Which hypothesis proposes that a cloud of gas and dust collapsed and flattened due to gravity, leading to the formation of the solar system?
Lesson 2.1: The Origin of the Solar System

Quiz
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Science
•
11th Grade
•
Medium
Rafael Nanas
Used 44+ times
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20 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Nebular Hypothesis
Planetesimal Hypothesis
Tidal Theory
Protoplanet Hypothesis
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the key weakness of the Nebular Hypothesis?
Difficulty in explaining initial trigger
Inability to explain the diversity of planetary compositions
Lack of evidence for protoplanetary disks
Ignoring the role of gas giants in solar system formation
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
According to the Nebular Hypothesis, what role does conservation of angular momentum play in the formation of the solar system?
It causes the solar nebula to contract
It triggers nuclear fusion in the Sun
It leads to the formation of planetesimals
It causes the spinning solar nebula to flatten into a disk
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
The Planetesimal Hypothesis focuses on the idea that planets formed through the collision and coalescence of _______________.
gas clouds
protoplanets
star clusters
solid planetesimals
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What evidence supports the Planetesimal Hypothesis?
Observations of protoplanetary disks
Observations of interstellar gas clouds
Kuiper Belt and Asteroid Belt
Presence of multiple stars in the solar system
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Which hypothesis suggests that a passing star or external perturbation triggers the collapse of a diffuse gas cloud, leading to star and planetary system formation?
Nebular Theory
Planetesimal Hypothesis
Tidal Theory
Protoplanet Hypothesis
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is a major weakness of Tidal Theory?
It fails to explain the role of external influences.
It doesn't address the presence of interstellar gas clouds.
It is too complex to understand.
It lacks a clear mechanism for protostar formation.
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