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Because Earth's rotation is gradually slowing, the length of each day increases: The day at the end of \(1.0\) century is \(1.0 \mathrm{~ms}\) longer than the day at the start of the century. In 20 centuries, what is the total of the daily increases in time?

Short Answer

Expert verified
The total increase in daily time over 20 centuries is 20.0 ms.

Step by step solution

01

Understand the Problem

We are given that the length of the day increases by 1.0 ms over a century. We need to find the total daily increase for 20 centuries.
02

Calculate the Daily Increase for One Century

The daily increase in time for one century is given as 1.0 ms. This means by the end of one century, each day is 1.0 ms longer than at the start.
03

Calculate the Total Increase Over 20 Centuries

Multiply the daily increase per century by the total number of centuries. Since the increase is 1.0 ms per century, for 20 centuries, the total increase is:\[ 1.0 \text{ ms/century} \times 20 \text{ centuries} = 20.0 \text{ ms}. \]
04

Conclusion

The increase in the length of the day over 20 centuries is 20.0 ms. This is the cumulative increase in daily time over this period.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Earth's Rotation
The rotation of Earth is a fascinating phenomenon that greatly affects our daily lives. Imagine Earth as a spinning top; it revolves around its axis, which results in day and night. This rotation takes approximately 24 hours to complete a full cycle. However, Earth doesn't spin at a constant speed. Over millennia, its rotation is gradually slowing down.

The gradual slowing of Earth's rotation means that each day becomes slightly longer. Factors causing this change include gravitational interactions with the Moon and even movements within our planet, such as its molten core movements. This slowing effect might not be noticeable daily, but over extended periods, like centuries, the impact accumulates. Understanding the slowing rotation helps in predicting changes in time measurement and adapting various global systems.

Key points to remember about Earth's rotation:
  • Earth completes a full rotation in about 24 hours.
  • Due to gravitational forces and internal dynamics, Earth's rotation is slowing.
  • The slowing rotation can affect time measurement over long periods.
Time Measurement
Time measurement is an essential practice in human society, enabling us to organize, predict, and plan activities efficiently. Precision in timekeeping affects everything from navigation to communication technologies. With Earth's rotation speed changing, historical methods of time measurement must adapt to newer and more accurate technologies.

Traditionally, time was based on the apparent movement of the Sun across the sky – the sundial era. As Earth's rotation changes, technologies have evolved. Today, atomic clocks provide extremely precise timekeeping, minimizing errors resulting from Earth's variable rotation.

Understanding time measurement in the context of physics involves appreciating the ongoing adjustments needed for when our planet's rotational velocity alters:
  • Atomic clocks provide precise time management despite Earth's slowing rotation.
  • Historically, time was linked to Earth's rotation (e.g., sundials, water clocks).
  • Modern systems may require adjustments, like leap seconds, to stay accurate.
Century Calculation
Century calculations play a significant role in understanding long-term changes on Earth, such as assessing the cumulative effect of Earth's slowing rotation. In the given problem, each century witnesses a 1.0 millisecond increase in the length of a day. This may seem minor, but over many centuries, the cumulative effect can be significant.

When dealing with century calculations, it's essential to understand the timescale involved and how small changes can accumulate. In this exercise, a systematic approach enabled us to establish that over 20 centuries, the increase in daily time sums up to 20 milliseconds. Such calculations help quantify long-term trends that can influence global activities and technologies.

Key insights into century calculations:
  • Small changes over long periods lead to significant accumulations (e.g., 1 ms per century).
  • Understanding these trends allows for better adaptation of timekeeping technologies.
  • Long-term calculations affect navigation, space sciences, and more.

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Most popular questions from this chapter

Earth is approximately a sphere of radius \(6.37 \times 10^{6} \mathrm{~m}\). What are (a) its circumference in kilometers, (b) its surface area in square kilometers, and (c) its volume in cubic kilometers?

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