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7th Grade Life Science at the Observatory: Life Throughout the Universe
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This classroom activity will show students that there is a lot we don't know about science, for example life throughout the universe. It will hopefully encourage students to question what we know and don't know, and exploration and study of the unknown.

Author:
Brad Snyder
Antimatter Matters
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Antimatter, the charge reversed equivalent of matter, has captured the imaginations of science fiction fans for years as a perfectly efficient form of energy. While normal matter consists of atoms with negatively charged electrons orbiting positively charged nuclei, antimatter consists of positively charged positrons orbiting negatively charged anti-nuclei. When antimatter and matter meet, both substances are annihilated, creating massive amounts of energy. Instances in which antimatter is portrayed in science fiction stories (such as Star Trek) are examined, including their purposes (fuel source, weapons, alternate universes) and properties. Students compare and contrast matter and antimatter, learn how antimatter can be used as a form of energy, and consider potential engineering applications for antimatter.

Author:
TeachEngineering.org
Rachel Howser
Christine Hawthorne
National Science Foundation GK-12 and Research Experience for Teachers (RET) Programs,
Asteroids
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In this lesson, students learn some basic facts about asteroids in our solar system. The main focus is on the size of asteroids and how that relates to the potential danger of an asteroid colliding with the Earth. Students are briefly introduced to the destruction that would ensue should a large asteroid hit, as it did 65 million years ago.

Author:
Janet Yowell
Integrated Teaching and Learning Program ,
TeachEngineering.org
Brian Kay
Karen King
Ball Bounce Experiment
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Students investigate different balls' abilities to bounce and represent the data they collect graphically.

Author:
TeachEngineering.org
Center for Engineering Educational Outreach,
Center for Engineering Educational Outreach, Tufts University
Tufts University
Benham's Disk
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In this optics activity, learners discover that when they rotate a special black and white pattern called a Benham's Disk, it produces the illusion of colored rings. Learners experiment with the speed of rotation and direction of rotation to observe varying patterns. Use this activity to explain to learners how our eyes detect color and how different color receptors in the eye respond at different rates.

Author:
National Science Foundation
NEC Foundation of America
California Department of Education
The Exploratorium
Don Rathjen
Blue Sky
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In this optics activity, learners explore why the sky is blue and the sunset is red, using a simple setup comprising a transparent plastic box, water, and powdered milk. Learners use a flashlight to shine a beam of light through the container. Learners look at the beam from the side of the container and then from the end of the tank, and compare the colors that they see. Learners also examine a narrower beam of light. Use this activity to introduce learners to the light spectrum, wavelengths, frequency, scattering, and how all this effects what we see in the sky at different times of the day.

Author:
The Exploratorium
California Department of Education
NEC Foundation of America
National Science Foundation
Bone Stress
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In this optics activity, learners examine how polarized light can reveal stress patterns in clear plastic. Learners place a fork between two pieces of polarizing material and induce stress by squeezing the tines together. Learners will observe the colored stress pattern in the image of the plastic that is projected onto a screen using an overhead projector. Learners rotate one of the polarizing filters to explore which orientations give the most dramatic color effects. This activity can be related to bones, as bones develop stress patterns from the loads imposed upon them every day.

Author:
The Exploratorium
California Department of Education
NEC Foundation of America
National Science Foundation
Cosmology and Astronomy: Intergalactic Scale
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This 11-minute video lesson looks at intergalactic scale or the distance between galaxies. [Cosmology and Astronomy playlist: Lesson 5 of 85]

Author:
Khan, Salman
Destination Outer Space
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Students acquire a basic understanding of the science and engineering of space travel as well as a brief history of space exploration. They learn about the scientists and engineers who made space travel possible and briefly examine some famous space missions. Finally, they learn the basics of rocket science (Newton's third law of motion), the main components of rockets and the U.S. space shuttle, and how engineers are involved in creating and launching spacecraft.

Author:
Integrated Teaching and Learning Program,
Denise W. Carlson
Jessica Butterfield
Jessica Todd
Geoff Hill
TeachEngineering.org
Denise Carlson
Sam Semakula
The Earth and Sky in a 24 Hour Day
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This is an indoor and outdoor activity where students understand the distance the earth is from the sun. The students understand that the earth rotates on it's axis once in a 24 hour period thus providing us with day and night.

Eddy Currents
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In this activity related to magnetism and electricity, learners discover that a magnet falls more slowly through a metallic tube than it does through a nonmetallic tube. Use this activity to illustrate how eddy currents in an electrical conductor create a magnetic field that exerts an opposing force on the falling magnet, which makes it fall at a slower rate. This activity guide also includes demonstration instructions involving two thick, flat pieces of aluminum to illustrate the same principle.

Author:
National Science Foundation
NEC Foundation of America
California Department of Education
The Exploratorium
Don Rathjen
Engineering Apollo: The Moon Project as a Complex System, Spring 2007
Conditional Remix & Share Permitted
CC BY-NC-SA
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This course is a detailed technical and historical exploration of the Apollo project to "fly humans to the moon and return them safely to earth" as an example of a complex engineering system. Emphasis is on how the systems worked, the technical and social processes that produced them, mission operations, and historical significance. Guest lectures are featured by MIT-affiliated engineers who contributed to and participated in the Apollo missions. Students work in teams on a final project analyzing an aspect of the historical project to articulate and synthesize ideas in engineering systems.

Subject:
Astronomy
Physical Science
Material Type:
Full Course
Textbook
Author:
Mindell, David
Date Added:
01/01/2007
Exploration of Shadows in the Earth, Moon, and Sun System: Moon Phases and Eclipses
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This guided inquiry activity has students using models to create variations of alignment of the Earth, Moon, and Sun. By varying their arrangement, students will discover how the positions of the Earth, Moon and Sun interact, how shadows can be cast on the Moon and on the Earth, and how Earth's view of the lit portion of the Moon changes.

Author:
Jill Baumtrog
Jill Baumtrog
Finding Our Top Speed
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"This lesson sets the stage for a discussion of travel in the solar system. By considering a real-world, hands-on activity, students develop their understanding of time and distance. Finally, students plot the data they have collected." from NCTM Illuminations.

Author:
Thinkfinity/Verizon Foundation
NCTM Illuminations
National Council of Teachers of Mathematics
A Fridge in Space: A Case Study in Thermodynamics
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This case analyzes the principles of thermodynamics and the operating cycle of an adiabatic demagnetizing refrigerator (ADR), a piece of equipment NASA uses to keep x-ray detectors cold enough to work. A synthesis of all the basic principles of thermodynamics, the case would be appropriate for students enrolled in a thermal physics course, typically taught at a sophomore level.

Author:
Lok C. Lew Yan Voon
From Sunlight to Electric Current
Read the Fine Print
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The lesson will first explore the concept of current in electrical circuits. Current will be defined as the flow of electrons. Photovoltaic (PV) cell properties will then be introduced. Generally constructed of silicon, photovoltaic cells contain a large number of electrons BUT they can be thought of as "frozen" in their natural state. A source of energy is required to "free" these electrons if we wish to create current. Light from the sun provides this energy. This will lead to the principle of "Conservation of Energy." Finally, with a basic understanding of the circuits through Ohm's law, students will see how the energy from the sun can be used to power everyday items, including vehicles. This lesson utilizes the engineering design activity of building a solar car to help students learn these concepts.

Subject:
Applied Science
Engineering
Physical Science
Physics
Space Science
Material Type:
Activity/Lab
Lesson Plan
Author:
Rahmin Sarabi
Roni Prucz
TeachEngineering.org
Techtronics Program,
Date Added:
09/18/2014
GPS on the Move
Read the Fine Print
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During a scavenger hunt and an art project, students learn how to use a handheld GPS receiver for personal navigation. Teachers can request assistance from the Institute of Navigation to find nearby members with experience in using GPS and in locating receivers to use.

Subject:
Applied Science
Ecology
Engineering
Geoscience
Life Science
Physical Science
Space Science
Technology
Material Type:
Activity/Lab
Lesson Plan
Author:
Integrated Teaching and Learning Program,
Janet Yowell
Malinda Schaefer Zarske
Matt Lundberg
Penny Axelrad
TeachEngineering.org
Date Added:
09/18/2014
Galaxies and Dark Matter
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This video lesson has the goal of introducing students to galaxies as large collections of gravitationally bound stars. It explores the amount of matter needed for a star to remain bound and then brings in the idea of Dark Matter, a new kind of matter that does not interact with light. It is best if students have had some high school level mechanics, ideally Newton's laws, orbital motion and centripetal force. The teacher guide segment has a derivation of centripetal acceleration. This lesson should be mostly accessible to students with no physics background. The video portion of this lesson runs about 30 minutes, and the questions and demonstrations will give a total activity time of about an hour if the materials are all at hand and the students work quickly. However, 1 1/2 hours is a more comfortable amount of time. There are several demonstrations that can be carried out using string, ten or so balls of a few inches in diameter, a stopwatch or clock with a sweep second hand and some tape. The demonstrations are best done outside, but can also be carried out in a gymnasium or other large room. If the materials or space are not available, there are videos of the demonstrations in the module and these may be used.

Author:
Peter Fisher