Solar eclipses can be predicted with much precision using mathematical

equations which take into account the motion and size of the earth, moon,

and sun. The data presented in this set were computed by NASA long before

the solar eclipse of February 26, 1998,took place. Mathematical models of

the event enable observers to station themselves at prime viewing locations

which allow them to see a rare phenomenon - a total solar eclipse. The data

can also be used to predict the appearance of the partial eclipse for a given

observer position.

In this activity, we will download the calculated data into spreadsheets for sorting
and graphing variables which are involved in the eclipse.

Steps involved in this activity are:

FOR ADDITIONAL ASSISTANCE,
The buttons on the left are provided to enhance your understanding of activities.