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Earth's rotation

earth science Maturity 7-9

Our big Earth spins around.

EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif
It turns in a circle. This spin makes day and night. It helps us know when to sleep. It is very cool!
Earth Rotation (Nepal, Himalayas).jpg
Earth Rotation (Nepal, Himalayas).jpg
Can you feel the spin?

37 words

Our big Earth spins around.

EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif
This spin makes day and night. It takes about 24 hours to spin once.
Earth Rotation (Nepal, Himalayas).jpg
Earth Rotation (Nepal, Himalayas).jpg
The spin is actually slowing down a little bit. The Moon helps cause this change. In the past, days were even shorter. Some years, the Earth even spins faster. This can happen because of the oceans and air.
Starry Spin-up.jpg
Starry Spin-up.jpg
It is amazing to think our world is always moving!

74 words

Earth spins around on an axis. An axis is an imaginary line through the center.

EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif
The North Pole and South Pole are the ends of this line. Earth spins toward the east. This spin takes about 24 hours.
Sidereal day (prograde).svg
Sidereal day (prograde).svg
This creates day and night.

Earth's spin is not always the same. The Moon's pull on the oceans slows the spin down. This means days were shorter a long time ago. In 2020, Earth began to spin faster again. This change might come from the oceans or the air. Melting ice can also change how fast Earth spins. When ice melts, mass moves closer to the center. This makes the planet spin faster.

Starry Spin-up.jpg
Starry Spin-up.jpg

Not all parts of Earth move at the same speed. The equator is the middle of the Earth. It is the widest part. Speed is highest at the equator. Speed gets lower as you move toward the poles. At the very poles, the speed is zero.

Earth rotation tangential speed.svg
Earth rotation tangential speed.svg

164 words

Earth is constantly spinning around on an imaginary line called an axis. This movement is known as rotation.

EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif
The axis runs through the North Pole and the South Pole. Earth rotates toward the east, which is called prograde motion.
Sidereal day (prograde).svg
Sidereal day (prograde).svg
This spin is what gives us our days and nights. If you look at the stars from the North Pole, the Earth seems to turn counterclockwise. It takes about 24 hours to spin once relative to the Sun. However, it takes 23 hours, 56 minutes, and 4 seconds to spin once relative to distant stars.

The speed of this spin changes depending on where you stand. The Earth is widest at the equator, which is the middle part of the planet. Because the equator is so large, the speed is highest there at about 1,670 kilometers per hour. As you move toward the poles, the speed decreases. For example, at 45 degrees latitude, the speed is roughly 1,180 kilometers per hour. At the very North or South Pole, the speed is zero. This happens because there is no distance to cover in a full rotation at the poles.

Earth rotation tangential speed.svg
Earth rotation tangential speed.svg

People have wondered about this spin for a very long time. Ancient Greeks like Philolaus believed the Earth moved, but their ideas were quite complex. In 499 CE, an Indian astronomer named Aryabhata suggested the Earth rotates on its axis. He said it is like a person in a boat seeing the river banks move backward.

Earth Rotation (Nepal, Himalayas).jpg
Earth Rotation (Nepal, Himalayas).jpg
Later, Nicolaus Copernicus helped establish our modern view in 1543. He showed that planets circle a central Sun. Other scientists like Galileo and Newton later provided more support for the idea of a rotating Earth.

Scientists use many tools to study how the Earth spins. They use atomic clocks to measure time very precisely. These clocks show that the length of a day is changing. For a long time, the Moon's pull on the oceans slowed the spin down. This meant days were getting longer by about 2.3 milliseconds every century. But in 2020, scientists reported that the Earth began to rotate faster. On June 29, 2022, the Earth set a record by completing a rotation in 1.59 milliseconds under 24 hours.

Many things can change the speed of our planet. The movement of the molten core, oceans, and atmosphere all play a part. Climate change might also be a factor. When ice at the poles melts, the Earth's shape changes slightly. The Earth is an oblate spheroid, which means it bulges at the equator. As ice melts, the poles rebound and the Earth becomes more spherical. This moves mass closer to the center of gravity. Because of the laws of physics, spinning mass moves faster when it is closer to the center.

AxialTiltObliquity.png
AxialTiltObliquity.png

473 words

Earth's rotation is the planet's spin around its own axis. This movement is known as prograde motion because Earth rotates toward the east.

Sidereal day (prograde).svg
Sidereal day (prograde).svg
This rotation creates our cycle of day and night. It also causes the apparent movement of stars across the sky. The axis of rotation connects the North Pole to the South Pole. The North Pole is a specific point in the Northern Hemisphere. It is different from the magnetic north pole.
EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif

Rotation speed varies depending on your latitude. At the equator, the Earth's circumference is at its largest. This means the rotational speed is highest there, at about 1,670 kilometers per hour. As you move toward the poles, the speed decreases. At 45 degrees latitude, the speed drops to roughly 1,180 kilometers per hour. At the poles, the speed is effectively zero. This happens because there is no distance to travel during a rotation at those points.

Earth rotation tangential speed.svg
Earth rotation tangential speed.svg

We measure the length of a rotation in two different ways. A solar day is the time from one noon to the next. This takes about 24 hours. A sidereal day is the time it takes to rotate relative to distant stars. This takes 23 hours, 56 minutes, and 4 seconds. The solar day changes slightly throughout the year. This is due to the eccentricity and inclination of Earth's orbit. For example, the true solar day is longer near perihelion. This is when Earth is closest to the Sun.

For centuries, thinkers have debated how the Earth moves. Some ancient Greeks, like Philolaus, believed the Earth rotated. However, Aristotle argued that the stars were fixed in a sphere. He believed the heavens rotated around a stationary Earth. This view lasted a long time. In 499 CE, the Indian astronomer Aryabhata suggested the Earth rotates. He used a clever analogy. He said a person in a boat sees the river banks moving backward.

Earth Rotation (Nepal, Himalayas).jpg
Earth Rotation (Nepal, Himalayas).jpg
Later, Nicolaus Copernicus established the heliocentric system in 1543. He showed that planets circle the Sun. Scientists like Galileo and Newton later provided more evidence for this rotation.

Scientists use precise tools to track changes in rotation speed. Atomic clocks show that the length of a day is not constant. For a long time, the Moon's tidal effects slowed Earth down. This increased the length of a day by 2.3 milliseconds per century. However, in 2020, Earth began to rotate faster. On June 29, 2022, Earth completed a rotation in 1.59 milliseconds under 24 hours. This was a new record. Engineers are now discussing a "negative leap second" to manage this.

Several factors influence how fast the planet spins. The movement of the molten core, oceans, and atmosphere all matter. Climate change may also play a role. Melting ice at the poles changes the Earth's shape. Earth is an oblate spheroid, which means it bulges at the equator.

AxialTiltObliquity.png
AxialTiltObliquity.png
When ice melts, the poles rebound from the loss of weight. This makes the Earth more spherical. This brings mass closer to the center of gravity. The law of conservation of angular momentum says that mass spinning closer to the center moves faster.

Rotation also creates the Coriolis effect. This is an apparent path that moving objects follow in a rotating system. In the Northern Hemisphere, projectiles veer to the right. In the Southern Hemisphere, they veer to the left. This effect is very important for meteorology. It causes cyclones to rotate in different directions in each hemisphere. Scientists once tested this by dropping weights from tall towers. The most famous test was the Foucault pendulum in 1851. This device uses a heavy sphere to show the Earth rotating underneath it.

Starry Spin-up.jpg
Starry Spin-up.jpg

620 words
🖼️ Images & Media (9)
File:EpicEarth-Globespin-tilt-23.4.gif
EpicEarth-Globespin-tilt-23.4.gif
File:Earth Rotation (Nepal, Himalayas).jpg
Earth Rotation (Nepal, Himalayas).jpg
File:Starry Spin-up.jpg
Starry Spin-up.jpg
File:Sidereal day (prograde).svg
Sidereal day (prograde).svg
File:Earth_rotation_tangential_speed.svg
Earth_rotation_tangential_speed.svg
File:AxialTiltObliquity.png
AxialTiltObliquity.png
File:Simulated evolution of Earth's day length over time.png
Simulated evolution of Earth's day length...
File:Deviation of day length from SI day.svg
Deviation of day length from SI day.svg
File:The_Mysterious_Case_of_the_Disappearing_Dust.jpg
The_Mysterious_Case_of_the_Disappearing_Dust.jpg
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