As a high school science educator at Lac Courte Oreilles Ojibwe school,  indigenous culture and teachings are incorporated into my instruction as much as possible. This text set was incorporated in my Astronomy class tying in Ojibwe Moons and seasonal constellations with northern Wisconsin phenology. A discussion of text set implementation is also included in this OER.Lac Courte Oreilles Ojibwe School is a Bureau of Indian Education/Tribally controlled school catering to students who are themselves tribally enrolled or descendants of a tribal member.

Intended for all audiences, this textbook is an introduction to the nature of the universe. Use it to research or review our solar system, stars, galaxies, and the history of the universe. Each chapter has a set of corresponding homework questions.

This activity is a chance for students to apply the diffraction grating equation m*Λ/d = Θ to solve a real life problem: find the wavelength of given source of light. It is also useful for them to apply trigonometry to real life scenarios.

Background for and techniques of visual observation, electronic imaging, and spectroscopy of the Moon, planets, satellites, stars, and brighter deep-space objects. Weekly outdoor observing sessions using 8-inch diameter telescopes when weather permits. Indoor sessions introduce needed skills. Introduction to contemporary observational astronomy including astronomical computing, image and data processing, and how astronomers work. Student must maintain a careful and complete written log which is graded. In this seminar we explore the background and techniques of visual observation and imaging of the Moon, planets, and brighter deep-space objects using 8-inch telescopes. (Some sample images appear in our "photo album".) Telescope work begins with visual observing, then we advance to CCD (charge-coupled device) cameras. Each class observing session meets one evening a week. Whenever weather conditions permit us to observe outdoors we do so! In cloudy weather we'll try some astronomical computing and image processing indoors instead. Either way, virtually all the work for the seminar is done during the evening sessions, so students must attend section every week in order to pass. Past experience has been that if you're really enthusiastic about hands-on out-under-the-sky astronomy, enough to be willing to deal with dressing warmly, tinkering with equipment, and committing one evening a week, 12.409 is great fun! One student wrote, "Unlike most seminars, you will earn your units and, unlike most other MIT courses, you will look forward to doing it!" But we'll be direct: 12.409 is not for everyone, and in past years many whose interest was merely casual found themselves unwilling to devote one entire evening every week to the class. If your interest is only casual then consider whether a more typical astronomy survey subject might be a better choice, since it'll have more outside preparation time that you can rearrange at your discretion and less in-class time that you can't.

This resource is an interactive Hertzsprung-Russell diagram along with a student handout that could be used.  The interactive H-R diagram allows the user to change the luminosity(or magnitude) and temperature which moves the red X to show where that star would be placed on the diagram.

This course includes Quantitative introduction to physics of the solar system, stars, interstellar medium, the Galaxy, and Universe, as determined from a variety of astronomical observations and models. Topics: planets, planet formation; stars, the Sun, "normal" stars, star formation; stellar evolution, supernovae, compact objects (white dwarfs, neutron stars, and black holes), plusars, binary X-ray sources; star clusters, globular and open clusters; interstellar medium, gas, dust, magnetic fields, cosmic rays; distance ladder; galaxies, normal and active galaxies, jets; gravitational lensing; large scaling structure; Newtonian cosmology, dynamical expansion and thermal history of the Universe; cosmic microwave background radiation; big-bang nucleosynthesis. No prior knowledge of astronomy necessary. Not usable as a restricted elective by physics majors.

Applications of physics (Newtonian, statistical, and quantum mechanics) to fundamental processes that occur in celestial objects. Includes main-sequence stars, collapsed stars (white dwarfs, neutron stars, and black holes), pulsars, supernovae, the interstellar medium, galaxies, and as time permits, active galaxies, quasars, and cosmology. Observational data discussed. No prior knowledge of astronomy is required.

Physics for Future Presidents Spring, 2006. The title is serious. The official designation is Physics 10 and is sometimes called qualitative physics -- but this is not trivial physics. You will be learning material that is generally not learned by the physicist until after earning a Ph.D. After every lecture, you should come away with the feeling that what was just covered is important for every world leader to know. Topics covered may vary and may include energy and conservation, radioactivity, nuclear physics, the Theory of Relativity, lasers, explosions, earthquakes, superconductors, and quantum physics.

This activity is based on an activity from NASA's Solar Math.  This activity has students analyzing sunspot cycle data.  Students find patterns within the data to explore sunspot cycles.

This resource is a lab in which students will use spectroscopes to look at emissions from known emission tubes and lights.  They will use this knowledge/skill to understand how scientists know what elements make up stars.  There are two handouts for students, one is to record observations and the other asks the students questions.

YouTube video comparing the relative size of objects that students are familiar with (planets) and those that they are not (stars, galaxies, etc.) to allow for development of abstract concepts of massive sizes.

This is a computer lab activity where students view images of stars, nebulas, and galaxies and discover factors in telescope design that allow scientists to study the universe. The students will write questions about the images and produce a power point presentation on features of the universe.

Students learn about an astrophysicist that is working in science to open possible ideas for themselves in science careers. Pursuits addressed: Identity-Students will learn about people who they can relate to who are currently working in STEM related careers and study possible STEM related careers that could be meaningful to their own lives/cultures.Skills-The students will research scientists who they can relate to culturally who are working on STEM related careers and then write letters to these scientists in a way that is interesting, genuine, authentic, and allows them to use their own voice.Intellect-Students will choose which scientists they would each like to study by finding scientists who they can relate to culturally who are currently working in STEM related careers and showing examples of Black Excellence.Details: This lesson can be added to 5th Grade Amplify Patterns of Earth and Sky: Analyzing Stars on Ancient Artifacts, with Lesson 2.1 after looking for patterns, making observations, and reflecting on the Model. Explain to the students that this is exactly what astrophysicists do.