WorksheetsEarth's Early History Review
Total questions: 33
Worksheet time: 17mins
The formation of the solar system from a huge cloud of dust and gases is called the (a) theory.
The image shows the formation of the solar system from a cloud of gas.
Based on the image, which explanation best describes how gravity helped to form the solar system?
the disintegration of the protosun into planets
accumulation of leftover materials that formed into planets
collisions between gas molecules that resulted in planet formation
condensation of gas and dust molecules that formed the protosun
Which of the following processes is responsible for the formation of stars from a nebula?
Erosion
Radioactive decay
Gravitational collapse
Nuclear fusion
What is the primary reason Earth has fewer visible craters compared to the Moon?
The Moon has a stronger gravitational pull
Earth's atmosphere burns up small meteors
The Moon is closer to the asteroid belt
Earth's surface is constantly changing due to erosion
Which of the following best describes the role of gravity in the formation of the solar system?
It caused the planets to form from leftover materials
It led to the disintegration of the protosun
It caused the solar system to expand indefinitely
It prevented the formation of gaseous planets
Which process is responsible for the transformation of a protostar into a main-sequence star?
Nuclear fusion
Gravitational collapse
Radioactive decay
Erosion
What is the primary reason Earth has less visible cratering compared to the Moon?
Earth's atmosphere burns up smaller meteors
The Moon attracts more meteors due to its gravitational pull
Earth's surface is constantly changing due to erosion and tectonics
The Moon's surface is more resistant to impacts
Which process is responsible for the formation of a planetary disk around a young star?
Nuclear fusion
Gravitational collapse
Electrostatic forces
Magnetic field interactions
What is the main component of the early solar nebula that led to the formation of the Sun and planets?
Silicon dust
Carbon dioxide
Hydrogen gas
Iron particles
