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Lesson: Get Me Off This Planet Contributed by: Integrated Teaching and Learning Program, College of Engineering, University of Colorado at Boulder
Learning Objectives (Return to Contents) After this lesson, students should:
Introduction/Motivation (Return to Contents) Ask the students, "How does a rocket physically get from the Earth to Mars?" Students should realize that it takes a very large rocket to get there. Ask them, "Why do you need such a large rocket?" They will probably come up with answers such as: we need to overcome gravity, Mars is a long ways away, when we go to Mars, we have to take a lot of supplies and equipment, and maybe even, we have to overcome gravity and the drag of our atmosphere. So, as soon as we leave the atmosphere, are we free to travel to Mars? Not quite yet, we are still even in the grip of Earth's gravity even though the astronauts feel weightless. There is a misconception that once you leave the Earth's atmosphere, there is no gravity. The truth is that there is gravity acting on a person in orbit around the Earth, but they do not feel it. A comparison can be made to a sky diver. Do you think a sky diver feels the effects of gravity? The answer is no, the sky diver cannot feel gravity. They can feel the air rushing by and they can see the ground coming up but they can't actually feel gravity. This feeling is called weightlessness, and it does not mean that gravity is not there. It is as if both the astronaut and spacecraft are perpetually falling, but never actually get any closer to the surface of the Earth. So, once a rocket has gotten us out of the Earth's atmosphere, we enter into an orbit around the Earth. Ask students if they can explain what an orbit is. (Answer: An orbit is a regular, repeating path that one object in space takes around another one.) Ask students what the shape of most orbits is. (Answer: Elliptical, but students will probably say that they think orbits are in the shape of a circle.) An ellipse is essentially an oval. While a circle is a special kind of ellipse, engineers and scientists use the term ellipse to describe orbits around Earth and other bodies such as the Sun. So, if a spacecraft is in orbit around Earth, how does it get to Mars? (Answer: It uses another rocket.) If the rocket moves the craft fast enough, it will escape the Earth's gravity and start heading for Mars. Elliptical orbits also help to move a rocket between planets. However, there are many other factors to take into consideration when traveling between planets. Today we are going to talk about the basics of traveling from Earth to Mars. Lesson Background & Concepts for Teachers (Return to Contents) Getting off Earth - Launch The first step on the trip to Mars is the launch. Launch is the act of getting a spacecraft off the surface of the Earth and into an orbit around it. It takes a lot of energy to reach an orbit above Earth. Consider that just to jump a couple feet off the ground takes all the energy we can muster. To get a thousand kilogram spacecraft off the ground takes an incredible amount of energy. Not only do we have to overcome Earth's gravity, but also the drag of the atmosphere. To figure out how much velocity we need to get into an orbit around Earth, we use the following equation:
where, ∆ means change and V means velocity. So ∆VLaunch is the total change in velocity needed to launch a spacecraft into an orbit around Earth. ∆V is the final velocity minus the initial velocity. Since the velocity of the spacecraft is initially zero while it is on the ground, ∆V is simply the final velocity. ∆Vburnout is the leftover velocity that we need to maintain and orbit around Earth. We will talk about this velocity a little later. ∆Vgravity is the change in velocity needed to overcome the gravity of Earth. ∆Vdrag is the change in velocity required to overcome drag. To achieve the required ∆V, engineers at NASA use huge rockets. The actual size and mass of the rocket, which engineers call the launch vehicle, dwarfs the actual spacecraft, which is referred to as the payload. For a typical mission into Low Earth Orbit (LEO) the mass of the launch vehicle and the fuel is roughly 40 times the mass of the actual payload. So, how does a rocket create the ∆V we need? (Answer: Rockets use Newton's 3rd Law of Motion.) Newton's 3rd Law states that for every action there is an equal and opposite reaction. If you were to stand on a skateboard and push against a wall you would move in the opposite direction. This is an example of Newton's 3rd Law. Cars use their tires to push backwards against the road, which cause the car to move in the opposite direction. True, rockets do not actually push against the air, but the movement of a rocket is still described by Newton's 3rd Law of Motion. A rocket works by creating super hot gasses and "throwing" them backwards very quickly. This "throwing" of the air is the action. The reaction is that the rocket moves in the opposite direction, forwards. There are two basic numbers that we use to characterize a rocket. The first of these is the thrust — the force that pushes the rocket into orbit. We calculate the amount of thrust a rocket produces by using the following equation:
where the thrust force (F) is equal to the mass flow rate (m) multiplied by the exhaust velocity (Ve). The mass flow rate is how fast mass is coming out of the rocket. The mass is the exhaust gas that comes from the burning fuel. Mass flow rate is measured in kilograms per second (kg/s). The exhaust velocity is a measure of how fast the hot gas leaves the rocket nozzle. The other number we use to characterize a rocket is the specific impulse (Isp) — a measure of the energy content of a propellant and how efficiently it is converted into thrust. Basically, the specific impulse tells us how much bang for the buck we get out a certain type of rocket. To calculate the specific impulse, we divide the thrust by the weight flow rate:
The weight flow rate is the mass flow rate (m) multiplied by the gravitational acceleration of Earth (g = 9.81 m/s2). The specific impulse has units of seconds. The Isp measures how much thrust we are getting for how much fuel weight we are using. A higher Isp means that we are getting more thrust for less fuel, and it is more efficient system. There are three different kinds of rockets that are currently used in space applications: chemical, electrical and cold gas. Chemical rockets are the most common rockets in use today, and include liquid fuel rockets, solid fuel rockets and a hybrid of the two. Chemical rockets rely on a chemical combustion that creates a super-heated, high-pressure gas. This high pressure gas can only escape through the nozzle. According to Newton's 3rd Law, this gas leaving the rocket at a very high velocity is the action, while the rocket moving in the opposite direction is the opposite reaction.
Liquid fuels are stored in large tanks and are pumped into a combustion chamber where they ignite before leaving the rocket through the nozzle. Figure 1 shows a diagram of a liquid fuel rocket. Liquid fuel systems are complicated since they require several tanks, complex valves and intricate piping, but they create a lot of thrust, have a high Isp, and can be throttled and restarted if needed. The space shuttles main engines use a liquid fuel that is a mixture of liquid oxygen and liquid hydrogen. Figure 2 shows the liquid fuel tank and the liquid fuel main engine on the space shuttle.
Solid fuel rockets can be described as a tube, filled with a solid fuel, capped at one end and with a nozzle at the other end. The solid fuel is highly flammable and works in the same way the liquid fuel system works. As the fuel burns, a hot and high-pressure gas comes out of the nozzle creating thrust. Solid fuel systems are very simple, cheap and reliable, but they cannot be turned off once they start and they are not as efficient as liquid fuels. An example of a solid fuel system is the Solid Rocket Boosters (SRB) on the space shuttle (see Figure 2). They are the two white rockets strapped to the side of the vehicle and are used to help get the space shuttle off the ground. Once the fuel inside the boosters is exhausted, they are released from the shuttle and dropped into the ocean. Bottle rockets and model rockets are both considered solid fuel rockets. Electrical rockets use electricity to accelerate particles that are directed out the back end of the spacecraft, thus creating thrust. The rockets generally use charged atoms called ions that have a positive or negative charge associated with them. An electrical source, such as solar cells, or a nuclear reactor is used to charge plates in the engine with different charges so that the ions are pushed and pulled out of the spacecraft. The downside to electrical rockets is that they cannot create much thrust. If you hold one sheet of paper in your hand, the force with which the paper pushes on your hand due to its weight is roughly equal to the thrust of an electrical rocket. The plus side to electric rockets is that they are very efficient and have a high Isp. Since the thrust of an electrical rocket is so small, it is impossible to launch a rocket into space; but, once a spacecraft is in an orbit around Earth, an electrical rocket can be used to escape the Earth's gravity and head to different places around our solar system. The small thrust means it takes a long time for the craft to build up sufficient escape velocity, but the high efficiency of the system means less fuel is needed to achieve the desired velocity. The first use of electrical rockets in space was onboard Deep Space 1, which launched onboard a conventional liquid fuel rocket on October 24, 1998. Once it was in orbit, it started its own engine and eventually reached the Comet Borrelly in September of 2001. Cold gas rockets use pressurized gas that is not ignited. This is usually a nonflammable gas such as nitrogen or helium. A balloon that is filled and then released is an example of a cold gas system. The pressurized gas can only escape out the nozzle, and as it does, it creates thrust. Cold gas systems have very low thrusts and are very inefficient (low Isp), but they are very simple and cheap. They are often used on spacecraft to make very small velocity changes where large rockets are overkill. The rocket packs that astronauts use when they are outside the space shuttle or international space station use cold gas rockets. Table 1 shows the different types of rockets and the typical thrusts and specific impulses for each system.
Orbits Once a launch vehicle has gotten the spacecraft out of the Earth's atmosphere, it now must enter into an orbit. An orbit is a circular or elliptical path around a celestial body (sun, star, planet, asteroid, etc.) on which an object such as a spacecraft will follow. There is a misconception that on the space shuttle and international space station there is no gravity. There is gravity acting on a person in orbit around the Earth, but they do not feel it like we feel it on Earth, because there is no ground to push back on us in space. So, why doesn't a spacecraft just fall back to Earth once the rockets shut off? This is because the velocity of the spacecraft wants to move it past the Earth, while gravity pulls it back. These two actions cancel out to form an orbit. An orbit can be explained by Newton's 1st Law of Motion which tells us that an object in motion stays in motion unless a force acts against it. This means that an object will move in a straight line unless a force pushes it in a different direction. For any object to change the direction in which it is moving, there must be a force acting on it. For example, when you are on a bike and want to turn (change directions), your tire must apply a force to the ground. This force is called friction; without friction, it would be like biking on perfectly smooth ice. If you tried to turn, there would be no frictional force; you would keep moving in a straight line as Newton's 1st Law dictates. Just like your bike, a spacecraft will not turn unless there is a force acting on it. The force that acts on objects — ultimately causing it to orbit a planet or a star — is gravity. An orbit is just a balance between the velocity of an object and gravity.
Figure 3 shows how gravity affects the path of a spacecraft. The diagram on the left shows the path of a spacecraft if there was no gravity. In this case, the spacecraft would continue along in a straight line. The diagram on the right shows the path of a spacecraft under the influence of gravity. Gravity is pulling the spacecraft towards the center of the Earth, while the velocity of the spacecraft makes the spacecraft want to keep going past the Earth. The balance of these two opposing actions is known as an orbit. For a Low Earth Orbit (LEO), which has an altitude between 600 and 2000 kilometers above the Earth's surface, the spacecraft must have a velocity of about 8 kilometers per second. That means that it can go all the way around the Earth in 90 minutes. So, what happens if the spacecraft is not moving (i.e., has no velocity)? If there is no velocity, then the only force acting on the spacecraft is gravity. This means that a spacecraft would fall to Earth just as a stone falls to the ground when you drop it. So, what happens if the spacecraft is moving much faster than the 8 km/s needed to maintain a LEO? In that case, the gravity will not be able to hold the spacecraft as close to the Earth, and the spacecraft will either move into an orbit that is further away from the Earth, or if it is moving fast enough it will escape Earth's gravity entirely. This is called the escape velocity, and it is the minimum velocity needed to escape the Earth's gravity. Sir Isaac Newton performed a famous mind experiment to demonstrate how an orbit works that involves shooting cannons off the top of a mountain. There is a demonstration of the cannon ball orbit on the NASA website at http://spaceplace.nasa.gov/en/kids/orbits1.shtml. Getting to Mars Now that our spacecraft has left Earth's gravity, our mission is to arrive at Mars. We have left the influence of Earth's gravity, but we are not free of gravity altogether. Since we are now orbiting around the Sun, we are now under the influence of the Sun's gravity. Thus far, we have talked about circular orbits — the simplest kind of orbit. However, most orbits are actually ellipses, a stretched circle. Ellipses are often called ovals. Figure 4 shows a diagram of an elliptical orbit.
There are two foci (each one called a focus) that define an ellipse: the periapsis, which is the point on the elliptical orbit that is closest to the planet or sun; and the apoapis, the point furthest from the planet or sun. You may have also heard these points called perigee and apogee. These are the periapsis and apoapsis for an elliptical orbit around Earth, respectively. In an elliptical orbit, the Earth (or other massive body) is located at one of the two foci. Elliptical orbits enable movement between planets. Using the Sun as one of the foci, and the Earth as the periapsis, the spacecraft will actually be closer to the Sun when it is at the periapsis. When the spacecraft is at the apoapsis, it will be further away from the sun. This is useful for traveling to planets further from the sun such as Mars. Figure 6 shows how half an elliptical orbit can be used to get from Earth to Mars.
In addition to great engineering and excellent calculations by scientists, it takes good timing to reach Mars. Since the Earth and Mars are both moving, it is like standing on a moving platform and trying to shoot a basketball into a hoop that is moving as well. To make things worse, since it takes about 6 months for a spacecraft to go from the Earth to Mars, scientists and engineers have to anticipate where Mars is going to be when the spacecraft gets there. If we try to shoot a spacecraft right at Mars, by the time it actually gets there, the great Red Planet will be long gone. Once we get to Mars, we have to slow down so that we are in an orbit around our destination. From our orbit, we can take pictures of Mars, take scientific readings, or even land on the planet itself. Vocabulary/Definitions (Return to Contents)
Associated Activities (Return to Contents)
Lesson Closure (Return to Contents) In this lesson, the students should learn what it takes to get a spacecraft from the launch pad to Mars. We learned that rockets use Newton's 3rd Law of Motion to propel upward/forward. We covered the basics of orbits and learned that an orbit is where the velocity of the spacecraft and the gravity balance to form an elliptical path. Finally, we talked about elliptical orbits and how elliptical orbits allow us to travel from Earth to Mars. Assessment (Return to Contents) Pre-Lesson Assessment Discussion Question: Solicit, integrate and summarize student responses.
Voting: Ask a true/false question and have students vote by holding thumbs up for true and thumbs down for false. Count the votes and write the totals on the board. Give the right answer.
Post-Introduction Assessment Discussion Question: Ask the students and discuss as a class:
Lesson Summary Assessment Numbered Heads: Break the class up into teams of three to five. Students on the team should pick numbers so each member has a different number. Ask the students a question and give them a short time frame for solving it (~1 minute). The members of each team should work together on the question. Everyone on the team must know the answer. Call a number at random. Students with that number should raise their hands to answer the question. If not all the students with that number raise their hands, allow the teams to work on the question a little longer. Example questions:
Lesson Extension Activities (Return to Contents) There are types of orbits other than circular and elliptical orbits. There are also parabolic and hyperbolic orbits. Have the students research these types of orbits to determine what is special about them and how they are used. References (Return to Contents) National Aeronautics and Space Administration, Mars Exploration Program, http://mars.jpl.nasa.gov - accessed October 4, 2005. National Aeronautics and Space Administration, Space Place http://spaceplace.nasa.gov/en/kids/orbits1.shtml - accessed October 4, 2005. Wertz, James R. and Larson, Wiley J. Space Mission Analysis and Design, 3rd Edition, Space Technology Library, Volume 8, New York, NY: Springer Publishing Company, 1999. Contributors Geoffrey Hill, Daria Kotys-Schwartz, Chris Yakacki, Janet Yowell, Malinda Schaefer ZarskeCopyright © 2004 by Regents of the University of Colorado.The contents of this digital library curriculum were developed under a grant from the Fund for the Improvement of Postsecondary Education (FIPSE), U.S. Department of Education and National Science Foundation GK-12 grant no. 0226322. However, these contents do not necessarily represent the policies of the Department of Education or National Science Foundation, and you should not assume endorsement by the federal government. Supporting Program (Return to Contents) Integrated Teaching and Learning Program, College of Engineering, University of Colorado at BoulderLast Modified: September 26, 2008 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||
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