Chapter 23: Problem 6
How long does it take for the Moon to rotate once? A) 24 hours C) \(27.3\) hours ?) 365 days D) \(27.3\) days
Short Answer
Expert verified
The Moon takes 27.3 days to rotate once.
Step by step solution
01
Understanding the Question
The question is asking for the duration it takes for the Moon to complete one full rotation on its axis. This is known as the Moon's rotation period.
02
Identifying the Correct Rotation Period
The Moon rotates on its axis at the same rate that it orbits the Earth, a phenomenon called synchronous rotation. This means the Moon completes one rotation in the same amount of time it takes to orbit Earth once.
03
Finding the Moon's Orbital Period
The Moon's orbital period, and therefore its rotational period, is approximately 27.3 days. This value corresponds with option D.
04
Verifying Against Given Options
Among the given options for the rotation period: 24 hours, 27.3 hours, 365 days, and 27.3 days, the correct duration is 27.3 days, which matches the fact that the Moon takes 27.3 days to rotate once.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
synchronous rotation
Synchronous rotation is a concept that occurs when an astronomical body rotates on its axis in the same amount of time it takes to orbit around another body. In the case of the Moon, this phenomenon is what causes us to always see the same side of the Moon from Earth.
This happens because the gravitational pull between the Earth and the Moon has caused the Moon's rotation to slow over time until it reached this state of balance. Now, the Moon completes one rotation on its axis in exactly the same time it takes to complete one orbit around Earth: approximately 27.3 days.
This happens because the gravitational pull between the Earth and the Moon has caused the Moon's rotation to slow over time until it reached this state of balance. Now, the Moon completes one rotation on its axis in exactly the same time it takes to complete one orbit around Earth: approximately 27.3 days.
- This matching of rotation and orbital periods is not unusual in space and is termed as being tidally locked.
- It leads to one hemisphere of the Moon constantly facing the Earth.
- Understanding synchronous rotation helps explain why human beings have only seen one side of the Moon until satellites were sent to orbit it.
Moon's orbital period
The Moon's orbital period refers to the time it takes for the Moon to make one complete orbit around Earth. This period is approximately 27.3 days. During this time, the Moon travels around the Earth in an elliptical path.
The idea of a 27.3-day period may seem specific, but it is a result of the gravitational interactions within the Earth-Moon system and the velocity at which the Moon orbits.
The idea of a 27.3-day period may seem specific, but it is a result of the gravitational interactions within the Earth-Moon system and the velocity at which the Moon orbits.
- The Moon's orbital path is slightly elliptical, meaning it isn’t a perfect circle.
- Because of this orbit, the distance between the Earth and the Moon changes as the Moon moves around Earth.
- The period of 27.3 days aligns with both its rotation and its orbital times because of gravitational forces.
- This orbital period is crucial for creating lunar cycles like new moons or full moons, which affect things like tides and calendars.
Earth-Moon system
The Earth-Moon system is a fascinating example of the gravitational interactions that govern much of what occurs in our universe. This system consists of Earth and its natural satellite, the Moon, which together create a complex gravitational dance.
The Moon's gravitational pull is responsible for creating tides in Earth's oceans due to the differences in gravitational strength at various points around the Earth.
The Moon's gravitational pull is responsible for creating tides in Earth's oceans due to the differences in gravitational strength at various points around the Earth.
- The Earth-Moon system helps stabilize Earth's axial tilt, which is why we have predictable seasons.
- The long-term nature of the Moon's gravitational pull slows the Earth's rotation very gradually over time.
- Together, Earth and Moon share a barycenter—a common center of mass around which both objects revolve. For the Earth-Moon system, this point is located inside Earth due to its substantially larger mass.