Eclipses
The Moon passes between Earth and the Sun every single month. So why doesn't the Sun go dark every single month?
What You'll Be Able to Do
By the end of this lesson, you will be able to:
- Set targets for modeling how and why eclipses happen.
- Name the month puzzle up front as a goal to explain.
- Goal setting
- Advance organizers
- Understand to Analyze
- DOK 1 to 3
- Student-facing "I can" language
- One goal per card, short lines
- Standard badge kept separate from the goal text
Vocabulary to Know
Choose a card to see what each word means.
- Pre-teach shadow and orbit terms the lesson leans on.
- Give a reference students can jump back to during the lab.
- Pre-teaching vocabulary
- Reduced extraneous load
- Remember to Understand
- DOK 1
- One card open at a time
- Click to reveal, no hover
- Jump link ties each term to the lesson
Two Kinds of Eclipse
Before you investigate, here's the setup. Two types of eclipse exist, and they work in completely opposite ways.
- Set up the two eclipse types, then pose the month puzzle.
- Force a prediction before instruction so the explanation has something to resolve.
- Curiosity gap
- Phenomenon-based learning
- Understand
- DOK 2
- Prediction locks in one tap, no penalty
- Reveal appears only after a choice
- Labeled diagrams paired with the text
Eclipse Discovery Lab
Scientists can predict eclipses centuries in advance. The positions are exact. Can you find them?
New moon + crossing the orbital plane = solar eclipse. Most months the Moon passes above or below this line, and the shadow misses Earth completely.
Full moon + crossing the orbital plane = lunar eclipse. Both conditions have to be true at exactly the same time.
- Let students find eclipse alignments themselves instead of being told.
- Show that both a phase and a crossing must line up at once.
- Productive struggle
- Evidence-based reasoning
- Dual coding
- Apply to Analyze
- DOK 2
- Interactive with clear success feedback
- Large drag and click targets
- No penalty for repeated tries
What You Discovered
Here's what you found. The two eclipses look similar from a distance; but the geometry, the phase, and the experience are completely different.
| Solar Eclipse | Lunar Eclipse | |
|---|---|---|
| What happens | Moon blocks sunlight from reaching Earth | Earth's shadow falls on the Moon |
| Moon phase | New Moon, Moon between Sun and Earth | Full Moon, Moon on far side of Earth |
| Alignment | Sun → Moon → Earth | Sun → Earth → Moon |
| Seen from | Only the narrow path of totality on Earth | Anywhere the Moon is visible in the sky |
- Name what the lab revealed about each eclipse type.
- Set up the orbit question the next section answers.
- Comparison and contrast
- Concrete to abstract
- Elaboration
- Understand to Analyze
- DOK 2
- Side-by-side comparison table
- Short, parallel rows
- Bridge callout restates the open question
The Tilted Orbit
New moon happens every 29.5 days, the exact phase a solar eclipse needs. So why don't eclipses happen every month? A single 5-degree tilt in the Moon's orbit changes everything.
The Moon's tilted orbit crosses Earth's orbital plane at exactly two points, called nodes, the only places where an eclipse is geometrically possible. Both conditions must be true at the same time:
A new moon happens every ~29.5 days, but the Moon is near a node for only a few days each orbit. That rare overlap is exactly why eclipses feel special.
- Resolve the month puzzle with the 5-degree orbital tilt.
- Trace the chain from tilt to missed shadow to node alignment.
- Cause-and-effect modeling
- Misconception checking
- Dual coding
- Understand to Analyze
- DOK 3
- Flat and tilted orbits shown side by side
- Key terms defined in place
- Short paragraphs, one idea each
The Anatomy of a Shadow
The Moon casts two shadow zones during a solar eclipse, and they produce completely different experiences. Which one you're in determines everything.
The umbra is the innermost, darkest cone of the Moon's shadow. Stand inside it and the Moon completely covers the Sun, the sky goes dark, stars appear, and the Sun's corona glows around the Moon's edge. The umbra can be as narrow as a few kilometers and rarely exceeds about 270 km wide on Earth's surface.
- Sun completely covered by the Moon
- Sky noticeably darkens, stars and planets may appear
- Solar corona glows around the Moon's edge
- Only a narrow path on Earth experiences totality
The penumbra is the outer, lighter shadow zone. Here, the Moon covers only part of the Sun, you see a partial solar eclipse, a crescent Sun still bright enough to need eye protection. The penumbra spreads wider than the umbra across Earth's surface. Most people observing a solar eclipse are in the penumbra and see only a partial eclipse.
- Part of the Sun remains visible
- Daylight stays relatively bright
- Sun appears crescent-shaped
- Eclipse glasses are still required
- Separate the umbra from the penumbra as two shadow zones.
- Tie which zone you stand in to what you actually see.
- Comparison and contrast
- Dual coding
- Elaboration
- Understand to Analyze
- DOK 2
- Labeled shadow diagram paired with text
- Umbra and penumbra named where shown
- Short, parallel descriptions
Brain Check
Three quick questions before we put it all together. These are not graded. Pulling answers from memory now will help them stick.
- Pull key eclipse facts from memory before the wrap-up.
- Surface gaps early, while there is still time to reread.
- Retrieval practice
- Generation effect
- Understand to Apply
- DOK 1 to 2
- Ungraded and low stakes
- Immediate feedback
- Try Again resets each item
Why Not Every Month?
You started with a puzzle: the Moon lines up with the Sun every month, so why don't eclipses happen every month? Here is the whole answer, step by step.
- Answer the opening puzzle in one connected chain.
- Return to the prediction students made so the loop closes.
- Schema building
- Coherent narrative
- Elaboration
- Understand to Analyze
- DOK 3
- Steps shown as ordered chips
- One idea per step
- Plain summary sentence at the end
Eclipses Quiz
10 questions covering solar and lunar eclipses, shadows, orbital tilt, and nodes. Answer every question, then submit.
Scientists don't just know the answer. They explain their thinking.
Write your own explanation first. Then submit your work to compare your thinking with a model answer.
The Moon reaches new moon every single month, the exact phase a solar eclipse needs. Yet a solar eclipse is rare. Explain why we do not get an eclipse every month. Build the whole chain: what lines up every month, why the Moon's tilted orbit usually makes the shadow miss Earth, and what has to be true about the Moon's position for an eclipse to actually happen. Use the word node.
- Assess solar and lunar eclipses, shadows, tilt, and nodes.
- Give a quick check of understanding after the wrap-up.
- Retrieval practice
- Feedback loops
- Understand to Apply
- DOK 1 to 2
- Answer explanations provided
- Plausible, evenly placed options
- Try Again to review missed items
More Learning
Ready to push your eclipse knowledge deeper? These optional extensions are waiting for you.
- Offer optional depth for students who want to keep going.
- Let learners test tilt and node ideas in a simulation.
- Interest-driven extension
- Transfer
- Apply to Analyze
- DOK 2 to 3
- Optional and self-paced
- No penalty for skipping
- Clear label on the card
Connections
An eclipse is all about alignment. Here are the ideas that help explain how it happens.