5.5Unit 6: Sound, the Earth and eclipses
Solar and lunar eclipses — Cambridge Checkpoint Earth & Space 0893 Revision Notes & Topical Questions
5 min read 11 parts Lesson 5 of 5 1 quiz
Lesson summary
5.5 Solar and lunar eclipses — CHECKPOINT EARTH AND SPACE 0893 notes: Explain how shadows form and how solar and lunar eclipses happen.Opaque = not allowing light to pass throughFormation — an opaque object blocks light rays and leaves a dark shadowLight rays — light travels in s…
- Surroundings
- Solar eclipse
- Total and partial
- Orbit time
- White ball
- Tennis ball
Section 1 of 11Shadows
Opaque
Opaque not allowing light to pass through
Formation
- Formation an opaque object blocks light rays and leaves a dark shadow
Light rays
- Light rays light travels in straight lines called rays
Surroundings
- Surroundings areas around the shadow are brighter because light reaches them
Section 2 of 11Solar eclipse
Solar eclipse
Solar eclipse the Moon comes between the Sun and the Earth
Blocking
- Blocking the Moon is made of rock, so it is opaque and blocks the Sun's light rays
Shadow
- Shadow the Moon's shadow forms on the Earth
Daytime
- Daytime a solar eclipse can only be seen in the daytime
Section 3 of 11Total and partial solar eclipses
Total and partial solar eclipses
Total
- Total people in the middle of the Moon's shadow see all of the Sun's light blocked
Partial
- Partial away from the middle some rays still reach the Earth
Safety
- Safety never look directly at the Sun, even during an eclipse, because it can permanently damage the eyes
Section 4 of 11Lunar eclipse
Lunar eclipse
Lunar eclipse
Lunar eclipse the Earth comes between the Sun and the Moon
Blocking
- Blocking the Earth is opaque and blocks light from the Sun
Shadow
- Shadow the Earth's shadow forms on the Moon
Total and partial
- Total and partial a total lunar eclipse happens when the whole Moon is in the shadow and a partial one when only part is
Section 5 of 11Why eclipses are not monthly
1Orbit time
- Orbit time the Moon takes about 28 days to orbit the Earth
2Tilt
- Tilt the Moon's orbit is tilted slightly from the plane of the Earth's orbit
3Condition
- Condition eclipses happen only when the Sun, Earth and Moon are in the same straight line
Section 6 of 11Comparing eclipses
| Solar eclipse | Lunar eclipse | |
|---|---|---|
| Object in the middle | Moon | Earth |
| Shadow falls on | Earth | Moon |
| Sun, Moon, Earth order | Sun, Moon, Earth | Sun, Earth, Moon |
| Seen from | Part of the daytime side of Earth | Anywhere the Moon is above the horizon |
Section 7 of 11Classroom model of eclipses
Lamp
- Lamp it represents the Sun
White ball
- White ball it represents the Earth, with a lit side as day and a dark side as night
Tennis ball
- Tennis ball it represents the Moon
Solar eclipse
- Solar eclipse moving the Moon between the lamp and the Earth puts the Moon's shadow on the Earth
Lunar eclipse
- Lunar eclipse moving the Moon into the shadow of the Earth shows a lunar eclipse
Section 8 of 11Predicting eclipses
Early astronomers
- Early astronomers about 3000 years ago astronomers in the Middle East made the earliest known predictions of eclipses
Pattern
- Pattern solar eclipses repeat after every 223 lunar months, and one lunar month is 29.5 days
Method
- Method a pattern of observations is used to make predictions
Past eclipses
- Past eclipses modern calculations of past eclipses date events such as a battle in Greece in 585 BCE
Section 9 of 11More from the specification
More from the specification
Ray tracing geometrical eclipse model
- Ray tracing geometrical eclipse model constructing straight light ray paths around Moon and Earth illustrates a predictive geometrical shadow model.
Solar eclipse conditions
- Occurs during the new moon phase when the Moon aligns directly between Earth and Sun, casting its shadow upon Earth's surface.
Lunar eclipse conditions
- Occurs during the full moon phase when Earth moves directly between Sun and Moon, casting Earth's shadow across the lunar disc.
Umbral and penumbral shadows
- The umbra is the darkest core where sunlight is totally blocked;
- the penumbra experiences partial illumination.
Scales and angles in astronomy
- Although the Moon is 400 times smaller than the Sun, it is 400 times closer to Earth, so both appear almost identical in angular diameter.
Section 10 of 11Key terms
| Term | Meaning |
|---|---|
| Opaque | Not allowing light to pass through. |
| Shadow | Dark area where light is blocked. |
| Solar eclipse | The Moon blocks light from the Sun to Earth. |
| Lunar eclipse | The Earth blocks light from the Sun to the Moon. |
| Total | Whole of the light is blocked. |
| Partial | Only part of the light is blocked. |
| Ray | A straight line along which light travels. |
Section 11 of 11Exam technique
1
Thinking an eclipse is a different kind of light from the Sun — it is a shadow of the Moon or Earth.
2
Mixing up solar and lunar eclipses — in a solar eclipse the Moon is in the middle, in a lunar eclipse the Earth is.
3
Thinking eclipses happen every month — the Moon's orbit is tilted so they are rare.
4
Looking at the Sun during an eclipse — it damages the eyes permanently.
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