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Thomas Chrowder Chamberlin

Thomas Chrowder Chamberlin is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Thomas Chrowder Chamberlin rather than just read about it. In short: Thomas Chrowder Chamberlin (; September 25, 1843 – November 15, 1928) was an American geologist and educator. In 1893 he founded the Journal of Geology, of which he was editor for many years.

Thomas Chrowder Chamberlin — main illustration
Thomas Chrowder Chamberlin — illustration

Key takeaways

  • Thomas Chrowder Chamberlin belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Thomas Chrowder Chamberlin to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Thomas Chrowder Chamberlin from memory before moving on to harder problems.

Reference excerpt

Thomas Chrowder Chamberlin (; September 25, 1843 – November 15, 1928) was an American geologist and educator. In 1893 he founded the Journal of Geology, of which he was editor for many years.

Biography Chamberlin was born September 25, 1843, in Mattoon, Illinois. When he was three years old his family moved north to near Beloit, Wisconsin. His father was a Methodist circuit minister and farmer. He attended a preparatory academy before entering Beloit College, where he received a classical education in Greek and Latin, while becoming interested in natural science. While a student at Beloit he directed a church choir and participated in athletics and debate. After graduation from Beloit College in 1866, Chamberlin worked for two years as a teacher and later principal in a high school near Beloit. He was married to Alma Wilson in 1867. In 1868–1869, Chamberlin spent a year taking graduate courses, including geology, at the University of Michigan to strengthen his scientific background. Subsequently (1869–1873), he became professor of natural science at Whitewater Normal School in Wisconsin. He joined the Beloit faculty in 1873, where he was professor of geology, zoology, and botany. In 1873 he also became one of several part-time participants in conducting a comprehensive geological survey of Wisconsin. His geological mapping work in southeastern Wisconsin, a region mantled with thick glacial deposits, led him to recognize multiple episodes of glaciation during the Pleistocene. His terminology for glacial stages in North America is still in use, with minor modifications. In 1875 he started a business with his brother and sold spring water, a popular brand at the time. In 1876 Chamberlin became chief geologist for the Wisconsin geological survey, supervising the completion of the survey and the publication of the four-volume report, for which he authored sections on glacial deposits, Paleozoic and Precambrian bedrock geology, lead-zinc ore deposits, artesian wells, and soils. The project brought him national attention and led to his appointment as head of the glacial division of the US Geological Survey in 1881. He later was president of the University of Wisconsin (1887 to 1892). In 1890, and again in 1897, Chamberlin wrote "The method of multiple working hypotheses", in which he advocated the importance of simultaneously evaluating several hypotheses, rejecting those that conflict with available data, and ending with the one hypothesis supported by the data. This stood in contrast to what he called the single ruling theory, which encouraged scientists to find supporting data and not challenge it with difficult tests. The paper is considered a landmark on the scientific method, was an inspiration for the approach called strong inference, and was reprinted in 1965. In 1892 Chamberlin accepted the offer to organize a department of geology at the new University of Chicago, where he remained as a professor until 1918. From 1898 to 1914 he was president of the Chicago Academy of Sciences. In 1899 Chamberlin wrote, An Attempt to Frame a Working Hypothesis of the Cause of Glacial Periods on an Atmospheric Basis, and developed at length the idea that changes in climate could result from changes in the concentration of atmospheric carbon dioxide, and wrote about climate actions:

When the temperature is rising after a glacial episode, dissociation is promoted, and the ocean gives forth its carbon dioxide at an increased rate, and thereby assists in accelerating the amelioration of climate. A study of the life of the geological periods seems to indicate that there were very notable fluctuations in the total mass of living matter. To be sure there was a reciprocal relation between the life of the land and that of the sea, so that when the latter was extended upon the continental platforms and greatly augmented, the former was contracted, but notwithstanding this it seems clear that the sum of life activity fluctuated notably during the ages. It is believed that on the whole it was greatest at the periods of sea extension and mild climates, and least at the times of disruption and climatic intensification. This factor then acted antithetically to the carbonic acid freeing previously noted, and, so far as it went, tended to offset its effects

It now becomes necessary to assign agencies capable of removing carbon dioxide from the atmosphere at a rate sufficiently above the normal rate of supply, at certain times, to produce glaciation; and on the other hand, capable of restoring it to the atmosphere at certain other times in sufficient amounts to produce mild climates. Chamberlin was elected to the American Academy of Arts and Sciences in 1901 and the United States National Academy of Sciences in 1903. In 1905, Chamberlin and Forest Ray Moulton developed a theory of the formation of the Solar System that challenged the Laplacian nebular hypothesis. Their theory, the Chamberlin-Moulton planetesimal hypothesis, received favorable support for almost a third of a century, but passed out of favor by the late 1930s. It ultimately was discarded in the 1940s by the realization it was incompatible with the angular momentum of Jupiter. A portion of the theory stating that smaller objects — planetesimals — gradually collided to build the planets by accretion is still well-regarded. From his theories and other geological evidence he concluded that Earth was much older than assumed by Lord Kelvin (ca 100 million years) at the time. His speculations about the source of energy for such a long-lived Sun were prescient, involving the ability of the Sun to somehow extract energy from the inner structures of the atom. In 1905, Chamberlin was elected to the American Philosophical Society.

In 1909, he and his son Rollin Thomas Chamberlin traveled to the East as members of the Oriental Educational Investigation Commission led by Ernest DeWitt Burton, and supported by John D. Rockefeller to reconnoiter the Eastern world as a potential site for the humanitarian projects of the nascent Rockefeller Foundation. Chamberlin was awarded the inaugural Penrose Gold Medal of the Society of Economic Geologists in 1924, and the inaugural Penrose Medal of the Geological Society of America in 1927. He was president of the Geological Society of America in 1894. Chamberlin remained active professionally up until his death in Chicago on November 15, 1928.

… excerpt ends here. Continue reading the full article.

Illustrations

Thomas Chrowder Chamberlin illustration
Thomas Chrowder Chamberlin: From left to right, E. D. Burton, T. C. Chamberlin, Joseph Beech, Y. T. Wang (interpreter), and R. T. Chamberlin (T. C. Chamberlin's son) at Santai County, Sichuan, during an exploratory trip through China in 1909 as part of the Oriental Educational Investigation Commission.
From left to right, E. D. Burton, T. C. Chamberlin, Joseph Beech, Y. T. Wang (interpreter), and R. T. Chamberlin (T. C. Chamberlin's son) at Santai County, Sichuan, during an exploratory trip through China in 1909 as part of the Oriental Educational Investigation Commission.

Worked examples

Example 1 — a first encounter with Thomas Chrowder Chamberlin

Start with the simplest possible case. Write down what Thomas Chrowder Chamberlin claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Thomas Chrowder Chamberlin before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Thomas Chrowder Chamberlin ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Thomas Chrowder Chamberlin

In research
Thomas Chrowder Chamberlin appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Thomas Chrowder Chamberlin in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Thomas Chrowder Chamberlin is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1843 births, 1928 deaths, American academic journal editors, so understanding it makes those chapters shorter.
In everyday life
Look for Thomas Chrowder Chamberlin outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

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How to study Thomas Chrowder Chamberlin in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Thomas Chrowder Chamberlin means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Thomas Chrowder Chamberlin out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Thomas Chrowder Chamberlin in simple terms?

Thomas Chrowder Chamberlin (; September 25, 1843 – November 15, 1928) was an American geologist and educator. In 1893 he founded the Journal of Geology, of which he was editor for many years.

Why does Thomas Chrowder Chamberlin matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Thomas Chrowder Chamberlin?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Thomas Chrowder Chamberlin.

Tags

  • 1843 births
  • 1928 deaths
  • American academic journal editors
  • American geologists
  • American science teachers
  • American science writers
  • Beloit College alumni
  • Beloit College faculty
  • Leaders of the University of Wisconsin-Madison
  • Members of the American Philosophical Society
  • Penrose Medal winners
  • People from Beloit, Wisconsin

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