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Galilean Orbiting Object's Frequencies. GOOF. Original Objective. To determine the rotational frequencies of Jupiter's moons Also to determine to orbital periods of the Moons. What We Tried To Do.
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Original Objective • To determine the rotational frequencies of Jupiter's moons • Also to determine to orbital periods of the Moons
What We Tried To Do • Measure the relative brightness of two of Jupiter's moons, Europa and Callisto using the photometer and the 20” telescope. • This would allow us to determine the rotational period of these two moons by determining how long it took to form a distinctive pattern.
More of What We Tried To Do • Using the 12” and a CCD camera, we attempted to take pictures of Jupiter (and its moons) to determine the orbital period of the moons. • By seeing when the moons came back into original positions, then we could determine how long the moons took to orbit Jupiter.
“Results” • Most of the data was corrupted. • Both the data for the comparison star that we used (SAO 187992) and the data for the moons fluctuated in weird ways...
Day 1 • Comparison Star, then Europa and Callisto
Day 2 • Again, the comparison star and the 2 moons.
Day 3 • DANCE PARTY!!! • and then cloudy data. cry. • Finally, robotic beings rule the world. • Woohoo
So.. • In the end, we just got unlucky. But that's the way it goes.