Chemistry Review for Physiology: Atoms, Ions, and Molecules

Matter and the Basis of Biology

  • Matter is anything that has mass and occupies space.

  • The three forms of matter we commonly refer to are:

    • Solid

    • Liquid

    • Gas

    • In physiology, there are many bodily solids (e.g., bone) and liquids (e.g., blood).

    • Gases in life: oxygen (O₂) and carbon dioxide (CO₂).

  • We start from the smallest unit that has chemical properties of an element: the atom.

    • An atom is the smallest particle exhibiting the chemical properties of an element.

    • Subatomic particles include:

    • Protons: mass ≈ 1 AMU, charge = +1

    • Neutrons: mass ≈ 1 AMU, charge = 0

    • Electrons: mass ≈ 1/1836 AMU, charge = −1

    • The nucleus contains protons and neutrons; electrons orbit the nucleus in regions called electron orbitals (often simplified as shells).

  • In brief, atoms form matter and build up to molecules and cells, which we’ll tie back to cellular organization later.

Atoms, Elements, and the Periodic Table

  • An element is a pure chemical substance consisting of only one type of atom.

  • There are 92 naturally occurring elements that make up matter, organized in the Periodic Table.

  • Element symbols can be simple (e.g., H, C, O) or derived from Latin or other languages (e.g., Fe for iron from ferrum; Na for sodium from natrium).

  • The Periodic Table is organized by:

    • Electric structure influences: the arrangement of electrons and their shells.

    • Columns (groups) reflect elements with related properties, particularly valence electron configurations.

    • Rows (periods) reflect increasing atomic number across the table.

    • A top-number reference (as discussed in the lecture) is shown above the symbol and relates to trends such as atomic size in this teaching context.

  • Important features highlighted in class:

    • Electronegativity tends to increase across a period (left to right) and affects how atoms interact.

    • The outermost shell (valence shell) largely determines chemical behavior.

    • The first electron shell holds a maximum of 2 electrons; all subsequent shells hold up to 8 electrons.

  • Major vs minor elements in the human body:

    • Major elements collectively make up about 99% of body mass (e.g., carbon-based life).

    • Minor elements collectively compose less than about 1% of body weight but are essential.

    • Trace elements exist in even smaller amounts (about 0.01%), but are physiologically important.

  • How we describe an element:

    • Chemical symbol (often one letter, sometimes two; sometimes from Latin).

    • Atomic number Z: number of protons. Shown above the symbol on the periodic table.

    • Atomic mass (often shown below the symbol): total mass of protons and neutrons.

    • Mass number A ≈ Z + N (N = number of neutrons).

  • Example: iron (Fe)

    • Symbol: Fe (from ferrum, Latin)

    • Atomic number Z = 26

    • Atomic mass ≈ 55.845

    • Mass number A ≈ 56 (rounded for some calculations)

    • If A = 56 and Z = 26, neutrons N = A − Z = 56 − 26 = 30

    • In a neutral atom, electrons = protons → 26 electrons when Fe is neutral

Isotopes and Atomic Mass

  • Isotopes have the same number of protons and electrons (same Z) but different numbers of neutrons.

    • Prefix iso- means "same"; tope means "place"; so isotopes share the same place in the periodic table (same element) but differ in mass.

    • Chemical properties are nearly identical because Z (and thus electron configuration) is the same.

    • Mass differs due to different neutron counts.

  • Common example: carbon isotopes

    • ^12C, ^13C, and ^14C are naturally existing isotopes.

    • ^14C is radioactive; ^12C and ^13C are stable.

  • Atomic mass on the periodic table is a weighted average of the isotopes’ masses (
    the relative abundances).

  • Practical uses of isotopes in physiology and medicine:

    • Scintigraphy (radiolabeled isotopes) to image metabolically active tissues (e.g., thyroid activity).

    • PET scans often use radiolabeled glucose to detect areas with high glucose uptake (cancer cells).

  • Biological half-life: time required for half of the radioactive material (or other tracer) to be eliminated from the body.

    • This varies widely: some molecules have very short half-lives (seconds) like mycosanoids; others like insulin can have half-lives of minutes to hours.

Ions and Ionic Compounds

  • Ions are atoms with a charge produced by loss or gain of one or more electrons.

    • Neutral atoms have equal numbers of protons and electrons.

    • If an atom gains electrons, it becomes negatively charged (anion).

    • If an atom loses electrons, it becomes positively charged (cation).

  • Anions: negative charge (e.g., Cl⁻).

  • Cations: positive charge (e.g., Na⁺, Mg²⁺).

  • Basic examples:

    • Chlorine gains one electron to form Cl⁻ (charge −1).

    • Sodium loses one electron to form Na⁺ (charge +1).

    • Magnesium loses two electrons to form Mg²⁺ (charge +2).

  • Polyatomic ions: ions that contain more than one atom (e.g., bicarbonate HCO₃⁻, phosphate PO₄³⁻).

  • Ionic bonds and salts:

    • Ionic bonds are electrostatic attractions between a cation and an anion, formed by transfer (not sharing) of electrons.

    • Resulting structures are lattices (crystalline salts).

    • Example salts:

    • Sodium chloride: extNaClext{NaCl} — Na⁺ transfers an electron to Cl⁻, forming a crystalline lattice.

    • Magnesium chloride: extMgCl2ext{MgCl}_2 — Mg²⁺ pairs with two Cl⁻ ions.

Molecular Compounds and Covalent Bonds

  • Molecular compounds are stable associations between two or more elements held together by covalent bonds (shared electrons).

    • Note: Not all molecules with more than one atom are compounds; for example, O₂ is a molecule but not a compound because it has only one element.

  • Covalent bonds share electrons between atoms, allowing each atom to fill its valence shell.

  • Common elements forming covalent bonds in physiology:

    • Hydrogen (H): needs 1 more electron to fill its valence shell; typically forms 1 covalent bond.

    • Oxygen (O): needs 2 electrons; typically forms 2 covalent bonds.

    • Nitrogen (N): needs 3 electrons; typically forms 3 covalent bonds.

    • Carbon (C): needs 4 electrons; typically forms 4 covalent bonds.

  • Bond types:

    • Single covalent bond: one pair of electrons shared (depicted as a single line); e.g., H–H.

    • Double covalent bond: two pairs shared (depicted as a double line); e.g., O═O (and as in CO₂ where carbon shares two electrons with each oxygen).

    • Triple covalent bond: three pairs shared (depicted as a triple line); e.g., N≡N.

  • Carbon skeletons:

    • Carbon can form straight chains, branched chains, or rings.

    • Carbon often forms four covalent bonds, resulting in various structures: methane (CH₄), carbon dioxide (CO₂), ethanol (C₂H₅OH), formic acid (HCOOH), etc.

  • Representation conventions:

    • Line-angle (bond-line) drawings show bonds as lines; vertices/endpoints represent carbon atoms; implicit hydrogens complete the valence.

  • Polar vs nonpolar covalent bonds:

    • Electronegativity is the atoms’ attraction for electrons.

    • Nonpolar covalent bonds: equal sharing of electrons (approximately equal electronegativities).

    • Polar covalent bonds: unequal sharing due to differences in electronegativity (e.g., O–H, N–H, C–O).

    • A molecule may be nonpolar even if it contains polar bonds if the bond dipoles cancel (e.g.,
      extCO2ext{CO}_2 has two polar C=O bonds arranged linearly such that the dipoles cancel).

  • Examples of polarity:

    • Water (H₂O) is a polar molecule due to its bent geometry and polar O–H bonds.

    • Glucose is polar; it dissolves in water.

    • Oil and triglycerides are largely nonpolar; oil does not mix with water due to nonpolar–polar incompatibility.

  • Amphipathic molecules:

    • Contain both polar and nonpolar regions (e.g., phospholipids with a polar head and nonpolar tails).

    • Phospholipids form the bilayer of cell membranes, with polar heads facing aqueous environments and nonpolar tails in the interior.

Intermolecular and Intramolecular Forces

  • Intermolecular attractions: weak attractions between molecules that influence structure, shape, and interactions.

    • Hydrogen bonding: attraction between a partially positive hydrogen atom and a partially negative atom (commonly O or N) in another molecule; e.g., as in water and glucose.

    • Temporary dipole (induced dipole) interactions can occur in nonpolar molecules due to momentary unequal electron distribution; these are weaker but cumulatively significant.

    • Hydrophobic interactions: nonpolar molecules aggregate in polar solvents (e.g., oil droplets in water) due to unfavorable interactions between nonpolar groups and water.

  • Intermolecular forces contribute to properties like surface tension (e.g., hydrogen bonding in water).

  • Intramolecular forces: forces within the same molecule that influence its shape and stability (e.g., hydrogen bonding within a protein or nucleic acid can influence folding; strong covalent bonds within a molecule determine its core structure).

  • The balance of these forces helps explain structure–function relationships in biology (structure equals function).

Isomerism

  • Isomer: molecules with the same molecular formula but different arrangement of atoms in space.

  • Why it matters: different structures can yield different properties and reactivity; enzyme specificity often distinguishes between isomers.

  • Common example in physiology: the hexose family — glucose, galactose, and fructose share the same molecular formula extC<em>6extH</em>12extO6ext{C}<em>6 ext{H}</em>{12} ext{O}_6 but differ in structure.

    • Glucose and galactose form similar ring structures, with a key difference at one carbon’s orientation.

    • Fructose is structurally different (a five-membered ring with additional carbon attachments).

  • Consequences for biology: enzymes recognize specific isomers; transporters may differentiate between closely related sugars; glucose is a key energy currency, while galactose and fructose are often converted into glucose or used in other pathways.

Practical Implications and Applications in Physiology

  • The chemistry of life underpins biology: understanding atoms, ions, molecules, and their interactions helps explain cellular processes.

  • Common physiological ions and molecules (examples):

    • Sodium Na⁺, potassium K⁺, calcium Ca²⁺, chloride Cl⁻, bicarbonate HCO₃⁻, phosphate PO₄³⁻.

    • Important covalent molecules: water (H₂O), carbon dioxide (CO₂), organic molecules (carbohydrates, lipids, proteins, nucleic acids).

  • Medical imaging and lab techniques rely on isotopes and chemical behavior:

    • Radiolabeled isotopes used in scintigraphy and PET scans.

    • Biological half-life informs how long a tracer remains active in the body.

  • Quick reference formulas and concepts:

    • Mass number: A=Z+NA = Z + N

    • Neutrons: N=AZN = A - Z

    • Neutral atom electron count: e=Ze^- = Z

    • Ionic charge: extCharge=Zeext{Charge} = Z - e^-

    • Covalent bonds: single, double, triple (1, 2, or 3 electron pairs shared)

    • Ionic bond: transfer of electrons; electrostatic attraction; lattice structure

    • Polar covalent bond: unequal sharing due to electronegativity differences; polar molecules arise from net dipoles

    • Nonpolar covalent bond: equal sharing; may still have polar bonds that cancel in the molecule (e.g., extCO2ext{CO}_2)

    • Hydrophobic interactions: aggregation of nonpolar regions in polar solvents

    • Amphipathic molecules: phospholipids with polar heads and nonpolar tails; form membranes

Quick Cross-References to What’s Next

  • Monday: macromolecules (proteins, nucleic acids, carbohydrates, lipids) and their chemistry.

  • Later: cellular level organization and physiology applications of these chemical principles.