Chapter 12: Problem 12
T/F: Comet tails always point away from the Sun.
Short Answer
Expert verified
True.
Step by step solution
01
Understanding Comet Tails
Comet tails are created by the solar wind and radiation pressure from the Sun. This means they point away from the Sun, regardless of the comet's direction.
02
Considering Solar Wind
Solar wind consists of charged particles emitted by the Sun. These particles exert force on the comet's tail, pushing it away from the Sun.
03
Evaluating Radiation Pressure
Radiation pressure is due to sunlight photons striking comet material, again pushing it away from the Sun.
04
Conclusion
Both solar wind and radiation pressure influence the comet's tail, confirming that the tail always points away from the Sun.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Solar Wind
The **solar wind** plays a fundamental role in shaping a comet's tail. Solar wind is a stream of charged particles, mostly protons and electrons, ejected from the Sun's upper atmosphere, known as the corona.
These charged particles move at incredibly high speeds, often exceeding 1 million miles per hour.
The interaction between the solar wind and the comet causes the particles in the comet's coma (the cloud surrounding the comet's nucleus) to ionize.
This ionization process generates a force that pushes the comet's tail away from the Sun. This happens regardless of the direction the comet is traveling.
Key points about solar wind’s effect on comet tails:
These charged particles move at incredibly high speeds, often exceeding 1 million miles per hour.
The interaction between the solar wind and the comet causes the particles in the comet's coma (the cloud surrounding the comet's nucleus) to ionize.
This ionization process generates a force that pushes the comet's tail away from the Sun. This happens regardless of the direction the comet is traveling.
Key points about solar wind’s effect on comet tails:
- The solar wind is made up of charged particles like protons and electrons.
- It originates from the Sun’s corona.
- It pushes the comet's tail away from the Sun.
Radiation Pressure
Radiation pressure is the other major force acting upon a comet’s tail. This is the force exerted by sunlight itself. Light is composed of photons, which are particles that exert pressure when they collide with other particles.
When photons from the Sun strike the particles in a comet’s coma, they impart momentum. This pressure pushes the tail material away from the Sun.
Here are some additional points about radiation pressure:
When photons from the Sun strike the particles in a comet’s coma, they impart momentum. This pressure pushes the tail material away from the Sun.
Here are some additional points about radiation pressure:
- Radiation pressure comes from sunlight photons.
- It pushes the small particles in a comet’s tail away from the Sun.
- This force is significant enough to shape the direction and structure of the comet's tail.
Astronomy Education
Understanding the forces behind comet tails provides valuable insights and strengthens our grasp of fundamental astronomical concepts. In **astronomy education**, learning about comet tails can enrich one’s comprehension of solar and space phenomena.
This knowledge helps students understand how various factors in space interact with one another. Here’s why grasping these concepts is essential:
This knowledge helps students understand how various factors in space interact with one another. Here’s why grasping these concepts is essential:
- It enhances understanding of solar phenomena and space weather.
- It illustrates the relevance of theories like electromagnetism and photon momentum in practical scenarios.
- It fosters curiosity about the dynamic nature of celestial bodies and their interactions.