This is an easy and fun way for students to visually understand why the Transit of Venus is so rarely seen, using a paper plate. Paper Plate Demo-Modified by University of Montana

This problem book covers 17 specific mathematics problems that are common to studying the transit of Venus more critically. These include: geometry of chords and triangles, working with angular measure, unit conversion exercises, parallax and angular size, angular speed, time zone conversions, working with proportions, and a few problems involving trig! The majority of the problems may be undertaken by grade 7-9 students. This resource is also helpful for the amateur astronomer wishing to gain a better understanding of parallax, transit geometry and how the Astronomical Unit can be deduced. The book contains 16 math problems, 37 pages, 20 illustrations 2.5 Mby PDF file.

NASA press releases are a great source of topics that highlight how mathematics is used in the process of discovery. Here are the titles and links to recent news announcements in chronological order, together with their related math problems. The press releases appear on the front page of the NASA Home Page, and are frequently covered the same day by news organizations such as CNN.com or Space.com. This collection does not include numerous other discoveries made by NASA missions, which are published in technical journals.

This problem book allows students to explore astronomical eclipses, transits and occultations to learn about their unique geometry, and how modern observations by NASA's Kepler satellite will use simple transit math to discover planets orbiting distant stars. A series of Appendices reveal the imagery and history through news paper articles of the Transits of Venus observed during the 1700 and 1800s. Contains 44 math problems, 250 pages, 120 illustrations 14.6 Mby PDF file.

- Transit Mathematics (without answer keys)
- Transit Mathematics (with answer keys)
- Space Math @ NASA - Transit of Venus 2012 Resources

Kepler-Math SpaceMath@NASA introduces students to the use of mathematics in today's scientific discoveries. Through press releases and other articles, explore how mathematics skills are vital in exploring the universe. (Content is below Transit Mathematics)

This archive provides a sampling of various kinds of data that can lead to answering very interesting questions. All you have to do is provide the question, and then work with the data to come up with your own answers. How you choose to analyze the data, or which data set or combination of them you choose to work with, is entirely up to you. SpaceMath@NASA, through its hundreds of math problems has provided many examples of how data can be investigated to extract new information. Among these 'worked' problems you may come up with new questions for you to research using these data sets. Great Inquiry Activity

Solar Math (2008) 15 Problems Exploring solar storms and solar structure using simple math activities. Calculating speeds of solar flares from photographs, and investigating solar magnetism.

17 Problems An exploration of the moon using NASA photographs and scaling activities. Mathematical modeling of the lunar interior, and problems involving estimating its total mass and the mass of its atmosphere.

37 Problems Six hands-on exercises, plus 37 math problems, allow students to explore magnetism and magnetic fields, both through drawing and geometric construction, and by using simple algebra to quantitatively examine magnetic forces, energy, and magnetic field lines and their mathematical structure.

96 Problems Students explore the way in which the sun interacts with Earth to produce space weather, and the ways in which astronomers study solar storms to predict when adverse conditions may pose a hazard for satellites and human operation in space. Six appendices and an extensive provide a rich 150-year context for why space whether is an important issue.

84 Problems Students explore the simple mathematics behind light and other forms of electromagnetic energy including the properties of waves, wavelength, frequency, the Doppler shift, and the various ways that astronomers image the universe across the electromagnetic spectrum to learn more about the properties of matter and its movement.

44 Problems Students explore astronomical eclipses, transits and occultations to learn about their unique geometry, and how modern observations by NASA's Kepler Satellite will use transit math to discover planets orbiting distant stars. A series of Appendices reveal the imagery and history through news paper articles of the Transits of Venus observed during the 1700 and 1800s.

103 Problems This book covers many topics in remote sensing, satellite imaging, image analysis and interpretation. Examples are culled from earth science and astronomy missions. Students learn about instrument resolution and sensitivity as well as how to calibrate a common digital camera, and how to design a satellite imaging system.

Use this physical model to demonstrate how an eclipse occurs.

This is a complete teachers guide on magnetism. It is designed for students to explore magnets and to develop an operational definition of a magnetic "field" and an operational definition for magnetic "pole."

Use this physical model to demonstrate how an eclipse occurs.

Students will act as scientists discovering magnetic fields and electromagnetism through inquiry and measurement. Included at the beginning of each session is a summary of the session, a list of national education standards that the session covers, and a list of materials required for the session. Each session is broken into several activities, with each activity outlined for the teacher. In the Background Material section, you can find science background for the lessons. A glossary can be found after the background section. At the end we recommend different resources to help you teach and learn more about magnetism.

Students will make sun shadow plots by marking ends of shadows made by the Sun and a gnomon (a stick used to cast shadows). After students have made their sun shadow plot, they will use it to determine the direction of true north.

This bulletin board activity is designed to focus student attention on the role that sun watching has played in humankind's survival through time. As part of this display you may wish to use your own world map or download one we have created for you.

These activities are designed to help you make connections between events in your life and the seasons of the year. One major connection relates the concept of the seasons to past observations.

Let the Exploratorium show you how to build a working Sun Clock.

Enjoy this unit based on the Space and Time gallery at the Liverpool Museum, with both formal and informal activities.

"Learn about these accomplished early astronomers. This site is concise, clearly written, and easy to navigate. It's a great starting point for exploration into the fascinating culture of the Maya." (Selected by the Exploratorium as a Cool Site in Feb. 1998)

There are hundreds of Native American cultures, each with distinctive views of the heavens. In this program, students visit five cultures: the Hupa people of Northern California, Medicine Wheel in Northern Wyoming, Chaco Canyon in New Mexico, the Mayan people and the Incan people.

From NASA's Quest's Learning Technologies Channel (at NASA Ames) and the Stanford Solar Center, learn more about the sun from this impressive archive of video clips and materials from past webcasts.

You and your middle-school students will open up the Sun and explore phenomena most people have never seen before. Your students will calculate the period of the solar cycle and predict its shapes, and calculate the rotation period of the Sun.

Students will make a flip book that shows the progression of two solar events on reversible sides of the flip book. Event choices include the sunspot cycle, differential rotation of the sun using sunspots, a total solar eclipse, progression of a coronal mass ejection, and a sungrazing comet.

A typical galaxy like the Milky Way has a magnetic field strength of about 0.000003 Gauss.