Planetary Systems Unit Readings and Assignments Name ___________________ Table of Contents Part 1: Earth in Space Pages 2-4 Homework Assignment #1 Page 3 Homework Assignment #2 Page 4 Part 2: The Earth, Moon, and Sun System Pages 5-11 Homework Assignment #3 Page 6 Homework Assignment #4 Page 9 Homework Assignment #5 Page 11 Part 3: The Solar System Page 12-?? Homework Assignment #6 Page 12 Homework Assignment #7 Page 13 Homework Assignment #8 Page 15 1 Part 1: Earth in Space Day and Night Day/Night are caused by the rotation of the Earth. When the Sun is shining on one side of the Earth, that side is in daylight. The side away from the Sun is experiencing night. As the Earth rotates counterclockwise, the Sun rises in the eastern sky and sets in the western sky. Planets and stars also rise and set in the night sky is due to the Earth’s rotation. At any given time, half of the Earth is in day and half in night. A big misconception among students is that the moon is always up during night. This is not true, as you will learn later in this unit. As a certain place on Earth is entering the Sun’s light, we call that sunrise. When that place is leaving the Sun’s light, we call it sunset. When there are equal amounts of light on either side (as one would see looking at Earth from space), it is referred to as noon. Opposite of noon is midnight, when the location on Earth we are referencing is exactly halfway between sunset and sunrise. However, depending where you are on Earth, you may experience different amounts of sunlight due to the tilt of the earth’s axis. Seasons on Earth Seasons are caused by two factors: Earth’s tilted axis (23.5 degrees) and the fact it revolves around the Sun. This causes the Earth to be tilted towards and away from the Sun during the summer and winter months. Because of this tilt, two factors come into play in heating the Earth’s surface. First, and most importantly, in the summer radiant energy (heat and light) from the Sun hits the Earth at a more direct angle causing the energy to be more concentrated in a given area. 2 Secondly, areas that are experiencing summer receive the energy for a longer period of time due to increased day length. These two factors cause mid-latitude and Polar Regions of our planet to experience energy variations over a 12 month period. While the equatorial regions also receive energy variations, the Sun’s energy hits these regions at a relatively direct angle all year long causing it to experience warmer temperatures throughout the entire year. Also, it should be noted that the Northern and Southern Hemisphere experience seasons that are opposite to each other. When the Northern Hemisphere is tilted towards the Sun and experiencing summer, the Southern Hemisphere is tilted away from the Sun and experiencing winter. The opposite is true six months later. The spring/fall relationships have a similar converse relationship. Homework Assignment #1 Label the Northern and Southern Hemispheres and what seasons they are experiencing. The axis and equator are drawn in for your convenience Northern Hemisphere Season: ____________________________ Southern Hemisphere Season: ____________________________ Explain why you chose those seasons… _________________________________________________________________ _________________________________________________________________ 3 Light Concentration and Seasons Only latitudes between the Tropic of Cancer and Tropic of Capricorn can receive direct rays. The maximum angle of insolation is 90 degrees. As Latitude increases, the angle of insolation decreases. The poles are at about 90 degrees North and South. The maximum angle of insolation, maximum duration, and maximum intensity occur during the summer. From morning to noon, the angle of insolation increases. The angle of insolation decreases from noon to evening. As the Sun moves higher in the sky, the length of the shadow decreases, and as the Sun moves lower in the sky, the length of shadow increases, causing warmer temperatures when the sun is at its mid-point in the sky. Think of it this way: if someone were to throw a ball at you and hit you directly, you would receive more of the ball’s energy than if the ball deflected off you at an angle. This is the same as far as light hitting you at an angle of insolation of 90 degrees (direct) as opposed to an angle of insolation of 60 or 30 degrees. In general, the mornings are cooler and as the Sun’s ray become more direct during the day and the temperature increases. As the Sun sets, temperatures usually will fall. When there is a surplus of heat energy, the temperatures go up. When there is a deficit of heat energy, the temperatures go down. Maximum temperatures never occur at the time of the maximum angle of insolation. This is because a surplus occurs from June to August (in northern hemisphere) of heat energy and the temperatures go up. From December to March, there is a deficit of heat energy, so the temperatures go down. Homework Assignment #2 Draw the sun at three different angles of insolation: 30, 60, and 90 degrees. 4 Part 2: The Earth, Moon, and Sun System What is Gravity? Many years ago a young scientist sat beneath an apple tree and an apple fell on his head. This young person was named Isaac Newton and this event would shape the rest of his scientific career. He wondered why the apple fell and if this force, called gravity, affected other objects such as the planets. Gravity is one of the four fundamental forces in our universe. It is an attractive (pulling) force between objects, and the objects can exert a gravity force on one another without even touching. It is for this reason that gravity is sometimes called the invisible force. The amount of force between the objects depends on the masses of the objects and the distance between them. If the mass increases, so does the force of gravity. If the distance between the objects increases, the force of gravity decreases; but the force of gravity never goes to zero. All objects exert their force of gravity (we could even calculate your own personal “gravity force” if we wished), but in most cases, objects are too small to really concern ourselves with their affects. The force involves two objects and will change size based upon the characteristics of the second object. This is not the case with large objects such as planets, stars and asteroids. What Newton discovered is that the force of gravity was universal-it behaves the same way everywhere in the universe. The Sun and the planets have a gravitational pull on each other, but because the Sun is so much more massive, its gravity dominates the solar system and is the reason why the planets orbit the Sun, not the other way around. The Earth’s gravity is responsible for keeping our Moon in orbit around our planet. 5 Gravity and Planets – Why are most space objects spherical? On Earth, we typically say that gravity pulls things straight downward, but the truth is that gravity actually pulls toward the center of the Earth. If you look at a globe, vertically downward in Delaware is not the same direction as vertically downward in Hawaii. So, when talking about the force of gravity on a global or astronomical scale, it would be more accurate to say that gravity acts inward, towards the Earth’s center. When our solar system was forming, there were many small pieces of gas and dust, each having their own very small amount of gravity. As these small pieces started to stick together, the combined (now larger and more massive) object increased its gravity and pulled more and more pieces together from all directions. This caused the formation of objects in a spherical shape. Homework Assignment #3 Draw a picture to represent gravity. Do not use any words. 6 Defining Tides A tide is the distortion of the shape of one object (Earth) produced by the gravitational pull of another nearby object (Moon and Sun). The Sun is the more massive object and it would appear that it would influence tides on Earth more so than the Moon, but the Moon is much more influential in tidal action because it is so much closer to the Earth than the Sun. Even though the Sun exerts a greater gravitational force on the Earth, its pull is nearly constant over the diameter of the planet. The Moon’s gravitational pull, on the other hand, varies across the diameter of our planet. It is this variation in the strength of the Moon’s gravity that influences tides. Gravity and Tides The Moon does not simply revolve around the Earth, both the Earth and the Moon are in motion together and therefore require forces to keep them moving in this circular pattern. It is the force of gravity that makes these two objects move this way and since they are locked together by the forces of gravity that they exert on one another, they are commonly referred to as the Earth-Moon system. Remember that gravity weakens with distance, so the side of the Earth that is closest to the Moon will experience the greatest force of gravity and the side farthest from the Moon will experience the smallest force of gravity. This is outlined in the figure below. 7 This difference in the force of gravity causes the Earth and its oceans to become egg-shaped. This produces tidal bulges on both sides of the Earth, through which the land masses and oceans pass through on a daily basis. The underlying geology of the land masses also contributes to the variations in tides associated with particular regions about the globe. It may also surprise you that both the land and the atmosphere also experience tides due to gravitational effects. The Predictable Time Schedule for Tides … Variations in tides occur around the world due to many factors. The combination of land (continents) and water create shorelines which can vary from one location to another. The topography of the coastal area (shape of sea floor and the mouths of bays and rivers) can also cause great variations in the tides. Most coastal areas on Earth experience 2 high tides and 2 low tides every day. A 24 hour day is caused by the rotation of the Earth on its axis. As a result, the tide in most coastal areas of the Earth changes every 6 hours, 12 minutes and 30 seconds. For example: If the first high tide of the day was 9:00 AM, then a low tide would be expected at 3:12:30 PM (9:00 AM + 6hrs 12 minutes and 30 seconds.. The second high tide would be expected at 9:25 PM with the next low tide expected at 3:37:30 AM (9:25 AM + 6 hrs 12 minutes and 30 seconds.. The first high tide of the following day would be expected at 9:50 AM. This is a very predictable pattern. The Role of the Sun on Tidal Action The gravitational attraction between the Moon and the waters of the Earth is the main cause of the tides, but the Sun certainly plays a part. The tide generating force of the Sun is about half of the Moon. When the Earth, Moon and Sun are in alignment, the force is additive. The gravity of the Moon and Sun work together causing extra-high tides and very low (low) tides. These tides are called Spring tides and occur twice per lunar 8 cycle. Spring tides occur during the full and New Moon phases. The highest high tides occur during the New Moon phase since the Moon and Sun are on the same side of the Earth and their gravity is pulling in the same direction. Homework Assignment # 4 The gravity of the Moon has more of an affect on tides than the Sun because the Moon is closer. BUT!! The Sun DOES have an effect! During New Moon and Full Moon phases high tides are higher than other phases because the gravity of the Moon and Sun “work together”. These are called SPRING TIDES. During First Quarter and Third Quarter phases high tides are lower than other phases. These are called NEAP TIDES. Look at the diagram and explanations above. Do your best to describe why Neap tides are the lowest high tides. _________________________________________________________________ _________________________________________________________________ _________________________________________________________________ If it is high tide in Delaware at 12:00 P.M., what time will the next low tide occur? _________________ …the next high tide? _________________ Moon Phases 9 Moon Phases and Eclipses The Moon appears to change shape throughout the month. The Moon is not actually changing shape, but the part that we see illuminated here from Earth is changing. The major phases of the Moon include New Moon, Waxing and Waning Crescent, First and Last Quarter, Waxing and Waning Gibbous and Full Moon. The Moon rotates and revolves counterclockwise. The illuminated part of the Moon always points the way to the Sun. If the right side of the Moon is illuminated, the Sun is on the right. If the left half of the Moon is illuminated, the Sun is on the left. The phases of the Moon always proceed with the lighted part of the Moon growing from right to left until the Full Moon, then receding from the right to left until you reach New Moon. If the Moon is light on the right side, the light will continue to expand to the left (Waxing). If the Moon is dark on the right side, the shadow will continue to expand to the left (Waning). The edge of light that moves across the Moon’s surface is called the terminator. The terminator always moves from right to left on the Moon’s surface. The Full Moon occurs when the Moon is on the opposite side of the Sun from the Earth. In this position, the Moon receives full light on the side of the Moon facing Earth. The period after the Full Moon up until the New Moon is called a waning Moon because the visible lighted surface is decreasing. One lunar cycle from New Moon to New Moon lasts about 29 ½ days. A lunar eclipse occurs during Full Moon when the Earth’s shadow falls on the Moon. This would happen every month during Full Moon if the Moon orbited around Earth in the same plane as the Earth orbits around the Sun. The Moon’s orbit is tilted about 5 degrees above the Earth-Sun plane. This tilt also moves and rotates which allows eclipses to happen when the Earth, Sun and Moon end up in a straight line, therefore blocking Sunlight. A lunar eclipse is visible to an entire hemisphere and is seen by all persons able to view the 10 Full Moon. Lunar eclipses can last for hours because the Moon and Earth are moving slowly in relation to each other, and the shadow cast by the Earth is very large. A solar eclipse occurs when the Moon comes directly between the Earth and Sun (New Moon), and blocks the Sun’s rays. The Moon’s path is usually too high or too low for a solar eclipse to occur most of the time. A solar eclipse always occurs two weeks after or two weeks before a total lunar eclipse. Solar eclipses last for a matter of minutes and are visible in a narrow path around the Earth. Homework Assignment #5 Label the diagram with the correct moon phase. The outer images are how the Moon appears from Earth…these are the images you should label. There are 8 in all. (You may need to look at your vocab words or do some extra searching to help guide you) 11 Part 3: The Solar System Galactic Address Most students know their home address, but do they know their galactic address? We are but a small spot on Earth in an immense solar system, galaxy and universe. We live in the Milky Way Galaxy. Most galaxies belong to groups called clusters of galaxies. The Milky Way Galaxy belongs to a cluster called the local group which contains more than 20 galaxies in a great sphere. There are thousands of other clusters of galaxies that contain over one thousand galaxies called rich clusters. The closest one is in Virgo (holds 2500 galaxies). Superclusters are the largest known formations in the universe and we belong to the Virgo super cluster. Where are we in the universe? Our home, planet Earth, is part of the solar system which is in the Milky Way Galaxy. The Milky Way Galaxy is part of a cluster of galaxies. These clusters make up super clusters, such as the Virgo super cluster. A map is a representation of a particular area and may be drawn or photographed and labeled from different points of view. The amount of human made or natural objects seen in satellite images varies depending on your point of view. The higher the elevation, the less human made objects we see and the more natural objects that will be visible. Homework Assignment #6 You are an employee of Google maps. Someone from a distant planet (outside the Virgo supercluster) asks you for directions to your house. In the space below, provide them with the directions they need… 12 Scale Models of Our Solar System Models are important to demonstrate size of objects in our solar system. There are different types of models that are used in the science classroom. Conceptual models are used to explain something that we cannot directly see. Physical models are a simplified construction of real objects.We use a model of the Solar System because it is very large, and models may also be used for things that are very small, like cells. Most depictions of the solar system, whether in posters, videos, or films, give the impression that the distances between planets are only somewhat larger than the diameters of the planets themselves. To a great extent, this impression results from the limitations of 2-dimensional or even threedimensional artwork. Thus, in some ways, our natural, human visual sense betrays us when it comes to making sense of something as outsized as the solar system, not to mention the Universe. Homework Assignment #7 Bodes’ Law: In 1766, Johann Titius developed a mathematical relationship between the distances of the planets from the Sun and it was published in 1772 by Johann Bode. The law states this relationship between planets can be found by using a series of numbers starting with zero and jumping to 3 and then doubling the following numbers, Then 4 was added to each number, divided by 10 and this value represented the AU (Astronomical Unit) from Sun. Find the missing numbers for Jupiter and Saturn! Numbers Add 4 Divide by 10 AU Planet 0 4 .4 0.39 Mercury 3 7 .7 0.72 Venus 6 10 1.0 1.0 Earth 12 16 1.6 1.6 Mars 24 28 2.8 2.8 48 _____ _____ _____ Jupiter _____ _____ _____ _____ Saturn 13 Asteroid belt More Gravity Remember the two factors that influence gravitational pull: mass and distance. Since the Sun’s mass is roughly 99% of the mass in the solar system, all objects in the solar system revolves around our star. But what happens when we travel farther away from Earth? Even though we are still affected by the Sun’s gravity, we begin to be less affected by the Earth’s gravity. However, there is nowhere in the universe you can go and not be affected by gravity…that we know of!! So How Do Astronauts Float Around in Space? We have all seen the images and videos of astronauts floating around in space and it is generally referred to as a “weightless” or “microgravity” environment. But this contradicts our previous discussion that gravity never goes to zero, let alone for astronauts that are only a few hundred miles from the surface of the Earth. The terms weightlessness, zero gravity, and microgravity refer to a sensation of being weightless. By all appearances, gravity has disappeared, but this is not true. The space shuttle, the space station, and satellites are actually falling towards the Earth because the Earth’s gravity is pulling them downward just like it would do to any object that get tossed up into the air. The spacecraft and astronauts are moving forward while they are also falling downward. Since the Earth is a sphere, the astronauts and the spacecraft actually fall around the Earth. You would feel the same sensation, for a short amount of time if you were to ride the Free Fall ride at Six Flags Great Adventure in New Jersey or if you rode in the Vomit Comet, which is a plane that is used to train astronauts for this free fall condition. Due to this free fall situation, it appears as if all objects have no weight, when actually they have not traveled far enough away from the center of the Earth to experience any significant weight loss. What is really happening is that all of the objects are falling at the same rate around the Earth. Since things in this free fall 14 environment behave like there is no gravity at all, scientists use the terms weightlessness, zero gravity, and microgravity to describe it even though the gravity is not zero or “micro”. How Do Humans React to Space? Humans may live in space for longer periods of time in the future. Past missions in space travel have revealed that this free fall (or microgravity) environment can have negative effects on the human body. Our bodies have evolved to handle the Earth’s always-present downward force of gravity, but when put into a situation, such as in orbit, where the body feels as if the force of gravity was turned off, the human body adapts to the new environment. This is the reason that astronauts must exercise regularly in space. As scientists study ways to combat gravity related problems in space, such as bone degeneration, they have also made advances in similar problems already existing on our planet. Homework Assignment #8 Think of an Olympic or sports event (running, diving, basketball, soccer, etc.). Now think of how that event would be played on the Moon (where there is less gravity and humans can jump higher and throw farther). Write down how you would change the equipment, rules, goals, etc. so it could be played on the Moon. _________________________________________________________________ _________________________________________________________________ _________________________________________________________________ _________________________________________________________________ _________________________________________________________________ _________________________________________________________________ 15