1.1: Introduction and Objectives
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Chapter Introduction
Welcome to the fascinating study of Planet Earth! In this chapter, we begin our exploration of the dynamic planet we call home. From the fiery core to the outermost atmosphere, Earth is a complex, interconnected system composed of diverse components that work in harmony. We'll study several of the components in detail, commonly referred to as Earth's major spheres—the geosphere, hydrosphere, atmosphere, and biosphere—and examine how they interact with each other and with human activities.
Understanding Earth Science isn't just about memorizing facts; it's about appreciating the intricate relationships that sustain life and recognizing the impact of our actions on these delicate systems. Through case studies like California's water crisis, we'll see the real-world implications of human impacts on this system, including pollution, resource extraction, and climate change. By examining the branches of Earth Science, the scientific method, and the foundations of early scientific thought, we'll build a solid framework for evaluating sources and confronting science denial. Let's embark on this adventure together and unravel the mysteries of our ever-changing planet!
- Explain the components and interactions of Earth's systems, including the geosphere, hydrosphere, atmosphere, and biosphere.
- Analyze the significance of Earth Science in understanding natural phenomena and addressing environmental challenges.
- Evaluate the impact of human activities on Earth's spheres, with a focus on climate change and resource extraction.
- Apply the scientific method and principles of early scientific thought to investigate Earth Science phenomena and assess scientific claims.
- Critically assess sources of information in Earth Science, distinguishing between credible scientific evidence and science denial.
Let's begin!
Throughout its entire 4.5 Ga (i.e., giga annum, or billion years) history, every event in the history of our planet happened because something forced it to happen. An asteroid once caused an extinction. Extinctions led to novel new evolutionary pathways for species origination. As we will see, Earth's surface if comprised of lithospheric plates that are in continual, albeit gradual, motion. This process, referred to as plate tectonics, led to the current spatial arrangement of the continents. We might be tempted to describe each of these events as was explained in the preceding sentences, linearly (e.g., A caused B). We could leave it at that. However, is it rarely that simple!
Contained within our galactic system is a solar system powered by an average G type star. “On a mote of dust suspended in a sunbeam” (Carl Sagan) resides our Earth system. Like any system, it is composed of many moving parts, powered by flows of energy and sustained in a state of dynamic equilibrium. A system is a naturally occurring group of interacting, interrelated, or interdependent elements that form a complex whole.

Within the Earth system, there are subsystems. These subsystems encompass the space environment (exosphere), gaseous environment (atmosphere), water environment (hydrosphere), solid environment (geosphere and its subcomponent the lithosphere), and living environment (biosphere). In some cases, the icy environment (cryosphere) is broken away from the hydrosphere and the anthroposphere (human environment) from the biosphere, for emphasis. Energy, coming from the Sun on one hand and the Earth’s interior on the other, powers these systems. As energy flows through and between these systems, so too does matter, such as nutrients and elements. These flows of matter are often referred to as biogeochemical cycles. Examples of these include the carbon and nitrogen cycles.

Energy does not flow through these systems in a linear fashion. Its pathways are complex, taking advantage of the points where systems interact to transfer from one system to another and back again. In order to understand how our planet works today and how it has worked in the past (uniformitarianism), we need to use the principles of systems analysis. If we think in terms of systems, we begin to think in terms of cycles, feedbacks, forcing mechanisms, storage, sinks, and flows of energy and material.
Remember the extinction caused by an asteroid mentioned above? While the asteroid (from the exosphere) did indeed cause the extinction, it was the effect that asteroid had on the hydrosphere, atmosphere, and lithosphere that led to the subsequent destruction of life that occurred in the biosphere. In systems thinking, the asteroid was a forcing mechanism that disrupted the entire Earth system, past a tipping point of no return. While some organisms were directly crushed by the impending rock from space, most were killed by the subsequent cascading effects as energy rippled across the interconnected systems.
“To everything, there is a season”.