Lesson Plans:
Orbital Forces
To demonstrate orbital motions and forces using a tennis ball swung by
a ribbon.
Gravity Gauge
To make a simple accelerometer to measure "G-forces" when you change
your motion.
Sunspot
Races
After you've looked at your images, you should be able to predict when
sunspot groups or active regions will disappear behind the Sun's limb
and, perhaps, eventually reappear from around the back side of the
Sun.
Gravity Is As Gravity Does
Gravity, whether it is holding you to the Earth’s surface or
swallowing light in a black hole, is the same force obeying the same
laws at all places in the observable Universe. We can measure it with
this simple lab.
Celestial Navigation
The gnomon, a fancy name for a vertical stick (must be thin and round)
stuck in the ground, is the most ancient of all astronomical
instruments. It can be used to chart the Sun's motion across the sky
so as to determine one's latitude and longitude, as well as the time
of true noon.
Sidereal Day
To find the difference between a solar day and a sidereal day you will
measure the intervals between the times when a star returns to a given
spot over successive evenings.
Motion of the Moon
The moon changes its position in the sky from day to day as a
consequence of its orbital motion around the earth. In this project,
we ask you to chart the motion of the moon against the background
stars.
Kepler's Laws
By reproducing ellipses via the "string-and-pencil method," the
students will draw ellipses and determine the eccentricities; by
measuring the orbits of five of Jupiter's moons, the students will
test Kepler's third law; and by using characteristics of Pluto's
orbit, the students will confirm Kepler's second law.
Motion of the Earth
Lab to show the motion of the Earth
Sun
Activities
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