Earth, Moon & Sun: Moon Phases — Drills · Grade 9 Science
Chapter: Earth, Moon & Solar SystemWhat these drills covers
By the end of Earth, Moon & Sun: Moon Phases you should be able to:
- I can explain that moon phases are caused by our changing view of the Moon's sunlit half, not by Earth's shadow.
- I can put the eight phases of the Moon in order, from new moon to full moon and back.
- I can explain why lunar and solar eclipses are rare compared to the regular monthly phases.
8 questions, multiple choice, numeric and written answer, each with a worked explanation.
Vocabulary used: phase, waxing, waning, new moon, synodic month.
Problem 1
- Earth's shadow on the Moon
- the changing angle from which we see the Moon's sunlit half
- clouds
- the Moon's own light
Answer and explanation
the changing angle from which we see the Moon's sunlit half
Half the Moon is always lit; the phase is how much of that half faces Earth.
Problem 2
Answer and explanation
29.5 days
About 29.5 days from new moon to new moon.
Problem 3
- between Earth and the Sun
- behind Earth from the Sun
- at right angles
- in Earth's shadow
Answer and explanation
between Earth and the Sun
Its sunlit side faces away from Earth, so it appears dark.
Problem 4
- full moon
- new moon
- first quarter
- any phase
Answer and explanation
new moon
The Moon must be between Earth and the Sun to block it.
Problem 5
- the Moon's orbit is tilted relative to Earth's orbit
- the Moon disappears
- Earth stops rotating
- the Sun moves
Answer and explanation
the Moon's orbit is tilted relative to Earth's orbit
The roughly 5° tilt means the three bodies usually fail to line up exactly.
Problem 6
- the Moon does not rotate
- its rotation period equals its orbital period
- Earth does not rotate
- of its phases
Answer and explanation
its rotation period equals its orbital period
Tidal locking makes one rotation take exactly one orbit.
Problem 7
Answer and explanation
In a lunar eclipse Earth's shadow falls on the Moon, so anyone on the night side of Earth who can see the Moon sees it darken — roughly half the planet at once. In a solar eclipse the Moon's much smaller shadow falls on Earth, and totality is confined to a narrow track a few hundred kilometres wide, so only people within that track see it.
Response criteria
- State a scientifically accurate conclusion.
- Show the data, mechanism, or calculation that supports it.
- Include units, conditions, or limits where relevant.
Problem 8
Answer and explanation
Phases come from the changing angle at which we view the Moon's permanently sunlit half, not from Earth's shadow. The evidence is that a full moon occurs when the Moon is opposite the Sun — exactly where Earth's shadow would fall — yet it is fully lit rather than dark, and phases cycle smoothly every month while eclipses are rare. Earth's shadow does cause lunar eclipses, which is a separate and occasional event.
Response criteria
- State a scientifically accurate conclusion.
- Show the data, mechanism, or calculation that supports it.
- Include units, conditions, or limits where relevant.