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The Solar System and it's Formation

The Solar System and it's Formation

Assessment

Presentation

Science

9th Grade

Hard

NGSS
HS-ESS1-4, HS-ESS1-3, MS-ESS1-1

+4

Standards-aligned

Created by

Joyce Windrow

Used 19+ times

FREE Resource

19 Slides • 22 Questions

1

The Solar System and it's Formation

Chapter 25

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2

Fill in the Blank

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3

Multiple Select

The solar system contains many objects that orbit our sun. Check off the objects that are in our solar system.

1

Sun

2

Planets and Dwarf Planets

3

Other Stars

4

Moons

5

Asteroids, Comets, Meteoroids

4

Multiple Select

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Which of these shows a Model of the Heliocentric Solar System?

1

Image on the Left

2

Image on the Right

5

Multiple Choice

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Ptolomy proposed the Geocentric (Earth Centered Model) to explain what we saw in the sky, who first created the Heliocentric Model?

1

Aristotle

2

Copernicus

3

Galileo

6

Multiple Choice

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Which person used the telescope and his observations about the phases of Venus to argue that the Heliocentric Model was correct?

1

Aristotle

2

Copernicus

3

Galileo

4

Ptolomy

7

Fill in the Blank

Type answer...

8

Multiple Choice

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Which of these has the planets in the correct order from the sun outward?

1

Pluto, Neptune, Uranus, Saturn, Jupiter, Mercury, Venus, Earth, Mars

2

Mars, Venus, Earth, Mercury, Jupiter, Saturn, Neptune, Uranus

3

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune

9

Multiple Select

Check off all the planets that are classified as Gas Giants as they are huge and composed of mostly Hydrogen and Helium.

1

Mercury

2

Jupiter

3

Saturn

4

Neptune

5

Uranus

10

Keplers Three Laws of Orbital Motion

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11

Multiple Choice

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Kepler described the orbital motion of the planets as being perfect circles.

1

True

2

False

12

Fill in the Blank

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13

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14

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15

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16

Multiple Choice

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According to Kepler's Second Law, during which section of this planets orbit would it be travelling the fastest?

1

From Section A-B

2

From Section X-Y

17

Multiple Choice

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Large rocks that mostly orbit in a "belt" between Mars and Jupiter.

1

Meteors

2

Asteroids

3

Dwarf Planets

4

Comets

18

Fill in the Blank

Type answer...

19

Dwarf Planets

  • Pluto is not alone!

  • These are just the ones that have been observed.

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20

Characteristics of a Orbits of the Dwarf Planets



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21

Multiple Select

Which characteristics of a planet does Pluto have? (check all that are true)

1

is it a celestial body in the Solar Systemthat orbits the sun?

2

is it massive enough for its own gravity to make it round?

3

Has it cleared its orbit of smaller objects?

22

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23

The Formation of our Solar System

25.5

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24

Fill in the Blank

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25

Multiple Choice

What is one hypothesis that could explain the force that may have started the collapse of our solar nebula?

1

the big bang theory

2

the shockwave from the explosion of a nearby star

3

gravity alone

26

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27

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28

Solar Nebula

  • A large thin cloud of gas and dust (range form light years to millions of light years across)

  • nebulae are made of dust and gases (mostly hydrogen and helium) which are remnants of old stars.

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29

About 5 billion years ago..

  • The solar nebula starts to contract due to the gravitational forces

  • As it contracted it started to spin

  • As the nebula shrank the spinning forces increased flattening it into a disk

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30

Fill in the Blank

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31

Fill in the Blank

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32

The Sun Forms (c)

  • after about 10 million years the density of this protostar will reach over 1,000,000 degrees

  • This is enough heat and pressure to cause nuclear fusion to begin and it becomes a real star!

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33

The Gas Giants

  •  The solar wind swept away lighter elements, such as hydrogen and helium, from the closer regions, leaving only heavy, rocky materials to create smaller terrestrial worlds.

  • But farther away, the solar winds had less impact on lighter elements, allowing them to coalesce into gas giants.

  • In this way, asteroids, comets, planets, and moons were created.

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34

Fill in the Blank

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35

Planetesimals

  • The planetesimals (c) continue colliding and growing

  • Once they become about 1 km in diameter they have significant gravitational attraction on nearby objects

  • now they start to become moonsized (d)

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36

Fill in the Blank

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37

The Solar System

Once gravity/accretion pull most of the material together the area between the planets gets clearer and we now have the Solar System we see today.

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38

Hubble Evidence of the Nebular Theory


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39

Fill in the Blank

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40

Fill in the Blank

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41

Exosolar system!

The star TYC 8998-760-1 (top center) was photographed with two giant exoplanets (arrows), the first time astronomers have directly imaged more than one planet orbiting a sunlike star. The bright spots above star TYC 8998-760-1 are other stars in the background.

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The Solar System and it's Formation

Chapter 25

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