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Polflucht

Polflucht is a physics 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 Polflucht rather than just read about it. In short: Polflucht (from German, flight from the poles) is a geophysical concept invoked in 1922 by Alfred Wegener to explain his ideas of continental drift. The pole-flight force F P f {\displaystyle F_{\mathrm {Pf} }} is that component of the centrifugal force during the rotation of the Earth that acts tangentially to the Earth's surface.

Key takeaways

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

Reference excerpt

Polflucht (from German, flight from the poles) is a geophysical concept invoked in 1922 by Alfred Wegener to explain his ideas of continental drift. The pole-flight force F P f {\displaystyle F_{\mathrm {Pf} }} is that component of the centrifugal force during the rotation of the Earth that acts tangentially to the Earth's surface. The daily rotation of the Earth (more precisely: within a sidereal day of 23.93447 hours) around its axis of rotation causes everybody on Earth to experience a centrifugal force that points away perpendicularly from the Earth's axis, i.e. diagonally to the Earth's surface, depending on the degree of latitude. The centrifugal force contains a component tangential to the surface of the Earth away from the pole; this component is called the Polfluchtkraft, or pole-flight force.

Mathematics The magnitude of the centrifugal force is:

F C f = m ⋅ ω 2 ⋅ r {\displaystyle F_{\mathrm {Cf} }=m\cdot \omega ^{2}\cdot r}

where

m {\displaystyle m} is the mass of the body (not the Earth's mass!)

r {\displaystyle r} is its distance from the Earth's axis

ω = 0.00007292116 / s {\displaystyle \omega =0.00007292116/\mathrm {s} } is the angular velocity of the Earth's rotation in radians per second The distance depends on the geographical latitude φ over a mean Earth radius R = 6371 km, resulting in:

⇒ F C f = m ⋅ ω 2 ⋅ R ⋅ cos ⁡ φ {\displaystyle \Rightarrow F_{\mathrm {Cf} }=m\cdot \omega ^{2}\cdot R\cdot \cos \varphi }

Only at the equator does the centrifugal force exactly counteract the gravitational force. At all other degrees of latitude it acts at an angle α = 90° – φ to the horizontal. The following now applies to the pole-flight force:

F P f = F C f ⋅ sin ⁡ φ = m ⋅ ω 2 ⋅ R ⋅ cos ⁡ φ ⋅ sin ⁡ φ {\displaystyle {\begin{aligned}F_{\mathrm {Pf} }&=F_{\mathrm {Cf} }\cdot \sin \varphi \\&=m\cdot \omega ^{2}\cdot R\cdot \cos \varphi \cdot \sin \varphi \end{aligned}}}

Effect If one considers only that component of the force which acts parallel to the Earth's surface, then it is directed to the south in the Northern Hemisphere and to the north in the Southern Hemisphere. The constant action of this force is why the Earth is not a perfect sphere but is flattened at the poles. The somewhat elastic nature of the Earth adjusts to the prevailing rotation, so that its mass distribution yields to the polar-flight force and the equatorial radius increases at the expense of the polar radius. Today the flattening of the poles is 0.3353%, or 21 km. Isaac Newton formulated this deformation mathematically for the first time. The resulting Polfluchtkraft was postulated by the German geologist Damian Kreichgauer in 1902 and the Hungarian physicist Loránd Eötvös in 1912. Around 1920 Alfred Wegener postulated the pole flight of the continents and suspected that the centrifugal force was the cause of continental drift hypothesized by him and others. This was refuted a few years later, but the terms Polflucht and Polfluchtkraft found their way into the scientific literature. Wegener suggested that the differential gravitational force resulting from the horizontal component of the centrifugal could cause continental masses to drift slowly towards the equator. Wegener's hypothesis was expanded by Paul Sophus Epstein in 1920, but the force is now known to be far too weak to cause plate tectonics. The strength of the layers of the Earth's crust is much stronger than assumed by Wegener and Epstein.

Literature The Concise Oxford Dictionary of Earth Sciences (topic 'Polflucht'), Oxford 1990 Laszlo Egyed: Physik der festen Erde (Physics of solid Earth), 368p. Akadémiai Kiadó, Budapest 1969 Über die Polflucht der Kontinente, F.Nölke 1921 Damian Kreichgauer, Die Äquatorfrage in der Geologie, Missionsdruckerei in Steyl, Steyl (1902) Loránd Eötvös, Verhandlungen der 17. Allgemeinen Conferenz der Internationalen Erdmessung, Volume 1, Georg Reimer, Berlin (1913) Alfred Wegener, Die Entstehung der Kontinente und Ozeane, Second Edition, Friedrich Vieweg & Sohn, Braunschweig (1920) Alfred Wegener, The Origin of Continents and Oceans, Translated from the Third German Edition by John George Anthony Skerl, E P Dutton and Company, New York (1924)

Worked examples

Example 1 — a first encounter with Polflucht

Start with the simplest possible case. Write down what Polflucht claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, 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 Polflucht 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 Polflucht 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 Polflucht

In research
Polflucht appears in physics 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 Polflucht 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
Polflucht is common in secondary-school and first-year university syllabi. It links to neighbouring topics Geophysics, Obsolete geology theories, Plate tectonics, so understanding it makes those chapters shorter.
In everyday life
Look for Polflucht 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 Polflucht in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Polflucht 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 Polflucht out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Polflucht in simple terms?

Polflucht (from German, flight from the poles) is a geophysical concept invoked in 1922 by Alfred Wegener to explain his ideas of continental drift. The pole-flight force F P f {\displaystyle F_{\mathrm {Pf} }} is that component of the centrifugal force during the rotation of the Earth that acts ta…

Why does Polflucht matter?

Because it connects several physics 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 Polflucht?

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 Polflucht.

Tags

  • Geophysics
  • Obsolete geology theories
  • Plate tectonics

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