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    Astronomy 101

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    • Introduction to Astronomy
      • 1.1What is Astronomy?
      • 1.2History of Astronomy
      • 1.3Overview of the Universe
    • The Solar System
      • 2.1Overview of the Solar System
      • 2.2Planets and their Characteristics
      • 2.3Other Celestial Bodies in the Solar System
    • Stars and Galaxies
      • 3.1Introduction to Stars
      • 3.2Life Cycle of Stars
      • 3.3Introduction to Galaxies
      • 3.4Types of Galaxies
    • The Milky Way and Other Galaxies
      • 4.1Overview of the Milky Way
      • 4.2Other Notable Galaxies
      • 4.3Interstellar Medium and Cosmic Dust
    • Telescopes and Observatories
      • 5.1Introduction to Telescopes
      • 5.2Types of Telescopes
      • 5.3Famous Observatories
    • The Sun and the Moon
      • 6.1Overview of the Sun
      • 6.2Solar Phenomena
      • 6.3Overview of the Moon
      • 6.4Lunar Phenomena
    • The Earth and the Sky
      • 7.1Earth's Rotation and Revolution
      • 7.2Seasons and Climate
      • 7.3Sky Phenomena
    • Space Exploration
      • 8.1History of Space Exploration
      • 8.2Notable Space Missions
      • 8.3Future of Space Exploration
    • Astrobiology
      • 9.1Introduction to Astrobiology
      • 9.2Search for Extraterrestrial Life
      • 9.3Extremophiles on Earth
    • Cosmology
      • 10.1Introduction to Cosmology
      • 10.2The Big Bang Theory
      • 10.3Dark Matter and Dark Energy
    • Space-Time and Relativity
      • 11.1Introduction to Space-Time
      • 11.2Special Relativity
      • 11.3General Relativity
    • Black Holes and Neutron Stars
      • 12.1Introduction to Black Holes
      • 12.2Properties of Black Holes
      • 12.3Introduction to Neutron Stars
      • 12.4Properties of Neutron Stars
    • Wrap-up and Future Study
      • 13.1Review of Key Concepts
      • 13.2Current Research in Astronomy
      • 13.3How to Continue Studying Astronomy

    The Earth and the Sky

    Module 7, Unit 1: Earth's Rotation and Revolution

    angle between the rotational axis and orbital axis of a body

    Angle between the rotational axis and orbital axis of a body.

    Introduction

    Understanding the Earth's rotation and revolution is fundamental to understanding many aspects of our daily lives, from the cycle of day and night to the changing of the seasons. In this unit, we will explore these movements and their effects in detail.

    Earth's Rotation

    The Earth rotates on its axis, an imaginary line that runs from the North Pole to the South Pole. This rotation happens once every 24 hours and is the reason we experience day and night.

    When one side of the Earth faces the Sun, it experiences daylight. As the Earth continues to rotate, this side moves away from the Sun, transitioning into night. Meanwhile, the other side of the Earth begins to face the Sun, transitioning from night to day. This continuous rotation creates the 24-hour cycle of day and night that we are all familiar with.

    The speed of Earth's rotation is not uniform across the planet. At the equator, the Earth's surface is moving at a speed of about 1,670 kilometers per hour due to rotation. However, as you move towards the poles, this speed decreases because the circles of rotation become smaller.

    Earth's Revolution

    While the Earth is rotating on its axis, it is also revolving around the Sun. This revolution takes about 365.25 days, which we round down to 365 for convenience in our calendar year. The extra 0.25 days is why we have a leap year every four years - to account for those extra hours.

    The path that the Earth takes around the Sun is called its orbit. The Earth's orbit is not a perfect circle, but an ellipse, meaning it is slightly elongated. This means that the Earth is not always the same distance from the Sun. However, contrary to popular belief, the changing distance to the Sun is not what causes our seasons. That has more to do with the tilt of the Earth's axis, which we will discuss in the next unit.

    Conclusion

    The Earth's rotation and revolution are fundamental to our experience of time. The rotation of the Earth on its axis gives us our cycle of day and night, while its revolution around the Sun gives us our year. Understanding these movements helps us understand many other aspects of our world, from the changing of the seasons to the behavior of the stars in the night sky. In the next unit, we will explore how the tilt of the Earth's axis affects our seasons and climate.

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    Next up: Seasons and Climate