Difficulty: Easy
Correct Answer: All of the above
Explanation:
Introduction / Context:
The nightly motion of stars across the sky is a foundational concept in astronomical surveying, navigation, and observational astronomy. Understanding the origin and geometry of this motion explains why some stars are circumpolar, why their trails are circular in long-exposure photographs, and how the celestial pole provides a stable reference direction.
Given Data / Assumptions:
Concept / Approach:
Because Earth rotates once every roughly 24 hours, the entire sky appears to rotate the other way. This apparent rotation causes stars to follow circular paths centered on the celestial pole. The axis of rotation of Earth defines a fixed direction through the celestial sphere; where this axis meets the sphere are the north and south celestial poles. All stars share the same instantaneous angular speed with respect to the pole but have different circle radii depending on their declinations.
Step-by-Step Solution:
Verification / Alternative check:
Star-trail photography shows concentric circles around the pole. The near-fixity of Polaris (close to the north celestial pole) and the rotation of the rest of the sky around it corroborate the model.
Why Other Options Are Wrong:
Each individual statement (a)–(d) is correct; therefore the collective correct choice is “All of the above.”
Common Pitfalls:
Confusing apparent motion with actual stellar motion; overlooking that circumpolarity depends on observer latitude; and forgetting that the pole is a direction, not a single star.
Final Answer:
All of the above
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