118
Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking the next arrow at the bottom right of each slide. Click the previous arrow to go to the slide before. 2. On the menu slide (next page) you can jump around to any topic. You can return to the menu page at any time by clicking the “home” button. 3. There will be a small quiz at the end, so take your time while completing the tutorial. J. Furcron

Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Embed Size (px)

Citation preview

Page 1: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Introduction

Before we get started, let’s look at what we need to do in order to complete the tutorial:

1.You can go straight through the tutorial by clicking the next arrow at the bottom right of each slide. Click the previous arrow to go to the slide before.

2. On the menu slide (next page) you can jump around to any topic. You can return to the menu page at any time by clicking the “home” button.

3. There will be a small quiz at the end, so take your time while completing the tutorial.

J. Furcron

Page 2: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

MenuClick on the name of any topic to skip right to that section. If you prefer to continue straight through, click the next arrow at the bottom. Remember, clicking the “home”

button at any time will bring you back to this page.

Earth- Moon- Sun

Misconceptions

Scale

Earth

The Sun

Day and Night

The Seasons

The Moon

Phases of the Moon

Planets

Introduction

Mercury

Venus

Mars

Jupiter

Saturn

Uranus

Neptune

Pluto

Deep Space

Light Years

Galaxies

Other Planets

The Universe

At the End

Key Vocabulary

Quiz Time

References

J. Furcron

Page 3: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

What is a Misconception?

Have you ever believed that something is correct only to find out later that it is actually wrong? That is called a misconception.

Everyone has a misconception about something. Misconceptions are often very common beliefs. Many people don’t even know that their misconceptions even exist.

Astronomy may have more misconceptions than any other field of science.

J. Furcron

Page 4: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Why is the Sky Blue?

Why do you think that the sky is blue? Many people believe that the sky is blue because the blue from water is reflected up into the sky.

This is not true and is an example of a misconception.

The sky is actually blue because of sunlight. When it passes through our atmosphere, it creates a blue color.

J. Furcron

Page 5: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Fixing Misconceptions

When you hear something that is different from your misconception, does that automatically fix it? Sometimes it might, but normally it will not.

It can actually take hearing and seeing new information seven times in order to correct the misconception.

People that have misconceptions must work hard to overcome them. Unfortunately, astronomy is filled with misconceptions.

Do you know why this diagram of Earth’s orbit around the sun is a misconception?

J. Furcron

Page 6: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

What is Scale?

With scale, we are not talking about the kind that you weigh yourself with. Think back to geography and scale should start to sound familiar.

A map scale simply helps you to understand how large or far something is in real life. Take a look at the scale in the picture. The scale is 1inch = 100 miles.

So, that means that every inch on the map is 100 miles in real life.

J. Furcron

Page 7: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Scale in the Solar System

Our solar system isn’t quite like a map you are used to using. It is much larger and things are not always in the same place. The distances between places require huge measurements.

The size and distances are almost too large to completely understand. That is why we need a scale to help give us an idea of how large and far the solar system is.

Let’s take a look at what our normal scale in the solar system will look like.

J. Furcron

Earth

Sun

In this scale, 1mm =1,000 miles

Page 8: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Example of Scale

When using a map, the scale may often be 1 inch = 100 miles. However with the solar system, that scale is much too small.

The scale that we will be using the most (but not all the time) will be the scale of 1inch = 1,000 miles.

So for example, the earth is about 8,000 miles in diameter in real life, so according to our scale, how large would the earth be? If you said 8 inches, you are correct. If 1 inch = 1,000 miles, then 8 inches = 8,000 miles.

8 inch model of the Earth

J. Furcron

Page 9: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Earth

From space, some say that earth looks like a blue marble. The combination of water, breathable air, and the perfect temperature make Earth unlike any other planet in our solar system.

While there is still much to be discovered, Earth is the only known planet in the universe that is able to sustain life.

J. Furcron

Page 10: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Earth in the Solar System

Earth is the third planet from the sun. A HUGE misconception is that the earth has an oval-shaped orbit around the sun. That is not true at all. Earth actually has a circular orbit around the sun.

Earth is the perfect distance from the sun. It’s not too hot or too cold. The distance that we are from the sun is actually referred to as the “Goldilocks’ Zone”.

Earth has a diameter of about 8,000 miles.

8,000 miles

J. Furcron

Page 11: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Small is the Earth?

When we often think of the earth, we view it as a huge place. While Earth is very large, it is actually extremely tiny when we look at the big picture.

The next few slides will be taking you on a journey away from Earth. This will help to show just how small we really are.

The first picture shows the earth from our moon. Here, the distance is about 240,000 miles.

J. Furcron

Page 12: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Small is the Earth?

This next image shows how the Earth looks from Saturn. As you can see, the earth looks no larger than just a small dot. Without the arrow, you probably wouldn’t have even realized that you were looking at your home planet.

This is about 800,000,000 miles (that’s 800 million) miles away from Earth.

J. Furcron

Page 13: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Small is the Earth?

This next image shows Earth in comparison to our entire galaxy (we will discuss galaxies later). Although this is a computer generated image, it is still generally accurate.

From this far away, Earth, the other planets, and even the sun are impossible to see.

J. Furcron

Page 14: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Small is the Earth?

Do you know what this last picture is? It looks like many stars, but it is not. These are all galaxies! In the last picture, we saw our own galaxy and couldn’t even see our sun. Here, we have billions of galaxies and ours is just a tiny speck.

Each galaxy has billions of stars and potentially billions of planets. In the grand scheme of things, Earth is invisible.

J. Furcron

Page 15: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

The SunThe sun is the center of our solar system. The planets are all caught in the sun’s gravitational pull.

Solar means sun, so a solar system is a ‘system of the sun’. Without the sun’s gravity, all of the planets (including Earth) would be floating randomly throughout space.

Most importantly, without the sun, there would be no life on Earth.

J. Furcron

Page 16: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Large is the Sun?The sun is about 870,000 miles in diameter. If you remember, the Earth is only about 8,000 miles in diameter. Without a scale, it is hard to realize just how large the sun actually is.

Let’s use the scale we discussed before, 1in. =1,000 miles. Here the earth has a diameter of 8 inches. In this scale, the sun has a diameter of over 72 feet!

Let’s make a smaller scale; this time 1millimeter = 1,000 miles. The earth now has a diameter of 8mm (that’s not even 1 cm.), while the sun has a diameter of 87cm. The image to the right shows the size comparison using this scale.

J. Furcron

Page 17: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Does the Sun Compare to Other Stars?

The sun is by far the closest star to the earth. Other stars are so far away that is it extremely difficult to really tell just how massive they are.

While we saw in our last slide that our sun is huge, in reality it is only an average sized star. Some stars are much smaller than our sun. However, there are also stars that make our sun look tiny (see picture to the right).

Our sun is actually very small when compared to these larger stars.

J. Furcron

Page 18: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Does the Sun Compare to Other Stars?

But how does the Sun compare to the largest stars? Take a look for yourself.

In this picture, the Sun is basically invisible.

Compared to Earth, the Sun is massive. Compare the Sun to other stars and…the picture to the left says it all.

J. Furcron

Compared to the largest stars, the Sun is basically invisible.

Page 19: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Far is the Earth from the Sun?

The earth is about 93 million (93,000,000) miles away from the sun. It is so far that is takes the light from the sun 8 minutes to reach Earth (we will discuss light speed later)!

Let’s use out scale to help us see just how far 93 million miles really is. For this, we need to use our 1mm = 1,000 miles scale. Remember, the earth is 8mm and the sun is 87 cm. In this scale, they are about 93 meters apart. The picture to the right shows this distance. (The light pole represents the correct distance).

Location of the sun

Earth

J. Furcron

Page 20: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Why Do We Have Day and Night?

We have day and night on Earth because the earth rotates. Rotation means that the earth spins on its axis in place. It takes about 24 hours for the earth to complete one rotation.

Half of the earth is always light and half is always dark. The light side has daytime and it is night on the dark side.

J. Furcron

Page 21: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Why Do We Have Seasons?

The Earth and the sun work together to give us seasons. The most common misconception is that the earth is closer to the sun in the summer and farther away during the winter.

This is not correct at all. In reality, we are actually closer to the sun during the winter and farther away during the summer.

This is NOT how we have seasons

J. Furcron

Page 22: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Earth’s Tilt

The main reason that we have seasons is due to the tilt of the earth. This means that poles of the earth are not straight up and down, but are slightly titled to the side instead.

This means that half of the earth is always facing the sun a little bit more than the other half.

Northern Hemisphere

Southern Hemisphere

J. Furcron

Page 23: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How does the Tilt Cause Seasons?

Because of the tilt, different parts of the earth face towards the sun at different times of the year.

During our summer, the northern hemisphere is tilted towards the sun and is receiving direct rays of sunlight. During our summer, the southern hemisphere is actually having their winter because they are tilted away and are receiving indirect rays.

N

S

Direct rays

Northern H.=summerSouthern H.=winter

J. Furcron

Page 24: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How does the Tilt Cause Seasons?

During our winter, the northern hemisphere is titled away from the sun and therefore receives indirect rays. The southern hemisphere however is now titled towards the sun.

When we are having winter, the southern hemisphere is enjoying summer.

NS

Direct rays

Northern H. = winterSouthern H. = summer

J. Furcron

Page 25: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Earth’s Revolution

The other factor that causes seasons is the earth’s revolution around the sun. Revolution simply means that Earth orbits or travels around the sun. The orbit is like a circle, NOT like an oval.

The revolution allows for a different end of the earth to be titled towards the sun at different times of the year.

A complete revolution takes one year.

J. Furcron

Page 26: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Earth-Sun Relationship

Let’s review some key ideas with the earth and the sun:

We have day and night because the earth rotates. Half of the earth is always light, while half is always dark.

We have seasons because of the earth’s tilt and revolution around the sun. The hemisphere tilted towards the sun has summer, while the hemisphere tilted away has winter.

J. Furcron

Page 27: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

The Moon

The moon is a natural satellite that orbits the earth. A satellite is an object that orbits another. Just like how the earth revolves around the sun, the moon revolves around the earth. The moon is caught in the gravitational pull of the earth.

The moon has an effect on the earth too. The gravitational pull from the moon gives us tides on earth.

J. Furcron

Page 28: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Large is the Moon?

In the sky at night, the moon looks very large, but just how large is it? The moon has a diameter of about 2,000 miles. In order to compare it to earth, let’s use our scale of

1 inch = 1,000 miles.

Remember, the earth is a sphere 8 inches in diameter using this scale. That means that the moon would be 2 inches.

Moon

Earth

2 inches

8 inches

J. Furcron

Page 29: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Far is the Moon from the Earth?

When we see the moon, it is very difficult to tell just how far away it really is from earth. The actual distance is 240,000 miles. Let’s use our scale to get a better idea of that distance.

Just like the last slide, we are still using the 1 in. = 1,000 miles scale. So the 8 inch earth and the 2 inch moon would be 240 inches apart, or 20 feet! The picture to the right shows the distance using our scale.

Earth Moon

J. Furcron

Page 30: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Phases of the Moon

A huge misconception is that the earth’s shadow on the moon is the cause of the moon phases. This is NOT true at all.

The actual cause of the moon phases is how much of the light side of the moon we can see from earth. Just like the earth, half of the moon is always light and half of it is dark.

J. Furcron

Page 31: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

New Moon

The first phase in the moon cycle is called the New Moon. At this part of the of the cycle, the moon is between the earth and the sun.

Because the entire lighted side is facing away from Earth, the moon is not visible during this phase.

J. Furcron

Page 32: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Waxing Crescent

The moon phases will always go right to left. The waxing crescent shows the very right side of the moon lit up. “Waxing” phases will always mean that the moon is gaining light.

As you can see by this image, only a very small portion of the moon is visible from Earth.

J. Furcron

Page 33: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

First Quarter

The next phase in the cycle is the First Quarter. Here, the right half of the moon is lit and visible from Earth.

Notice the position of the moon orbiting Earth is changing. This allows for more of the moon to be visible from the dark side of the Earth.

J. Furcron

Page 34: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Waxing Gibbous

The next phase in the cycle is the Waxing Gibbous. The waxing gibbous is almost a full moon, but not quite yet. The majority of the moon is lit, except for a small portion on the left side.

Notice so far that the moon has been gradually getting lighter from the right to the left.

Also, remember that waxing means more and more of the moon is becoming visible from Earth.

J. Furcron

Page 35: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Full Moon

The Full Moon is probably the most recognizable moon phase. Here, the complete lighted side of the moon is visible from Earth. The moon is lined up directly behind the Earth.

Remember, even though the moon is full, we can still only see half of the moon. The dark side is not visible from Earth.

J. Furcron

Page 36: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Waning Gibbous

The Waning Gibbous comes after the full moon. Here, only a slight part of the moon is not visible. This time however, it is the right side that is getting darker.

Where waxing meant that the moon is getting lighter, waning refers to the moon now getting darker.

Remember, the phases always work right to left. Now the moon will be getting darker starting on the right side and moving left.

J. Furcron

Page 37: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Third Quarter

The Third Quarter is a half moon, but now with the left side visible from earth and the right side is now dark.

Notice how the moon is not getting darker from the right side moving left. The phases are essentially now going backwards from earlier.

J. Furcron

Page 38: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Waning Crescent

The Waning Crescent is the final phase before the process starts over again with the new moon. Here, only a small sliver of the moon is visible on the left side of the moon. The complete cycle is just about completed.

It takes 27 days for the entire moon cycle to occur.

J. Furcron

Page 39: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Moon Review

Let’s do a quick review of the moon:

The moon is about 2,000 miles is diameter and 240,000 miles from Earth.

Half of the moon is always lit by the sun.

Phases are caused by the amount of the lighted half of the moon that we can see from Earth.

Phases of the moon always for right to left when getting lighter (waxing) and getting darker (waning). The entire process takes 27 days.

J. Furcron

Page 40: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Moon Review

For one final review, click on the link at the bottom to review your knowledge of the moon phases.

This site is a great way to either learn about the phases or to simply review and refresh your memory.

Moon Phase Review

J. Furcron

Page 41: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

The Planets

Nine planets (including Earth and Pluto) orbit or revolve around the sun. This makes up most of our solar system. Some of the planets are similar to each other, while others are quite different. All of them are very different from Earth in a number of ways.

We will be looking at all of the planets, starting with the closest to the sun (Mercury) and working all the way back to the farthest (Pluto).

J. Furcron

Page 42: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Mercury

Mercury is the closest planet to the sun. It orbits at only 36 million miles away (remember the Earth orbits at around 93 million miles).

The diameter of Mercury is about 3,000 miles, only one thousand miles larger than our moon.

Mercury completes a revolution around the sun in only 88 days, but it also takes Mercury 59 days to make one rotation. However, because the orbit around the sun is so short, it actually causes a day to last for 176 days!

J. Furcron

Page 43: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Mercury

Mercury is so close to the sun that it is not possible for it to even have an atmosphere (the atmosphere would just burn away). Because of this, the temperature on Mercury is a little crazy.

During the day (side facing the sun) it is about 662 degrees F., However, the temperature at night (facing away from the sun) averages -274 degrees F. because there is no atmosphere to hold in the heat.

J. Furcron

Page 44: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Venus

Venus has been called Earth’s sister planet because it is very similar in size. Size however, is where the similarities end.

The diameter of Venus is just slightly smaller than Earth at 7,500 miles. Venus is also about 67 million miles away from the sun. It takes the planet 225 days to make a revolution around the sun and 243 days to make one rotation…that’s a long day.

J. Furcron

Page 45: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Venus

Mercury has no atmosphere to hold in heat, but Venus has the complete opposite problem. The atmosphere on Venus is so thick, that no heat at all can escape. Because of this, the temperature averages 900 degrees F. This makes it the hottest place in the solar system other than the sun. (The picture to the left show what Venus looks like under the clouds).

At times during the year, Venus can be easily seen in the night sky. Aside from the moon, Venus is the brightest light in the sky.

J. Furcron

Page 46: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Mars

Mars is often called the “Red Planet” due to its red color.

Mars has a diameter of over 4,200 miles, a little larger than half the Earth. Mars is about 142 million miles from the sun.

A day on Mars is a little over 24 hours, almost the same as on Earth. It takes Mars 687 days to make a revolution around the sun.

J. Furcron

Page 47: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Mars

The surface temperature (soil) on Mars is a surprising 73 degrees F. in some locations. The air temperature rarely reaches 32 degrees. At the poles, the temperature becomes much colder.

Mars is the next major destination to travel to in the solar system. Within your lifetime, people may actually walk on the Red Planet.

J. Furcron

Page 48: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Jupiter

Jupiter is the largest planet in our solar system. With a diameter of nearly 90,000 miles, it makes Earth seem very small.

On average, Jupiter is about 484 million miles away from the sun. A year on Jupiter lasts for almost 12 earth years. However, a day lasts less than 10 hours!

J. Furcron

Page 49: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Jupiter

Probably the most notable feature on Jupiter is the Red Spot. The Red Spot (picture to the right) is an ongoing storm that is 3x larger than earth! Winds in this storm can reach up to 250 mph.

The average temperature in the clouds of Jupiter is about -238 degrees.

Jupiter has at least 66 moons orbiting the planet. Chances are that there are other moons that just have not been discovered yet.

J. Furcron

Page 50: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Saturn

Saturn is the second largest planet in the solar system with a diameter of almost 75,000 miles. Saturn is an average distance of 887 million miles from the sun.

It takes Saturn almost 30 years to make one revolution around the sun. Similar to Jupiter, Saturn has a short rotation time of only about 11 hours.

J. Furcron

Page 51: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Saturn

Saturn is most noted for its massive and stunning rings (picture to the right). The rings however are not solid. They are actually formed from a large collection of dust, rocks, and ice.

Also like Jupiter, Saturn is called a gas giant. The average temperature in the clouds of Saturn is -292 degrees.

Saturn has 62 known moons. One of the moons, Titan, is actually larger than Mars!

J. Furcron

Page 52: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Uranus

Uranus comes next in our journey to the planets. Although it is much smaller than Saturn and Jupiter, it is still much larger than Earth with a diameter of about 32,400 miles.

Uranus averages a distance of 1.78 billion (that’s 1,780,000,000) miles from the sun. It takes about 84 years to make one revolution around the sun, and only about 17 hours to complete a rotation.

J. Furcron

Page 53: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Uranus

The feature of Uranus that really stands out is its tilt. If you notice in the picture, Uranus has a 90 degree tilt so it is actually sideways. The exact reason for the extreme tilt is unknown, but scientists believe that it could have been the result of a major collision.

The average cloud temperature on Uranus is about -346 degrees. There are 27 known moons that orbit Uranus.

J. Furcron

Page 54: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Neptune

In size, Neptune is almost identical to Uranus. Neptune has a diameter of about 30,800 miles.

On average, Neptune is about 2.78 billion miles away from the sun. It takes Neptune almost 165 years to make a complete revolution around the sun. A day though, only lasts for a little over 16 hours.

J. Furcron

Page 55: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Neptune

Like Jupiter, Neptune also has very powerful storms. Some of the winds (like in the former Dark Spot) can reach speeds over 1,000 mph!

The cloud temperature on Neptune averages around -346 degrees.

At certain times, Neptune is actually farther away from the sun than Pluto. The path of the orbits allows for this to occur.

J. Furcron

Page 56: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Pluto

Much is not known about Pluto. It has a diameter less than our own moon at about 1,400 miles.

It takes Pluto 248 years to make a revolution around the sun, and over 6 days to make a rotation.

Pluto was officially downgraded to a dwarf planet in 2006. Pluto even has its own moon named Charon (both pictured to the right).

J. Furcron

Page 57: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Planet Review

From this section, these are some of the key ideas to remember:•All planets revolve around the sun. In other words, this is their path/orbit in space.

•Rotation is when a planet spins on its axis. This causes day and night.

•The larger planets are primarily gas giants. The smaller planets (and moons) are rocky.

•Planets do not give off their own light. They just reflect light from the sun.

J. Furcron

Page 58: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

What is a Light Year?

A light year is simply a way to measure distance in space. It refers to the amount of distance that light can travel in one year.

Space is so large that using miles or kilometers would just be too small.

J. Furcron

Page 59: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

How Far is a Light Year?

A light years is the distance that light travels in the time of one year.

Light travels at an amazing speed of 186,000 miles per second! That means that a beam of light could travel around the equator of the Earth 7 times in one second.

In one year, light can travel 5.8 trillion (5,800,000,000,000) miles. A distance that large is almost too much to truly grasp.

J. Furcron

Page 60: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

What Does a Light Year Look Like?

Let’s look at an example of deep space. This picture is of a galaxy named the Sombrero Galaxy..

Traveling at 186,000 miles per second or 5.8 trillion miles a year, how long do you think it would take light to get from one end to the other?

J. Furcron

Page 61: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Light Year Distances

These objects in deep space are much larger than they appear.

If we were to travel from one end of this galaxy to the other, it would take 50,000 years of light travel to go complete the trip. Not to mention that this galaxy is only about 28 million light years away from Earth!

This is just a glimpse of how massive the universe is.

50,000 light years

J. Furcron

Page 62: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Looking in the Past

Every time that you look at the stars at night, you are actually looking back into the past.

Let’s say a star that you see is 70 light years away from Earth. That means that it takes the light from the star 70 years to actually reach Earth. So, the light from that star is actually how it looked 70 years ago! Other stars are hundreds of light years away.

Confusing? Yes, I know. Let’s take a look at a much closer example.

J. Furcron

Page 63: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Light Minutes from the Sun

The sun is actually about 8 light minutes from Earth. That means that it takes the light from the sun 8 minutes to actually reach Earth.

For example, if the sun were to suddenly go dark this moment, we would not notice on Earth for 8 minutes.

So when you see the sun, you are really seeing the sun how it was 8 minutes ago.

J. Furcron

Page 64: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Our Galaxy

We live in the Milky Way Galaxy. Our entire solar system is a part of this galaxy.

A galaxy is a very large collection of stars and other bodies in space.

Our solar system only makes up a very small part of the galaxy. There are billions of other stars and possible planets.

J. Furcron

Page 65: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Other Galaxies

Our galaxy is only one of billions of other galaxies. Each galaxy has billions of stars and probably billions of planets.

Although each galaxy is massive, they only make up a very small section of the entire universe.

J. Furcron

Page 66: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Other Planets

As said before, each galaxy contains billions of stars and therefore billions of planets. Have you ever wondered what those other planets could be like?

Here is one example of another planet in our own galaxy, Wasp-17. Although the picture is just a created image, this planet is unlike any in our solar system. It is slowly being drawn into its own sun.

J. Furcron

Page 67: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Other Planets

Here is another example of another planet discovered named Kepler.-22b. What makes this planet so different from others is that it is in the “Goldilocks Zone”. Scientists believe that the surface temperature of this planet could be around 72 degrees F.

Is there life on this planet? Nobody has that answer. This planet is 600 light years away from Earth.

J. Furcron

Page 68: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

The Universe

In simple terms, the universe contains absolutely everything. Every planet, star, solar system, and galaxy are part of the universe.

The universe it simply HUGE! There is no number large enough to give its size. The picture to the right is not of stars, but rather entire galaxies! This section of the universe only makes up a very small portion.

J. Furcron

Page 69: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

The Universe

As we saw, the universe contains everything. Think about it…there are billions of galaxies, with billions of stars, with billions of planets. If we look at the big picture, the Earth is a microscopic speck.

Although we have not found any other planets with life, do you think that it is possible? In my opinion, the universe is just too massive just for us.

J. Furcron

Page 70: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Key Vocabulary

Misconception: a belief someone has that is incorrect

Scale: a smaller version used to represent actual distance and size

Star: a large body in space that gives off heat and light

Planet: a body that orbits a star, but does not give off its own light

Moon: a natural satellite that orbits a planet

Gravity: the force that keeps planets and moons in orbit

Rotation: a planet spinning on its axis; the reason that we have day and night

J. Furcron

Page 71: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Key Vocabulary

Revolution: a planet traveling around the sun, or a moon traveling around a planet

Tilt: responsible for the Earth’s seasons along with revolution; Earth is not straight up and down, but rather slightly on its side

Moon Phases: the part of the light side of the moon that we can see from Earth; takes about a month to complete the entire cycle

Light Year: Distance that light can travel in one year

Galaxy: a large collection of stars and planets

Universe: everything in space; most of the universe contains nothing

J. Furcron

Page 72: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Quiz Time

1. About how far is Earth from the sun?

a) 240,000 miles c) 3 light years

b) 93 million miles d) 8,000 miles

2. A natural satellite of Earth is:

a) the sun c) the moon

b) the planetsd) the atmosphere

3. What is rotation?

a) traveling around the sun c) moon phases

b) Earth’s tilt d) spinning on its axis

4. What is revolution?

a) Traveling around the sun c) scale

b) Earth’s tiltd) spinning on

axis

5. Why do we have seasons?

a) rotation c) tilt

b) revolution d) tilt and revolution

6. A way to measure distance in space is:

a) galaxy c) light year

b) nebula d) cosmos

Click on the best answer for each question

J. Furcron

Page 73: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Quiz Time

7. What is the solar system?

a) everything in the universe c) a galaxy

b) Everything revolving d) planet and around a star moon

8. The universe mostly contains:

a) nothing c) stars

b) galaxies d) nebulas

9. Our galaxy is named:

a) Andromeda c) Milky Way

b) P.S 90 d) Universe

10. What causes moon phases?

a) the amount of the light side we see from Earth

b) the Earth’s shadow blocking light on the moon

c) the moon actually changes shape

d) the sun blocks part of the moon from our view

11. What body gives off light and heat?

a) Planet c) Star

b) Moon d) Titan

Click on the best answer for each question

J. Furcron

Page 74: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

The Earth is about 93 million miles away from the sun.

Hubblesite.org

J. Furcron

Page 75: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

240,000 miles refers to the distance that the Earth is from the moon.

J. Furcron

Page 76: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

3 light years is not the correct distance. This amount of distance would end up being over 16 trillion miles. In reality,

the Earth is 8 light minutes from the sun.

J. Furcron

Page 77: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

8,000 miles refers to the diameter of the Earth.

J. Furcron

Page 78: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

The moon is a natural satellite of the Earth. The moon is a satellite because it orbits (or travels) around Earth.

Hubblesite.org

J. Furcron

Page 79: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The sun is not a satellite of the Earth. Actually, the Earth is a satellite of the sun. Remember, a satellite is the one orbiting

another body in space.

J. Furcron

Page 80: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The planets are not satellites of Earth. All the planets are actually satellites of the sun. A satellite is the one that orbits

another body in space.

J. Furcron

Page 81: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The atmosphere is not a satellite of the Earth. The atmosphere is the layer of gases that surrounds a planet.

J. Furcron

Page 82: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

Rotation means a planet or other body spinning on its axis. On Earth, this is what helps to give us day and night.

Hubblesite.org

J. Furcron

Page 83: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Earth traveling around the sun refers to revolution.

J. Furcron

Page 84: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The tilt of the Earth is not rotation. While the Earth is tilted, is has nothing to do with rotation.

J. Furcron

Page 85: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The moon orbiting the Earth is not rotation. In this case, the moon is revolving around the Earth.

J. Furcron

Page 86: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

Revolution means that the Earth is orbiting (or traveling) around the sun. All the planets revolve around the sun.

Hubblesite.org

J. Furcron

Page 87: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The tilt of the Earth is not called revolution. The tilt and revolution do work together though to help something else

happen.

J. Furcron

Page 88: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Revolution is not a form of scale. Scale is what helps us see what actual distance and size look like in a smaller way.

J. Furcron

Page 89: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Spinning on its axis is not revolution. When the Earth spins, it is referred to as rotation.

J. Furcron

Page 90: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

We have seasons because of both the tilt of the Earth and the revolution around the sun. Without both, our weather would

remain pretty much the same.

Hubblesite.org

J. Furcron

Page 91: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Rotation does not cause seasons. Rotation helps to give us day and night.

J. Furcron

Page 92: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Revolution is a part of the reason that we have seasons, but it is not the only reason.

J. Furcron

Page 93: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The Earth’s tilt is part of the reason that we have seasons, but it is not the only reason.

J. Furcron

Page 94: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

A light year is a way to measure distance in space. Other units of measurement are just too small.

Hubblesite.org

J. Furcron

Page 95: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A galaxy is a large collection of stars and planets. It is not a unit of measurement in space.

J. Furcron

Page 96: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A nebula is created during the death of a star. It is not a unit of measurement in space.

J. Furcron

Page 97: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Cosmos is a term that can be used to define space.

J. Furcron

Page 98: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

A solar system involves everything revolving around a star. The sun is the center of our solar system.

Hubblesite.org

J. Furcron

Page 99: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A solar system does not contain everything in the universe. A solar system is much much smaller.

J. Furcron

Page 100: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A galaxy is not a solar system. Galaxies actually contain billions of solar systems.

J. Furcron

Page 101: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A planet and a moon are a part of a solar system, but not the entire thing.

J. Furcron

Page 102: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

The universe mostly contains nothing. Although stars and galaxies are massive, they do not take up a lot of space in the

universe.

Hubblesite.org

J. Furcron

Page 103: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

There are billions of galaxies in the universe, but they don’t take up too much space.

J. Furcron

Page 104: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

There are an infinite amount of stars in all the galaxies, but they don’t take up too much space.

J. Furcron

Page 105: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

There are billions of nebulas in the universe, but they do not take up too much space.

J. Furcron

Page 106: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

Our galaxy is named the Milky Way Galaxy.

Hubblesite.org

J. Furcron

Page 107: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Andromeda is a name for a nearby galaxy, but not ours.

J. Furcron

Page 108: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

P.S. 90 is not the name of our galaxy.

J. Furcron

Page 109: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The universe is not the name of our galaxy. Our galaxy is part of the universe.

J. Furcron

Page 110: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

The moon has phases because the lighted amount of the moon we see from Earth changes.

Hubblesite.org

J. Furcron

Page 111: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The Earth’s shadow does not block light from the sun on the moon. This is a huge misconception. When this does

happen, we see a lunar eclipse.

J. Furcron

Page 112: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The moon never changes its actual shape. The only thing that changes is the part of the moon we are able to see.

J. Furcron

Page 113: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The sun does not block the moon from our view. The sun is 93 million miles away, while the moon is only 240,000 miles

away from Earth.

J. Furcron

Page 114: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Correct!

A star gives off its own heat and light. While other planets and moons may appear to have light, they are just reflecting

the light of the star (sun).

Hubblesite.org

J. Furcron

Page 115: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

The moon does not give off its own light. The light we see from the moon is reflected light from another source.

J. Furcron

Page 116: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

A planet does not give off its own light. Some planets appear to be very bright in the night sky, but they are just reflecting

light from another source.

J. Furcron

Page 117: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

Incorrect

Titan is a moon of Saturn and it does not give off its own light.

J. Furcron

Page 118: Introduction Before we get started, let’s look at what we need to do in order to complete the tutorial: 1.You can go straight through the tutorial by clicking

ReferencesAstronomy Picture of the Day. (2006). Retrieved March 11, 2012 from: apod.nasa.gov/.../0609/earth2_cassini_big.jpg

Astro Pix. Retrieved March 11, 2012 from: www.astropix.com/HTML/D_SUM_S/MILKYWAY.HTM

Crystal Links. Retrieved March 11, 2012 from: http://www.crystalinks.com/mercury.html

Geography For Kids. Retrieved March 25, 2012 from: http://www.kidsgeo.com/geography-for-kids/0027-map-key-and-scale.php

Geography 4 Kids. Retrieved March 18, 2012 from: http://www.geography4kids.com/extras/dtop_space/moonearth.html

Hubble Site. Retrieved March 11, 2012 from: http://hubblesite.org/gallery/

Info Barrel. Retrieved March 18, 2012 from: http://www.infobarrel.com/8_phases_of_the_moon

LaCapria, K. (2009). The inquisitir Retrieved March 11, 2012 from: http://www.inquisitr.com/33198/weird-new-planet-discovered-named-wasp-17/

Library Think Quest. Retrieved March 11, 2012 from: http://library.thinkquest.org/06aug/02405/sun.html

Mail Colonial. Retrieved March 18, 2012 from: http://mail.colonial.net/~hkaiter/solarsysteminfo.html

Mapas. Retrieved March 11, 2012 from: http://mapas.owje.com/maps/10593_the-earth-moon-and-sun.html

McNab, D., & Younger, J. (1999). The planets. New Haven: Yale University Press

National Geographic. Retrieved March 25, 2012 from: http://science.nationalgeographic.com/science/photos/galaxies-gallery/

NASA. Retrieved March 11, 2012 from: http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html

Our Earth. Retrieved March 25, 2012 from: http://www.our-earth.net/Planets-Orbits.asp

Potter, N. (2011). Retrieved March 11, 2012 from:  http://abcnews.go.com/Technology/planet-found-600-light-years-nasa-kepler-telescope/story?id=15094976

Wikiversity. Retrieved March 18, 2012 from: http://en.wikiversity.org/wiki/Solar_System/Earth/Solar_System_overview, 21 February 2010,

J. Furcron