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How Would Weather Change if Earth Rotated Twice as Fast?

How weather affected if Earth rotated twice as fast

Question:

I don’t know if this is something you can answer, but I was wondering how the weather patterns on earth would change if it rotated about twice as fast. I heard that the centrifugal force would pull the water to the equator, would something similar happen to the air currents? How do you think this would affect the temperature and weather? – Zoe

Answer:

Thank you for your fun question! This is the sort of question professors LOVE to add to their exams.

If Earth rotated about twice as fast (with a 12-hour day instead of a 24-hour one), it would have significant effects on weather patterns, atmospheric circulation, and the distribution of temperatures. Here’s how the changes could play out:

1. Centrifugal Force and Distribution of Water and Air

  • Centrifugal Force: With a faster rotation, the centrifugal force would indeed increase, becoming more pronounced at the equator. This would pull water towards the equator, leading to a bulging effect where sea levels rise at the equator and fall at the poles.
  • Impact on Air Currents: Air would also be affected by the increased centrifugal force. The atmosphere would become thicker at the equator and thinner at higher latitudes. This would influence pressure gradients and shift wind patterns closer to the equator, as more air is pulled toward these regions.
 

Suggested Reading

The Dynamic Earth: An Introduction to Physical Geology by Brian J. Skinner and Stephen C. Porter.

Atmospheric Science: An Introductory Survey by John M. Wallace and Peter V. Hobbs – Chapter 3, “Basic Physical Processes in the Atmosphere” (sections on pressure gradients and forces). It discusses in more detail how centrifugal force affects atmospheric circulation.

2. Increased Coriolis Effect

  • Stronger Deflection of Winds: The Coriolis effect, which causes moving air to deflect to the right in the Northern Hemisphere and to the left in the Southern Hemisphere, would become stronger due to the faster rotation. This means that winds would curve more sharply, resulting in more pronounced and tighter circulation patterns.
  • More Jet Streams and Faster Winds: With an increased Coriolis effect, we might see additional jet streams develop, with stronger and faster winds aloft. The existing jet streams could become narrower and more intense, leading to greater atmospheric turbulence.
 

Suggested Reading

The Atmosphere: An Introduction to Meteorology by Frederick Lutgens and Edward Tarbuck – Chapter 7, “Winds and Global Circulation.” This chapter covers the Coriolis effect and its role in deflecting wind patterns, with explanations on how it strengthens with faster rotation.
 
Introduction to Atmospheric Dynamics by David G. Andrews – Chapter 4, “Midlatitude Synoptic Systems” (section on jet streams and their formation)

3. Changes in Atmospheric Circulation Cells

  • More but Smaller Circulation Cells: Currently, Earth has three main circulation cells in each hemisphere: the Hadley, Ferrel, and Polar cells. With a faster rotation, these cells could be split into more, smaller cells. For example, the Hadley cells could be narrower and closer to the equator, while additional cells might form in the mid-latitudes.
  • Stronger Trade Winds: The trade winds, which blow from east to west in the tropics, could strengthen due to the intensified Coriolis effect, leading to more persistent and intense tropical weather systems.

Suggested Reading

Global Physical Climatology (2nd Edition) by Dennis L. Hartmann – Chapter 6, “General Circulation of the Atmosphere.” This chapter explains how the Earth’s atmospheric circulation cells would adjust with different rotational speeds.

Climatology by Robert V. Rohli and Anthony J. Vega – Chapter 5, “The Global Energy Balance and Temperature” (sections on large-scale wind systems). It includes discussions on how the Coriolis effect influences trade winds and global circulation.

4. Impact on Weather Patterns

  • More Extreme Weather at Mid-Latitudes: The more intense and frequent jet streams could lead to increased weather variability in the mid-latitudes, causing rapid changes between weather conditions. The stronger Coriolis effect could also enhance the formation of cyclones, making storms more frequent and severe.
  • Changes in Rainfall Patterns: The shift of atmospheric cells and changes in wind patterns could alter where and how rain falls. Regions that currently experience steady rainfall might see a shift in precipitation patterns, with some areas becoming wetter and others drier. The equatorial region might see more concentrated rainfall, while mid-latitude regions could experience more variability and intense storms.

Suggested Reading

Synoptic-Dynamic Meteorology in Midlatitudes (Volume I, 2nd Edition) by Howard Bluestein – Chapter 8, “Extratropical Cyclones” (section on the dynamics of mid-latitude weather systems). This chapter explains how increased rotational speeds could affect storm formation and variability.

Meteorology Today: An Introduction to Weather, Climate, and the Environment (13th Edition) by C. Donald Ahrens – Chapter 13, “Weather Patterns and Severe Storms.” This chapter covers how shifts in circulation can alter rainfall distribution and weather patterns.

5. Temperature Distribution

  • More Temperature Variation Between Day and Night: With a faster rotation, days and nights would be shorter, which could lead to reduced time for heating during the day and cooling at night. This might create a sharper contrast between daytime and nighttime temperatures, particularly in regions far from the equator.
  • Equator-to-Pole Temperature Gradient: The stronger centrifugal force pulling air and water toward the equator could make polar regions even colder while concentrating warmer temperatures closer to the equator. The result would be a steeper temperature gradient, potentially intensifying atmospheric circulation and weather dynamics.
 

Suggested Reading

Principles of Planetary Climate (1st Edition) by Raymond T. Pierrehumbert – Chapter 4, “Radiative Energy Balance” (section on rotation and temperature profiles). This discusses how changes in the length of day affect planetary temperature variations.

Atmospheric and Oceanic Fluid Dynamics (2nd Edition) by Geoffrey K. Vallis –  Chapter 2, “The Governing Equations” (sections on temperature gradients and atmospheric circulation). This chapter elaborates on how temperature differences drive global weather patterns.

Overall, a faster-rotating Earth would likely have more intense and complex weather patterns, with stronger winds, more pronounced atmospheric circulation, and altered temperature distributions.

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