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How Eclipses
Happen

Discover why the Sun, Moon, and Earth sometimes align to create the most spectacular events in our sky: solar and lunar eclipses.

Earth & Space Science

What Is an Eclipse?

An eclipse occurs when one celestial body moves into the shadow of another. In our solar system, eclipses happen when the Sun, Earth, and Moon line up in a nearly straight path called syzygy.

The Three Key Players

★ The Sun
Our star: a massive ball of hot gas about 109 times Earth's diameter. It is the light source in every eclipse.
★ The Earth
Our home planet orbits the Sun once per year. Earth casts a long shadow into space behind it.
★ The Moon
Earth's natural satellite orbits us about once every 29.5 days. It can block the Sun or enter Earth's shadow.

Shadows in Space

Every object in sunlight casts a shadow. That shadow has two parts:

Sun Earth Umbra (total shadow) Penumbra (partial shadow)
Umbra
The darkest, innermost part of the shadow where all sunlight is blocked.
Penumbra
The lighter, outer part of the shadow where only some sunlight is blocked.

The Moon's Tilted Orbit

The Moon's orbit around Earth is tilted about \(5^\circ\) relative to Earth's orbit around the Sun. This is why eclipses don't happen every month: the Moon usually passes slightly above or below the Sun-Earth line.

Earth's orbital plane Earth Moon
\(5^\circ\)
Node Node

How a Solar Eclipse Works

A solar eclipse occurs during a new moon when the Moon passes directly between the Sun and Earth, casting its shadow on Earth's surface.

Sun Moon Earth Moon's shadow Sun, Moon, and Earth aligned (New Moon phase)

Types of Solar Eclipses

Total
The Moon completely covers the Sun. The sky goes dark and the Sun's corona becomes visible. Only from within the umbra.
Partial
Only part of the Sun is covered. Observers are in the penumbra. The Sun looks like a "cookie with a bite."
Annular
The Moon is farther from Earth (smaller apparent size), so a bright "ring of fire" remains around the Moon.

How a Lunar Eclipse Works

A lunar eclipse occurs during a full moon when the Earth passes directly between the Sun and Moon, casting Earth's shadow onto the Moon.

Sun Earth Moon Earth's shadow Sun, Earth, and Moon aligned (Full Moon phase)

Types of Lunar Eclipses

Total
The entire Moon enters Earth's umbra. The Moon glows red/copper for up to 1 hour 40 minutes.
Partial
Only part of the Moon enters the umbra. A dark "bite" appears on one edge of the Moon.
Penumbral
The Moon passes through Earth's penumbra only. The dimming is so subtle it is hard to notice.

Solar vs. Lunar Eclipses

Solar Eclipse Lunar Eclipse
Moon Phase New Moon Full Moon
What's Shadowed? Part of Earth The Moon
Who Sees It? Small area on Earth (narrow path) Anyone on Earth's night side (half the planet)
Duration Minutes (totality up to ~7.5 min) Hours (totality up to ~100 min)
Safe to Watch? Requires special glasses Safe with naked eyes
Shadow Caster The Moon The Earth

Why Not Every Month?

1
The Moon's orbit is tilted \(5^\circ\). Most months, the Moon passes above or below the Sun-Earth line, missing the shadow entirely.
2
Eclipses require alignment at a node. The Moon must cross Earth's orbital plane at the same time it is in new moon or full moon phase.
3
Eclipse seasons shift each year. The nodes slowly rotate, creating eclipse windows roughly every 6 months: typically 2-5 eclipses per year.

How to Identify an Eclipse

1
Check the Moon phase. New Moon → possible solar eclipse. Full Moon → possible lunar eclipse.
2
Check the alignment. The Sun, Earth, and Moon must be nearly in a straight line (near a node).
3
Identify the shadow. Solar: Moon's shadow on Earth. Lunar: Earth's shadow on the Moon.
4
Determine total vs. partial. If the object is fully in the umbra → total. If only in the penumbra → partial (or annular for solar).

Example: A Total Solar Eclipse

Sun Moon Earth A B C New Moon phase: Moon between Sun and Earth
Observer A
In the umbra: sees a total solar eclipse. The sky goes dark, the corona appears.
Observer B
In the penumbra: sees a partial solar eclipse. Part of the Sun is still visible.
Observer C
Outside the shadow: sees no eclipse at all. A normal sunny day.

Example: A Total Lunar Eclipse

Stage 1 Stage 2 Stage 3 Stage 4 Penumbral Slight dimming Partial Dark bite appears Total Blood Moon Recovery Moon exits shadow

Example: An Annular Solar Eclipse

Moon (appears smaller) "Ring of Fire" Moon is farther from Earth, so it appears smaller than the Sun

Common Mistakes

✕ Confusing the order
In a solar eclipse the order is Sun → Moon → Earth. In a lunar eclipse it is Sun → Earth → Moon. Students often reverse these.
✕ Wrong Moon phase
Solar eclipses happen at new moon, lunar eclipses at full moon. A common error is mixing up which phase goes with which eclipse.
✕ Eclipses every month
The Moon's \(5^\circ\) orbital tilt means alignment at the nodes is rare. Eclipses do not happen every new or full moon.

Summary at a Glance

Feature Solar Eclipse Lunar Eclipse
Alignment order Sun → Moon → Earth Sun → Earth → Moon
Moon phase New Moon Full Moon
Shadow caster Moon Earth
Visibility Narrow path on Earth Entire night side of Earth
Types Total, Partial, Annular Total, Partial, Penumbral
Eye safety Special glasses needed Safe to view
Why not monthly? Moon's orbit tilted \(5^\circ\): alignment at nodes required

Question 1 of 5

During a solar eclipse, which object casts a shadow on Earth?

Question 2 of 5

A lunar eclipse can only occur during which Moon phase?

Question 3 of 5

Why don't eclipses happen every month?

Question 4 of 5

An observer in the penumbra during a solar eclipse would see:

Question 5 of 5

What causes the Moon to appear red during a total lunar eclipse?