Solar and lunar eclipses
Grade 6 Science Worksheet - Challenge Me

Circle the best answer.
Read this first
Table (model data), Model data: Moon dates
Date Phase and Moon near Earth's orbit plane? A. February new moon Moon near the plane of Earth's orbit: no B. April full moon: yes. C. June full moon: no. D. October new moon: yes.
Esme studies the example table of four Moon dates. Which date could have a lunar eclipse?
- D: the October new moon
- A: the February new moon
- B: the April full moon
- C: the June full moon
Using the same example table, Jun looks for a date that could have a solar eclipse. Which date fits?
- C: the June full moon
- D: the October new moon
- A: the February new moon
- B: the April full moon
Side view, not to scale
The Moon's tilted orbit crossing the plane of Earth's orbit at two points, on opposite sides; the April line-up is marked at one crossing.
A lunar eclipse happens at an April full moon. About when does Kira expect the Moon to line up with the Sun and Earth again?
- Exactly 12 months later, on the same date
- Next month, at the very next full moon
- About 6 months later, at the other crossing
- Next month, since a full moon's dark edge is Earth's shadow
Side view, not to scale; with the shadow not yet drawn. Luz's friend says a solar eclipse happens when Earth's shadow falls on the Sun. Which response is best?
- Agree: and it happens at each new moon
- Agree: Earth's shadow darkens the Sun
- Disagree: the Moon's shadow falls on Earth
- Disagree: it happens at full moon, when the Moon is bright
Milo's cousin says a lunar eclipse is just the Moon's new moon phase. Which response is best?
Orbit diagram, top view, not to scale: sunlight from the left; Earth in the center with its shadow pointing right; the Moon at new moon (left) and inside the shadow (right). Orbit diagram, top view, not to scale: sunlight from the left; Earth in the center with its shadow pointing right; the Moon at new moon (left) and inside the shadow (right). Orbit diagram, top view, not to scale sunlight Earth new moon Moon inside shadow shadow - Disagree: it happens at full moon, in Earth's shadow
- Disagree: it is seen from just a narrow path
- Agree: the new moon is Earth's shadow on the Moon
- Agree: the Moon's shadow covers the Moon then
“not to scale” A post claims that everyone on Earth's daytime side sees each total solar eclipse. Noah checks it. Which response is best?
Earth seen from space, not to scale: the day side lit, with a small dark spot where the Moon's inner shadow touches it. Earth seen from space, not to scale: the day side lit, with a small dark spot where the Moon's inner shadow touches it. Earth day side Moon's inner shadow - Agree: the Moon's shadow covers the whole day side
- Agree: Earth's shadow covers the whole Sun
- Disagree: totality is seen only along a narrow path
- Disagree: the Moon is as big as the Sun, so the path is wide
Sun diameter about 1,391,400 km; Moon diameter about 3,475 km. Pia reads the NASA size table. About how many times wider is the Sun than the Moon?
- About the same width
- About 40 times wider
- About 400 times wider
- About 4 times wider
“Classroom model, top view:” In a class model, a lamp is the Sun, a foam ball is the Moon and Zee's head is Earth. Where should Zee hold the ball to model a lunar eclipse?
Classroom model, top view: a lamp on the left; a student in the middle; ball spots W (between the head and the lamp), X (beside the head), Y (behind the head, inside its shadow) and Y-high (behind the head, raised above the shadow). Classroom model, top view: a lamp on the left; a student in the middle; ball spots W (between the head and the lamp), X (beside the head), Y (behind the head, inside its shadow) and Y-high (behind the head, raised above the shadow). lamp student W X Y Y-high shadow - At W, between the head and the lamp
- At Y, inside the head's shadow
- At X, beside the head
- At Y-high, just above the head's shadow
In the lamp model, where should Ari hold the ball so its shadow lands on Ari's face, modeling a solar eclipse?
Classroom model, top view: a lamp on the left; a student in the middle; ball spots W (exactly between the head and the lamp), W-high (between them but raised above the line) and Y (behind the head). Classroom model, top view: a lamp on the left; a student in the middle; ball spots W (exactly between the head and the lamp), W-high (between them but raised above the line) and Y (behind the head). lamp student W W-high Y - Anywhere, since the shadow fills the room
- At W, exactly in line with the lamp and the head
- At Y, behind the head
- At W-high, raised above the line
In the model, the ball's shadow on Bo's face is a small spot, not the whole face. What does this show about solar eclipses?
Close-up drawing of the model: a lamp, a ball and a face, with a small dark spot of shadow on one cheek. Close-up drawing of the model: a lamp, a ball and a face, with a small dark spot of shadow on one cheek. lamp ball face - The ball must be as big as the lamp to work
- The whole day side sees totality at once
- A small area of Earth sees totality
- The head's shadow is what makes a solar eclipse