Here's a possible outline for such a class activity:
Review Newton's Law (Proportionally): Start by stating the law of gravitation as a proportionality: F ~ m1m2/r². Emphasize the dimensionless nature of the proportion. Centripetal Force (Proportionally): Introduce centripetal force, also as a proportionality: F_c ~ mv²/r. Stable Orbits: Explain that stable orbits represent a balance between these proportions: m1m2/r² ~ mv²/r. Kepler's Third Law (Proportionally): Derive the proportional form of Kepler's Third Law: M ~ r³/T². Introduce "Luna Mass": Define "1 luna mass" as the unit of mass. Explain that we'll be expressing all masses relative to the Moon. Earth's Mass in Luna Masses: Provide the Earth-Moon mass ratio (approximately 81.3) and show how to express Earth's mass in luna masses. Calculate the Sun's Mass (in Luna Masses): Guide students through the calculation of the Sun's mass in luna masses, using the proportional relationship derived earlier and the known orbital parameters of the Earth and Moon. Challenge Problems: Present additional problems, such as: Calculating the mass of Jupiter (in luna masses) given its orbital period and distance from the Sun. Calculating the mass of a hypothetical planet orbiting a different star, given its orbital parameters and the star's mass (expressed relative to the Sun). Discussing how uncertainties in the orbital measurements would affect the calculated masses.
Connect to G (Later): After students have worked through these exercises, you can then introduce G as a scaling factor that allows us to work with standard units (kg, m, s, N) and calculate absolute forces. This way, G is presented as a practical tool, not a fundamental mystery.
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