
Earth's Early History reteach
Presentation
•
Science
•
10th Grade
•
Medium
+15
Standards-aligned
Stephanie Ard
Used 3+ times
FREE Resource
10 Slides • 24 Questions
1
Nebular Theory
Review for Nebular Theory Quiz
2
Multiple Choice
3
4
Multiple Choice
What is the FIRST event in the formation of the solar system?
About 4.5 billion years ago pieces of rock and ice accumulate more material until they grow into planets and moons.
About 4.6 billion years ago, a cloud of stellar dust or nebula exists within the Milky Way.
None of the above.
5
Multiple Choice
6
Multiple Choice
The energy enriched nebula begins to contract further due to gravity. Then what?
The center of the nebula begins to get hot and dense.
Shock waves hit the nebula causing it to collapse.
The nebula begins to spin and flatten.
7
Multiple Choice
The collapsed cloud of interstellar gas and dust results to a smaller radius which means it will _______ faster.
spin
degrade
revolve
explode
8
Multiple Choice
when dust and gas gravitate together and form ever larger bodies
absolution
attrition
accretion
erosion
9
10
planetesimals stick together to form protoplanets
11
Multiple Choice
The protoplanets keep:
12
Multiple Choice
As the solar system continued to evolve, material in the disk collided with other material and grew into planetesimals, then protoplanets, and then planets. This process of growth by collision created a lot of heat, melting the early Earth. Growth by collision is called ___.
differentiation
accretion
adsorption
kinetic molecular theory
13
14
Multiple Choice
Sun + orbiting planets =
nebula
solar system
asteroids
meteroids
15
Reorder
Reorder the following
The nebula started to collapse and condense; this continued for some time.
Pockets of dust and gas began to collect in denser regions and it began rotating.
The solar nebula rotated faster and faster as it shrank in radius AND flatten.
Most of the material ended up in a ball in the middle as the Sun's protostar.
The rest of the nebula was left in the form of a disk called a protoplanetary disk.
16
17
Heavy Bombardment Period
Asteroids collide with young planets
During the Heavy Bombardment Period failed planets and large asteroids slammed into larger worlds, including young Earth. When these objects struck Earth, they left craters.
18
Multiple Choice
When did frequent large impacts stop?
about 9,000 years ago
about 3 million years ago
about 9 billion years ago
about 3.9 billion years ago
19
Multiple Choice
20
The earth moves!
Our earth moves! We have many pieces of evidence for this some we can even feel; like earthquakes. So what is causes the movement? Magma! Deep in the Earth, molten rock churns as it heats and cools in convection currents. This moves the crustlike plates on top, and even creates and new and destroys old plates. *VIDEO TIME*
21
One problem with dating rocks and minerals on Earth is the presence of the rock cycle. During the rock cycle, rocks are constantly changing between forms, going back and forth from igneous to metamorphic to sedimentary. Old rocks may even be destroyed as they slide back into the Earth's mantle, to be replaced by newer rocks formed by solidified lava. This makes finding an exact age for the Earth difficult, because the original rocks that formed on the Earth at the earliest stages of its creation are no longer here. The oldest rocks that have been found are about 3.8 billion years old, though some tiny minerals have been dated at 4.2 billion years.
22
To get around the difficulty presented by the rock cycle, scientists have looked elsewhere in the solar system for even older rock samples. They have examined rocks from the moon and from meteorites, neither of which have been altered by the rock cycle. The same techniques of radiometric dating have been used on those rocks. All of the data from this planet and beyond has led to the estimated age for the Earth of 4.5 billion years.
23
Multiple Choice
Scientists currently estimate that Earth is approximately ____ years old.
600 years old
4.5 million years
4.5 billion years
53 million years
24
Multiple Choice
How long has the recycling of Earth’s crust been going on?
about 4 billion years
about 4,000 years
about 4 million years
about 400 years
25
Multiple Choice
26
Multiple Choice
Why are meteorites important to evidence when estimating the age of Earth?
Meteorites are most likely debris ejected from the sun and moon.
Meteorites come from bodies in space that formed along with the planets and are thought to have similar compositions to Earth's layers.
Meteorites formed far outside the solar system at the same time Earth formed.
27
Dropdown
28
Drag and Drop
29
Multiple Choice
Why is Moon covered with craters, but Earth is not?
Moon has no tectonic activity.
More asteroids hit Moon than Earth
Moon is older than Earth
30
Multiple Choice
Why is Moon covered with craters, but Earth is not?
Earth's atmosphere protects Earth and weathers craters away
Moon's rocks are harder to wear away than Earth's
31
Multiple Choice
True or False: Earth, Moon, and all the other objects in the solar system (meteorites, asteroids, other planets) are all the same age since they all formed at about the same time.
True
False
32
Multiple Choice
T/F: Geologists can use radioactive dating to find the absolute age of rocks
33
Multiple Choice
34
Multiple Choice
When S-waves reach the outer core of the Earth they stop and when P-waves reach the outer core of the Earth they slow down. What is the reason for this speed change?
The outer core is a solid and P-waves don't go through solids.
The outer core is a liquid and P-waves slow down in liquids and S-waves don't go through liquids.
The outer core is made of iron and S-waves don't go through iron and P-waves always slow down in iron.
The outer core is a putty-like material and S-waves don't go through putty and P-waves slow down in putty like material.
Nebular Theory
Review for Nebular Theory Quiz
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