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Six original Cambridge-style questions on orbital speed: using v = 2(pi)r / T, rearranging it, and comparing orbits.
Write down the equation for orbital speed, and state what each symbol means.
A planet orbits a star in a circle of radius 6.0 x 10 to the 10 m, with a period of 2.0 x 10 to the 7 s. Calculate its orbital speed.
v = 1.9 x 10 to the 4 m/s (about 19000 m/s)
A satellite moves at 7500 m/s in a circular orbit of radius 7.0 x 10 to the 6 m. Calculate its period.
T = 5900 s (to 2 significant figures)
Two satellites have the same period, but one orbits at twice the radius of the other. Compare their orbital speeds.
Explain why a satellite with a longer period, at the same orbital radius, moves more slowly.
The Moon orbits the Earth at a radius of about 3.8 x 10 to the 8 m with a period of about 2.4 x 10 to the 6 s. Estimate its orbital speed.
v = 1000 m/s (about 1.0 x 10 to the 3 m/s)
Mark this once you have attempted all six and checked your working. It records a Practiced badge on the topic and adds a one-time bonus. Revealing the solutions alone does not count.