A method suitable for intermediate level astronomy courses is presented for the calculations of solar eclipses. The results are surprisingly good considering the simplifications used and the avoidance of spherical trigonometry.

This content is only available via PDF.
AAPT members receive access to the American Journal of Physics and The Physics Teacher as a member benefit. To learn more about this member benefit and becoming an AAPT member, visit the Joining AAPT page.