Skip over navigation
Cambridge University Faculty of Mathematics NRich logo
menu search
  • Teachers expand_more
    • Early years
    • Primary
    • Secondary
    • Post-16
    • Events
    • Professional development
  • Students expand_more
    • Primary
    • Secondary
    • Post-16
  • Parents expand_more
    • Early Years
    • Primary
    • Secondary
    • Post-16
  • Problem-Solving Schools
  • About NRICH expand_more
    • About us
    • Impact stories
    • Support us
    • Our funders
    • Contact us
  • search

Or search by topic

Number and algebra

  • The Number System and Place Value
  • Calculations and Numerical Methods
  • Fractions, Decimals, Percentages, Ratio and Proportion
  • Properties of Numbers
  • Patterns, Sequences and Structure
  • Algebraic expressions, equations and formulae
  • Coordinates, Functions and Graphs

Geometry and measure

  • Angles, Polygons, and Geometrical Proof
  • 3D Geometry, Shape and Space
  • Measuring and calculating with units
  • Transformations and constructions
  • Pythagoras and Trigonometry
  • Vectors and Matrices

Probability and statistics

  • Handling, Processing and Representing Data
  • Probability

Working mathematically

  • Thinking mathematically
  • Developing positive attitudes
  • Cross-curricular contexts

Advanced mathematics

  • Decision Mathematics and Combinatorics
  • Advanced Probability and Statistics
  • Mechanics
  • Calculus

For younger learners

  • Early Years Foundation Stage

Perfect Eclipse

Age 14 to 16
Challenge Level Yellow starYellow starYellow star
  • Problem
  • Getting Started
  • Student Solutions
  • Teachers' Resources

Why do this problem?

This problem gives a good opportunity to practise some trigonometry in context. Students have the opportunity to make decisions about how to model the situation and what diagrams to draw in order to address the questions raised. Students will need to take into account considerations of lower and upper bounds, and the effects of changing measurements.

Possible approach

Perhaps start with some discussion about the apparent sizes of the sun and the moon, as viewed from Earth, and how the very similar apparent sizes makes solar eclipses possible.

Explain that the task is to work out the apparent sizes of the sun and the moon. In order to display this, students could cut out circles to represent the sun and the moon.

Ask students to consider in pairs what information they think they would need in order to work this out, and then provide any information they ask for from the data in the problem or using these information cards.

It may not be obvious to students at first that they can work out angles to the edge of the sun or moon, or how to use this to compare the apparent sizes of the sun and moon. The diagram in the Hint may help.

Key questions

What assumptions do you need to make to model the situation?
Can you draw a diagram to represent the appropriate lengths and angles?
What difference does it make that the orbits involved are elliptical?

Possible extension

Once students have had a chance to work out the necessary data for our moon, and drawn a diagram to show their findings, the problem provides data for other moons so that students can investigate how rare a perfect eclipse is within our solar system. This task could be divided up between groups with each group looking at the moons of a different planet, with everyone presenting their findings at the end of the lesson.

Possible support

The problem can be scaffolded by discussing modelling assumptions together as a class and working out what sort of diagrams will be helpful - the image in the Hint could be used as a starting point for discussion.


You may also like

Shaping the Universe I - Planet Earth

This article explores ths history of theories about the shape of our planet. It is the first in a series of articles looking at the significance of geometric shapes in the history of astronomy.

Shaping the Universe II - the Solar System

The second in a series of articles on visualising and modelling shapes in the history of astronomy.

Shaping the Universe III - to Infinity and Beyond

The third installment in our series on the shape of astronomical systems, this article explores galaxies and the universe beyond our solar system.

  • Tech help
  • Accessibility Statement
  • Sign up to our newsletter
  • Twitter X logo

The NRICH Project aims to enrich the mathematical experiences of all learners. To support this aim, members of the NRICH team work in a wide range of capacities, including providing professional development for teachers wishing to embed rich mathematical tasks into everyday classroom practice.

NRICH is part of the family of activities in the Millennium Mathematics Project.

University of Cambridge logo NRICH logo