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Bio 100 LEC Chapter 8 Modules 1-3

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Bio 100 LEC Chapter 8

Chapter 8: An Introduction to Metabolism

Overview of Metabolism

Metabolism encompasses all chemical reactions that occur within a cell, integrating the transformation of matter and energy. These reactions are organized into metabolic pathways, which are sequences of enzymatically catalyzed steps that convert specific molecules into final products. Understanding metabolism requires knowledge of large biological molecules, solute concentration, ion movement, and pH values, as these factors influence metabolic reactions.

Diagram of interconnected metabolic pathways for carbohydrates, lipids, nucleotides, and amino acids

Metabolic Pathways

Metabolic pathways begin with a starting molecule and end with a product, with each step catalyzed by a specific enzyme. The product of one reaction often serves as the substrate for the next, allowing for precise regulation and integration of cellular activities.

  • Catabolic pathways: Break down complex molecules into simpler ones, releasing energy.

  • Anabolic pathways: Build complex molecules from simpler ones, consuming energy.

  • Energy released from catabolic pathways can drive anabolic processes.

Linear metabolic pathway with enzymes catalyzing each step

Diagram showing catabolic and anabolic pathways, energy flow, and biosynthesis

Energy and Life

Forms of Energy

Energy is the capacity to cause change. In biological systems, energy exists primarily as:

  • Kinetic energy: Energy of motion (e.g., muscle contraction, molecular movement).

  • Potential energy: Stored energy due to position or structure (e.g., chemical bonds, concentration gradients).

Energy can be transformed from one form to another, such as potential energy being converted to kinetic energy during movement.

Diagram showing conversion between potential and kinetic energy using a diver

The Laws of Thermodynamics

Thermodynamics is the study of energy transformations. Biological systems are considered open systems, exchanging energy and matter with their surroundings.

  • First Law of Thermodynamics: Energy cannot be created or destroyed, only transformed from one form to another.

  • Second Law of Thermodynamics: Every energy transfer increases the entropy (disorder) of the universe; some energy is lost as heat.

Comparison of open and closed systems in thermodynamics

Bear eating fish, illustrating chemical energy transfer

Bear running, illustrating energy transformation and heat loss

Biological Order and Entropy

Living organisms maintain order and structure by increasing the entropy of their surroundings. While cells create ordered structures, the overall entropy of the universe increases due to the release of heat and other byproducts.

Starfish and succulent plant illustrating biological order

Free Energy and Spontaneity of Reactions

Free Energy (ΔG)

Free energy (G) is the portion of a system's energy that can perform work when temperature and pressure are uniform. The change in free energy (ΔG) determines whether a reaction is spontaneous.

  • ΔG < 0: Spontaneous (exergonic) reaction; energy is released.

  • ΔG > 0: Non-spontaneous (endergonic) reaction; energy is required.

  • ΔG = 0: Reaction is at equilibrium; no net work can be done.

The standard equation for free energy change is:

  • = change in enthalpy (total energy)

  • = change in entropy (disorder)

  • = temperature in Kelvin

Equation for free energy change and its components

Summary of exergonic and endergonic reactions

Free Energy, Stability, and Work Capacity

Systems tend to move from higher free energy (less stable) to lower free energy (more stable). The released free energy can be harnessed to do work, as seen in gravitational motion, diffusion, and chemical reactions.

Diagram showing the relationship between free energy, stability, and spontaneous change

Exergonic and Endergonic Reactions

Exergonic reactions release energy and are spontaneous, while endergonic reactions require energy input and are non-spontaneous. Graphical representations help visualize the energy changes during these reactions.

Graph of exergonic reaction showing energy release

Graph of endergonic reaction showing energy requirement

Equilibrium and Metabolism

In a closed system, reactions eventually reach equilibrium (ΔG = 0), and no more work can be done. Living cells avoid equilibrium by remaining open systems, allowing continuous input and output of energy and materials, thus sustaining life and cellular processes.

Diagram showing equilibrium and inability to do work in a closed system

Diagram of a multistep open hydroelectric system, analogous to cellular metabolism

ATP and Cellular Work

ATP: The Energy Currency of the Cell

Adenosine triphosphate (ATP) powers cellular work by coupling exergonic reactions (energy-releasing) to endergonic reactions (energy-consuming). Cells perform three main types of work:

  • Mechanical work: Movement (e.g., muscle contraction)

  • Transport work: Pumping substances across membranes against gradients

  • Chemical work: Driving endergonic reactions (e.g., biosynthesis)

Diagram showing ATP coupling to mechanical, transport, and chemical work

Structure and Hydrolysis of ATP

ATP consists of a ribose sugar, adenine base, and three phosphate groups. The bonds between phosphate groups are high-energy due to electrostatic repulsion. Hydrolysis of ATP (removal of a phosphate group) releases energy that can be used for cellular work:

  • Hydrolysis of the terminal phosphate releases the most energy.

  • ATP hydrolysis is an exergonic reaction.

Structure of ATP and hydrolysis reaction

Regeneration of ATP

ATP is a renewable resource, continually regenerated from ADP and inorganic phosphate. The energy for ATP synthesis comes from exergonic (energy-releasing) processes, such as cellular respiration. Cells maintain small pools of ATP, constantly cycling between ATP and ADP to meet energy demands.

Diagram showing the ATP cycle: energy from catabolism regenerates ATP, which is used for cellular work

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