Learning Path
Question & Answer1
Understand Question2
Review Options3
Learn Explanation4
Explore TopicChoose the Best Answer
A
B → C → A → D
B
B → A → C → D
C
C → B → A → D
D
B → C → D → A
Understanding the Answer
Let's break down why this is correct
Answer
The first step is the formation of a flat disk of gas and dust around the newborn Sun (B). From that disk, material in the warmer inner region collapsed into rocky planets (C). Farther out, where temperatures were low, ice-rich chunks began to stick together, forming the seeds of outer planets and comets (A). Finally, as the outer planets grew, their gravity reshaped the paths of comets and other icy bodies, pulling them into new orbits (D). This sequence explains how the Sun, planets, and cometary belts came into being.
Detailed Explanation
The correct order is B → C → A → D. Other options are incorrect because This option mixes up the timing of ice gathering and planet building; It reverses the order by placing planet formation before the disk, which cannot happen.
Key Concepts
Formation of Solar System
Planetary differentiation
Gravitational effects on celestial bodies
Topic
Formation of Solar System
Difficulty
hard level question
Cognitive Level
understand
Practice Similar Questions
Test your understanding with related questions
1
Question 1How did the formation of the Solar System influence the differences between inner and outer planets?
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2
Question 2The formation of the Solar System involved a flat disk of material around the Sun, leading to the creation of planets, asteroids, and comets. This process is largely influenced by the gravitational effects of larger bodies, which can be best described as _______.
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3
Question 3Order the following events to describe the process of how comets from the Oort Cloud are formed and interact with the solar system: A) Gravitational disturbances from nearby stars influence Oort Cloud objects, B) Icy bodies in the Oort Cloud are perturbed into the inner solar system, C) These bodies exhibit long orbital periods as they approach the sun, D) The objects coalesce to form larger bodies in the outer solar system.
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