📚 Learning Guide
Outer Solar System Features
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How does Neptune's migration influence the orbits of icy objects in the Outer Solar System?

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Choose the Best Answer

A

It stabilizes their orbits, making them circular.

B

It ejects them into highly elliptical orbits.

C

It causes them to collide with each other frequently.

D

It prevents them from entering the Kuiper Belt.

Understanding the Answer

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Answer

Neptune’s migration refers to the planet’s slow outward drift after the Sun’s protoplanetary disk cleared. As it moved, its gravity pulled nearby icy planetesimals, trapping some in resonant orbits and scattering others into distant, highly eccentric paths. This explains why many Kuiper Belt objects share similar orbital periods—such as Pluto’s 3:2 resonance with Neptune—and why scattered‑disk bodies have elongated orbits. The migration process therefore shapes both the structure and the dynamical families of icy objects beyond Neptune. For instance, Pluto remains locked in a 3:2 resonance because it was captured during Neptune’s outward journey.

Detailed Explanation

Neptune moves farther from the Sun and pulls on nearby icy bodies. Other options are incorrect because Some think Neptune smooths the paths, but actually its pull disturbs them; It’s easy to imagine many collisions, yet most icy objects are far apart.

Key Concepts

Neptune's gravitational influence
Orbital dynamics of icy bodies
Migration of planets
Topic

Outer Solar System Features

Difficulty

medium level question

Cognitive Level

understand

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