Using the nebular theory, explain the formation of our solar system from the formation of the solar nebula through the present day
What will be an ideal response?
Answer: The gases and dust in the solar nebula contracted and began to rotate. The majority of materials fell into the center of this rotating mass to form the protosun. The remaining materials flattened out into a disk, which allowed heat to escape more quickly. Cooling resulted in condensation of larger grains of icy, rocky material. These grains collided repeatedly to create protoplanets, which eventually became the planets we have today.
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Clastic sedimentary rocks are formed
A. from the broken-up fragments of preexisting rocks. B. at very high temperatures because the grains must be fused together to make rock. C. from chemicals dissolved in solution. D. All of the choices are correct.
Molecules in a constant-temperature mixture of gasses have the same average
A. velocity. B. kinetic energy. C. speed. D. all of the above
The site on the accompanying figure that would most likely form a rock that has a nonwelded texture with many fine particles is
A) A.
B) B.
C) C.
D) D.
E) E.
Volcanic activity always results in a loss of biodiversity due to habitat destruction. Indicate whether the statement is true or false