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  Earth Science News
A geologist in the field, here on the shore of Kangaroo Island, Australia. Such field observations have allowed geologists to work out the history of Earth.
CreditStephen Marshak
Guide to Reading

The last chapter dealt with how Earth’s history has been worked out; this one deals with the story itself. It’s presented in chronological order and in terms of the major divisions of geologic time: the Precambrian (from Earth’s beginning 4.6 billion years ago up to 545 million years ago) and its subdivisions (Hadean Eon, Archean Eon, and Proterozoic Eon) and the rest of all time, the Phanerozoic, including its subdivisions (the Paleozoic Era, including the Cambrian, Ordovician, Silurian, Devonian, Carboniferous, and Permian Periods; the Mesozoic Era, including the Triassic, Jurassic, and Cretaceous Periods; and the Cenozoic Era, with special attention paid to the Pleistocene Ice Age of the Quaternary Period). That’s a lot of names, but do learn them. They’re basic to any discussion of Earth history.

Basically, Chapter 11 is narrating the highlights of 4.6 billion years of change. This presents a problem. Even the most concise summary of 4.6 billion of anything is going to be long. What is essential to learn? The author has chosen major milestones in Earth’s development that any well-informed general geologist should know. This guide narrows the focus even further. Still, basic literacy means different things to different students, to different teachers, and in different situations. For example, the particular facts required of you could depend on the location of your school. If you’re in the Denver area, no doubt you’ll have to know about the Ancestral Rockies, the Laramide Revolution, and the Western Interior Seaway. If you’re located in Boston or Seattle, other particulars may seem more important to you or to your teacher. This chapter presents a wonderful opportunity to bring basic concepts to life by indulging your curiosity about the history of your present (or hometown) surroundings.

Whatever your goal, it’s easy to get mired down in all the details and proper nouns. To avoid this, as you study, try to picture our planet as it was in the past—a truly alien world. It’s not dull stuff; it’s been the subject matter for popular comics and blockbuster movies for decades. Who hasn’t heard of the Flintstones or Jurassic Park? Asteroid encounters have been exciting from Superman days up to Deep Impact. People everywhere wonder why the dinosaurs became extinct; maybe after reading this chapter you’ll also wonder why the trilobites became extinct. As you read, remind yourself that this is not a fanciful movie plot; it’s all based on scientific data and reasoning. Truth really is stranger than fiction.

Key Terms
Acadian orogeny Laurentia, Gondwana, Baltica, and Siberia
Alleghenian orogeny organic carbon
Antler orogeny Pannotia
basement uplifts photosynthetic organisms
Cambrian explosion of life prokaryotic cells
conodonts Rodinia
cratonic (or continental) platform Sevier orogeny
cratons shield
cyanobacteria Sierran arc
epicontinental seas stromatolites
eukaryotic cells super plumes
greenhouse gas Taconic orogeny
gymnosperms vascular plants
Laramide orogeny