charge = number of protons − number of electrons

As will be discussed in more detail later in this chapter, atoms (and molecules) typically acquire charge by gaining or losing electrons. An atom that gains one or more electrons will exhibit a negative charge and is called an anion. Positively charged atoms called cations are formed when an atom loses one or more electrons. For example, a neutral sodium atom (Z = 11) has 11 electrons. If this atom loses one electron, it will become a cation with a 1+ charge (11 − 10 = 1+). A neutral oxygen atom (Z = 8) has eight electrons, and if it gains two electrons it will become an anion with a 2− charge (8 − 10 = 2−).

Chemical Symbols

A chemical symbol is an abbreviation that we use to indicate an element or an atom of an element. For example, the symbol for mercury is Hg (Figure 2). We use the same symbol to indicate one atom of mercury (microscopic domain) or to label a container of many atoms of the element mercury (macroscopic domain).



A jar is shown with a small amount of liquid mercury in it.
Figure 2 The symbol Hg represents the element mercury regardless of the amount; it could represent one atom of mercury or a large amount of mercury. Image used with permission from Wikipedia (user: Materialscientist).



The symbols for several common elements and their atoms are listed in Table 2. Some symbols are derived from the common name of the element; others are abbreviations of the name in another language. Symbols have one or two letters, for example, H for hydrogen and Cl for chlorine. To avoid confusion with other notations, only the first letter of a symbol is capitalized. For example, Co is the symbol for the element cobalt, but CO is the notation for the compound carbon monoxide, which contains atoms of the elements carbon (C) and oxygen (O). All known elements and their symbols are in the periodic table.

Table 2: Some Common Elements and Their Symbols
ElementSymbolElementSymbol
aluminumAlironFe (from ferrum)
bromineBrleadPb (from plumbum)
calciumCamagnesiumMg
carbonCmercuryHg (from hydrargyrum)
chlorineClnitrogenN
chromiumCroxygenO
cobaltCopotassiumK (from kalium)
copperCu (from cuprum)siliconSi
fluorineFsilverAg (from argentum)
goldAu (from aurum)sodiumNa (from natrium)
heliumHesulfurS
hydrogenHtinSn (from stannum)
iodineIzincZn

Traditionally, the discoverer (or discoverers) of a new element names the element. However, until the name is recognized by the International Union of Pure and Applied Chemistry (IUPAC), the recommended name of the new element is based on the Latin word(s) for its atomic number. For example, element 106 was called unnilhexium (Unh), element 107 was called unnilseptium (Uns), and element 108 was called unniloctium (Uno) for several years. These elements are now named after scientists or locations; for example, element 106 is now known as seaborgium (Sg) in honor of Glenn Seaborg, a Nobel Prize winner who was active in the discovery of several heavy elements.


Summary

An atom consists of a small, positively charged nucleus surrounded by electrons. The nucleus contains protons and neutrons; its diameter is about 100,000 times smaller than that of the atom. The mass of one atom is usually expressed in atomic mass units (amu), which is referred to as the atomic mass. An amu is defined as exactly 1/12 of the mass of a carbon-12 atom and is equal to 1.6605  10−24 g.

Protons are relatively heavy particles with a charge of 1+ and a mass of 1.0073 amu. Neutrons are relatively heavy particles with no charge and a mass of 1.0087 amu. Electrons are light particles with a charge of 1− and a mass of 0.00055 amu. The number of protons in the nucleus is called the atomic number (Z) and is the property that defines an atom’s elemental identity. The sum of the numbers of protons and neutrons in the nucleus is called the mass number and, expressed in amu, is approximately equal to the mass of the atom. An atom is neutral when it contains equal numbers of electrons and protons.