Western Governors University

C895: Astronomy

A study guide to WGU's C895, the graduate astronomy course for science teachers, from moon phases to stellar evolution and cosmology.

Updated October 2026 · 5 min read

C895 gives science teachers the astronomy they need: the sky as seen from Earth, the solar system, the life of stars and the scale of the universe.

WGU describes the course as giving graduate students seeking licensure or endorsement, or an M.A., in secondary or middle grades science education essential knowledge of astronomy.

It explores Western history and basic physics of astronomy; phases of the moon and seasons; composition and properties of solar system bodies; stellar evolution and remnants; properties and scale of objects and distances within the universe; and introductory cosmology.

Astronomy is full of persistent misconceptions, including among adults. Explaining seasons or moon phases correctly is harder than it sounds, and it is exactly what you will need to teach.

Course at a Glance

ItemDetails
UniversityWestern Governors University (WGU)
Course codeC895
LevelGraduate, competency-based
AudienceMiddle grades and secondary science education candidates
Subject areaAstronomy and astrophysics basics
Typical workWritten explanation or exam; check your course page

What C895 Covers

TopicKey ideas
History and physicsGeocentric to heliocentric models, Kepler, Newton's gravity
Moon phases and seasonsSun-Earth-Moon geometry, axial tilt
Solar system bodiesTerrestrial and giant planets, moons, small bodies
Stellar evolutionStar formation, main sequence, red giants, remnants
Scale and distanceAstronomical units, light-years, parallax
CosmologyExpanding universe and the Big Bang model

Key Concepts Explained

Seasons Come from Axial Tilt

Seasons are caused by Earth's 23.5-degree axial tilt, not by changing distance from the Sun. When a hemisphere tilts towards the Sun, sunlight strikes it more directly and days are longer, so it receives more energy.

Example: Earth is actually closest to the Sun in early January, during the Northern Hemisphere's winter. If distance caused seasons, both hemispheres would have summer at the same time, but Australia has summer while Canada has winter.

Moon Phases Come from Viewing Angle

The Moon is always half lit by the Sun. Phases depend on how much of that lit half we see from Earth as the Moon orbits. Earth's shadow causes eclipses, not phases.

Example: At full moon, the Moon is on the opposite side of Earth from the Sun, so we see the whole lit half. It rises around sunset. At new moon, it is between Earth and the Sun and we see the unlit side.

Stellar Evolution Depends on Mass

Stars form from collapsing gas clouds and spend most of their lives fusing hydrogen on the main sequence. A star like the Sun becomes a red giant and ends as a white dwarf. Much more massive stars explode as supernovae, leaving neutron stars or black holes.

Kepler and Newton

Kepler showed that planets move in ellipses, sweep out equal areas in equal times, and that a planet's orbital period squared is proportional to the cube of its average distance from the Sun.

Newton's law of gravitation later explained why. These laws let astronomers calculate masses and distances, and they are a strong example of the history and physics strand in the course description.

Getting a Feel for Scale

Distances in astronomy defeat intuition. Light from the Sun takes about 8 minutes to reach Earth. The nearest star beyond the Sun is a little over 4 light-years away. The Milky Way spans roughly 100,000 light-years, and it is one of billions of galaxies.

Scale models help both you and future students. If the Sun were a 1-meter ball, Earth would be about 1 centimeter across and roughly 100 meters away. Building such a model shows why textbook diagrams, drawn to fit a page, are always badly out of scale.

Typical Tasks and How to Approach Them

Task typeWhat it testsHow to approach it
Phenomenon explanationCorrect modelsUse a labeled diagram and plain language
Misconception analysisTeaching insightState the wrong idea and the evidence against it
Stellar life cycleSequence and massCompare low-mass and high-mass paths
Scale calculationUnits and distanceConvert carefully and check orders of magnitude

Where Students Get Stuck

Study Tips for C895

How We Help with C895

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Frequently Asked Questions

What does C895 cover?

The history and basic physics of astronomy, moon phases and seasons, solar system bodies, stellar evolution and remnants, the scale of the universe and introductory cosmology.

What causes the seasons?

Earth's axial tilt, which changes how directly sunlight strikes each hemisphere and how long days last. Distance from the Sun is not the cause.

What causes moon phases?

Our changing view of the Moon's sunlit half as it orbits Earth.

Does C895 have prerequisites?

Check your degree plan, as prerequisites can vary by program version.

Can you take my C895 exam?

No. We never take exams or log in for students. We provide explanations and study notes.

Is GradeEssays affiliated with WGU?

No. We are independent and not connected with Western Governors University.