Timing the Transit of Venus.
Introduction:
During the four previous transits of Venus in 1761, 1769, 1874 and 1882 astronomers carefully noted the start and stop times of the passage of Venus across the face of the Sun. When these times were combined with the latitude and longitudes of the various observers, astronomers could calculate the distance between Earth and Venus in terms of actual miles using the properties of triangles. This is similar to the method used by surveyors to determine the distance to remote, or inaccessible, objects on the surface of Earth.
In this activity, students will use the actual transit times recorded by astronomers during the 1882 and 1874 transits to determine the duration of the transit, and the time intervals between specific moments in the transit called 'Contacts'.
Benchmark:
The graphical display of numbers may help to show patterns such as trends or varying rates of change. Such patterns sometimes can be used to make predictions about the phenomenon being graphed.
Objective:
Students will calculate elapsed time and look for patterns.
Materials:
Vocabulary:
Ingress
Egress
1st Contact
2nd Contact
3rd Contact
4th Contact
Procedures: